---
_id: '11562'
abstract:
- lang: eng
text: We present the CAlibrating LYMan-α with Hα (CALYMHA) pilot survey and new
results on Lyman α (Lyα) selected galaxies at z ∼ 2. We use a custom-built Lyα
narrow-band filter at the Isaac Newton Telescope, designed to provide a matched
volume coverage to the z = 2.23 Hα HiZELS survey. Here, we present the first results
for the COSMOS and UDS fields. Our survey currently reaches a 3σ line flux limit
of ∼4 × 10−17 erg s−1 cm−2, and a Lyα luminosity limit of ∼1042.3 erg s−1. We
find 188 Lyα emitters over 7.3 × 105 Mpc3, but also find significant numbers of
other line-emitting sources corresponding to He II, C III] and C IV emission lines.
These sources are important contaminants, and we carefully remove them, unlike
most previous studies. We find that the Lyα luminosity function at z = 2.23 is
very well described by a Schechter function up to LLy α ≈ 1043 erg s−1 with L∗=1042.59+0.16−0.08
erg s−1, ϕ∗=10−3.09+0.14−0.34 Mpc−3 and α = −1.75 ± 0.25. Above LLy α ≈ 1043 erg
s−1, the Lyα luminosity function becomes power-law like, driven by X-ray AGN.
We find that Lyα-selected emitters have a high escape fraction of 37 ± 7 per cent,
anticorrelated with Lyα luminosity and correlated with Lyα equivalent width. Lyα
emitters have ubiquitous large (≈40 kpc) Lyα haloes, ∼2 times larger than their
Hα extents. By directly comparing our Lyα and Hα luminosity functions, we find
that the global/overall escape fraction of Lyα photons (within a 13 kpc radius)
from the full population of star-forming galaxies is 5.1 ± 0.2 per cent at the
peak of the star formation history. An extra 3.3 ± 0.3 per cent of Lyα photons
likely still escape, but at larger radii.
acknowledgement: 'We thank the reviewer for his/her helpful comments and suggestions
that have greatly improved this work. DS and JM acknowledge financial support from
the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship.
DS also acknowledges funding from FCT through an FCT Investigator Starting Grant
and Start-up Grant (IF/01154/2012/CP0189/CT0010). PNB is grateful for support from
the UK STFC via grant ST/M001229/1. IRS acknowledges support from STFC (ST/L00075X/1),
the ERC Advanced Investigator programme DUSTYGAL 321334 and a Royal Society/Wolfson
merit award. We thank Matthew Hayes, Ryan Trainor, Kimihiko Nakajima and Anne Verhamme
for many helpful discussions and Ana Sobral, Carolina Duarte and Miguel Domingos
for taking part in observations with the NB392 filter. We also thank Sergio Santos
for helpful comments. This research is based on observations obtained on the Isaac
Newton Telescope (INT), programs: I13AN002, I14AN002, 088-INT7/14A, I14BN006, 118-INT13/14B
& I15AN008. The authors acknowledge the award of time from programmes: I13AN002,
I14AN002, 088-INT7/14A, I14BN006, 118-INT13/14B, I15AN008 on the INT. INT is operated
on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio
del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. Based on
observations made with ESO Telescopes at the La Silla Paranal Observatory under
programme ID 098.A 0819. We have benefited greatly from the publicly available programming
language PYTHON, including the NUMPY, MATPLOTLIB, PYFITS, SCIPY and ASTROPY packages,
the astronomical imaging tools SEXTRACTOR, SWARP (Bertin & Arnouts 1996; Bertin
2010), SCAMP (Bertin 2006) and TOPCAT (Taylor 2005). Dedicated to the memory of
M. L. Nicolau and M. C. Serrano.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: David
full_name: Sobral, David
last_name: Sobral
- 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: Philip
full_name: Best, Philip
last_name: Best
- first_name: Andra
full_name: Stroe, Andra
last_name: Stroe
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
- first_name: Iván
full_name: Oteo, Iván
last_name: Oteo
- first_name: Ian
full_name: Smail, Ian
last_name: Smail
- first_name: Leah
full_name: Morabito, Leah
last_name: Morabito
- first_name: Ana
full_name: Paulino-Afonso, Ana
last_name: Paulino-Afonso
citation:
ama: 'Sobral D, Matthee JJ, Best P, et al. The CALYMHA survey: Lyα luminosity function
and global escape fraction of Lyα photons at z = 2.23. Monthly Notices of the
Royal Astronomical Society. 2017;466(1):1242-1258. doi:10.1093/mnras/stw3090'
apa: 'Sobral, D., Matthee, J. J., Best, P., Stroe, A., Röttgering, H., Oteo, I.,
… Paulino-Afonso, A. (2017). The CALYMHA survey: Lyα luminosity function and global
escape fraction of Lyα photons at z = 2.23. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stw3090'
chicago: 'Sobral, David, Jorryt J Matthee, Philip Best, Andra Stroe, Huub Röttgering,
Iván Oteo, Ian Smail, Leah Morabito, and Ana Paulino-Afonso. “The CALYMHA Survey:
Lyα Luminosity Function and Global Escape Fraction of Lyα Photons at z = 2.23.”
Monthly Notices of the Royal Astronomical Society. Oxford University Press,
2017. https://doi.org/10.1093/mnras/stw3090.'
ieee: 'D. Sobral et al., “The CALYMHA survey: Lyα luminosity function and
global escape fraction of Lyα photons at z = 2.23,” Monthly Notices of the
Royal Astronomical Society, vol. 466, no. 1. Oxford University Press, pp.
1242–1258, 2017.'
ista: 'Sobral D, Matthee JJ, Best P, Stroe A, Röttgering H, Oteo I, Smail I, Morabito
L, Paulino-Afonso A. 2017. The CALYMHA survey: Lyα luminosity function and global
escape fraction of Lyα photons at z = 2.23. Monthly Notices of the Royal Astronomical
Society. 466(1), 1242–1258.'
mla: 'Sobral, David, et al. “The CALYMHA Survey: Lyα Luminosity Function and Global
Escape Fraction of Lyα Photons at z = 2.23.” Monthly Notices of the Royal Astronomical
Society, vol. 466, no. 1, Oxford University Press, 2017, pp. 1242–58, doi:10.1093/mnras/stw3090.'
short: D. Sobral, J.J. Matthee, P. Best, A. Stroe, H. Röttgering, I. Oteo, I. Smail,
L. Morabito, A. Paulino-Afonso, Monthly Notices of the Royal Astronomical Society
466 (2017) 1242–1258.
date_created: 2022-07-12T12:04:16Z
date_published: 2017-04-01T00:00:00Z
date_updated: 2022-08-19T07:18:20Z
day: '01'
doi: 10.1093/mnras/stw3090
extern: '1'
external_id:
arxiv:
- '1609.05897'
intvolume: ' 466'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: haloes'
- 'galaxies: high-redshift'
- 'galaxies: luminosity function'
- mass function
- 'galaxies: statistics'
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1609.05897
month: '04'
oa: 1
oa_version: Preprint
page: 1242-1258
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 CALYMHA survey: Lyα luminosity function and global escape fraction of
Lyα photons at z = 2.23'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 466
year: '2017'
...
