---
_id: '10698'
abstract:
- lang: eng
text: This is the second of three talks describing the observation and characterization
of a ferromagnetic moiré heterostructure based on twisted bilayer graphene aligned
to hexagonal boron nitride. I will compare the qualitative and quantitative features
of this observed quantum anomalous Hall state to traditional systems engineered
from thin film (Bi,Sb)2Te3 topological insulators. In particular, we find that
the measured electronic energy gap of ~30K is several times higher than the Curie
temperature, consistent with a lack of disorder associated with magnetic dopants.
In this system, the quantization arises from spontaneous ferromagnetic polarization
into a single spin and valley moiré subband, which is topological despite the
lack of spin orbit coupling. I will also discuss the observation of current induced
switching, which allows the magnetic state of the heterostructure to be controllably
reversed with currents as small as a few nanoamperes.
acknowledgement: I would like to thank the MURI Program, AFOSR, Sloan Foundation,
and the ARO for their generous support of this work.
alternative_title:
- Bulletin of the American Physical Society
article_number: B59.00011
article_processing_charge: No
arxiv: 1
author:
- first_name: Marec
full_name: Serlin, Marec
last_name: Serlin
- first_name: Charles
full_name: Tschirhart, Charles
last_name: Tschirhart
- first_name: Hryhoriy
full_name: Polshyn, Hryhoriy
id: edfc7cb1-526e-11ec-b05a-e6ecc27e4e48
last_name: Polshyn
orcid: 0000-0001-8223-8896
- first_name: Yuxuan
full_name: Zhang, Yuxuan
last_name: Zhang
- first_name: Jiacheng
full_name: Zhu, Jiacheng
last_name: Zhu
- first_name: Martin E.
full_name: Huber, Martin E.
last_name: Huber
- first_name: Leon
full_name: Balents, Leon
last_name: Balents
- first_name: Kenji
full_name: Watanabe, Kenji
last_name: Watanabe
- first_name: Takashi
full_name: Tanaguchi, Takashi
last_name: Tanaguchi
- first_name: Andrea
full_name: Young, Andrea
last_name: Young
citation:
ama: 'Serlin M, Tschirhart C, Polshyn H, et al. Intrinsic quantized anomalous Hall
effect in a moiré heterostructure, part II: Temperature dependence and current
switching. In: APS March Meeting 2020. Vol 65. American Physical Society;
2020.'
apa: 'Serlin, M., Tschirhart, C., Polshyn, H., Zhang, Y., Zhu, J., Huber, M. E.,
… Young, A. (2020). Intrinsic quantized anomalous Hall effect in a moiré heterostructure,
part II: Temperature dependence and current switching. In APS March Meeting
2020 (Vol. 65). Denver, CO, United States: American Physical Society.'
chicago: 'Serlin, Marec, Charles Tschirhart, Hryhoriy Polshyn, Yuxuan Zhang, Jiacheng
Zhu, Martin E. Huber, Leon Balents, Kenji Watanabe, Takashi Tanaguchi, and Andrea
Young. “Intrinsic Quantized Anomalous Hall Effect in a Moiré Heterostructure,
Part II: Temperature Dependence and Current Switching.” In APS March Meeting
2020, Vol. 65. American Physical Society, 2020.'
ieee: 'M. Serlin et al., “Intrinsic quantized anomalous Hall effect in a
moiré heterostructure, part II: Temperature dependence and current switching,”
in APS March Meeting 2020, Denver, CO, United States, 2020, vol. 65, no.
1.'
ista: 'Serlin M, Tschirhart C, Polshyn H, Zhang Y, Zhu J, Huber ME, Balents L, Watanabe
K, Tanaguchi T, Young A. 2020. Intrinsic quantized anomalous Hall effect in a
moiré heterostructure, part II: Temperature dependence and current switching.
APS March Meeting 2020. APS: American Physical Society, Bulletin of the American
Physical Society, vol. 65, B59.00011.'
mla: 'Serlin, Marec, et al. “Intrinsic Quantized Anomalous Hall Effect in a Moiré
Heterostructure, Part II: Temperature Dependence and Current Switching.” APS
March Meeting 2020, vol. 65, no. 1, B59.00011, American Physical Society,
2020.'
short: M. Serlin, C. Tschirhart, H. Polshyn, Y. Zhang, J. Zhu, M.E. Huber, L. Balents,
K. Watanabe, T. Tanaguchi, A. Young, in:, APS March Meeting 2020, American Physical
Society, 2020.
conference:
end_date: 2020-03-06
location: Denver, CO, United States
name: 'APS: American Physical Society'
start_date: 2020-03-02
date_created: 2022-01-28T10:46:57Z
date_published: 2020-03-01T00:00:00Z
date_updated: 2023-02-21T15:57:52Z
day: '01'
extern: '1'
external_id:
arxiv:
- '1907.00261'
intvolume: ' 65'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://meetings.aps.org/Meeting/MAR20/Session/B59.11
month: '03'
oa: 1
oa_version: Published Version
publication: APS March Meeting 2020
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
related_material:
record:
- id: '10619'
relation: other
status: public
status: public
title: 'Intrinsic quantized anomalous Hall effect in a moiré heterostructure, part
II: Temperature dependence and current switching'
type: conference
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
volume: 65
year: '2020'
...
---
_id: '10699'
abstract:
- lang: eng
text: This is the third of three talks describing the observation and characterization
of a ferromagnetic moiré heterostructure based on twisted bilayer graphene aligned
to hexagonal boron nitride. In this segment I will present scanning probe magnetometry
data acquired using a nanoSQUID-on-tip microscope, which provides ~150 nm spatial
resolution and a field sensitivity of ~10 nT/rtHz. We study the distribution of
magnetic domains within the device as a function of density, magnetic field training,
and DC current. Our data allow us to constrain the magnitude of the orbital magnetic
moment of the electrons in the QAH state. Comparison with simultaneously acquired
transport data allows us to precisely correlate single domain dynamics with discrete
jumps in the observed anomalous Hall signal.
acknowledgement: I would like to thank the MURI program, Sloan foundation, AFOSR,
and ARO for their generous support of this work. I would also like to thank the
NSF GRFP and the Hertz foundation for their generous support of my graduate studies.
alternative_title:
- Bulletin of the American Physical Society
article_number: B59.00013
article_processing_charge: No
arxiv: 1
author:
- first_name: Charles
full_name: Tschirhart, Charles
last_name: Tschirhart
- first_name: Marec
full_name: Serlin, Marec
last_name: Serlin
- first_name: Hryhoriy
full_name: Polshyn, Hryhoriy
id: edfc7cb1-526e-11ec-b05a-e6ecc27e4e48
last_name: Polshyn
orcid: 0000-0001-8223-8896
- first_name: Yuxuan
full_name: Zhang, Yuxuan
last_name: Zhang
- first_name: Jiacheng
full_name: Zhu, Jiacheng
last_name: Zhu
- first_name: Leon
full_name: Balents, Leon
last_name: Balents
- first_name: Martin E.
full_name: Huber, Martin E.
last_name: Huber
- first_name: Kenji
full_name: Watanabe, Kenji
last_name: Watanabe
- first_name: Takashi
full_name: Tanaguchi, Takashi
last_name: Tanaguchi
- first_name: Andrea
full_name: Young, Andrea
last_name: Young
citation:
ama: 'Tschirhart C, Serlin M, Polshyn H, et al. Intrinsic quantized anomalous Hall
effect in a moiré heterostructure, part III: Scanning probe magnetometry. In:
APS March Meeting 2020. Vol 65. American Physical Society; 2020.'
apa: 'Tschirhart, C., Serlin, M., Polshyn, H., Zhang, Y., Zhu, J., Balents, L.,
… Young, A. (2020). Intrinsic quantized anomalous Hall effect in a moiré heterostructure,
part III: Scanning probe magnetometry. In APS March Meeting 2020 (Vol.
65). Denver, CO, United States: American Physical Society.'
chicago: 'Tschirhart, Charles, Marec Serlin, Hryhoriy Polshyn, Yuxuan Zhang, Jiacheng
Zhu, Leon Balents, Martin E. Huber, Kenji Watanabe, Takashi Tanaguchi, and Andrea
Young. “Intrinsic Quantized Anomalous Hall Effect in a Moiré Heterostructure,
Part III: Scanning Probe Magnetometry.” In APS March Meeting 2020, Vol.
65. American Physical Society, 2020.'
ieee: 'C. Tschirhart et al., “Intrinsic quantized anomalous Hall effect in
a moiré heterostructure, part III: Scanning probe magnetometry,” in APS March
Meeting 2020, Denver, CO, United States, 2020, vol. 65, no. 1.'
ista: 'Tschirhart C, Serlin M, Polshyn H, Zhang Y, Zhu J, Balents L, Huber ME, Watanabe
K, Tanaguchi T, Young A. 2020. Intrinsic quantized anomalous Hall effect in a
moiré heterostructure, part III: Scanning probe magnetometry. APS March Meeting
2020. APS: American Physical Society, Bulletin of the American Physical Society,
vol. 65, B59.00013.'
mla: 'Tschirhart, Charles, et al. “Intrinsic Quantized Anomalous Hall Effect in
a Moiré Heterostructure, Part III: Scanning Probe Magnetometry.” APS March
Meeting 2020, vol. 65, no. 1, B59.00013, American Physical Society, 2020.'
short: C. Tschirhart, M. Serlin, H. Polshyn, Y. Zhang, J. Zhu, L. Balents, M.E.
Huber, K. Watanabe, T. Tanaguchi, A. Young, in:, APS March Meeting 2020, American
Physical Society, 2020.
conference:
end_date: 2020-03-06
location: Denver, CO, United States
name: 'APS: American Physical Society'
start_date: 2020-03-02
date_created: 2022-01-28T10:57:49Z
date_published: 2020-03-01T00:00:00Z
date_updated: 2023-02-21T15:57:52Z
day: '01'
extern: '1'
external_id:
arxiv:
- '1907.00261'
intvolume: ' 65'
issue: '1'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://meetings.aps.org/Meeting/MAR20/Session/B59.13
month: '03'
oa: 1
oa_version: Published Version
publication: APS March Meeting 2020
publication_identifier:
issn:
- 0003-0503
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
related_material:
record:
- id: '10619'
relation: other
status: public
status: public
title: 'Intrinsic quantized anomalous Hall effect in a moiré heterostructure, part
III: Scanning probe magnetometry'
type: conference
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
volume: 65
year: '2020'
...
---
_id: '10701'
abstract:
- lang: eng
text: Partially filled Landau levels host competing electronic orders. For example,
electron solids may prevail close to integer filling of the Landau levels before
giving way to fractional quantum Hall liquids at higher carrier density1,2. Here,
we report the observation of an electron solid with non-collinear spin texture
in monolayer graphene, consistent with solidification of skyrmions3—topological
spin textures characterized by quantized electrical charge4,5. We probe the spin
texture of the solids using a modified Corbino geometry that allows ferromagnetic
magnons to be launched and detected6,7. We find that magnon transport is highly
efficient when one Landau level is filled (ν=1), consistent with quantum Hall
ferromagnetic spin polarization. However, even minimal doping immediately quenches
the magnon signal while leaving the vanishing low-temperature charge conductivity
unchanged. Our results can be understood by the formation of a solid of charged
skyrmions near ν=1, whose non-collinear spin texture leads to rapid magnon decay.
Data near fractional fillings show evidence of several fractional skyrmion solids,
suggesting that graphene hosts a highly tunable landscape of coupled spin and
charge orders.
acknowledgement: We acknowledge discussions with B. Halperin, C. Huang, A. Macdonald
and M. Zalatel. Experimental work at UCSB was supported by the Army Research Office
under awards nos. MURI W911NF-16-1-0361 and W911NF-16-1-0482. K.W. and T.T. acknowledge
support from the Elemental Strategy Initiative conducted by MEXT (Japan) and CREST
(JPMJCR15F3), JST. A.F.Y. acknowledges the support of the David and Lucile Packard
Foundation and and Alfred. P. Sloan Foundation.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Haoxin
full_name: Zhou, Haoxin
last_name: Zhou
- first_name: Hryhoriy
full_name: Polshyn, Hryhoriy
id: edfc7cb1-526e-11ec-b05a-e6ecc27e4e48
last_name: Polshyn
orcid: 0000-0001-8223-8896
- first_name: Takashi
full_name: Taniguchi, Takashi
last_name: Taniguchi
- first_name: Kenji
full_name: Watanabe, Kenji
last_name: Watanabe
- first_name: Andrea F.
full_name: Young, Andrea F.
last_name: Young
citation:
ama: Zhou H, Polshyn H, Taniguchi T, Watanabe K, Young AF. Skyrmion solids in monolayer
graphene. Nature Physics. 2020;16(2):154-158. doi:10.1038/s41567-019-0729-8
apa: Zhou, H., Polshyn, H., Taniguchi, T., Watanabe, K., & Young, A. F. (2020).
Skyrmion solids in monolayer graphene. Nature Physics. Springer Nature.
https://doi.org/10.1038/s41567-019-0729-8
chicago: Zhou, Haoxin, Hryhoriy Polshyn, Takashi Taniguchi, Kenji Watanabe, and
Andrea F. Young. “Skyrmion Solids in Monolayer Graphene.” Nature Physics.
Springer Nature, 2020. https://doi.org/10.1038/s41567-019-0729-8.
ieee: H. Zhou, H. Polshyn, T. Taniguchi, K. Watanabe, and A. F. Young, “Skyrmion
solids in monolayer graphene,” Nature Physics, vol. 16, no. 2. Springer
Nature, pp. 154–158, 2020.
ista: Zhou H, Polshyn H, Taniguchi T, Watanabe K, Young AF. 2020. Skyrmion solids
in monolayer graphene. Nature Physics. 16(2), 154–158.
mla: Zhou, Haoxin, et al. “Skyrmion Solids in Monolayer Graphene.” Nature Physics,
vol. 16, no. 2, Springer Nature, 2020, pp. 154–58, doi:10.1038/s41567-019-0729-8.
short: H. Zhou, H. Polshyn, T. Taniguchi, K. Watanabe, A.F. Young, Nature Physics
16 (2020) 154–158.
date_created: 2022-01-28T12:04:09Z
date_published: 2020-02-01T00:00:00Z
date_updated: 2022-01-31T07:10:07Z
day: '01'
doi: 10.1038/s41567-019-0729-8
extern: '1'
external_id:
arxiv:
- '1904.11485'
intvolume: ' 16'
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1904.11485
month: '02'
oa: 1
oa_version: Preprint
page: 154-158
publication: Nature Physics
publication_identifier:
eissn:
- 1745-2481
issn:
- 1745-2473
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
status: public
title: Skyrmion solids in monolayer graphene
type: journal_article
user_id: 8b945eb4-e2f2-11eb-945a-df72226e66a9
volume: 16
year: '2020'
...
---
_id: '10862'
abstract:
- lang: eng
text: We consider the sum of two large Hermitian matrices A and B with a Haar unitary
conjugation bringing them into a general relative position. We prove that the
eigenvalue density on the scale slightly above the local eigenvalue spacing is
asymptotically given by the free additive convolution of the laws of A and B as
the dimension of the matrix increases. This implies optimal rigidity of the eigenvalues
and optimal rate of convergence in Voiculescu's theorem. Our previous works [4],
[5] established these results in the bulk spectrum, the current paper completely
settles the problem at the spectral edges provided they have the typical square-root
behavior. The key element of our proof is to compensate the deterioration of the
stability of the subordination equations by sharp error estimates that properly
account for the local density near the edge. Our results also hold if the Haar
unitary matrix is replaced by the Haar orthogonal matrix.
acknowledgement: Partially supported by ERC Advanced Grant RANMAT No. 338804.
article_number: '108639'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Zhigang
full_name: Bao, Zhigang
id: 442E6A6C-F248-11E8-B48F-1D18A9856A87
last_name: Bao
orcid: 0000-0003-3036-1475
- first_name: László
full_name: Erdös, László
id: 4DBD5372-F248-11E8-B48F-1D18A9856A87
last_name: Erdös
orcid: 0000-0001-5366-9603
- first_name: Kevin
full_name: Schnelli, Kevin
last_name: Schnelli
citation:
ama: Bao Z, Erdös L, Schnelli K. Spectral rigidity for addition of random matrices
at the regular edge. Journal of Functional Analysis. 2020;279(7). doi:10.1016/j.jfa.2020.108639
apa: Bao, Z., Erdös, L., & Schnelli, K. (2020). Spectral rigidity for addition
of random matrices at the regular edge. Journal of Functional Analysis.
Elsevier. https://doi.org/10.1016/j.jfa.2020.108639
chicago: Bao, Zhigang, László Erdös, and Kevin Schnelli. “Spectral Rigidity for
Addition of Random Matrices at the Regular Edge.” Journal of Functional Analysis.
Elsevier, 2020. https://doi.org/10.1016/j.jfa.2020.108639.
ieee: Z. Bao, L. Erdös, and K. Schnelli, “Spectral rigidity for addition of random
matrices at the regular edge,” Journal of Functional Analysis, vol. 279,
no. 7. Elsevier, 2020.
ista: Bao Z, Erdös L, Schnelli K. 2020. Spectral rigidity for addition of random
matrices at the regular edge. Journal of Functional Analysis. 279(7), 108639.
mla: Bao, Zhigang, et al. “Spectral Rigidity for Addition of Random Matrices at
the Regular Edge.” Journal of Functional Analysis, vol. 279, no. 7, 108639,
Elsevier, 2020, doi:10.1016/j.jfa.2020.108639.
short: Z. Bao, L. Erdös, K. Schnelli, Journal of Functional Analysis 279 (2020).
date_created: 2022-03-18T10:18:59Z
date_published: 2020-10-15T00:00:00Z
date_updated: 2023-08-24T14:08:42Z
day: '15'
department:
- _id: LaEr
doi: 10.1016/j.jfa.2020.108639
ec_funded: 1
external_id:
arxiv:
- '1708.01597'
isi:
- '000559623200009'
intvolume: ' 279'
isi: 1
issue: '7'
keyword:
- Analysis
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1708.01597
month: '10'
oa: 1
oa_version: Preprint
project:
- _id: 258DCDE6-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '338804'
name: Random matrices, universality and disordered quantum systems
publication: Journal of Functional Analysis
publication_identifier:
issn:
- 0022-1236
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: Spectral rigidity for addition of random matrices at the regular edge
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 279
year: '2020'
...
---
_id: '10865'
abstract:
- lang: eng
text: "We introduce the notion of Witness Maps as a cryptographic notion of a proof
system. A Unique Witness Map (UWM) deterministically maps all witnesses for an
\ NP statement to a single representative witness, resulting in a computationally
sound, deterministic-prover, non-interactive witness independent proof system.
A relaxation of UWM, called Compact Witness Map (CWM), maps all the witnesses
to a small number of witnesses, resulting in a “lossy” deterministic-prover, non-interactive
proof-system. We also define a Dual Mode Witness Map (DMWM) which adds an “extractable”
mode to a CWM.\r\nOur main construction is a DMWM for all NP relations, assuming
sub-exponentially secure indistinguishability obfuscation ( iO ), along with
standard cryptographic assumptions. The DMWM construction relies on a CWM and
a new primitive called Cumulative All-Lossy-But-One Trapdoor Functions (C-ALBO-TDF),
both of which are in turn instantiated based on iO and other primitives. Our
instantiation of a CWM is in fact a UWM; in turn, we show that a UWM implies Witness
Encryption. Along the way to constructing UWM and C-ALBO-TDF, we also construct,
from standard assumptions, Puncturable Digital Signatures and a new primitive
called Cumulative Lossy Trapdoor Functions (C-LTDF). The former improves up on
a construction of Bellare et al. (Eurocrypt 2016), who relied on sub-exponentially
secure iO and sub-exponentially secure OWF.\r\nAs an application of our constructions,
we show how to use a DMWM to construct the first leakage and tamper-resilient
signatures with a deterministic signer, thereby solving a decade old open problem
posed by Katz and Vaikunthanathan (Asiacrypt 2009), by Boyle, Segev and Wichs
(Eurocrypt 2011), as well as by Faonio and Venturi (Asiacrypt 2016). Our construction
achieves the optimal leakage rate of 1−o(1) ."
acknowledgement: We would like to thank the anonymous reviewers of PKC 2019 for their
useful comments and suggestions. We thank Omer Paneth for pointing out to us the
connection between Unique Witness Maps (UWM) and Witness encryption (WE). The first
author would like to acknowledge Pandu Rangan for his involvement during the initial
discussion phase of the project.
article_processing_charge: No
author:
- first_name: Suvradip
full_name: Chakraborty, Suvradip
id: B9CD0494-D033-11E9-B219-A439E6697425
last_name: Chakraborty
- first_name: Manoj
full_name: Prabhakaran, Manoj
last_name: Prabhakaran
- first_name: Daniel
full_name: Wichs, Daniel
last_name: Wichs
citation:
ama: 'Chakraborty S, Prabhakaran M, Wichs D. Witness maps and applications. In:
Kiayias A, ed. Public-Key Cryptography. Vol 12110. LNCS. Cham: Springer
Nature; 2020:220-246. doi:10.1007/978-3-030-45374-9_8'
apa: 'Chakraborty, S., Prabhakaran, M., & Wichs, D. (2020). Witness maps and
applications. In A. Kiayias (Ed.), Public-Key Cryptography (Vol. 12110,
pp. 220–246). Cham: Springer Nature. https://doi.org/10.1007/978-3-030-45374-9_8'
chicago: 'Chakraborty, Suvradip, Manoj Prabhakaran, and Daniel Wichs. “Witness Maps
and Applications.” In Public-Key Cryptography, edited by A Kiayias, 12110:220–46.
LNCS. Cham: Springer Nature, 2020. https://doi.org/10.1007/978-3-030-45374-9_8.'
ieee: 'S. Chakraborty, M. Prabhakaran, and D. Wichs, “Witness maps and applications,”
in Public-Key Cryptography, vol. 12110, A. Kiayias, Ed. Cham: Springer
Nature, 2020, pp. 220–246.'
ista: 'Chakraborty S, Prabhakaran M, Wichs D. 2020.Witness maps and applications.
In: Public-Key Cryptography. vol. 12110, 220–246.'
mla: Chakraborty, Suvradip, et al. “Witness Maps and Applications.” Public-Key
Cryptography, edited by A Kiayias, vol. 12110, Springer Nature, 2020, pp.
220–46, doi:10.1007/978-3-030-45374-9_8.
short: S. Chakraborty, M. Prabhakaran, D. Wichs, in:, A. Kiayias (Ed.), Public-Key
Cryptography, Springer Nature, Cham, 2020, pp. 220–246.
date_created: 2022-03-18T11:35:51Z
date_published: 2020-04-29T00:00:00Z
date_updated: 2023-09-05T15:10:02Z
day: '29'
doi: 10.1007/978-3-030-45374-9_8
editor:
- first_name: A
full_name: Kiayias, A
last_name: Kiayias
intvolume: ' 12110'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://eprint.iacr.org/2020/090
month: '04'
oa: 1
oa_version: Preprint
page: 220-246
place: Cham
publication: Public-Key Cryptography
publication_identifier:
eissn:
- 1611-3349
isbn:
- '9783030453732'
- '9783030453749'
issn:
- 0302-9743
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
series_title: LNCS
status: public
title: Witness maps and applications
type: book_chapter
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 12110
year: '2020'
...
---
_id: '10866'
abstract:
- lang: eng
text: Recent discoveries have shown that, when two layers of van der Waals (vdW)
materials are superimposed with a relative twist angle between them, the electronic
properties of the coupled system can be dramatically altered. Here, we demonstrate
that a similar concept can be extended to the optics realm, particularly to propagating
phonon polaritons–hybrid light-matter interactions. To do this, we fabricate stacks
composed of two twisted slabs of a vdW crystal (α-MoO3) supporting anisotropic
phonon polaritons (PhPs), and image the propagation of the latter when launched
by localized sources. Our images reveal that, under a critical angle, the PhPs
isofrequency curve undergoes a topological transition, in which the propagation
of PhPs is strongly guided (canalization regime) along predetermined directions
without geometric spreading. These results demonstrate a new degree of freedom
(twist angle) for controlling the propagation of polaritons at the nanoscale with
potential for nanoimaging, (bio)-sensing, or heat management.
acknowledgement: "J.T.-G. and G.Á.-P. acknowledge support through the Severo Ochoa
Program from the\r\nGovernment of the Principality of Asturias (nos. PA-18-PF-BP17-126
and PA20-PF-BP19-053,\r\nrespectively). J. M-S acknowledges financial support through
the Ramón y Cajal Program from\r\nthe Government of Spain (RYC2018-026196-I). A.Y.N.
acknowledges the Spanish Ministry of\r\nScience, Innovation and Universities (national
project no. MAT201788358-C3-3-R). P.A.-G.\r\nacknowledges support from the European
Research Council under starting grant no. 715496,\r\n2DNANOPTICA."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jiahua
full_name: Duan, Jiahua
last_name: Duan
- first_name: Nathaniel
full_name: Capote-Robayna, Nathaniel
last_name: Capote-Robayna
- first_name: Javier
full_name: Taboada-Gutiérrez, Javier
last_name: Taboada-Gutiérrez
- first_name: Gonzalo
full_name: Álvarez-Pérez, Gonzalo
last_name: Álvarez-Pérez
- first_name: Ivan
full_name: Prieto Gonzalez, Ivan
id: 2A307FE2-F248-11E8-B48F-1D18A9856A87
last_name: Prieto Gonzalez
orcid: 0000-0002-7370-5357
- first_name: Javier
full_name: Martín-Sánchez, Javier
last_name: Martín-Sánchez
- first_name: Alexey Y.
full_name: Nikitin, Alexey Y.
last_name: Nikitin
- first_name: Pablo
full_name: Alonso-González, Pablo
last_name: Alonso-González
citation:
ama: 'Duan J, Capote-Robayna N, Taboada-Gutiérrez J, et al. Twisted nano-optics:
Manipulating light at the nanoscale with twisted phonon polaritonic slabs. Nano
Letters. 2020;20(7):5323-5329. doi:10.1021/acs.nanolett.0c01673'
apa: 'Duan, J., Capote-Robayna, N., Taboada-Gutiérrez, J., Álvarez-Pérez, G., Prieto
Gonzalez, I., Martín-Sánchez, J., … Alonso-González, P. (2020). Twisted nano-optics:
Manipulating light at the nanoscale with twisted phonon polaritonic slabs. Nano
Letters. American Chemical Society. https://doi.org/10.1021/acs.nanolett.0c01673'
chicago: 'Duan, Jiahua, Nathaniel Capote-Robayna, Javier Taboada-Gutiérrez, Gonzalo
Álvarez-Pérez, Ivan Prieto Gonzalez, Javier Martín-Sánchez, Alexey Y. Nikitin,
and Pablo Alonso-González. “Twisted Nano-Optics: Manipulating Light at the Nanoscale
with Twisted Phonon Polaritonic Slabs.” Nano Letters. American Chemical
Society, 2020. https://doi.org/10.1021/acs.nanolett.0c01673.'
ieee: 'J. Duan et al., “Twisted nano-optics: Manipulating light at the nanoscale
with twisted phonon polaritonic slabs,” Nano Letters, vol. 20, no. 7. American
Chemical Society, pp. 5323–5329, 2020.'
ista: 'Duan J, Capote-Robayna N, Taboada-Gutiérrez J, Álvarez-Pérez G, Prieto Gonzalez
I, Martín-Sánchez J, Nikitin AY, Alonso-González P. 2020. Twisted nano-optics:
Manipulating light at the nanoscale with twisted phonon polaritonic slabs. Nano
Letters. 20(7), 5323–5329.'
mla: 'Duan, Jiahua, et al. “Twisted Nano-Optics: Manipulating Light at the Nanoscale
with Twisted Phonon Polaritonic Slabs.” Nano Letters, vol. 20, no. 7, American
Chemical Society, 2020, pp. 5323–29, doi:10.1021/acs.nanolett.0c01673.'
short: J. Duan, N. Capote-Robayna, J. Taboada-Gutiérrez, G. Álvarez-Pérez, I. Prieto
Gonzalez, J. Martín-Sánchez, A.Y. Nikitin, P. Alonso-González, Nano Letters 20
(2020) 5323–5329.
date_created: 2022-03-18T11:37:38Z
date_published: 2020-07-01T00:00:00Z
date_updated: 2023-09-05T12:05:58Z
day: '01'
department:
- _id: NanoFab
doi: 10.1021/acs.nanolett.0c01673
external_id:
arxiv:
- '2004.14599'
isi:
- '000548893200082'
pmid:
- '32530634'
intvolume: ' 20'
isi: 1
issue: '7'
keyword:
- Mechanical Engineering
- Condensed Matter Physics
- General Materials Science
- General Chemistry
- Bioengineering
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2004.14599
month: '07'
oa: 1
oa_version: Preprint
page: 5323-5329
pmid: 1
publication: Nano Letters
publication_identifier:
eissn:
- 1530-6992
issn:
- 1530-6984
publication_status: published
publisher: American Chemical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Twisted nano-optics: Manipulating light at the nanoscale with twisted phonon
polaritonic slabs'
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 20
year: '2020'
...