---
_id: '11564'
abstract:
- lang: eng
text: We study the production rate of ionizing photons of a sample of 588 Hα emitters
(HAEs) and 160 Lyman-α emitters (LAEs) at z = 2.2 in the COSMOS field in order
to assess the implied emissivity from galaxies, based on their ultraviolet (UV)
luminosity. By exploring the rest-frame Lyman Continuum (LyC) with GALEX/NUV data,
we find fesc < 2.8 (6.4) per cent through median (mean) stacking. By combining
the Hα luminosity density with intergalactic medium emissivity measurements from
absorption studies, we find a globally averaged 〈fesc〉 of 5.9+14.5−4.2 per cent
at z = 2.2 if we assume HAEs are the only source of ionizing photons. We find
similarly low values of the global 〈fesc〉 at z ≈ 3–5, also ruling out a high 〈fesc〉
at z < 5. These low escape fractions allow us to measure ξion, the number of produced
ionizing photons per unit UV luminosity, and investigate how this depends on galaxy
properties. We find a typical ξion ≈ 1024.77 ± 0.04 Hz erg−1 for HAEs and ξion
≈ 1025.14 ± 0.09 Hz erg−1 for LAEs. LAEs and low-mass HAEs at z = 2.2 show similar
values of ξion as typically assumed in the reionization era, while the typical
HAE is three times less ionizing. Due to an increasing ξion with increasing EW(Hα),
ξion likely increases with redshift. This evolution alone is fully in line with
the observed evolution of ξion between z ≈ 2 and 5, indicating a typical value
of ξion ≈ 1025.4 Hz erg−1 in the reionization era.
acknowledgement: "We thank the referee for the many helpful and constructive comments
which have significantly improved this paper. JM acknowledges the support of a Huygens
PhD fellowship from Leiden University. DS acknowledges financial support from the
Netherlands Organization for Scientific research (NWO) through a Veni fellowship
and from FCT through an FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010).
PNB is grateful for support from the UK STFC via grant ST/M001229/1. IO acknowledges
support from the European Research Council in the form of the Advanced Investigator
Programme, 321302, COSMICISM. The authors thank Andreas Faisst, Michael Rutkowski
and Andreas Sandberg for answering questions related to this work and Daniel Schaerer
and Mark Dijkstra for discussions. We acknowledge the work that has been done by
both the COSMOS team in assembling such large, state-of-the-art multi-wavelength
data set, as this has been crucial for the results presented in this paper. We have
benefited greatly from the public available programming language PYTHON, including
the NUMPY, MATPLOTLIB, PYFITS, SCIPY (Jones et al. 2001; Hunter 2007; Van Der Walt,
Colbert & Varoquaux 2011) and ASTROPY (Astropy Collaboration et al. 2013) packages,
the astronomical imaging tools SEXTRACTOR and SWARP (Bertin & Arnouts 1996;\r\nBertin
2010) and the TOPCAT analysis program (Taylor 2013)."
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: David
full_name: Sobral, David
last_name: Sobral
- first_name: Philip
full_name: Best, Philip
last_name: Best
- first_name: Ali Ahmad
full_name: Khostovan, Ali Ahmad
last_name: Khostovan
- first_name: Iván
full_name: Oteo, Iván
last_name: Oteo
- first_name: Rychard
full_name: Bouwens, Rychard
last_name: Bouwens
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
citation:
ama: Matthee JJ, Sobral D, Best P, et al. The production and escape of Lyman-Continuum
radiation from star-forming galaxies at z ∼ 2 and their redshift evolution. Monthly
Notices of the Royal Astronomical Society. 2017;465(3):3637-3655. doi:10.1093/mnras/stw2973
apa: Matthee, J. J., Sobral, D., Best, P., Khostovan, A. A., Oteo, I., Bouwens,
R., & Röttgering, H. (2017). The production and escape of Lyman-Continuum
radiation from star-forming galaxies at z ∼ 2 and their redshift evolution. Monthly
Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stw2973
chicago: Matthee, Jorryt J, David Sobral, Philip Best, Ali Ahmad Khostovan, Iván
Oteo, Rychard Bouwens, and Huub Röttgering. “The Production and Escape of Lyman-Continuum
Radiation from Star-Forming Galaxies at z ∼ 2 and Their Redshift Evolution.” Monthly
Notices of the Royal Astronomical Society. Oxford University Press, 2017.
https://doi.org/10.1093/mnras/stw2973.
ieee: J. J. Matthee et al., “The production and escape of Lyman-Continuum
radiation from star-forming galaxies at z ∼ 2 and their redshift evolution,” Monthly
Notices of the Royal Astronomical Society, vol. 465, no. 3. Oxford University
Press, pp. 3637–3655, 2017.
ista: Matthee JJ, Sobral D, Best P, Khostovan AA, Oteo I, Bouwens R, Röttgering
H. 2017. The production and escape of Lyman-Continuum radiation from star-forming
galaxies at z ∼ 2 and their redshift evolution. Monthly Notices of the Royal Astronomical
Society. 465(3), 3637–3655.
mla: Matthee, Jorryt J., et al. “The Production and Escape of Lyman-Continuum Radiation
from Star-Forming Galaxies at z ∼ 2 and Their Redshift Evolution.” Monthly
Notices of the Royal Astronomical Society, vol. 465, no. 3, Oxford University
Press, 2017, pp. 3637–55, doi:10.1093/mnras/stw2973.
short: J.J. Matthee, D. Sobral, P. Best, A.A. Khostovan, I. Oteo, R. Bouwens, H.
Röttgering, Monthly Notices of the Royal Astronomical Society 465 (2017) 3637–3655.
date_created: 2022-07-12T12:12:14Z
date_published: 2017-03-01T00:00:00Z
date_updated: 2022-08-19T07:53:04Z
day: '01'
doi: 10.1093/mnras/stw2973
extern: '1'
external_id:
arxiv:
- '1605.08782'
intvolume: ' 465'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: high-redshift'
- 'cosmology: observations'
- dark ages
- reionization
- first stars
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1605.08782
month: '03'
oa: 1
oa_version: Preprint
page: 3637-3655
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 production and escape of Lyman-Continuum radiation from star-forming galaxies
at z ∼ 2 and their redshift evolution
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 465
year: '2017'
...
---
_id: '11565'
abstract:
- lang: eng
text: We use the hydrodynamical EAGLE simulation to study the magnitude and origin
of the scatter in the stellar mass–halo mass relation for central galaxies. We
separate cause and effect by correlating stellar masses in the baryonic simulation
with halo properties in a matched dark matter only (DMO) simulation. The scatter
in stellar mass increases with redshift and decreases with halo mass. At z = 0.1,
it declines from 0.25 dex at M200, DMO ≈ 1011 M⊙ to 0.12 dex at M200, DMO ≈ 1013
M⊙, but the trend is weak above 1012 M⊙. For M200, DMO < 1012.5 M⊙ up to 0.04
dex of the scatter is due to scatter in the halo concentration. At fixed halo
mass, a larger stellar mass corresponds to a more concentrated halo. This is likely
because higher concentrations imply earlier formation times and hence more time
for accretion and star formation, and/or because feedback is less efficient in
haloes with higher binding energies. The maximum circular velocity, Vmax, DMO,
and binding energy are therefore more fundamental properties than halo mass, meaning
that they are more accurate predictors of stellar mass, and we provide fitting
formulae for their relations with stellar mass. However, concentration alone cannot
explain the total scatter in the Mstar−M200,DMO relation, and it does not explain
the scatter in Mstar–Vmax, DMO. Halo spin, sphericity, triaxiality, substructure
and environment are also not responsible for the remaining scatter, which thus
could be due to more complex halo properties or non-linear/stochastic baryonic
effects.
acknowledgement: We thank the anonymous referee for their comments. JM acknowledges
the support of a Huygens PhD fellowship from Leiden University. JM thanks David
Sobral for useful discussions and help with fitting routines and Jonas Chavez Montero
and Ying Zu for providing data. We thank PRACE for the access to the Curie facility
in France. We have used the DiRAC system which is a part of National E-Infrastructure
at Durham University, operated by the Institute for Computational Cosmology on behalf
of the STFC DiRAC HPC Facility (www.dirac.ac.uk); the equipment was funded by BIS
National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1,
STFC DiRAC Operations grant ST/K003267/1 and Durham University. The study was sponsored
by the Dutch National Computing Facilities Foundation (NCF) for the use of supercomputer
facilities, with financial support from the Netherlands Organisation for Scientific
Research (NWO), through VICI grant 639.043.409, and the European Research Council
under the European Union’s Seventh Framework Programme (FP7/2007-2013)/ERC Grant
agreement 278594- GasAroundGalaxies, and from the Belgian Science Policy Office
([AP P7/08 CHARM]). We have benefited greatly from the public available programming
language PYTHON, including the NUMPY, MATPLOTLIB, PYFITS, SCIPY, H5PY and RPY2 packages,
and the TOPCAT analysis program (Taylor 2005).