---
_id: '10867'
abstract:
- lang: eng
text: In this paper we find a tight estimate for Gromov’s waist of the balls in
spaces of constant curvature, deduce the estimates for the balls in Riemannian
manifolds with upper bounds on the curvature (CAT(ϰ)-spaces), and establish similar
result for normed spaces.
acknowledgement: ' Supported by the Russian Foundation for Basic Research grant 18-01-00036.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Arseniy
full_name: Akopyan, Arseniy
id: 430D2C90-F248-11E8-B48F-1D18A9856A87
last_name: Akopyan
orcid: 0000-0002-2548-617X
- first_name: Roman
full_name: Karasev, Roman
last_name: Karasev
citation:
ama: Akopyan A, Karasev R. Waist of balls in hyperbolic and spherical spaces. International
Mathematics Research Notices. 2020;2020(3):669-697. doi:10.1093/imrn/rny037
apa: Akopyan, A., & Karasev, R. (2020). Waist of balls in hyperbolic and spherical
spaces. International Mathematics Research Notices. Oxford University Press.
https://doi.org/10.1093/imrn/rny037
chicago: Akopyan, Arseniy, and Roman Karasev. “Waist of Balls in Hyperbolic and
Spherical Spaces.” International Mathematics Research Notices. Oxford University
Press, 2020. https://doi.org/10.1093/imrn/rny037.
ieee: A. Akopyan and R. Karasev, “Waist of balls in hyperbolic and spherical spaces,”
International Mathematics Research Notices, vol. 2020, no. 3. Oxford University
Press, pp. 669–697, 2020.
ista: Akopyan A, Karasev R. 2020. Waist of balls in hyperbolic and spherical spaces.
International Mathematics Research Notices. 2020(3), 669–697.
mla: Akopyan, Arseniy, and Roman Karasev. “Waist of Balls in Hyperbolic and Spherical
Spaces.” International Mathematics Research Notices, vol. 2020, no. 3,
Oxford University Press, 2020, pp. 669–97, doi:10.1093/imrn/rny037.
short: A. Akopyan, R. Karasev, International Mathematics Research Notices 2020 (2020)
669–697.
date_created: 2022-03-18T11:39:30Z
date_published: 2020-02-01T00:00:00Z
date_updated: 2023-08-24T14:19:55Z
day: '01'
department:
- _id: HeEd
doi: 10.1093/imrn/rny037
external_id:
arxiv:
- '1702.07513'
isi:
- '000522852700002'
intvolume: ' 2020'
isi: 1
issue: '3'
keyword:
- General Mathematics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1702.07513
month: '02'
oa: 1
oa_version: Preprint
page: 669-697
publication: International Mathematics Research Notices
publication_identifier:
eissn:
- 1687-0247
issn:
- 1073-7928
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Waist of balls in hyperbolic and spherical spaces
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 2020
year: '2020'
...
---
_id: '11054'
abstract:
- lang: eng
text: In recent years, the nuclear pore complex (NPC) has emerged as a key player
in genome regulation and cellular homeostasis. New discoveries have revealed that
the NPC has multiple cellular functions besides mediating the molecular exchange
between the nucleus and the cytoplasm. In this review, we discuss non-transport
aspects of the NPC focusing on the NPC-genome interaction, the extreme longevity
of the NPC proteins, and NPC dysfunction in age-related diseases. The examples
summarized herein demonstrate that the NPC, which first evolved to enable the
biochemical communication between the nucleus and the cytoplasm, now doubles as
the gatekeeper of cellular identity and aging.
article_processing_charge: No
article_type: review
author:
- first_name: Ukrae H.
full_name: Cho, Ukrae H.
last_name: Cho
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: 'Cho UH, Hetzer M. Nuclear periphery takes center stage: The role of nuclear
pore complexes in cell identity and aging. Neuron. 2020;106(6):899-911.
doi:10.1016/j.neuron.2020.05.031'
apa: 'Cho, U. H., & Hetzer, M. (2020). Nuclear periphery takes center stage:
The role of nuclear pore complexes in cell identity and aging. Neuron.
Elsevier. https://doi.org/10.1016/j.neuron.2020.05.031'
chicago: 'Cho, Ukrae H., and Martin Hetzer. “Nuclear Periphery Takes Center Stage:
The Role of Nuclear Pore Complexes in Cell Identity and Aging.” Neuron.
Elsevier, 2020. https://doi.org/10.1016/j.neuron.2020.05.031.'
ieee: 'U. H. Cho and M. Hetzer, “Nuclear periphery takes center stage: The role
of nuclear pore complexes in cell identity and aging,” Neuron, vol. 106,
no. 6. Elsevier, pp. 899–911, 2020.'
ista: 'Cho UH, Hetzer M. 2020. Nuclear periphery takes center stage: The role of
nuclear pore complexes in cell identity and aging. Neuron. 106(6), 899–911.'
mla: 'Cho, Ukrae H., and Martin Hetzer. “Nuclear Periphery Takes Center Stage: The
Role of Nuclear Pore Complexes in Cell Identity and Aging.” Neuron, vol.
106, no. 6, Elsevier, 2020, pp. 899–911, doi:10.1016/j.neuron.2020.05.031.'
short: U.H. Cho, M. Hetzer, Neuron 106 (2020) 899–911.
date_created: 2022-04-07T07:43:36Z
date_published: 2020-06-17T00:00:00Z
date_updated: 2022-07-18T08:29:35Z
day: '17'
doi: 10.1016/j.neuron.2020.05.031
extern: '1'
external_id:
pmid:
- '32553207'
intvolume: ' 106'
issue: '6'
keyword:
- General Neuroscience
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1016/j.neuron.2020.05.031
month: '06'
oa: 1
oa_version: Published Version
page: 899-911
pmid: 1
publication: Neuron
publication_identifier:
issn:
- 0896-6273
publication_status: published
publisher: Elsevier
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Nuclear periphery takes center stage: The role of nuclear pore complexes in
cell identity and aging'
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 106
year: '2020'
...
---
_id: '11055'
abstract:
- lang: eng
text: Vascular dysfunctions are a common feature of multiple age-related diseases.
However, modeling healthy and pathological aging of the human vasculature represents
an unresolved experimental challenge. Here, we generated induced vascular endothelial
cells (iVECs) and smooth muscle cells (iSMCs) by direct reprogramming of healthy
human fibroblasts from donors of different ages and Hutchinson-Gilford Progeria
Syndrome (HGPS) patients. iVECs induced from old donors revealed upregulation
of GSTM1 and PALD1, genes linked to oxidative stress, inflammation and endothelial
junction stability, as vascular aging markers. A functional assay performed on
PALD1 KD VECs demonstrated a recovery in vascular permeability. We found that
iSMCs from HGPS donors overexpressed bone morphogenetic protein (BMP)−4, which
plays a key role in both vascular calcification and endothelial barrier damage
observed in HGPS. Strikingly, BMP4 concentrations are higher in serum from HGPS
vs. age-matched mice. Furthermore, targeting BMP4 with blocking antibody recovered
the functionality of the vascular barrier in vitro, hence representing a potential
future therapeutic strategy to limit cardiovascular dysfunction in HGPS. These
results show that iVECs and iSMCs retain disease-related signatures, allowing
modeling of vascular aging and HGPS in vitro.
article_number: e54383
article_processing_charge: No
article_type: original
author:
- first_name: Simone
full_name: Bersini, Simone
last_name: Bersini
- first_name: Roberta
full_name: Schulte, Roberta
last_name: Schulte
- first_name: Ling
full_name: Huang, Ling
last_name: Huang
- first_name: Hannah
full_name: Tsai, Hannah
last_name: Tsai
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: Bersini S, Schulte R, Huang L, Tsai H, Hetzer M. Direct reprogramming of human
smooth muscle and vascular endothelial cells reveals defects associated with aging
and Hutchinson-Gilford progeria syndrome. eLife. 2020;9. doi:10.7554/elife.54383
apa: Bersini, S., Schulte, R., Huang, L., Tsai, H., & Hetzer, M. (2020). Direct
reprogramming of human smooth muscle and vascular endothelial cells reveals defects
associated with aging and Hutchinson-Gilford progeria syndrome. ELife.
eLife Sciences Publications. https://doi.org/10.7554/elife.54383
chicago: Bersini, Simone, Roberta Schulte, Ling Huang, Hannah Tsai, and Martin Hetzer.
“Direct Reprogramming of Human Smooth Muscle and Vascular Endothelial Cells Reveals
Defects Associated with Aging and Hutchinson-Gilford Progeria Syndrome.” ELife.
eLife Sciences Publications, 2020. https://doi.org/10.7554/elife.54383.
ieee: S. Bersini, R. Schulte, L. Huang, H. Tsai, and M. Hetzer, “Direct reprogramming
of human smooth muscle and vascular endothelial cells reveals defects associated
with aging and Hutchinson-Gilford progeria syndrome,” eLife, vol. 9. eLife
Sciences Publications, 2020.
ista: Bersini S, Schulte R, Huang L, Tsai H, Hetzer M. 2020. Direct reprogramming
of human smooth muscle and vascular endothelial cells reveals defects associated
with aging and Hutchinson-Gilford progeria syndrome. eLife. 9, e54383.
mla: Bersini, Simone, et al. “Direct Reprogramming of Human Smooth Muscle and Vascular
Endothelial Cells Reveals Defects Associated with Aging and Hutchinson-Gilford
Progeria Syndrome.” ELife, vol. 9, e54383, eLife Sciences Publications,
2020, doi:10.7554/elife.54383.
short: S. Bersini, R. Schulte, L. Huang, H. Tsai, M. Hetzer, ELife 9 (2020).
date_created: 2022-04-07T07:43:48Z
date_published: 2020-09-08T00:00:00Z
date_updated: 2022-07-18T08:30:37Z
day: '08'
ddc:
- '570'
doi: 10.7554/elife.54383
extern: '1'
external_id:
pmid:
- '32896271'
file:
- access_level: open_access
checksum: f8b3821349a194050be02570d8fe7d4b
content_type: application/pdf
creator: dernst
date_created: 2022-04-08T06:53:10Z
date_updated: 2022-04-08T06:53:10Z
file_id: '11132'
file_name: 2020_eLife_Bersini.pdf
file_size: 4399825
relation: main_file
success: 1
file_date_updated: 2022-04-08T06:53:10Z
has_accepted_license: '1'
intvolume: ' 9'
keyword:
- General Immunology and Microbiology
- General Biochemistry
- Genetics and Molecular Biology
- General Medicine
- General Neuroscience
language:
- iso: eng
month: '09'
oa: 1
oa_version: Published Version
pmid: 1
publication: eLife
publication_identifier:
issn:
- 2050-084X
publication_status: published
publisher: eLife Sciences Publications
quality_controlled: '1'
scopus_import: '1'
status: public
title: Direct reprogramming of human smooth muscle and vascular endothelial cells
reveals defects associated with aging and Hutchinson-Gilford progeria syndrome
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 9
year: '2020'
...
---
_id: '11056'
abstract:
- lang: eng
text: Aging of the circulatory system correlates with the pathogenesis of a large
spectrum of diseases. However, it is largely unknown which factors drive the age-dependent
or pathological decline of the vasculature and how vascular defects relate to
tissue aging. The goal of the study is to design a multianalytical approach to
identify how the cellular microenvironment (i.e., fibroblasts) and serum from
healthy donors of different ages or Alzheimer disease (AD) patients can modulate
the functionality of organ-specific vascular endothelial cells (VECs). Long-living
human microvascular networks embedding VECs and fibroblasts from skin biopsies
are generated. RNA-seq, secretome analyses, and microfluidic assays demonstrate
that fibroblasts from young donors restore the functionality of aged endothelial
cells, an effect also achieved by serum from young donors. New biomarkers of vascular
aging are validated in human biopsies and it is shown that young serum induces
angiopoietin-like-4, which can restore compromised vascular barriers. This strategy
is then employed to characterize transcriptional/functional changes induced on
the blood–brain barrier by AD serum, demonstrating the importance of PTP4A3 in
the regulation of permeability. Features of vascular degeneration during aging
and AD are recapitulated, and a tool to identify novel biomarkers that can be
exploited to develop future therapeutics modulating vascular function is established.
article_number: '2000044'
article_processing_charge: No
article_type: original
author:
- first_name: Simone
full_name: Bersini, Simone
last_name: Bersini
- first_name: Rafael
full_name: Arrojo e Drigo, Rafael
last_name: Arrojo e Drigo
- first_name: Ling
full_name: Huang, Ling
last_name: Huang
- first_name: Maxim N.
full_name: Shokhirev, Maxim N.
last_name: Shokhirev
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: Bersini S, Arrojo e Drigo R, Huang L, Shokhirev MN, Hetzer M. Transcriptional
and functional changes of the human microvasculature during physiological aging
and Alzheimer disease. Advanced Biosystems. 2020;4(5). doi:10.1002/adbi.202000044
apa: Bersini, S., Arrojo e Drigo, R., Huang, L., Shokhirev, M. N., & Hetzer,
M. (2020). Transcriptional and functional changes of the human microvasculature
during physiological aging and Alzheimer disease. Advanced Biosystems.