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: Joop
full_name: Schaye, Joop
last_name: Schaye
- first_name: Robert A.
full_name: Crain, Robert A.
last_name: Crain
- first_name: Matthieu
full_name: Schaller, Matthieu
last_name: Schaller
- first_name: Richard
full_name: Bower, Richard
last_name: Bower
- first_name: Tom
full_name: Theuns, Tom
last_name: Theuns
citation:
ama: Matthee JJ, Schaye J, Crain RA, Schaller M, Bower R, Theuns T. The origin of
scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE
simulation. Monthly Notices of the Royal Astronomical Society. 2017;465(2):2381-2396.
doi:10.1093/mnras/stw2884
apa: Matthee, J. J., Schaye, J., Crain, R. A., Schaller, M., Bower, R., & Theuns,
T. (2017). The origin of scatter in the stellar mass–halo mass relation of central
galaxies in the EAGLE simulation. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stw2884
chicago: Matthee, Jorryt J, Joop Schaye, Robert A. Crain, Matthieu Schaller, Richard
Bower, and Tom Theuns. “The Origin of Scatter in the Stellar Mass–Halo Mass Relation
of Central Galaxies in the EAGLE Simulation.” Monthly Notices of the Royal
Astronomical Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stw2884.
ieee: J. J. Matthee, J. Schaye, R. A. Crain, M. Schaller, R. Bower, and T. Theuns,
“The origin of scatter in the stellar mass–halo mass relation of central galaxies
in the EAGLE simulation,” Monthly Notices of the Royal Astronomical Society,
vol. 465, no. 2. Oxford University Press, pp. 2381–2396, 2017.
ista: Matthee JJ, Schaye J, Crain RA, Schaller M, Bower R, Theuns T. 2017. The origin
of scatter in the stellar mass–halo mass relation of central galaxies in the EAGLE
simulation. Monthly Notices of the Royal Astronomical Society. 465(2), 2381–2396.
mla: Matthee, Jorryt J., et al. “The Origin of Scatter in the Stellar Mass–Halo
Mass Relation of Central Galaxies in the EAGLE Simulation.” Monthly Notices
of the Royal Astronomical Society, vol. 465, no. 2, Oxford University Press,
2017, pp. 2381–96, doi:10.1093/mnras/stw2884.
short: J.J. Matthee, J. Schaye, R.A. Crain, M. Schaller, R. Bower, T. Theuns, Monthly
Notices of the Royal Astronomical Society 465 (2017) 2381–2396.
date_created: 2022-07-12T12:25:08Z
date_published: 2017-02-01T00:00:00Z
date_updated: 2022-08-19T07:56:07Z
day: '01'
doi: 10.1093/mnras/stw2884
extern: '1'
external_id:
arxiv:
- '1608.08218'
intvolume: ' 465'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: formation'
- 'galaxies: haloes'
- 'cosmology: theory'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1608.08218
month: '02'
oa: 1
oa_version: Preprint
page: 2381-2396
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 origin of scatter in the stellar mass–halo mass relation of central galaxies
in the EAGLE simulation
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 465
year: '2017'
...
---
_id: '11566'
abstract:
- lang: eng
text: While traditionally associated with active galactic nuclei (AGN), the properties
of the C II] (λ = 2326 Å), C III] (λ, λ = 1907, 1909 Å) and C IV (λ, λ = 1549,
1551 Å) emission lines are still uncertain as large, unbiased samples of sources
are scarce. We present the first blind, statistical study of C II], C III] and
C IV emitters at z ∼ 0.68, 1.05, 1.53, respectively, uniformly selected down to
a flux limit of ∼4 × 10−17 erg s−1 cm−1 through a narrow-band survey covering
an area of ∼1.4 deg2 over COSMOS and UDS. We detect 16 C II], 35 C III] and 17
C IV emitters, whose nature we investigate using optical colours as well as Hubble
Space Telescope (HST), X-ray, radio and far-infrared data. We find that z ∼ 0.7
C II] emitters are consistent with a mixture of blue (UV slope β = −2.0 ± 0.4)
star-forming (SF) galaxies with discy HST structure and AGN with Seyfert-like
morphologies. Bright C II] emitters have individual X-ray detections as well as
high average black hole accretion rates (BHARs) of ∼0.1 M⊙ yr−1. C III] emitters
at z ∼ 1.05 trace a general population of SF galaxies, with β = −0.8 ± 1.1, a
variety of optical morphologies, including isolated and interacting galaxies and
low BHAR (<0.02 M⊙ yr−1). Our C IV emitters at z ∼ 1.5 are consistent with young,
blue quasars (β ∼ −1.9) with point-like optical morphologies, bright X-ray counterparts
and large BHAR (0.8 M⊙ yr−1). We also find some surprising C II], C III] and
C IV emitters with rest-frame equivalent widths (EWs) that could be as large as
50–100 Å. AGN or spatial offsets between the UV continuum stellar disc and the
line-emitting regions may explain the large EW. These bright C II], C III] and
C IV emitters are ideal candidates for spectroscopic follow-up to fully unveil
their nature.
acknowledgement: 'We would like to thank the anonymous referee for her/his valuable
input that helped improve the clarity and interpretation of our results. DS acknowledges
financial support from the Netherlands Organisation for Scientific research (NWO),
through a Veni fellowship. IO acknowledges support from the European Research Council
in the form of the Advanced Investigator Programme, 321302, COSMICISM. CALYMHA data
are based on observations made with the Isaac Newton Telescope (proposals 13AN002,
I14AN002, 088-INT7/14A, I14BN006, 118-INT13/14B, I15AN008) operated on the island
of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los
Muchachos of the Instituto de Astrofísica de Canarias. Also based on data products
from observations made with ESO Telescopes at the La Silla Paranal Observatory under
ESO programme IDs 098.A-0819 and 179.A-2005. We are grateful to E. L. Wright and
J. Schombert for their cosmology calculator. We would like to thank the authors
of NUMPY (van der Walt et al. 2011), SCIPY (Jones et al. 2001), MATPLOTLIB (Hunter
2007) and ASTROPY (Astropy Collaboration et al. 2013) for making these packages
publicly available. This research has made use of the NASA/IPAC Extragalactic Database
(NED), which is '
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Andra
full_name: Stroe, Andra
last_name: Stroe
- first_name: David
full_name: Sobral, David
last_name: Sobral
- 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: João
full_name: Calhau, João
last_name: Calhau
- first_name: Ivan
full_name: Oteo, Ivan
last_name: Oteo
citation:
ama: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. A 1.4 deg2 blind survey for
C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and equivalent
widths . Monthly Notices of the Royal Astronomical Society. 2017;471(3):2558-2574.
doi:10.1093/mnras/stx1712
apa: Stroe, A., Sobral, D., Matthee, J. J., Calhau, J., & Oteo, I. (2017). A
1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies
and equivalent widths . Monthly Notices of the Royal Astronomical Society.
Oxford University Press. https://doi.org/10.1093/mnras/stx1712
chicago: Stroe, Andra, David Sobral, Jorryt J Matthee, João Calhau, and Ivan Oteo.
“A 1.4 Deg2 Blind Survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature,
Morphologies and Equivalent Widths .” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1712.
ieee: A. Stroe, D. Sobral, J. J. Matthee, J. Calhau, and I. Oteo, “A 1.4 deg2 blind
survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and
equivalent widths ,” Monthly Notices of the Royal Astronomical Society,
vol. 471, no. 3. Oxford University Press, pp. 2558–2574, 2017.
ista: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. 2017. A 1.4 deg2 blind survey
for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature, morphologies and equivalent
widths . Monthly Notices of the Royal Astronomical Society. 471(3), 2558–2574.
mla: Stroe, Andra, et al. “A 1.4 Deg2 Blind Survey for C II], C III] and C IV at
z ∼ 0.7–1.5 – I. Nature, Morphologies and Equivalent Widths .” Monthly Notices
of the Royal Astronomical Society, vol. 471, no. 3, Oxford University Press,
2017, pp. 2558–74, doi:10.1093/mnras/stx1712.
short: A. Stroe, D. Sobral, J.J. Matthee, J. Calhau, I. Oteo, Monthly Notices of
the Royal Astronomical Society 471 (2017) 2558–2574.
date_created: 2022-07-12T12:33:16Z
date_published: 2017-11-01T00:00:00Z
date_updated: 2022-08-19T07:59:57Z
day: '01'
doi: 10.1093/mnras/stx1712
extern: '1'
external_id:
arxiv:
- '1703.10169'
intvolume: ' 471'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: active'
- 'galaxies: high-redshift'
- 'quasars: emission lines'
- 'galaxies: star formation'
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1703.10169
month: '11'
oa: 1
oa_version: Preprint
page: 2558-2574
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: 'A 1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – I. Nature,
morphologies and equivalent widths '
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '11567'
abstract:
- lang: eng
text: Recently, the C III] and C IV emission lines have been observed in galaxies
in the early Universe (z > 5), providing new ways to measure their redshift and
study their stellar populations and active galactic nuclei (AGN). We explore the
first blind C II], C III] and C IV survey (z ∼ 0.68, 1.05, 1.53, respectively)
presented in Stroe et al. (2017). We derive luminosity functions (LF) and study
properties of C II], C III] and C IV line emitters through comparisons to the
LFs of H α and Ly α emitters, UV selected star-forming (SF) galaxies and quasars
at similar redshifts. The C II] LF at z ∼ 0.68 is equally well described by a
Schechter or a power-law LF, characteristic of a mixture of SF and AGN activity.
The C III] LF (z ∼ 1.05) is consistent to a scaled down version of the Schechter
H α and Ly α LF at their redshift, indicating a SF origin. In stark contrast,
the C IV LF at z ∼ 1.53 is well fit by a power-law, quasar-like LF. We find that
the brightest UV sources (MUV < −22) will universally have C III] and C IV emission.
However, on average, C III] and C IV are not as abundant as H α or Ly α emitters
at the same redshift, with cosmic average ratios of ∼0.02–0.06 to H α and ∼0.01–0.1
to intrinsic Ly α. We predict that the C III] and C IV lines can only be truly
competitive in confirming high-redshift candidates when the hosts are intrinsically
bright and the effective Ly α escape fraction is below 1 per cent. While C III]
and C IV were proposed as good tracers of young, relatively low-metallicity galaxies
typical of the early Universe, we find that, at least at z ∼ 1.5, C IV is exclusively
hosted by AGN/quasars, especially at large line equivalent widths.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Andra
full_name: Stroe, Andra
last_name: Stroe
- first_name: David
full_name: Sobral, David
last_name: Sobral
- 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: João
full_name: Calhau, João
last_name: Calhau
- first_name: Ivan
full_name: Oteo, Ivan
last_name: Oteo
citation:
ama: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. A 1.4 deg2 blind survey for
C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity functions and cosmic average
line ratios. Monthly Notices of the Royal Astronomical Society. 2017;471(3):2575-2586.
doi:10.1093/mnras/stx1713
apa: Stroe, A., Sobral, D., Matthee, J. J., Calhau, J., & Oteo, I. (2017). A
1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity
functions and cosmic average line ratios. Monthly Notices of the Royal Astronomical
Society. Oxford University Press. https://doi.org/10.1093/mnras/stx1713
chicago: Stroe, Andra, David Sobral, Jorryt J Matthee, João Calhau, and Ivan Oteo.
“A 1.4 Deg2 Blind Survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity
Functions and Cosmic Average Line Ratios.” Monthly Notices of the Royal Astronomical
Society. Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1713.
ieee: A. Stroe, D. Sobral, J. J. Matthee, J. Calhau, and I. Oteo, “A 1.4 deg2 blind
survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity functions and
cosmic average line ratios,” Monthly Notices of the Royal Astronomical Society,
vol. 471, no. 3. Oxford University Press, pp. 2575–2586, 2017.
ista: Stroe A, Sobral D, Matthee JJ, Calhau J, Oteo I. 2017. A 1.4 deg2 blind survey
for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity functions and cosmic
average line ratios. Monthly Notices of the Royal Astronomical Society. 471(3),
2575–2586.
mla: Stroe, Andra, et al. “A 1.4 Deg2 Blind Survey for C II], C III] and C IV at
z ∼ 0.7–1.5 – II. Luminosity Functions and Cosmic Average Line Ratios.” Monthly
Notices of the Royal Astronomical Society, vol. 471, no. 3, Oxford University
Press, 2017, pp. 2575–86, doi:10.1093/mnras/stx1713.
short: A. Stroe, D. Sobral, J.J. Matthee, J. Calhau, I. Oteo, Monthly Notices of
the Royal Astronomical Society 471 (2017) 2575–2586.
date_created: 2022-07-12T12:54:57Z
date_published: 2017-11-01T00:00:00Z
date_updated: 2022-08-19T08:02:04Z
day: '01'
doi: 10.1093/mnras/stx1713
extern: '1'
external_id:
arxiv:
- '1703.10169'
intvolume: ' 471'
issue: '3'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: active'
- 'galaxies: high redshift'
- 'galaxies: luminosity function'
- mass function
- 'quasars: emission lines'
- star formation
- 'cosmology: observations'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1703.10169
month: '11'
oa: 1
oa_version: Preprint
page: 2575-2586
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: A 1.4 deg2 blind survey for C II], C III] and C IV at z ∼ 0.7–1.5 – II. Luminosity
functions and cosmic average line ratios
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '11572'
abstract:
- lang: eng
text: We present spectroscopic follow-up of candidate luminous Ly α emitters (LAEs)
at z = 5.7–6.6 in the SA22 field with VLT/X-SHOOTER. We confirm two new luminous
LAEs at z = 5.676 (SR6) and z = 6.532 (VR7), and also present HST follow-up of
both sources. These sources have luminosities LLy α ≈ 3 × 1043 erg s−1, very high
rest-frame equivalent widths of EW0 ≳ 200 Å and narrow Ly α lines (200–340 km s−1).
VR7 is the most UV-luminous LAE at z > 6.5, with M1500 = −22.5, even brighter
in the UV than CR7. Besides Ly α, we do not detect any other rest-frame UV lines
in the spectra of SR6 and VR7, and argue that rest-frame UV lines are easier to
observe in bright galaxies with low Ly α equivalent widths. We confirm that Ly α
line widths increase with Ly α luminosity at z = 5.7, while there are indications
that Ly α lines of faint LAEs become broader at z = 6.6, potentially due to reionization.
We find a large spread of up to 3 dex in UV luminosity for >L⋆ LAEs, but find
that the Ly α luminosity of the brightest LAEs is strongly related to UV luminosity
at z = 6.6. Under basic assumptions, we find that several LAEs at z ≈ 6–7 have
Ly α escape fractions ≳ 100 per cent, indicating bursty star formation histories,
alternative Ly α production mechanisms, or dust attenuating Ly α emission differently
than UV emission. Finally, we present a method to compute ξion, the production
efficiency of ionizing photons, and find that LAEs at z ≈ 6–7 have high values
of log10(ξion/Hz erg−1) ≈ 25.51 ± 0.09 that may alleviate the need for high Lyman-Continuum
escape fractions required for reionization.
acknowledgement: 'We thank the referee for a constructive report that has improved
the quality and clarity of this work. The authors thank Grecco Oyarzún for discussions.
JM acknowledges the support of a Huygens PhD fellowship from Leiden University.
DS acknowledges financial support from the Netherlands Organisation for Scientific
research (NWO) through a Veni fellowship and from Lancaster University through an
Early Career Internal Grant A100679. BD acknowledges financial support from NASA
through the Astrophysics Data Analysis Program (ADAP), grant number NNX12AE20G.
We thank Kasper Schmidt for providing measurements. Based on observations with the
W.M. Keck Observatory through programme C267D. The W.M. Keck Observatory is operated
as a scientific partnership amongst the California Institute of Technology, the
University of California and the National Aeronautics and Space Administration.