Wiley. https://doi.org/10.1002/adbi.202000044
chicago: Bersini, Simone, Rafael Arrojo e Drigo, Ling Huang, Maxim N. Shokhirev,
and Martin Hetzer. “Transcriptional and Functional Changes of the Human Microvasculature
during Physiological Aging and Alzheimer Disease.” Advanced Biosystems.
Wiley, 2020. https://doi.org/10.1002/adbi.202000044.
ieee: S. Bersini, R. Arrojo e Drigo, L. Huang, M. N. Shokhirev, and M. Hetzer, “Transcriptional
and functional changes of the human microvasculature during physiological aging
and Alzheimer disease,” Advanced Biosystems, vol. 4, no. 5. Wiley, 2020.
ista: Bersini S, Arrojo e Drigo R, Huang L, Shokhirev MN, Hetzer M. 2020. Transcriptional
and functional changes of the human microvasculature during physiological aging
and Alzheimer disease. Advanced Biosystems. 4(5), 2000044.
mla: Bersini, Simone, et al. “Transcriptional and Functional Changes of the Human
Microvasculature during Physiological Aging and Alzheimer Disease.” Advanced
Biosystems, vol. 4, no. 5, 2000044, Wiley, 2020, doi:10.1002/adbi.202000044.
short: S. Bersini, R. Arrojo e Drigo, L. Huang, M.N. Shokhirev, M. Hetzer, Advanced
Biosystems 4 (2020).
date_created: 2022-04-07T07:43:57Z
date_published: 2020-05-01T00:00:00Z
date_updated: 2022-07-18T08:30:48Z
day: '01'
ddc:
- '570'
doi: 10.1002/adbi.202000044
extern: '1'
external_id:
pmid:
- '32402127'
file:
- access_level: open_access
checksum: 5584d9a1609812dc75c02ce1e35d2ec0
content_type: application/pdf
creator: dernst
date_created: 2022-04-08T07:06:05Z
date_updated: 2022-04-08T07:06:05Z
file_id: '11134'
file_name: 2020_AdvancedBiosystems_Bersini.pdf
file_size: 2490829
relation: main_file
success: 1
file_date_updated: 2022-04-08T07:06:05Z
has_accepted_license: '1'
intvolume: ' 4'
issue: '5'
keyword:
- General Biochemistry
- Genetics and Molecular Biology
- Biomedical Engineering
- Biomaterials
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
pmid: 1
publication: Advanced Biosystems
publication_identifier:
issn:
- 2366-7478
- 2366-7478
publication_status: published
publisher: Wiley
quality_controlled: '1'
scopus_import: '1'
status: public
title: Transcriptional and functional changes of the human microvasculature during
physiological aging and Alzheimer disease
tmp:
image: /images/cc_by_nc_nd.png
legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
(CC BY-NC-ND 4.0)
short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 4
year: '2020'
...
---
_id: '11057'
abstract:
- lang: eng
text: During mitosis, transcription of genomic DNA is dramatically reduced, before
it is reactivated during nuclear reformation in anaphase/telophase. Many aspects
of the underlying principles that mediate transcriptional memory and reactivation
in the daughter cells remain unclear. Here, we used ChIP-seq on synchronized cells
at different stages after mitosis to generate genome-wide maps of histone modifications.
Combined with EU-RNA-seq and Hi-C analyses, we found that during prometaphase,
promoters, enhancers, and insulators retain H3K4me3 and H3K4me1, while losing
H3K27ac. Enhancers globally retaining mitotic H3K4me1 or locally retaining mitotic
H3K27ac are associated with cell type-specific genes and their transcription factors
for rapid transcriptional activation. As cells exit mitosis, promoters regain
H3K27ac, which correlates with transcriptional reactivation. Insulators also gain
H3K27ac and CCCTC-binding factor (CTCF) in anaphase/telophase. This increase of
H3K27ac in anaphase/telophase is required for posttranscriptional activation and
may play a role in the establishment of topologically associating domains (TADs).
Together, our results suggest that the genome is reorganized in a sequential order,
in which histone methylations occur first in prometaphase, histone acetylation,
and CTCF in anaphase/telophase, transcription in cytokinesis, and long-range chromatin
interactions in early G1. We thus provide insights into the histone modification
landscape that allows faithful reestablishment of the transcriptional program
and TADs during cell division.
article_processing_charge: No
article_type: original
author:
- first_name: Hyeseon
full_name: Kang, Hyeseon
last_name: Kang
- first_name: Maxim N.
full_name: Shokhirev, Maxim N.
last_name: Shokhirev
- first_name: Zhichao
full_name: Xu, Zhichao
last_name: Xu
- first_name: Sahaana
full_name: Chandran, Sahaana
last_name: Chandran
- first_name: Jesse R.
full_name: Dixon, Jesse R.
last_name: Dixon
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: Kang H, Shokhirev MN, Xu Z, Chandran S, Dixon JR, Hetzer M. Dynamic regulation
of histone modifications and long-range chromosomal interactions during postmitotic
transcriptional reactivation. Genes & Development. 2020;34(13-14):913-930.
doi:10.1101/gad.335794.119
apa: Kang, H., Shokhirev, M. N., Xu, Z., Chandran, S., Dixon, J. R., & Hetzer,
M. (2020). Dynamic regulation of histone modifications and long-range chromosomal
interactions during postmitotic transcriptional reactivation. Genes & Development.
Cold Spring Harbor Laboratory Press. https://doi.org/10.1101/gad.335794.119
chicago: Kang, Hyeseon, Maxim N. Shokhirev, Zhichao Xu, Sahaana Chandran, Jesse
R. Dixon, and Martin Hetzer. “Dynamic Regulation of Histone Modifications and
Long-Range Chromosomal Interactions during Postmitotic Transcriptional Reactivation.”
Genes & Development. Cold Spring Harbor Laboratory Press, 2020. https://doi.org/10.1101/gad.335794.119.
ieee: H. Kang, M. N. Shokhirev, Z. Xu, S. Chandran, J. R. Dixon, and M. Hetzer,
“Dynamic regulation of histone modifications and long-range chromosomal interactions
during postmitotic transcriptional reactivation,” Genes & Development,
vol. 34, no. 13–14. Cold Spring Harbor Laboratory Press, pp. 913–930, 2020.
ista: Kang H, Shokhirev MN, Xu Z, Chandran S, Dixon JR, Hetzer M. 2020. Dynamic
regulation of histone modifications and long-range chromosomal interactions during
postmitotic transcriptional reactivation. Genes & Development. 34(13–14),
913–930.
mla: Kang, Hyeseon, et al. “Dynamic Regulation of Histone Modifications and Long-Range
Chromosomal Interactions during Postmitotic Transcriptional Reactivation.” Genes
& Development, vol. 34, no. 13–14, Cold Spring Harbor Laboratory Press,
2020, pp. 913–30, doi:10.1101/gad.335794.119.
short: H. Kang, M.N. Shokhirev, Z. Xu, S. Chandran, J.R. Dixon, M. Hetzer, Genes
& Development 34 (2020) 913–930.
date_created: 2022-04-07T07:44:09Z
date_published: 2020-04-28T00:00:00Z
date_updated: 2022-07-18T08:31:08Z
day: '28'
ddc:
- '570'
doi: 10.1101/gad.335794.119
extern: '1'
external_id:
pmid:
- '32499403'
file:
- access_level: open_access
checksum: 84e92d40e67936c739628315c238daf9
content_type: application/pdf
creator: dernst
date_created: 2022-04-08T07:12:33Z
date_updated: 2022-04-08T07:12:33Z
file_id: '11136'
file_name: 2020_GenesDevelopment_Kang.pdf
file_size: 4406772
relation: main_file
success: 1
file_date_updated: 2022-04-08T07:12:33Z
has_accepted_license: '1'
intvolume: ' 34'
issue: 13-14
keyword:
- Developmental Biology
- Genetics
language:
- iso: eng
month: '04'
oa: 1
oa_version: Published Version
page: 913-930
pmid: 1
publication: Genes & Development
publication_identifier:
issn:
- 0890-9369
- 1549-5477
publication_status: published
publisher: Cold Spring Harbor Laboratory Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Dynamic regulation of histone modifications and long-range chromosomal interactions
during postmitotic transcriptional reactivation
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 34
year: '2020'
...
---
_id: '11058'
abstract:
- lang: eng
text: Nucleoporin 93 (Nup93) expression inversely correlates with the survival of
triple-negative breast cancer patients. However, our knowledge of Nup93 function
in breast cancer besides its role as structural component of the nuclear pore
complex is not understood. Combination of functional assays and genetic analyses
suggested that chromatin interaction of Nup93 partially modulates the expression
of genes associated with actin cytoskeleton remodeling and epithelial to mesenchymal
transition, resulting in impaired invasion of triple-negative, claudin-low breast
cancer cells. Nup93 depletion induced stress fiber formation associated with reduced
cell migration/proliferation and impaired expression of mesenchymal-like genes.
Silencing LIMCH1, a gene responsible for actin cytoskeleton remodeling and up-regulated
upon Nup93 depletion, partially restored the invasive phenotype of cancer cells.
Loss of Nup93 led to significant defects in tumor establishment/propagation in
vivo, whereas patient samples revealed that high Nup93 and low LIMCH1 expression
correlate with late tumor stage. Our approach identified Nup93 as contributor
of triple-negative, claudin-low breast cancer cell invasion and paves the way
to study the role of nuclear envelope proteins during breast cancer tumorigenesis.
article_number: e201900623
article_processing_charge: No
article_type: original
author:
- first_name: Simone
full_name: Bersini, Simone
last_name: Bersini
- first_name: Nikki K
full_name: Lytle, Nikki K
last_name: Lytle
- first_name: Roberta
full_name: Schulte, Roberta
last_name: Schulte
- first_name: Ling
full_name: Huang, Ling
last_name: Huang
- first_name: Geoffrey M
full_name: Wahl, Geoffrey M
last_name: Wahl
- first_name: Martin W
full_name: HETZER, Martin W
id: 86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed
last_name: HETZER
orcid: 0000-0002-2111-992X
citation:
ama: Bersini S, Lytle NK, Schulte R, Huang L, Wahl GM, Hetzer M. Nup93 regulates
breast tumor growth by modulating cell proliferation and actin cytoskeleton remodeling.
Life Science Alliance. 2020;3(1). doi:10.26508/lsa.201900623
apa: Bersini, S., Lytle, N. K., Schulte, R., Huang, L., Wahl, G. M., & Hetzer,
M. (2020). Nup93 regulates breast tumor growth by modulating cell proliferation
and actin cytoskeleton remodeling. Life Science Alliance. Life Science
Alliance. https://doi.org/10.26508/lsa.201900623
chicago: Bersini, Simone, Nikki K Lytle, Roberta Schulte, Ling Huang, Geoffrey M
Wahl, and Martin Hetzer. “Nup93 Regulates Breast Tumor Growth by Modulating Cell
Proliferation and Actin Cytoskeleton Remodeling.” Life Science Alliance.
Life Science Alliance, 2020. https://doi.org/10.26508/lsa.201900623.
ieee: S. Bersini, N. K. Lytle, R. Schulte, L. Huang, G. M. Wahl, and M. Hetzer,
“Nup93 regulates breast tumor growth by modulating cell proliferation and actin
cytoskeleton remodeling,” Life Science Alliance, vol. 3, no. 1. Life Science
Alliance, 2020.
ista: Bersini S, Lytle NK, Schulte R, Huang L, Wahl GM, Hetzer M. 2020. Nup93 regulates
breast tumor growth by modulating cell proliferation and actin cytoskeleton remodeling.
Life Science Alliance. 3(1), e201900623.
mla: Bersini, Simone, et al. “Nup93 Regulates Breast Tumor Growth by Modulating
Cell Proliferation and Actin Cytoskeleton Remodeling.” Life Science Alliance,
vol. 3, no. 1, e201900623, Life Science Alliance, 2020, doi:10.26508/lsa.201900623.
short: S. Bersini, N.K. Lytle, R. Schulte, L. Huang, G.M. Wahl, M. Hetzer, Life
Science Alliance 3 (2020).
date_created: 2022-04-07T07:44:18Z
date_published: 2020-01-01T00:00:00Z
date_updated: 2022-07-18T08:31:20Z
day: '01'
ddc:
- '570'
doi: 10.26508/lsa.201900623
extern: '1'
external_id:
pmid:
- '31959624'
file:
- access_level: open_access
checksum: 3bf33e7e93bef7823287807206b69b38
content_type: application/pdf
creator: dernst
date_created: 2022-04-08T07:33:01Z
date_updated: 2022-04-08T07:33:01Z
file_id: '11137'
file_name: 2020_LifeScienceAlliance_Bersini.pdf
file_size: 2653960
relation: main_file
success: 1
file_date_updated: 2022-04-08T07:33:01Z
has_accepted_license: '1'
intvolume: ' 3'
issue: '1'
keyword:
- Health
- Toxicology and Mutagenesis
- Plant Science
- Biochemistry
- Genetics and Molecular Biology (miscellaneous)
- Ecology
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
pmid: 1
publication: Life Science Alliance
publication_identifier:
issn:
- 2575-1077
publication_status: published
publisher: Life Science Alliance
quality_controlled: '1'
scopus_import: '1'
status: public
title: Nup93 regulates breast tumor growth by modulating cell proliferation and actin
cytoskeleton remodeling
tmp:
image: /images/cc_by.png
legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
short: CC BY (4.0)
type: journal_article
user_id: 72615eeb-f1f3-11ec-aa25-d4573ddc34fd
volume: 3
year: '2020'
...