Based on observations made with ESO Telescopes at the La Silla Paranal Observatory
under programme IDs 097.A-0943, 294.A 5018 and 098.A-0819 and on data products produced
by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium.
The authors acknowledge the award of observing time (W16AN004) and of service time
(SW2014b20) on the William Herschel Telescope (WHT). WHT and its service programme
are operated on the island of La Palma by the Isaac Newton Group in the Spanish
Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias.
Based on observations made with the NASA/ESA HST, obtained (from the Data Archive)
at the Space Telescope Science Institute, which is operated by the Association of
Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These
observations are associated with programme #14699. We are grateful for the excellent
data sets from the COSMOS, UltraVISTA, SXDS, UDS and CFHTLS survey teams; without
these legacy surveys, this research would have been impossible. We have benefited
from the public available programming language PYTHON, including the NUMPY, MATPLOTLIB,
PYFITS, SCIPY and ASTROPY packages, the astronomical imaging tools SEXTRACTOR, SWARP
and SCAMP and the TOPCAT analysis tool (Taylor 2013).'
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: David
full_name: Sobral, David
last_name: Sobral
- first_name: Behnam
full_name: Darvish, Behnam
last_name: Darvish
- first_name: Sérgio
full_name: Santos, Sérgio
last_name: Santos
- first_name: Bahram
full_name: Mobasher, Bahram
last_name: Mobasher
- first_name: Ana
full_name: Paulino-Afonso, Ana
last_name: Paulino-Afonso
- first_name: Huub
full_name: Röttgering, Huub
last_name: Röttgering
- first_name: Lara
full_name: Alegre, Lara
last_name: Alegre
citation:
ama: Matthee JJ, Sobral D, Darvish B, et al. Spectroscopic properties of luminous
Ly α emitters at z ≈ 6–7 and comparison to the Lyman-break population. Monthly
Notices of the Royal Astronomical Society. 2017;472(1):772-787. doi:10.1093/mnras/stx2061
apa: Matthee, J. J., Sobral, D., Darvish, B., Santos, S., Mobasher, B., Paulino-Afonso,
A., … Alegre, L. (2017). Spectroscopic properties of luminous Ly α emitters at
z ≈ 6–7 and comparison to the Lyman-break population. Monthly Notices of the
Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stx2061
chicago: Matthee, Jorryt J, David Sobral, Behnam Darvish, Sérgio Santos, Bahram
Mobasher, Ana Paulino-Afonso, Huub Röttgering, and Lara Alegre. “Spectroscopic
Properties of Luminous Ly α Emitters at z ≈ 6–7 and Comparison to the Lyman-Break
Population.” Monthly Notices of the Royal Astronomical Society. Oxford
University Press, 2017. https://doi.org/10.1093/mnras/stx2061.
ieee: J. J. Matthee et al., “Spectroscopic properties of luminous Ly α emitters
at z ≈ 6–7 and comparison to the Lyman-break population,” Monthly Notices of
the Royal Astronomical Society, vol. 472, no. 1. Oxford University Press,
pp. 772–787, 2017.
ista: Matthee JJ, Sobral D, Darvish B, Santos S, Mobasher B, Paulino-Afonso A, Röttgering
H, Alegre L. 2017. Spectroscopic properties of luminous Ly α emitters at z ≈ 6–7
and comparison to the Lyman-break population. Monthly Notices of the Royal Astronomical
Society. 472(1), 772–787.
mla: Matthee, Jorryt J., et al. “Spectroscopic Properties of Luminous Ly α Emitters
at z ≈ 6–7 and Comparison to the Lyman-Break Population.” Monthly Notices of
the Royal Astronomical Society, vol. 472, no. 1, Oxford University Press,
2017, pp. 772–87, doi:10.1093/mnras/stx2061.
short: J.J. Matthee, D. Sobral, B. Darvish, S. Santos, B. Mobasher, A. Paulino-Afonso,
H. Röttgering, L. Alegre, Monthly Notices of the Royal Astronomical Society 472
(2017) 772–787.
date_created: 2022-07-13T09:47:39Z
date_published: 2017-11-01T00:00:00Z
date_updated: 2022-08-19T08:05:37Z
day: '01'
doi: 10.1093/mnras/stx2061
extern: '1'
external_id:
arxiv:
- '1706.06591'
intvolume: ' 472'
issue: '1'
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/1706.06591
month: '11'
oa: 1
oa_version: Preprint
page: 772-787
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: Spectroscopic properties of luminous Ly α emitters at z ≈ 6–7 and comparison
to the Lyman-break population
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 472
year: '2017'
...
---
_id: '11573'
abstract:
- lang: eng
text: We present dynamical measurements from the KMOS (K-band multi-object spectrograph)
Deep Survey (KDS), which comprises 77 typical star-forming galaxies at z ≃ 3.5
in the mass range 9.0 < log (M⋆/M⊙) < 10.5. These measurements constrain the internal
dynamics, the intrinsic velocity dispersions (σint) and rotation velocities (VC)
of galaxies in the high-redshift Universe. The mean velocity dispersion of the
galaxies in our sample is σint=70.8+3.3−3.1kms−1, revealing that the increasing
average σint with increasing redshift, reported for z ≲ 2, continues out to z
≃ 3.5. Only 36 ± 8 per cent of our galaxies are rotation-dominated (VC/σint >
1), with the sample average VC/σint value much smaller than at lower redshift.
After carefully selecting comparable star-forming samples at multiple epochs,
we find that the rotation-dominated fraction evolves with redshift with a z−0.2
dependence. The rotation-dominated KDS galaxies show no clear offset from the
local rotation velocity–stellar mass (i.e. VC–M⋆) relation, although a smaller
fraction of the galaxies are on the relation due to the increase in the dispersion-dominated
fraction. These observations are consistent with a simple equilibrium model picture,
in which random motions are boosted in high-redshift galaxies by a combination
of the increasing gas fractions, accretion efficiency, specific star formation
rate and stellar feedback and which may provide significant pressure support against
gravity on the galactic disc scale.
acknowledgement: 'We wish to thank the anonymous referee for their comments, which
have improved the quality and clarity of this work. OJT acknowledges the financial
support of the Science and Technology Facilities Council through a studentship award.
MC and OJT acknowledge the KMOS team and all the personnel of the European Southern
Observatory Very Large Telescope for outstanding support during the KMOS GTO observations.
CMH, AMS and RMS acknowledge the Science and Technology Facilities Council through
grant code ST/L00075X/1. RJM acknowledges the support of the European Research Council
via the award of a Consolidator Grant (PI: McLure). JSD acknowledges the support
of the European Research Council via the award of an Advanced Grant (PI J. Dunlop),
and the contribution of the EC FP7 SPACE project ASTRODEEP (Ref.No: 312725). AMS
acknowledges the Leverhulme Foundation. JM acknowledges the support of a Huygens
PhD fellowship from Leiden University. DS acknowledges financial support from the
Netherlands Organization for Scientific research (NWO) through a Veni fellowship
and from FCT through an FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010).
This work is based on observations taken by the CANDELS Multi-Cycle Treasury Program
with the NASA/ESA HST, which is operated by the Association of Universities for
Research in Astronomy, Inc., under NASA contract NAS5-26555. This work is based
on observations taken by the 3D HST Treasury Program (GO 12177 and 12328) with the
NASA/ESA HST, which is operated by the Association of Universities for Research
in Astronomy, Inc., under NASA contract NAS5-26555. Based on data obtained with
the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large
Program 185.A-0791, and made available by the VUDS team at the CESAM data centre,
Laboratoire d’Astrophysique de Marseille, France. Based on observations obtained
at the Very Large Telescope of the European Southern Observatory. Programme IDs:
092.A 0399(A), 093.A-0122(A,B), 094.A-0214(A,B),095.A0680(A,B),096.A-0315(A,B,C).'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: O. J.
full_name: Turner, O. J.
last_name: Turner
- first_name: M.
full_name: Cirasuolo, M.
last_name: Cirasuolo
- first_name: C. M.
full_name: Harrison, C. M.
last_name: Harrison
- first_name: R. J.
full_name: McLure, R. J.
last_name: McLure
- first_name: J. S.
full_name: Dunlop, J. S.
last_name: Dunlop
- first_name: A. M.
full_name: Swinbank, A. M.
last_name: Swinbank
- first_name: H. L.
full_name: Johnson, H. L.
last_name: Johnson
- first_name: D.
full_name: Sobral, D.
last_name: Sobral
- 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: R. M.
full_name: Sharples, R. M.
last_name: Sharples
citation:
ama: Turner OJ, Cirasuolo M, Harrison CM, et al. The KMOS Deep Survey (KDS) – I.
Dynamical measurements of typical star-forming galaxies at z ≃ 3.5. Monthly
Notices of the Royal Astronomical Society. 2017;471(2):1280-1320. doi:10.1093/mnras/stx1366
apa: Turner, O. J., Cirasuolo, M., Harrison, C. M., McLure, R. J., Dunlop, J. S.,
Swinbank, A. M., … Sharples, R. M. (2017). The KMOS Deep Survey (KDS) – I. Dynamical
measurements of typical star-forming galaxies at z ≃ 3.5. Monthly Notices of
the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stx1366
chicago: Turner, O. J., M. Cirasuolo, C. M. Harrison, R. J. McLure, J. S. Dunlop,
A. M. Swinbank, H. L. Johnson, D. Sobral, Jorryt J Matthee, and R. M. Sharples.
“The KMOS Deep Survey (KDS) – I. Dynamical Measurements of Typical Star-Forming
Galaxies at z ≃ 3.5.” Monthly Notices of the Royal Astronomical Society.
Oxford University Press, 2017. https://doi.org/10.1093/mnras/stx1366.
ieee: O. J. Turner et al., “The KMOS Deep Survey (KDS) – I. Dynamical measurements
of typical star-forming galaxies at z ≃ 3.5,” Monthly Notices of the Royal
Astronomical Society, vol. 471, no. 2. Oxford University Press, pp. 1280–1320,
2017.
ista: Turner OJ, Cirasuolo M, Harrison CM, McLure RJ, Dunlop JS, Swinbank AM, Johnson
HL, Sobral D, Matthee JJ, Sharples RM. 2017. The KMOS Deep Survey (KDS) – I. Dynamical
measurements of typical star-forming galaxies at z ≃ 3.5. Monthly Notices of the
Royal Astronomical Society. 471(2), 1280–1320.
mla: Turner, O. J., et al. “The KMOS Deep Survey (KDS) – I. Dynamical Measurements
of Typical Star-Forming Galaxies at z ≃ 3.5.” Monthly Notices of the Royal
Astronomical Society, vol. 471, no. 2, Oxford University Press, 2017, pp.
1280–320, doi:10.1093/mnras/stx1366.
short: O.J. Turner, M. Cirasuolo, C.M. Harrison, R.J. McLure, J.S. Dunlop, A.M.
Swinbank, H.L. Johnson, D. Sobral, J.J. Matthee, R.M. Sharples, Monthly Notices
of the Royal Astronomical Society 471 (2017) 1280–1320.
date_created: 2022-07-13T10:03:01Z
date_published: 2017-10-01T00:00:00Z
date_updated: 2022-08-19T08:07:31Z
day: '01'
doi: 10.1093/mnras/stx1366
extern: '1'
external_id:
arxiv:
- '1704.06263'
intvolume: ' 471'
issue: '2'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'galaxies: evolution'
- 'galaxies: high-redshift'
- 'galaxies: kinematics and dynamics'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1704.06263
month: '10'
oa: 1
oa_version: Preprint
page: 1280-1320
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 KMOS Deep Survey (KDS) – I. Dynamical measurements of typical star-forming
galaxies at z ≃ 3.5
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 471
year: '2017'
...
---
_id: '1159'
abstract:
- lang: eng
text: Auxin steers numerous physiological processes in plants, making the tight
control of its endogenous levels and spatiotemporal distribution a necessity.
This regulation is achieved by different mechanisms, including auxin biosynthesis,
metabolic conversions, degradation, and transport. Here, we introduce cis-cinnamic
acid (c-CA) as a novel and unique addition to a small group of endogenous molecules
affecting in planta auxin concentrations. c-CA is the photo-isomerization product
of the phenylpropanoid pathway intermediate trans-CA (t-CA). When grown on c-CA-containing
medium, an evolutionary diverse set of plant species were shown to exhibit phenotypes
characteristic for high auxin levels, including inhibition of primary root growth,
induction of root hairs, and promotion of adventitious and lateral rooting. By
molecular docking and receptor binding assays, we showed that c-CA itself is neither
an auxin nor an anti-auxin, and auxin profiling data revealed that c-CA does not
significantly interfere with auxin biosynthesis. Single cell-based auxin accumulation
assays showed that c-CA, and not t-CA, is a potent inhibitor of auxin efflux.
Auxin signaling reporters detected changes in spatiotemporal distribution of the
auxin response along the root of c-CA-treated plants, and long-distance auxin
transport assays showed no inhibition of rootward auxin transport. Overall, these
results suggest that the phenotypes of c-CA-treated plants are the consequence
of a local change in auxin accumulation, induced by the inhibition of auxin efflux.
This work reveals a novel mechanism how plants may regulate auxin levels and adds
a novel, naturally occurring molecule to the chemical toolbox for the studies
of auxin homeostasis.
article_processing_charge: No
article_type: original
author:
- first_name: Ward
full_name: Steenackers, Ward
last_name: Steenackers
- first_name: Petr
full_name: Klíma, Petr
last_name: Klíma
- first_name: Mussa
full_name: Quareshy, Mussa
last_name: Quareshy
- first_name: Igor
full_name: Cesarino, Igor
last_name: Cesarino
- first_name: Robert
full_name: Kumpf, Robert
last_name: Kumpf
- first_name: Sander
full_name: Corneillie, Sander
last_name: Corneillie
- first_name: Pedro
full_name: Araújo, Pedro
last_name: Araújo
- first_name: Tom
full_name: Viaene, Tom
last_name: Viaene
- first_name: Geert
full_name: Goeminne, Geert
last_name: Goeminne
- first_name: Moritz
full_name: Nowack, Moritz
last_name: Nowack
- first_name: Karin
full_name: Ljung, Karin
last_name: Ljung
- first_name: Jirí
full_name: Friml, Jirí
id: 4159519E-F248-11E8-B48F-1D18A9856A87
last_name: Friml
orcid: 0000-0002-8302-7596
- first_name: Joshua
full_name: Blakeslee, Joshua
last_name: Blakeslee
- first_name: Ondřej
full_name: Novák, Ondřej
last_name: Novák
- first_name: Eva
full_name: Zažímalová, Eva
last_name: Zažímalová
- first_name: Richard
full_name: Napier, Richard
last_name: Napier
- first_name: Wout
full_name: Boerjan, Wout
last_name: Boerjan
- first_name: Bartel
full_name: Vanholme, Bartel
last_name: Vanholme
citation:
ama: Steenackers W, Klíma P, Quareshy M, et al. Cis-cinnamic acid is a novel natural
auxin efflux inhibitor that promotes lateral root formation. Plant Physiology.
2017;173(1):552-565. doi:10.1104/pp.16.00943
apa: Steenackers, W., Klíma, P., Quareshy, M., Cesarino, I., Kumpf, R., Corneillie,
S., … Vanholme, B. (2017). Cis-cinnamic acid is a novel natural auxin efflux inhibitor
that promotes lateral root formation. Plant Physiology. American Society
of Plant Biologists. https://doi.org/10.1104/pp.16.00943
chicago: Steenackers, Ward, Petr Klíma, Mussa Quareshy, Igor Cesarino, Robert Kumpf,
Sander Corneillie, Pedro Araújo, et al. “Cis-Cinnamic Acid Is a Novel Natural
Auxin Efflux Inhibitor That Promotes Lateral Root Formation.” Plant Physiology.