---
_id: '11501'
abstract:
- lang: eng
text: We investigated the ultraviolet (UV) spectral properties of faint Lyman-α
emitters (LAEs) in the redshift range 2.9 ≤ z ≤ 4.6, and we provide material to
prepare future observations of the faint Universe. We used data from the MUSE
Hubble Ultra Deep Survey to construct mean rest-frame spectra of continuum-faint
(median MUV of −18 and down to MUV of −16), low stellar mass (median value of
108.4 M⊙ and down to 107 M⊙) LAEs at redshift z ≳ 3. We computed various averaged
spectra of LAEs, subsampled on the basis of their observational (e.g., Lyα strength,
UV magnitude and spectral slope) and physical (e.g., stellar mass and star-formation
rate) properties. We searched for UV spectral features other than Lyα, such as
higher ionization nebular emission lines and absorption features. We successfully
observed the O III]λ1666 and [C III]λ1907+C III]λ1909 collisionally excited emission
lines and the He IIλ1640 recombination feature, as well as the resonant C IVλλ1548,1551
doublet either in emission or P-Cygni. We compared the observed spectral properties
of the different mean spectra and find the emission lines to vary with the observational
and physical properties of the LAEs. In particular, the mean spectra of LAEs with
larger Lyα equivalent widths, fainter UV magnitudes, bluer UV spectral slopes,
and lower stellar masses show the strongest nebular emission. The line ratios
of these lines are similar to those measured in the spectra of local metal-poor
galaxies, while their equivalent widths are weaker compared to the handful of
extreme values detected in individual spectra of z > 2 galaxies. This suggests
that weak UV features are likely ubiquitous in high z, low-mass, and faint LAEs.
We publicly released the stacked spectra, as they can serve as empirical templates
for the design of future observations, such as those with the James Webb Space
Telescope and the Extremely Large Telescope.
acknowledgement: 'We thank Margherita Talia, Stéphane Charlot, Adele Plat and Alba
Vidal-García for helpful discussions. This work is supported by the ERC advanced
grant 339659-MUSICOS (R. Bacon). AF acknowledges the support from grant PRIN MIUR
2017 20173ML3WW. MVM and JP would like to thank the Leiden/ESA Astrophysics Program
for Summer Students (LEAPS) for funding at the outset of this project. FL, HK, and
AV acknowledge support from the ERC starting grant ERC-757258-TRIPLE. TH was supported
by Leading Initiative for Excellent Young Researchers, MEXT, Japan. JB acknowledges
support by FCT/MCTES through national funds by the grant UID/FIS/04434/2019, UIDB/04434/2020
and UIDP/04434/2020 and through the Investigador FCT Contract No. IF/01654/2014/CP1215/CT0003.
HI acknowledges support from JSPS KAKENHI Grant Number JP19K23462. We would also
like to thank the organizers and participants of the Leiden Lorentz Center workshop:
Revolutionary Spectroscopy of Today as a Springboard to Webb. This work made use
of several open source python packages: NUMPY (van der Walt et al. 2011), MATPLOTLIB
(Hunter 2007), ASTROPY (Astropy Collaboration 2013) and MPDAF (MUSE Python Data
Analysis Framework, Piqueras et al. 2019).'
article_number: A118
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Anna
full_name: Feltre, Anna
last_name: Feltre
- first_name: Michael V.
full_name: Maseda, Michael V.
last_name: Maseda
- first_name: Roland
full_name: Bacon, Roland
last_name: Bacon
- first_name: Jayadev
full_name: Pradeep, Jayadev
last_name: Pradeep
- first_name: Floriane
full_name: Leclercq, Floriane
last_name: Leclercq
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- first_name: Lutz
full_name: Wisotzki, Lutz
last_name: Wisotzki
- first_name: Takuya
full_name: Hashimoto, Takuya
last_name: Hashimoto
- first_name: Kasper B.
full_name: Schmidt, Kasper B.
last_name: Schmidt
- first_name: Jeremy
full_name: Blaizot, Jeremy
last_name: Blaizot
- first_name: Jarle
full_name: Brinchmann, Jarle
last_name: Brinchmann
- first_name: Leindert
full_name: Boogaard, Leindert
last_name: Boogaard
- first_name: Sebastiano
full_name: Cantalupo, Sebastiano
last_name: Cantalupo
- first_name: David
full_name: Carton, David
last_name: Carton
- first_name: Hanae
full_name: Inami, Hanae
last_name: Inami
- first_name: Wolfram
full_name: Kollatschny, Wolfram
last_name: Kollatschny
- first_name: Raffaella A.
full_name: Marino, Raffaella A.
last_name: Marino
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Themiya
full_name: Nanayakkara, Themiya
last_name: Nanayakkara
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Laurence
full_name: Tresse, Laurence
last_name: Tresse
- first_name: Tanya
full_name: Urrutia, Tanya
last_name: Urrutia
- first_name: Anne
full_name: Verhamme, Anne
last_name: Verhamme
- first_name: Peter M.
full_name: Weilbacher, Peter M.
last_name: Weilbacher
citation:
ama: 'Feltre A, Maseda MV, Bacon R, et al. The MUSE Hubble Ultra Deep Field Survey:
XV. The mean rest-UV spectra of Lyα emitters at z > 3. Astronomy &
Astrophysics. 2020;641. doi:10.1051/0004-6361/202038133'
apa: 'Feltre, A., Maseda, M. V., Bacon, R., Pradeep, J., Leclercq, F., Kusakabe,
H., … Weilbacher, P. M. (2020). The MUSE Hubble Ultra Deep Field Survey: XV. The
mean rest-UV spectra of Lyα emitters at z > 3. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/202038133'
chicago: 'Feltre, Anna, Michael V. Maseda, Roland Bacon, Jayadev Pradeep, Floriane
Leclercq, Haruka Kusakabe, Lutz Wisotzki, et al. “The MUSE Hubble Ultra Deep Field
Survey: XV. The Mean Rest-UV Spectra of Lyα Emitters at z > 3.” Astronomy
& Astrophysics. EDP Sciences, 2020. https://doi.org/10.1051/0004-6361/202038133.'
ieee: 'A. Feltre et al., “The MUSE Hubble Ultra Deep Field Survey: XV. The
mean rest-UV spectra of Lyα emitters at z > 3,” Astronomy & Astrophysics,
vol. 641. EDP Sciences, 2020.'
ista: 'Feltre A, Maseda MV, Bacon R, Pradeep J, Leclercq F, Kusakabe H, Wisotzki
L, Hashimoto T, Schmidt KB, Blaizot J, Brinchmann J, Boogaard L, Cantalupo S,
Carton D, Inami H, Kollatschny W, Marino RA, Matthee JJ, Nanayakkara T, Richard
J, Schaye J, Tresse L, Urrutia T, Verhamme A, Weilbacher PM. 2020. The MUSE Hubble
Ultra Deep Field Survey: XV. The mean rest-UV spectra of Lyα emitters at z >
3. Astronomy & Astrophysics. 641, A118.'
mla: 'Feltre, Anna, et al. “The MUSE Hubble Ultra Deep Field Survey: XV. The Mean
Rest-UV Spectra of Lyα Emitters at z > 3.” Astronomy & Astrophysics,
vol. 641, A118, EDP Sciences, 2020, doi:10.1051/0004-6361/202038133.'
short: A. Feltre, M.V. Maseda, R. Bacon, J. Pradeep, F. Leclercq, H. Kusakabe, L.
Wisotzki, T. Hashimoto, K.B. Schmidt, J. Blaizot, J. Brinchmann, L. Boogaard,
S. Cantalupo, D. Carton, H. Inami, W. Kollatschny, R.A. Marino, J.J. Matthee,
T. Nanayakkara, J. Richard, J. Schaye, L. Tresse, T. Urrutia, A. Verhamme, P.M.
Weilbacher, Astronomy & Astrophysics 641 (2020).
date_created: 2022-07-06T09:38:16Z
date_published: 2020-09-18T00:00:00Z
date_updated: 2022-07-19T09:35:43Z
day: '18'
doi: 10.1051/0004-6361/202038133
extern: '1'
external_id:
arxiv:
- '2007.01878'
intvolume: ' 641'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution / galaxies: high-redshift / ISM: lines and bands / ultraviolet:
ISM / ultraviolet: galaxies'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2007.01878
month: '09'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The MUSE Hubble Ultra Deep Field Survey: XV. The mean rest-UV spectra of Lyα
emitters at z > 3'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 641
year: '2020'
...
---
_id: '11503'
abstract:
- lang: eng
text: "Context. The Lyα emitter (LAE) fraction, XLAE, is a potentially powerful
probe of the evolution of the intergalactic neutral hydrogen gas fraction. However,
uncertainties in the measurement of XLAE are still under debate.\r\nAims. Thanks
to deep data obtained with the integral field spectrograph Multi Unit Spectroscopic
Explorer (MUSE), we can measure the evolution of the LAE fraction homogeneously
over a wide redshift range of z ≈ 3–6 for UV-faint galaxies (down to UV magnitudes
of M1500 ≈ −17.75). This is a significantly fainter range than in former studies
(M1500 ≤ −18.75) and it allows us to probe the bulk of the population of high-redshift
star-forming galaxies.\r\nMethods. We constructed a UV-complete photometric-redshift
sample following UV luminosity functions and measured the Lyα emission with MUSE
using the latest (second) data release from the MUSE Hubble Ultra Deep Field Survey.\r\nResults.
We derived the redshift evolution of XLAE for M1500 ∈ [ − 21.75; −17.75] for the
first time with a equivalent width range EW(Lyα) ≥ 65 Å and found low values of
XLAE ≲ 30% at z ≲ 6. The best-fit linear relation is XLAE = 0.07+0.06−0.03z −
0.22+0.12−0.24. For M1500 ∈ [ − 20.25; −18.75] and EW(Lyα) ≥ 25 Å, our XLAE values
are consistent with those in the literature within 1σ at z ≲ 5, but our median
values are systematically lower than reported values over the whole redshift range.
In addition, we do not find a significant dependence of XLAE on M1500 for EW(Lyα)
≥ 50 Å at z ≈ 3–4, in contrast with previous work. The differences in XLAE mainly
arise from selection biases for Lyman Break Galaxies (LBGs) in the literature:
UV-faint LBGs are more easily selected if they have strong Lyα emission, hence
XLAE is biased towards higher values when those samples are used.\r\nConclusions.
Our results suggest either a lower increase of XLAE towards z ≈ 6 than previously
suggested, or even a turnover of XLAE at z ≈ 5.5, which may be the signature of
a late or patchy reionization process. We compared our results with predictions
from a cosmological galaxy evolution model. We find that a model with a bursty
star formation (SF) can reproduce our observed LAE fractions much better than
models where SF is a smooth function of time."
acknowledgement: We thank the anonymous referee for constructive comments and suggestions.
We would like to express our gratitude to Stephane De Barros and Pablo Arrabal Haro
for kindly providing their data plotted in Figs. 1, 2, and 8. We are grateful to
Kazuhiro Shimasaku, Masami Ouchi, Rieko Momose, Daniel Schaerer, Hidenobu Yajima,
Taku Okamura, Makoto Ando, and Hinako Goto for giving insightful comments and suggestions.
This work is based on observations taken by VLT, which is operated by European Southern
Observatory. This research made use of Astropy (http://www.astropy.org), which is
a community-developed core Python package for Astronomy (Astropy Collaboration 2013,
2018), MARZ, MPDAF, and matplotlib (Hunter 2007). H.K. acknowledges support from
Japan Society for the Promotion of Science (JSPS) through the JSPS Research Fellowship
for Young Scientists and Overseas Challenge Program for Young Researchers. AV acknowledges
support from the ERC starting grant 757258-TRIPLE and the SNF Professorship 176808-TRIPLE.
This work was supported by the project FOGHAR (Agence Nationale de la Recherche,
ANR-13-BS05-0010-02). JB acknowledges support from the ORAGE project from the Agence
Nationale de la Recherche under grant ANR-14-CE33-0016-03. JR acknowledges support
from the ERC starting grant 336736-CALENDS. T. H. acknowledges supports by the Grant-inAid
for Scientic Research 19J01620.
article_number: A12
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- first_name: Jérémy
full_name: Blaizot, Jérémy
last_name: Blaizot
- first_name: Thibault
full_name: Garel, Thibault
last_name: Garel
- first_name: Anne
full_name: Verhamme, Anne
last_name: Verhamme
- first_name: Roland
full_name: Bacon, Roland
last_name: Bacon
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: Takuya
full_name: Hashimoto, Takuya
last_name: Hashimoto
- first_name: Hanae
full_name: Inami, Hanae
last_name: Inami
- first_name: Simon
full_name: Conseil, Simon
last_name: Conseil
- first_name: Bruno
full_name: Guiderdoni, Bruno
last_name: Guiderdoni
- first_name: Alyssa B.
full_name: Drake, Alyssa B.
last_name: Drake
- first_name: Edmund
full_name: Christian Herenz, Edmund
last_name: Christian Herenz
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Pascal
full_name: Oesch, Pascal
last_name: Oesch
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Raffaella
full_name: Anna Marino, Raffaella
last_name: Anna Marino
- first_name: Kasper
full_name: Borello Schmidt, Kasper
last_name: Borello Schmidt
- first_name: Roser
full_name: Pelló, Roser
last_name: Pelló
- first_name: Michael
full_name: Maseda, Michael
last_name: Maseda
- first_name: Floriane
full_name: Leclercq, Floriane
last_name: Leclercq
- first_name: Josephine
full_name: Kerutt, Josephine
last_name: Kerutt
- first_name: Guillaume
full_name: Mahler, Guillaume
last_name: Mahler
citation:
ama: 'Kusakabe H, Blaizot J, Garel T, et al. The MUSE Hubble Ultra Deep Field Survey:
XIV. Evolution of the Lyα emitter fraction from z = 3 to z = 6. Astronomy &
Astrophysics. 2020;638. doi:10.1051/0004-6361/201937340'
apa: 'Kusakabe, H., Blaizot, J., Garel, T., Verhamme, A., Bacon, R., Richard, J.,
… Mahler, G. (2020). The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution of
the Lyα emitter fraction from z = 3 to z = 6. Astronomy & Astrophysics.
EDP Sciences. https://doi.org/10.1051/0004-6361/201937340'
chicago: 'Kusakabe, Haruka, Jérémy Blaizot, Thibault Garel, Anne Verhamme, Roland
Bacon, Johan Richard, Takuya Hashimoto, et al. “The MUSE Hubble Ultra Deep Field
Survey: XIV. Evolution of the Lyα Emitter Fraction from z = 3 to z = 6.” Astronomy
& Astrophysics. EDP Sciences, 2020. https://doi.org/10.1051/0004-6361/201937340.'
ieee: 'H. Kusakabe et al., “The MUSE Hubble Ultra Deep Field Survey: XIV.