American Society of Plant Biologists, 2017. https://doi.org/10.1104/pp.16.00943.
ieee: W. Steenackers et al., “Cis-cinnamic acid is a novel natural auxin
efflux inhibitor that promotes lateral root formation,” Plant Physiology,
vol. 173, no. 1. American Society of Plant Biologists, pp. 552–565, 2017.
ista: Steenackers W, Klíma P, Quareshy M, Cesarino I, Kumpf R, Corneillie S, Araújo
P, Viaene T, Goeminne G, Nowack M, Ljung K, Friml J, Blakeslee J, Novák O, Zažímalová
E, Napier R, Boerjan W, Vanholme B. 2017. Cis-cinnamic acid is a novel natural
auxin efflux inhibitor that promotes lateral root formation. Plant Physiology.
173(1), 552–565.
mla: Steenackers, Ward, et al. “Cis-Cinnamic Acid Is a Novel Natural Auxin Efflux
Inhibitor That Promotes Lateral Root Formation.” Plant Physiology, vol.
173, no. 1, American Society of Plant Biologists, 2017, pp. 552–65, doi:10.1104/pp.16.00943.
short: W. Steenackers, P. Klíma, M. Quareshy, I. Cesarino, R. Kumpf, S. Corneillie,
P. Araújo, T. Viaene, G. Goeminne, M. Nowack, K. Ljung, J. Friml, J. Blakeslee,
O. Novák, E. Zažímalová, R. Napier, W. Boerjan, B. Vanholme, Plant Physiology
173 (2017) 552–565.
date_created: 2018-12-11T11:50:28Z
date_published: 2017-01-01T00:00:00Z
date_updated: 2025-05-07T11:12:30Z
day: '01'
ddc:
- '580'
department:
- _id: JiFr
doi: 10.1104/pp.16.00943
ec_funded: 1
external_id:
isi:
- '000394135800041'
pmid:
- '27837086'
file:
- access_level: open_access
checksum: fd4d1cfe7ed70e54bb12ae3881f3fb91
content_type: application/pdf
creator: dernst
date_created: 2019-11-18T16:12:25Z
date_updated: 2020-07-14T12:44:36Z
file_id: '7040'
file_name: 2016_PlantPhysi_Steenackers.pdf
file_size: 4109142
relation: main_file
file_date_updated: 2020-07-14T12:44:36Z
has_accepted_license: '1'
intvolume: ' 173'
isi: 1
issue: '1'
language:
- iso: eng
month: '01'
oa: 1
oa_version: Submitted Version
page: 552 - 565
pmid: 1
project:
- _id: 25716A02-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '282300'
name: Polarity and subcellular dynamics in plants
publication: Plant Physiology
publication_identifier:
issn:
- 0032-0889
publication_status: published
publisher: American Society of Plant Biologists
publist_id: '6199'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Cis-cinnamic acid is a novel natural auxin efflux inhibitor that promotes lateral
root formation
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 173
year: '2017'
...
---
_id: '1160'
abstract:
- lang: eng
text: 'We investigate fundamental nonlinear dynamics of ferrofluidic Taylor-Couette
flow - flow confined be-tween two concentric independently rotating cylinders
- consider small aspect ratio by solving the ferro-hydrodynamical equations, carrying
out systematic bifurcation analysis. Without magnetic field, we find steady flow
patterns, previously observed with a simple fluid, such as those containing normal
one- or two vortex cells, as well as anomalous one-cell and twin-cell flow states.
However, when a symmetry-breaking transverse magnetic field is present, all flow
states exhibit stimulated, finite two-fold mode. Various bifurcations between
steady and unsteady states can occur, corresponding to the transitions between
the two-cell and one-cell states. While unsteady, axially oscillating flow states
can arise, we also detect the emergence of new unsteady flow states. In particular,
we uncover two new states: one contains only the azimuthally oscillating solution
in the configuration of the twin-cell flow state, and an-other a rotating flow
state. Topologically, these flow states are a limit cycle and a quasiperiodic
solution on a two-torus, respectively. Emergence of new flow states in addition
to observed ones with classical fluid, indicates that richer but potentially more
controllable dynamics in ferrofluidic flows, as such flow states depend on the
external magnetic field.'
article_number: '40012'
article_processing_charge: No
author:
- first_name: Sebastian
full_name: Altmeyer, Sebastian
id: 2EE67FDC-F248-11E8-B48F-1D18A9856A87
last_name: Altmeyer
orcid: 0000-0001-5964-0203
- first_name: Younghae
full_name: Do, Younghae
last_name: Do
- first_name: Ying
full_name: Lai, Ying
last_name: Lai
citation:
ama: Altmeyer S, Do Y, Lai Y. Dynamics of ferrofluidic flow in the Taylor-Couette
system with a small aspect ratio. Scientific Reports. 2017;7. doi:10.1038/srep40012
apa: Altmeyer, S., Do, Y., & Lai, Y. (2017). Dynamics of ferrofluidic flow in
the Taylor-Couette system with a small aspect ratio. Scientific Reports.
Nature Publishing Group. https://doi.org/10.1038/srep40012
chicago: Altmeyer, Sebastian, Younghae Do, and Ying Lai. “Dynamics of Ferrofluidic
Flow in the Taylor-Couette System with a Small Aspect Ratio.” Scientific Reports.
Nature Publishing Group, 2017. https://doi.org/10.1038/srep40012.
ieee: S. Altmeyer, Y. Do, and Y. Lai, “Dynamics of ferrofluidic flow in the Taylor-Couette
system with a small aspect ratio,” Scientific Reports, vol. 7. Nature Publishing
Group, 2017.
ista: Altmeyer S, Do Y, Lai Y. 2017. Dynamics of ferrofluidic flow in the Taylor-Couette
system with a small aspect ratio. Scientific Reports. 7, 40012.
mla: Altmeyer, Sebastian, et al. “Dynamics of Ferrofluidic Flow in the Taylor-Couette
System with a Small Aspect Ratio.” Scientific Reports, vol. 7, 40012, Nature
Publishing Group, 2017, doi:10.1038/srep40012.
short: S. Altmeyer, Y. Do, Y. Lai, Scientific Reports 7 (2017).
date_created: 2018-12-11T11:50:28Z
date_published: 2017-01-06T00:00:00Z
date_updated: 2023-09-20T11:28:49Z
day: '06'
ddc:
- '532'
department:
- _id: BjHo
doi: 10.1038/srep40012
external_id:
isi:
- '000391269700001'
file:
- access_level: open_access
checksum: 694aa70399444570825099c1a7ec91f2
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:10:16Z
date_updated: 2020-07-14T12:44:36Z
file_id: '4802'
file_name: IST-2017-743-v1+1_srep40012.pdf
file_size: 4546835
relation: main_file
file_date_updated: 2020-07-14T12:44:36Z
has_accepted_license: '1'
intvolume: ' 7'
isi: 1
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
publication: Scientific Reports
publication_identifier:
issn:
- '20452322'
publication_status: published
publisher: Nature Publishing Group
publist_id: '6198'
pubrep_id: '743'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Dynamics of ferrofluidic flow in the Taylor-Couette system with a small aspect
ratio
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: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 7
year: '2017'
...
---
_id: '1161'
abstract:
- lang: eng
text: Coordinated changes of cell shape are often the result of the excitable, wave-like
dynamics of the actin cytoskeleton. New work shows that, in migrating cells, protrusion
waves arise from mechanochemical crosstalk between adhesion sites, membrane tension
and the actin protrusive machinery.
article_processing_charge: No
author:
- first_name: Jan
full_name: Müller, Jan
id: AD07FDB4-0F61-11EA-8158-C4CC64CEAA8D
last_name: Müller
- first_name: Michael K
full_name: Sixt, Michael K
id: 41E9FBEA-F248-11E8-B48F-1D18A9856A87
last_name: Sixt
orcid: 0000-0002-6620-9179
citation:
ama: 'Müller J, Sixt MK. Cell migration: Making the waves. Current Biology.