Evolution of the Lyα emitter fraction from z = 3 to z = 6,” Astronomy &
Astrophysics, vol. 638. EDP Sciences, 2020.'
ista: 'Kusakabe H, Blaizot J, Garel T, Verhamme A, Bacon R, Richard J, Hashimoto
T, Inami H, Conseil S, Guiderdoni B, Drake AB, Christian Herenz E, Schaye J, Oesch
P, Matthee JJ, Anna Marino R, Borello Schmidt K, Pelló R, Maseda M, Leclercq F,
Kerutt J, Mahler G. 2020. The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution
of the Lyα emitter fraction from z = 3 to z = 6. Astronomy & Astrophysics.
638, A12.'
mla: 'Kusakabe, Haruka, et al. “The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution
of the Lyα Emitter Fraction from z = 3 to z = 6.” Astronomy & Astrophysics,
vol. 638, A12, EDP Sciences, 2020, doi:10.1051/0004-6361/201937340.'
short: H. Kusakabe, J. Blaizot, T. Garel, A. Verhamme, R. Bacon, J. Richard, T.
Hashimoto, H. Inami, S. Conseil, B. Guiderdoni, A.B. Drake, E. Christian Herenz,
J. Schaye, P. Oesch, J.J. Matthee, R. Anna Marino, K. Borello Schmidt, R. Pelló,
M. Maseda, F. Leclercq, J. Kerutt, G. Mahler, Astronomy & Astrophysics 638
(2020).
date_created: 2022-07-06T09:50:48Z
date_published: 2020-06-03T00:00:00Z
date_updated: 2022-07-19T09:35:20Z
day: '03'
doi: 10.1051/0004-6361/201937340
extern: '1'
external_id:
arxiv:
- '2003.12083'
intvolume: ' 638'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'dark ages / reionization / first stars / early Universe / cosmology: observations
/ galaxies: evolution / galaxies: high-redshift / intergalactic medium'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2003.12083
month: '06'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The MUSE Hubble Ultra Deep Field Survey: XIV. Evolution of the Lyα emitter
fraction from z = 3 to z = 6'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 638
year: '2020'
...
---
_id: '11504'
abstract:
- lang: eng
text: We present spatially resolved maps of six individually-detected Lyman α haloes
(LAHs) as well as a first statistical analysis of the Lyman α (Lyα) spectral signature
in the circum-galactic medium of high-redshift star-forming galaxies (−17.5 >
MUV > −21.5) using the Multi-Unit Spectroscopic Explorer. Our resolved spectroscopic
analysis of the LAHs reveals significant intrahalo variations of the Lyα line
profile. Using a three-dimensional two-component model for the Lyα emission, we
measured the full width at half maximum (FWHM), the peak velocity shift, and the
asymmetry of the Lyα line in the core and in the halo of 19 galaxies. We find
that the Lyα line shape is statistically different in the halo compared to the
core (in terms of width, peak wavelength, and asymmetry) for ≈40% of our galaxies.
Similarly to object-by-object based studies and a recent resolved study using
lensing, we find a correlation between the peak velocity shift and the width of
the Lyα line both at the interstellar and circum-galactic scales. This trend has
been predicted by radiative transfer simulations of galactic winds as a result
of resonant scattering in outflows. While there is a lack of correlation between
the spectral properties and the spatial scale lengths of our LAHs, we find a correlation
between the width of the line in the LAH and the halo flux fraction. Interestingly,
UV bright galaxies (MUV < −20) show broader, more redshifted, and less asymmetric
Lyα lines in their haloes. The most significant correlation found is for the FWHM
of the line and the UV continuum slope of the galaxy, suggesting that the redder
galaxies have broader Lyα lines. The generally broad and red line shapes found
in the halo component suggest that the Lyα haloes are powered either by scattering
processes through an outflowing medium, fluorescent emission from outflowing cold
clumps of gas, or a mix of both. Considering the large diversity of the Lyα line
profiles observed in our sample and the lack of strong correlation, the interpretation
of our results is still broadly open and underlines the need for realistic spatially
resolved models of the LAHs.
acknowledgement: F.L., R.B., and S.C. acknowledge support from the ERC advanced grant
339659-MUSICOS. F.L., T.G., H.K., and A.V. acknowledge support from the ERC starting
grant ERC-757258-TRIPLE. A.C. and J.R. acknowledge support from the ERC starting
grant 336736-CALENDS. J.B. acknowledges support by FCT/MCTES through national funds
(PID-DAC) by grant UID/FIS/04434/2019 and through Investigador FCT Contract No.IF/01654/2014/CP1215/CT0003.
T.H. was supported by Leading Initiative for Excellent Young Researchers, MEXT,
Japan.
article_number: A82
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Floriane
full_name: Leclercq, Floriane
last_name: Leclercq
- first_name: Roland
full_name: Bacon, Roland
last_name: Bacon
- first_name: Anne
full_name: Verhamme, Anne
last_name: Verhamme
- first_name: Thibault
full_name: Garel, Thibault
last_name: Garel
- first_name: Jérémy
full_name: Blaizot, Jérémy
last_name: Blaizot
- first_name: Jarle
full_name: Brinchmann, Jarle
last_name: Brinchmann
- first_name: Sebastiano
full_name: Cantalupo, Sebastiano
last_name: Cantalupo
- first_name: Adélaïde
full_name: Claeyssens, Adélaïde
last_name: Claeyssens
- first_name: Simon
full_name: Conseil, Simon
last_name: Conseil
- first_name: Thierry
full_name: Contini, Thierry
last_name: Contini
- first_name: Takuya
full_name: Hashimoto, Takuya
last_name: Hashimoto
- first_name: Edmund Christian
full_name: Herenz, Edmund Christian
last_name: Herenz
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- first_name: Raffaella Anna
full_name: Marino, Raffaella Anna
last_name: Marino
- first_name: Michael
full_name: Maseda, Michael
last_name: Maseda
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Peter
full_name: Mitchell, Peter
last_name: Mitchell
- first_name: Gabriele
full_name: Pezzulli, Gabriele
last_name: Pezzulli
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: Kasper Borello
full_name: Schmidt, Kasper Borello
last_name: Schmidt
- first_name: Lutz
full_name: Wisotzki, Lutz
last_name: Wisotzki
citation:
ama: 'Leclercq F, Bacon R, Verhamme A, et al. The MUSE Hubble Ultra Deep field survey:
XIII. Spatially resolved spectral properties of Lyman α haloes around star-forming
galaxies at z > 3. Astronomy & Astrophysics. 2020;635. doi:10.1051/0004-6361/201937339'
apa: 'Leclercq, F., Bacon, R., Verhamme, A., Garel, T., Blaizot, J., Brinchmann,
J., … Wisotzki, L. (2020). The MUSE Hubble Ultra Deep field survey: XIII. Spatially
resolved spectral properties of Lyman α haloes around star-forming galaxies at
z > 3. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/201937339'
chicago: 'Leclercq, Floriane, Roland Bacon, Anne Verhamme, Thibault Garel, Jérémy
Blaizot, Jarle Brinchmann, Sebastiano Cantalupo, et al. “The MUSE Hubble Ultra
Deep Field Survey: XIII. Spatially Resolved Spectral Properties of Lyman α Haloes
around Star-Forming Galaxies at z > 3.” Astronomy & Astrophysics.
EDP Sciences, 2020. https://doi.org/10.1051/0004-6361/201937339.'
ieee: 'F. Leclercq et al., “The MUSE Hubble Ultra Deep field survey: XIII.
Spatially resolved spectral properties of Lyman α haloes around star-forming galaxies
at z > 3,” Astronomy & Astrophysics, vol. 635. EDP Sciences, 2020.'
ista: 'Leclercq F, Bacon R, Verhamme A, Garel T, Blaizot J, Brinchmann J, Cantalupo
S, Claeyssens A, Conseil S, Contini T, Hashimoto T, Herenz EC, Kusakabe H, Marino
RA, Maseda M, Matthee JJ, Mitchell P, Pezzulli G, Richard J, Schmidt KB, Wisotzki
L. 2020. The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral
properties of Lyman α haloes around star-forming galaxies at z > 3. Astronomy
& Astrophysics. 635, A82.'
mla: 'Leclercq, Floriane, et al. “The MUSE Hubble Ultra Deep Field Survey: XIII.
Spatially Resolved Spectral Properties of Lyman α Haloes around Star-Forming Galaxies
at z > 3.” Astronomy & Astrophysics, vol. 635, A82, EDP Sciences,
2020, doi:10.1051/0004-6361/201937339.'
short: F. Leclercq, R. Bacon, A. Verhamme, T. Garel, J. Blaizot, J. Brinchmann,
S. Cantalupo, A. Claeyssens, S. Conseil, T. Contini, T. Hashimoto, E.C. Herenz,
H. Kusakabe, R.A. Marino, M. Maseda, J.J. Matthee, P. Mitchell, G. Pezzulli, J.
Richard, K.B. Schmidt, L. Wisotzki, Astronomy & Astrophysics 635 (2020).
date_created: 2022-07-06T09:56:20Z
date_published: 2020-03-11T00:00:00Z
date_updated: 2022-07-19T09:36:58Z
day: '11'
doi: 10.1051/0004-6361/201937339
extern: '1'
external_id:
arxiv:
- '2002.05731'
intvolume: ' 635'
keyword:
- Space and Planetary Science
- 'Astronomy and Astrophysics galaxies: high-redshift / galaxies: formation / galaxies:
evolution / cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2002.05731
month: '03'
oa: 1
oa_version: Published Version
publication: Astronomy & Astrophysics
publication_identifier:
eissn:
- 1432-0746
issn:
- 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The MUSE Hubble Ultra Deep field survey: XIII. Spatially resolved spectral
properties of Lyman α haloes around star-forming galaxies at z > 3'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 635
year: '2020'
...
---
_id: '11513'
abstract:
- lang: eng
text: We report the spectroscopic confirmation of a new protocluster in the COSMOS
field at z ∼ 2.2, COSMOS Cluster 2.2 (CC2.2), originally identified as an overdensity
of narrowband selected Hα emitting candidates. With only two masks of Keck/MOSFIRE
near-IR spectroscopy in both H (∼1.47–1.81 μm) and K (∼1.92–2.40 μm) bands (∼1.5
hr each), we confirm 35 unique protocluster members with at least two emission
lines detected with S/N > 3. Combined with 12 extra members from the zCOSMOS-deep
spectroscopic survey (47 in total), we estimate a mean redshift and a line-of-sight
velocity dispersion of zmean = 2.23224 ± 0.00101 and σlos = 645 ± 69 km s−1 for
this protocluster, respectively. Assuming virialization and spherical symmetry
for the system, we estimate a total mass of Mvir ∼ (1–2) ×1014M⊙ for the structure.
We evaluate a number density enhancement of δg ∼ 7 for this system and we argue
that the structure is likely not fully virialized at z ∼ 2.2. However, in a spherical
collapse model, δg is expected to grow to a linear matter enhancement of ∼1.9
by z = 0, exceeding the collapse threshold of 1.69, and leading to a fully collapsed
and virialized Coma-type structure with a total mass of Mdyn(z = 0) ∼ 9.2 × 1014M⊙
by now. This observationally efficient confirmation suggests that large narrowband
emission-line galaxy surveys, when combined with ancillary photometric data, can
be used to effectively trace the large-scale structure and protoclusters at a
time when they are mostly dominated by star-forming galaxies.
acknowledgement: We are thankful to the anonymous referee for useful comments and
suggestions that improved the quality of this paper. B.D. acknowledges financial
support from NASA through the Astrophysics Data Analysis Program (ADAP), grant number
NNX12AE20G, and the National Science Foundation, grant number 1716907. B.D. is thankful
to Andreas Faisst, Laura Danly, and Matthew Burlando for their companionship during
the observing run. B.D. is grateful to the COSMOS team for their useful comments
during the team meeting in New York City 2019 May 14–17. A.R. research was made
possible by Friends of W. M. Keck Observatory who philanthropically support the
Keck Science Collaborative (KSC) fund. The observations presented herein were obtained
at the W. M. Keck Observatory (program C236, PI Scoville), which is operated as
a scientific partnership among the California Institute of Technology, the University
of California, and the National Aeronautics and Space Administration. The Observatory
was made possible by the generous financial support of the W. M. Keck Foundation.
The authors would like to recognize and acknowledge the very prominent cultural
role and reverence that the summit of Maunakea has always had within the indigenous
Hawaiian community. We are fortunate to have the opportunity to perform observations
from this mountain.
article_number: '8'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Behnam
full_name: Darvish, Behnam
last_name: Darvish
- first_name: Nick Z.
full_name: Scoville, Nick Z.
last_name: Scoville
- first_name: Christopher
full_name: Martin, Christopher
last_name: Martin
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Bahram
full_name: Mobasher, Bahram
last_name: Mobasher
- first_name: Alessandro
full_name: Rettura, Alessandro
last_name: Rettura
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Peter
full_name: Capak, Peter
last_name: Capak
- first_name: Nima
full_name: Chartab, Nima
last_name: Chartab
- first_name: Shoubaneh
full_name: Hemmati, Shoubaneh
last_name: Hemmati
- first_name: Daniel
full_name: Masters, Daniel
last_name: Masters
- first_name: Hooshang
full_name: Nayyeri, Hooshang
last_name: Nayyeri
- first_name: Donal
full_name: O’Sullivan, Donal
last_name: O’Sullivan
- first_name: Ana
full_name: Paulino-Afonso, Ana
last_name: Paulino-Afonso
- first_name: Zahra
full_name: Sattari, Zahra
last_name: Sattari
- first_name: Abtin
full_name: Shahidi, Abtin
last_name: Shahidi
- first_name: Mara
full_name: Salvato, Mara
last_name: Salvato
- first_name: Brian C.
full_name: Lemaux, Brian C.
last_name: Lemaux
- first_name: Olivier Le
full_name: Fèvre, Olivier Le
last_name: Fèvre
- first_name: Olga
full_name: Cucciati, Olga
last_name: Cucciati
citation:
ama: Darvish B, Scoville NZ, Martin C, et al. Spectroscopic confirmation of a coma
cluster progenitor at z ∼ 2.2. The Astrophysical Journal. 2020;892(1).
doi:10.3847/1538-4357/ab75c3
apa: Darvish, B., Scoville, N. Z., Martin, C., Sobral, D., Mobasher, B., Rettura,
A., … Cucciati, O. (2020). Spectroscopic confirmation of a coma cluster progenitor
at z ∼ 2.2. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ab75c3
chicago: Darvish, Behnam, Nick Z. Scoville, Christopher Martin, David Sobral, Bahram
Mobasher, Alessandro Rettura, Jorryt J Matthee, et al. “Spectroscopic Confirmation
of a Coma Cluster Progenitor at z ∼ 2.2.” The Astrophysical Journal. IOP
Publishing, 2020. https://doi.org/10.3847/1538-4357/ab75c3.
ieee: B. Darvish et al., “Spectroscopic confirmation of a coma cluster progenitor
at z ∼ 2.2,” The Astrophysical Journal, vol. 892, no. 1. IOP Publishing,
2020.
ista: Darvish B, Scoville NZ, Martin C, Sobral D, Mobasher B, Rettura A, Matthee
JJ, Capak P, Chartab N, Hemmati S, Masters D, Nayyeri H, O’Sullivan D, Paulino-Afonso
A, Sattari Z, Shahidi A, Salvato M, Lemaux BC, Fèvre OL, Cucciati O. 2020. Spectroscopic
confirmation of a coma cluster progenitor at z ∼ 2.2. The Astrophysical Journal.
892(1), 8.
mla: Darvish, Behnam, et al. “Spectroscopic Confirmation of a Coma Cluster Progenitor
at z ∼ 2.2.” The Astrophysical Journal, vol. 892, no. 1, 8, IOP Publishing,
2020, doi:10.3847/1538-4357/ab75c3.
short: B. Darvish, N.Z. Scoville, C. Martin, D. Sobral, B. Mobasher, A. Rettura,
J.J. Matthee, P. Capak, N. Chartab, S. Hemmati, D. Masters, H. Nayyeri, D. O’Sullivan,
A. Paulino-Afonso, Z. Sattari, A. Shahidi, M. Salvato, B.C. Lemaux, O.L. Fèvre,
O. Cucciati, The Astrophysical Journal 892 (2020).
date_created: 2022-07-06T13:10:51Z
date_published: 2020-03-19T00:00:00Z
date_updated: 2022-07-19T09:31:35Z
day: '19'
doi: 10.3847/1538-4357/ab75c3
extern: '1'
external_id:
arxiv:
- '2002.06207'
intvolume: ' 892'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2002.06207
month: '03'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal
publication_identifier:
eissn:
- 1538-4357
issn:
- 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Spectroscopic confirmation of a coma cluster progenitor at z ∼ 2.2
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 892
year: '2020'
...
---
_id: '11528'
abstract:
- lang: eng
text: Ly α emission lines are typically found to be redshifted with respect to the
systemic redshifts of galaxies, likely due to resonant scattering of Ly α photons.
Here, we measure the average velocity offset for a sample of 96 z ≈ 3.3 Ly α emitters
(LAEs) with a median Ly α flux (luminosity) of ≈10−17 erg cm−2 s−1 (≈1042 erg
s−1) and a median star formation rate (SFR) of ≈1.3 M⊙ yr−1 (not corrected for
possible dust extinction), detected by the Multi-Unit Spectroscopic Explorer as
part of our MUSEQuBES circumgalactic medium (CGM) survey. By postulating that
the stacked CGM absorption profiles of these LAEs, probed by eight background
quasars, must be centred on the systemic redshift, we measure an average velocity
offset, Voffset = 171\pm 8 km s−1, between the Ly α emission peak and the systemic
redshift. The observed Voffset is lower by factors of ≈1.4 and ≈2.6 compared to
the velocity offsets measured for narrow-band-selected LAEs and Lyman break galaxies,
respectively, which probe galaxies with higher masses and SFRs. Consistent with
earlier studies based on direct measurements for individual objects, we find that
the Voffset is correlated with the full width at half-maximum of the red peak
of the Ly α line, and anticorrelated with the rest-frame equivalent width. Moreover,
we find that Voffset is correlated with SFR with a sub-linear scaling relation,
Voffset∝SFR0.16±0.03. Adopting the mass scaling for main-sequence galaxies, such
a relation suggests that Voffset scales with the circular velocity of the dark
matter haloes hosting the LAEs.
acknowledgement: 'We thank the anonymous referee for useful suggestions. This study
is based on observations collected at the European Organisation for Astronomical
Research in the Southern Hemisphere under ESO programme(s): 094.A-0131(B), 095.A
0200(A), 096.A0222(A), 097.A-0089(A), and 099.A-0159(A). SM acknowledges support
from the Alexander von Humboldt Foundation, Germany. SM thanks Christian Herenz
for useful discussion. SC gratefully acknowledges support from Swiss National Science
Foundation grant PP00P2 163824. JB acknowledges support by FCT/MCTES through national
funds by grant UID/FIS/04434/2019 and through Investigador FCT Contract No. IF/01654/2014/CP1215/CT0003.
NB and JZ acknowledge support from ANR grant ANR-17-CE31- 0017 (3DGasFlows). AC
and JR acknowledge support from the ERC starting grant 336736-CALENDS. MA acknowledges
support from European Union’s H2020 Marie Skłodowska-Curie Actions grant 721463
to the SUNDIAL ITN, and from the Spanish Ministry of Economy and Competitiveness
(MINECO) under grant number AYA2016-76219-P. MA also acknowledges support from the
Fundacion BBVA under its 2017 programme of assistance to ´scientific research groups,
for the project ‘Using machine-learning techniques to drag galaxies from the noise
in deep imaging’. FL and AV acknowledge support from the ERC starting grant ERC757258-TRIPLE.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Sowgat
full_name: Muzahid, Sowgat
last_name: Muzahid
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Raffaella Anna
full_name: Marino, Raffaella Anna
last_name: Marino
- first_name: Sebastiano
full_name: Cantalupo, Sebastiano
last_name: Cantalupo
- first_name: Jarle
full_name: Brinchmann, Jarle
last_name: Brinchmann
- first_name: Thierry
full_name: Contini, Thierry
last_name: Contini
- first_name: Martin
full_name: Wendt, Martin
last_name: Wendt
- first_name: Lutz
full_name: Wisotzki, Lutz
last_name: Wisotzki
- first_name: Johannes
full_name: Zabl, Johannes
last_name: Zabl
- first_name: Nicolas
full_name: Bouché, Nicolas
last_name: Bouché
- first_name: Mohammad
full_name: Akhlaghi, Mohammad
last_name: Akhlaghi
- first_name: Hsiao-Wen
full_name: Chen, Hsiao-Wen
last_name: Chen
- first_name: Adélaîde
full_name: Claeyssens, Adélaîde
last_name: Claeyssens
- first_name: Sean
full_name: Johnson, Sean
last_name: Johnson
- first_name: Floriane
full_name: Leclercq, Floriane
last_name: Leclercq
- first_name: Michael
full_name: Maseda, Michael
last_name: Maseda
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: Tanya
full_name: Urrutia, Tanya
last_name: Urrutia
- first_name: Anne
full_name: Verhamme, Anne
last_name: Verhamme
citation:
ama: 'Muzahid S, Schaye J, Marino RA, et al. MUSEQuBES: Calibrating the redshifts
of Lyα emitters using stacked circumgalactic medium absorption profiles. Monthly
Notices of the Royal Astronomical Society. 2020;496(2):1013-1022. doi:10.1093/mnras/staa1347'
apa: 'Muzahid, S., Schaye, J., Marino, R. A., Cantalupo, S., Brinchmann, J., Contini,
T., … Verhamme, A. (2020). MUSEQuBES: Calibrating the redshifts of Lyα emitters
using stacked circumgalactic medium absorption profiles. Monthly Notices of
the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staa1347'
chicago: 'Muzahid, Sowgat, Joop Schaye, Raffaella Anna Marino, Sebastiano Cantalupo,
Jarle Brinchmann, Thierry Contini, Martin Wendt, et al. “MUSEQuBES: Calibrating
the Redshifts of Lyα Emitters Using Stacked Circumgalactic Medium Absorption Profiles.”
Monthly Notices of the Royal Astronomical Society. Oxford University Press,
2020. https://doi.org/10.1093/mnras/staa1347.'
ieee: 'S. Muzahid et al., “MUSEQuBES: Calibrating the redshifts of Lyα emitters
using stacked circumgalactic medium absorption profiles,” Monthly Notices of
the Royal Astronomical Society, vol. 496, no. 2. Oxford University Press,
pp. 1013–1022, 2020.'
ista: 'Muzahid S, Schaye J, Marino RA, Cantalupo S, Brinchmann J, Contini T, Wendt
M, Wisotzki L, Zabl J, Bouché N, Akhlaghi M, Chen H-W, Claeyssens A, Johnson S,
Leclercq F, Maseda M, Matthee JJ, Richard J, Urrutia T, Verhamme A. 2020. MUSEQuBES:
Calibrating the redshifts of Lyα emitters using stacked circumgalactic medium
absorption profiles. Monthly Notices of the Royal Astronomical Society. 496(2),
1013–1022.'
mla: 'Muzahid, Sowgat, et al. “MUSEQuBES: Calibrating the Redshifts of Lyα Emitters
Using Stacked Circumgalactic Medium Absorption Profiles.” Monthly Notices of
the Royal Astronomical Society, vol. 496, no. 2, Oxford University Press,
2020, pp. 1013–22, doi:10.1093/mnras/staa1347.'
short: S. Muzahid, J. Schaye, R.A. Marino, S. Cantalupo, J. Brinchmann, T. Contini,
M. Wendt, L. Wisotzki, J. Zabl, N. Bouché, M. Akhlaghi, H.-W. Chen, A. Claeyssens,
S. Johnson, F. Leclercq, M. Maseda, J.J. Matthee, J. Richard, T. Urrutia, A. Verhamme,
Monthly Notices of the Royal Astronomical Society 496 (2020) 1013–1022.
date_created: 2022-07-07T10:20:11Z
date_published: 2020-08-01T00:00:00Z
date_updated: 2022-08-18T11:00:24Z
day: '01'
doi: 10.1093/mnras/staa1347
extern: '1'
external_id:
arxiv:
- '1910.03593'
intvolume: ' 496'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: haloes'
- 'galaxies: high-redshift'
- 'quasars: absorption lines'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1910.03593
month: '08'
oa: 1
oa_version: Preprint
page: 1013-1022
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
related_material:
link:
- relation: erratum
url: https://doi.org/10.1093/mnras/staa2668
scopus_import: '1'
status: public
title: 'MUSEQuBES: Calibrating the redshifts of Lyα emitters using stacked circumgalactic
medium absorption profiles'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 496
year: '2020'
...
---
_id: '11529'
abstract:
- lang: eng
text: CR7 is among the most luminous Ly α emitters (LAEs) known at z = 6.6 and consists
of at least three UV components that are surrounded by Ly α emission. Previous
studies have suggested that it may host an extreme ionizing source. Here, we present
deep integral field spectroscopy of CR7 with VLT/Multi Unit Spectroscopic Explorer
(MUSE). We measure extended emission with a similar halo scale length as typical
LAEs at z ≈ 5. CR7’s Ly α halo is clearly elongated along the direction connecting
the multiple components, likely tracing the underlying gas distribution. The Ly α
emission originates almost exclusively from the brightest UV component, but we
also identify a faint kinematically distinct Ly α emitting region nearby a fainter
component. Combined with new near-infrared data, the MUSE data show that the rest-frame
Ly α equivalent width (EW) is ≈100 Å. This is a factor 4 higher than the EW measured
in low-redshift analogues with carefully matched Ly α profiles (and thus arguably
H I column density), but this EW can plausibly be explained by star formation.
Alternative scenarios requiring active galactic nucleus (AGN) powering are also
disfavoured by the narrower and steeper Ly α spectrum and much smaller IR to UV
ratio compared to obscured AGN in other Ly α blobs. CR7’s Ly α emission, while
extremely luminous, resembles the emission in more common LAEs at lower redshifts
very well and is likely powered by a young metal-poor starburst.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Gabriele
full_name: Pezzulli, Gabriele
last_name: Pezzulli
- first_name: Ruari
full_name: Mackenzie, Ruari
last_name: Mackenzie
- first_name: Sebastiano
full_name: Cantalupo, Sebastiano
last_name: Cantalupo
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- first_name: Floriane
full_name: Leclercq, Floriane
last_name: Leclercq
- first_name: David
full_name: Sobral, David
last_name: Sobral
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: Lutz
full_name: Wisotzki, Lutz
last_name: Wisotzki
- first_name: Simon
full_name: Lilly, Simon
last_name: Lilly
- first_name: Leindert
full_name: Boogaard, Leindert
last_name: Boogaard
- first_name: Raffaella
full_name: Marino, Raffaella
last_name: Marino
- first_name: Michael
full_name: Maseda, Michael
last_name: Maseda
- first_name: Themiya
full_name: Nanayakkara, Themiya
last_name: Nanayakkara
citation:
ama: 'Matthee JJ, Pezzulli G, Mackenzie R, et al. The nature of CR7 revealed with
MUSE: A young starburst powering extended Ly α emission at z = 6.6. Monthly
Notices of the Royal Astronomical Society. 2020;498(2):3043-3059. doi:10.1093/mnras/staa2550'
apa: 'Matthee, J. J., Pezzulli, G., Mackenzie, R., Cantalupo, S., Kusakabe, H.,
Leclercq, F., … Nanayakkara, T. (2020). The nature of CR7 revealed with MUSE:
A young starburst powering extended Ly α emission at z = 6.6. Monthly Notices
of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staa2550'
chicago: 'Matthee, Jorryt J, Gabriele Pezzulli, Ruari Mackenzie, Sebastiano Cantalupo,
Haruka Kusakabe, Floriane Leclercq, David Sobral, et al. “The Nature of CR7 Revealed
with MUSE: A Young Starburst Powering Extended Ly α Emission at z = 6.6.” Monthly
Notices of the Royal Astronomical Society. Oxford University Press, 2020.
https://doi.org/10.1093/mnras/staa2550.'
ieee: 'J. J. Matthee et al., “The nature of CR7 revealed with MUSE: A young
starburst powering extended Ly α emission at z = 6.6,” Monthly Notices of the
Royal Astronomical Society, vol. 498, no. 2. Oxford University Press, pp.
3043–3059, 2020.'
ista: 'Matthee JJ, Pezzulli G, Mackenzie R, Cantalupo S, Kusakabe H, Leclercq F,
Sobral D, Richard J, Wisotzki L, Lilly S, Boogaard L, Marino R, Maseda M, Nanayakkara
T. 2020. The nature of CR7 revealed with MUSE: A young starburst powering extended
Ly α emission at z = 6.6. Monthly Notices of the Royal Astronomical Society. 498(2),
3043–3059.'
mla: 'Matthee, Jorryt J., et al. “The Nature of CR7 Revealed with MUSE: A Young
Starburst Powering Extended Ly α Emission at z = 6.6.” Monthly Notices of the
Royal Astronomical Society, vol. 498, no. 2, Oxford University Press, 2020,
pp. 3043–59, doi:10.1093/mnras/staa2550.'
short: J.J. Matthee, G. Pezzulli, R. Mackenzie, S. Cantalupo, H. Kusakabe, F. Leclercq,
D. Sobral, J. Richard, L. Wisotzki, S. Lilly, L. Boogaard, R. Marino, M. Maseda,
T. Nanayakkara, Monthly Notices of the Royal Astronomical Society 498 (2020) 3043–3059.
date_created: 2022-07-07T10:36:01Z
date_published: 2020-10-01T00:00:00Z
date_updated: 2022-08-18T11:04:05Z
day: '01'
doi: 10.1093/mnras/staa2550
extern: '1'
external_id:
arxiv:
- '2008.01731'
intvolume: ' 498'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: high-redshift'
- dark ages
- reionization
- first stars
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2008.01731
month: '10'
oa: 1
oa_version: Preprint
page: 3043-3059
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'The nature of CR7 revealed with MUSE: A young starburst powering extended
Ly α emission at z = 6.6'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 498
year: '2020'
...
---
_id: '11530'
abstract:
- lang: eng
text: A prediction of the classic active galactic nucleus (AGN) unification model
is the presence of ionization cones with different orientations depending on the
AGN type. Confirmations of this model exist for present times, but it is less
clear in the early Universe. Here, we use the morphology of giant Ly α nebulae
around AGNs at redshift z ∼ 3 to probe AGN emission and therefore the validity
of the AGN unification model at this redshift. We compare the spatial morphology
of 19 nebulae previously found around type I AGNs with a new sample of four Ly α
nebulae detected around type II AGNs. Using two independent techniques, we find
that nebulae around type II AGNs are more asymmetric than around type I, at least
at radial distances r > 30 physical kpc (pkpc) from the ionizing source. We conclude
that the type I and type II AGNs in our sample show evidence of different surrounding
ionizing geometries. This suggests that the classical AGN unification model is
also valid for high-redshift sources. Finally, we discuss how the lack of asymmetry
in the inner parts (r ≲ 30 pkpc) and the associated high values of the He II to
Ly α ratios in these regions could indicate additional sources of (hard) ionizing
radiation originating within or in proximity of the AGN host galaxies. This work
demonstrates that the morphologies of giant Ly α nebulae can be used to understand
and study the geometry of high-redshift AGNs on circumnuclear scales and it lays
the foundation for future studies using much larger statistical samples.
acknowledgement: SC and GP gratefully acknowledge support from Swiss National Science
Foundation grant PP00P2 163824. MK acknowledges support by DLR500R1904.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: J S
full_name: den Brok, J S
last_name: den Brok
- first_name: S
full_name: Cantalupo, S
last_name: Cantalupo
- first_name: R
full_name: Mackenzie, R
last_name: Mackenzie
- first_name: R A
full_name: Marino, R A
last_name: Marino
- first_name: G
full_name: Pezzulli, G
last_name: Pezzulli
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: S D
full_name: Johnson, S D
last_name: Johnson
- first_name: M
full_name: Krumpe, M
last_name: Krumpe
- first_name: T
full_name: Urrutia, T
last_name: Urrutia
- first_name: W
full_name: Kollatschny, W
last_name: Kollatschny
citation:
ama: den Brok JS, Cantalupo S, Mackenzie R, et al. Probing the AGN unification model
at redshift z ∼ 3 with MUSE observations of giant Lyα nebulae. Monthly Notices
of the Royal Astronomical Society. 2020;495(2):1874-1887. doi:10.1093/mnras/staa1269
apa: den Brok, J. S., Cantalupo, S., Mackenzie, R., Marino, R. A., Pezzulli, G.,
Matthee, J. J., … Kollatschny, W. (2020). Probing the AGN unification model at
redshift z ∼ 3 with MUSE observations of giant Lyα nebulae. Monthly Notices
of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staa1269
chicago: den Brok, J S, S Cantalupo, R Mackenzie, R A Marino, G Pezzulli, Jorryt
J Matthee, S D Johnson, M Krumpe, T Urrutia, and W Kollatschny. “Probing the AGN
Unification Model at Redshift z ∼ 3 with MUSE Observations of Giant Lyα Nebulae.”
Monthly Notices of the Royal Astronomical Society. Oxford University Press,
2020. https://doi.org/10.1093/mnras/staa1269.
ieee: J. S. den Brok et al., “Probing the AGN unification model at redshift
z ∼ 3 with MUSE observations of giant Lyα nebulae,” Monthly Notices of the
Royal Astronomical Society, vol. 495, no. 2. Oxford University Press, pp.
1874–1887, 2020.
ista: den Brok JS, Cantalupo S, Mackenzie R, Marino RA, Pezzulli G, Matthee JJ,
Johnson SD, Krumpe M, Urrutia T, Kollatschny W. 2020. Probing the AGN unification
model at redshift z ∼ 3 with MUSE observations of giant Lyα nebulae. Monthly Notices
of the Royal Astronomical Society. 495(2), 1874–1887.
mla: den Brok, J. S., et al. “Probing the AGN Unification Model at Redshift z ∼
3 with MUSE Observations of Giant Lyα Nebulae.” Monthly Notices of the Royal
Astronomical Society, vol. 495, no. 2, Oxford University Press, 2020, pp.
1874–87, doi:10.1093/mnras/staa1269.
short: J.S. den Brok, S. Cantalupo, R. Mackenzie, R.A. Marino, G. Pezzulli, J.J.
Matthee, S.D. Johnson, M. Krumpe, T. Urrutia, W. Kollatschny, Monthly Notices
of the Royal Astronomical Society 495 (2020) 1874–1887.
date_created: 2022-07-07T10:40:17Z
date_published: 2020-06-01T00:00:00Z
date_updated: 2022-08-18T11:17:47Z
day: '01'
doi: 10.1093/mnras/staa1269
extern: '1'
external_id:
arxiv:
- '2005.01732'
intvolume: ' 495'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: active'
- 'galaxies: high-redshift'
- intergalactic medium
- 'quasars: emission lines'
- 'quasars: general'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/2005.01732
month: '06'
oa: 1
oa_version: Preprint
page: 1874-1887
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Probing the AGN unification model at redshift z ∼ 3 with MUSE observations
of giant Lyα nebulae
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 495
year: '2020'
...
---
_id: '11531'
abstract:
- lang: eng
text: While low-luminosity galaxies dominate number counts at all redshifts, their
contribution to cosmic reionization is poorly understood due to a lack of knowledge
of their physical properties. We isolate a sample of 35 z ≈ 4–5 continuum-faint
Lyman-α emitters from deep VLT/MUSE spectroscopy and directly measure their H α
emission using stacked Spitzer/IRAC Ch. 1 photometry. Based on Hubble Space Telescope
imaging, we determine that the average UV continuum magnitude is fainter than
−16 (≈ 0.01 L⋆), implying a median Lyman-α equivalent width of 259 Å. By combining
the H α measurement with the UV magnitude, we determine the ionizing photon production
efficiency, ξion, a first for such faint galaxies. The measurement of log10 (ξion
[Hz erg−1]) = 26.28 (+0.28−0.40) is in excess of literature measurements of
both continuum- and emission line-selected samples, implying a more efficient
production of ionizing photons in these lower luminosity, Lyman-α-selected systems.
We conclude that this elevated efficiency can be explained by stellar populations
with metallicities between 4 × 10−4 and 0.008, with light-weighted ages less than
3 Myr.
acknowledgement: 'We would like to thank the anonymous referee for a thoughtful report
and suggestions that have improved this manuscript. We are also grateful to everyone
involved in the Spitzer Space Telescope mission and everyone at the Spitzer Science
Center: we are truly fortunate to have been able to use data from this facility.
J. B. acknowledges support by FCT/MCTES through national funds by this grant UID/FIS/04434/2019
and through the Investigador FCT contract no. IF/01654/2014/CP1215/CT0003. S. C.
gratefully acknowledges support from Swiss National Science Foundation grant PP00P2
163824. We would also like to thank Mauro Stefanon for his assistance with de-blending
the IRAC photometry, Pieter van Dokkum for a number of useful suggestions, and Daniel
Schaerer for information regarding the stellar population models. This study is
based on observations made with ESO telescopes at the La Silla Paranal Observatory
under programs IDs 094.A-2089(B), 095.A0010(A), 096.A-0045(A), and 096.A-0045(B).'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Michael V
full_name: Maseda, Michael V
last_name: Maseda
- first_name: Roland
full_name: Bacon, Roland
last_name: Bacon
- first_name: Daniel
full_name: Lam, Daniel
last_name: Lam
- first_name: Jorryt J
full_name: Matthee, Jorryt J
id: 7439a258-f3c0-11ec-9501-9df22fe06720
last_name: Matthee
orcid: 0000-0003-2871-127X
- first_name: Jarle
full_name: Brinchmann, Jarle
last_name: Brinchmann
- first_name: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Ivo
full_name: Labbe, Ivo
last_name: Labbe
- first_name: Kasper B
full_name: Schmidt, Kasper B
last_name: Schmidt
- first_name: Leindert
full_name: Boogaard, Leindert
last_name: Boogaard
- first_name: Rychard
full_name: Bouwens, Rychard
last_name: Bouwens
- first_name: Sebastiano
full_name: Cantalupo, Sebastiano
last_name: Cantalupo
- first_name: Marijn
full_name: Franx, Marijn
last_name: Franx
- first_name: Takuya
full_name: Hashimoto, Takuya
last_name: Hashimoto
- first_name: Hanae
full_name: Inami, Hanae
last_name: Inami
- first_name: Haruka
full_name: Kusakabe, Haruka
last_name: Kusakabe
- first_name: Guillaume
full_name: Mahler, Guillaume
last_name: Mahler
- first_name: Themiya
full_name: Nanayakkara, Themiya
last_name: Nanayakkara
- first_name: Johan
full_name: Richard, Johan
last_name: Richard
- first_name: Lutz
full_name: Wisotzki, Lutz
last_name: Wisotzki
citation:
ama: Maseda MV, Bacon R, Lam D, et al. Elevated ionizing photon production efficiency
in faint high-equivalent-width Lyman-α emitters. Monthly Notices of the Royal
Astronomical Society. 2020;493(4):5120-5130. doi:10.1093/mnras/staa622
apa: Maseda, M. V., Bacon, R., Lam, D., Matthee, J. J., Brinchmann, J., Schaye,
J., … Wisotzki, L. (2020). Elevated ionizing photon production efficiency in faint
high-equivalent-width Lyman-α emitters. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/staa622
chicago: Maseda, Michael V, Roland Bacon, Daniel Lam, Jorryt J Matthee, Jarle Brinchmann,
Joop Schaye, Ivo Labbe, et al. “Elevated Ionizing Photon Production Efficiency
in Faint High-Equivalent-Width Lyman-α Emitters.” Monthly Notices of the Royal
Astronomical Society. Oxford University Press, 2020. https://doi.org/10.1093/mnras/staa622.
ieee: M. V. Maseda et al., “Elevated ionizing photon production efficiency
in faint high-equivalent-width Lyman-α emitters,” Monthly Notices of the Royal
Astronomical Society, vol. 493, no. 4. Oxford University Press, pp. 5120–5130,
2020.
ista: Maseda MV, Bacon R, Lam D, Matthee JJ, Brinchmann J, Schaye J, Labbe I, Schmidt
KB, Boogaard L, Bouwens R, Cantalupo S, Franx M, Hashimoto T, Inami H, Kusakabe
H, Mahler G, Nanayakkara T, Richard J, Wisotzki L. 2020. Elevated ionizing photon
production efficiency in faint high-equivalent-width Lyman-α emitters. Monthly
Notices of the Royal Astronomical Society. 493(4), 5120–5130.
mla: Maseda, Michael V., et al. “Elevated Ionizing Photon Production Efficiency
in Faint High-Equivalent-Width Lyman-α Emitters.” Monthly Notices of the Royal
Astronomical Society, vol. 493, no. 4, Oxford University Press, 2020, pp.
5120–30, doi:10.1093/mnras/staa622.
short: M.V. Maseda, R. Bacon, D. Lam, J.J. Matthee, J. Brinchmann, J. Schaye, I.
Labbe, K.B. Schmidt, L. Boogaard, R. Bouwens, S. Cantalupo, M. Franx, T. Hashimoto,
H. Inami, H. Kusakabe, G. Mahler, T. Nanayakkara, J. Richard, L. Wisotzki, Monthly
Notices of the Royal Astronomical Society 493 (2020) 5120–5130.
date_created: 2022-07-07T10:46:41Z
date_published: 2020-04-01T00:00:00Z
date_updated: 2022-08-18T11:23:27Z
day: '01'
doi: 10.1093/mnras/staa622
extern: '1'
external_id:
arxiv:
- '2002.11117'
intvolume: ' 493'
issue: '4'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'Galaxies: evolution'
- 'Galaxies: high-redshift'
- 'Galaxies: ISM'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.1093/mnras/staa622
month: '04'
oa: 1
oa_version: Published Version
page: 5120-5130
publication: Monthly Notices of the Royal Astronomical Society
publication_identifier:
eissn:
- 1365-2966
issn:
- 0035-8711
publication_status: published
publisher: Oxford University Press
quality_controlled: '1'
scopus_import: '1'
status: public
title: Elevated ionizing photon production efficiency in faint high-equivalent-width
Lyman-α emitters
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 493
year: '2020'
...