2017;27(1):R24-R25. doi:10.1016/j.cub.2016.11.035'
apa: 'Müller, J., & Sixt, M. K. (2017). Cell migration: Making the waves. Current
Biology. Cell Press. https://doi.org/10.1016/j.cub.2016.11.035'
chicago: 'Müller, Jan, and Michael K Sixt. “Cell Migration: Making the Waves.” Current
Biology. Cell Press, 2017. https://doi.org/10.1016/j.cub.2016.11.035.'
ieee: 'J. Müller and M. K. Sixt, “Cell migration: Making the waves,” Current
Biology, vol. 27, no. 1. Cell Press, pp. R24–R25, 2017.'
ista: 'Müller J, Sixt MK. 2017. Cell migration: Making the waves. Current Biology.
27(1), R24–R25.'
mla: 'Müller, Jan, and Michael K. Sixt. “Cell Migration: Making the Waves.” Current
Biology, vol. 27, no. 1, Cell Press, 2017, pp. R24–25, doi:10.1016/j.cub.2016.11.035.'
short: J. Müller, M.K. Sixt, Current Biology 27 (2017) R24–R25.
date_created: 2018-12-11T11:50:29Z
date_published: 2017-01-09T00:00:00Z
date_updated: 2023-09-20T11:28:19Z
day: '09'
department:
- _id: MiSi
doi: 10.1016/j.cub.2016.11.035
external_id:
isi:
- '000391902500010'
intvolume: ' 27'
isi: 1
issue: '1'
language:
- iso: eng
month: '01'
oa_version: None
page: R24 - R25
publication: Current Biology
publication_identifier:
issn:
- '09609822'
publication_status: published
publisher: Cell Press
publist_id: '6197'
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'Cell migration: Making the waves'
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 27
year: '2017'
...
---
_id: '1162'
abstract:
- lang: eng
text: Selected universal experimental properties of high-temperature superconducting
(HTS) cuprates have been singled out in the last decade. One of the pivotal challenges
in this field is the designation of a consistent interpretation framework within
which we can describe quantitatively the universal features of those systems.
Here we analyze in a detailed manner the principal experimental data and compare
them quantitatively with the approach based on a single-band model of strongly
correlated electrons supplemented with strong antiferromagnetic (super)exchange
interaction (the so-called t−J−U model). The model rationale is provided by estimating
its microscopic parameters on the basis of the three-band approach for the Cu-O
plane. We use our original full Gutzwiller wave-function solution by going beyond
the renormalized mean-field theory (RMFT) in a systematic manner. Our approach
reproduces very well the observed hole doping (δ) dependence of the kinetic-energy
gain in the superconducting phase, one of the principal non-Bardeen-Cooper-Schrieffer
features of the cuprates. The calculated Fermi velocity in the nodal direction
is practically δ-independent and its universal value agrees very well with that
determined experimentally. Also, a weak doping dependence of the Fermi wave vector
leads to an almost constant value of the effective mass in a pure superconducting
phase which is both observed in experiment and reproduced within our approach.
An assessment of the currently used models (t−J, Hubbard) is carried out and the
results of the canonical RMFT as a zeroth-order solution are provided for comparison
to illustrate the necessity of the introduced higher-order contributions.
article_number: '024506'
article_processing_charge: No
author:
- first_name: Jozef
full_name: Spałek, Jozef
last_name: Spałek
- first_name: Michał
full_name: Zegrodnik, Michał
last_name: Zegrodnik
- first_name: Jan
full_name: Kaczmarczyk, Jan
id: 46C405DE-F248-11E8-B48F-1D18A9856A87
last_name: Kaczmarczyk
orcid: 0000-0002-1629-3675
citation:
ama: Spałek J, Zegrodnik M, Kaczmarczyk J. Universal properties of high temperature
superconductors from real space pairing t-J-U model and its quantitative comparison
with experiment. Physical Review B - Condensed Matter and Materials Physics.
2017;95(2). doi:10.1103/PhysRevB.95.024506
apa: Spałek, J., Zegrodnik, M., & Kaczmarczyk, J. (2017). Universal properties
of high temperature superconductors from real space pairing t-J-U model and its
quantitative comparison with experiment. Physical Review B - Condensed Matter
and Materials Physics. American Physical Society. https://doi.org/10.1103/PhysRevB.95.024506
chicago: Spałek, Jozef, Michał Zegrodnik, and Jan Kaczmarczyk. “Universal Properties
of High Temperature Superconductors from Real Space Pairing T-J-U Model and Its
Quantitative Comparison with Experiment.” Physical Review B - Condensed Matter
and Materials Physics. American Physical Society, 2017. https://doi.org/10.1103/PhysRevB.95.024506.
ieee: J. Spałek, M. Zegrodnik, and J. Kaczmarczyk, “Universal properties of high
temperature superconductors from real space pairing t-J-U model and its quantitative
comparison with experiment,” Physical Review B - Condensed Matter and Materials
Physics, vol. 95, no. 2. American Physical Society, 2017.
ista: Spałek J, Zegrodnik M, Kaczmarczyk J. 2017. Universal properties of high temperature
superconductors from real space pairing t-J-U model and its quantitative comparison
with experiment. Physical Review B - Condensed Matter and Materials Physics. 95(2),
024506.
mla: Spałek, Jozef, et al. “Universal Properties of High Temperature Superconductors
from Real Space Pairing T-J-U Model and Its Quantitative Comparison with Experiment.”
Physical Review B - Condensed Matter and Materials Physics, vol. 95, no.
2, 024506, American Physical Society, 2017, doi:10.1103/PhysRevB.95.024506.
short: J. Spałek, M. Zegrodnik, J. Kaczmarczyk, Physical Review B - Condensed Matter
and Materials Physics 95 (2017).
date_created: 2018-12-11T11:50:29Z
date_published: 2017-01-13T00:00:00Z
date_updated: 2023-09-20T11:25:56Z
day: '13'
department:
- _id: MiLe
doi: 10.1103/PhysRevB.95.024506
ec_funded: 1
external_id:
isi:
- '000391852800006'
intvolume: ' 95'
isi: 1
issue: '2'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1606.03247
month: '01'
oa: 1
oa_version: Submitted Version
project:
- _id: 25681D80-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '291734'
name: International IST Postdoc Fellowship Programme
publication: Physical Review B - Condensed Matter and Materials Physics
publication_identifier:
issn:
- '24699950'
publication_status: published
publisher: American Physical Society
publist_id: '6195'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Universal properties of high temperature superconductors from real space pairing
t-J-U model and its quantitative comparison with experiment
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 95
year: '2017'
...
---
_id: '1163'
abstract:
- lang: eng
text: 'We investigate the effect of the electron-hole (e-h) symmetry breaking on
d-wave superconductivity induced by non-local effects of correlations in the generalized
Hubbard model. The symmetry breaking is introduced in a two-fold manner: by the
next-to-nearest neighbor hopping of electrons and by the charge-bond interaction
- the off-diagonal term of the Coulomb potential. Both terms lead to a pronounced
asymmetry of the superconducting order parameter. The next-to-nearest neighbor
hopping enhances superconductivity for h-doping, while diminishes it for e-doping.
The charge-bond interaction alone leads to the opposite effect and, additionally,
to the kinetic-energy gain upon condensation in the underdoped regime. With both
terms included, with similar amplitudes, the height of the superconducting dome
and the critical doping remain in favor of h-doping. The influence of the charge-bond
interaction on deviations from symmetry of the shape of the gap at the Fermi surface
in the momentum space is briefly discussed.'
article_number: '085604'
article_processing_charge: No
author:
- first_name: Marcin
full_name: Wysokiński, Marcin
last_name: Wysokiński
- first_name: Jan
full_name: Kaczmarczyk, Jan
id: 46C405DE-F248-11E8-B48F-1D18A9856A87
last_name: Kaczmarczyk
orcid: 0000-0002-1629-3675
citation:
ama: 'Wysokiński M, Kaczmarczyk J. Unconventional superconductivity in generalized
Hubbard model role of electron–hole symmetry breaking terms. Journal of Physics:
Condensed Matter. 2017;29(8). doi:10.1088/1361-648X/aa532f'
apa: 'Wysokiński, M., & Kaczmarczyk, J. (2017). Unconventional superconductivity
in generalized Hubbard model role of electron–hole symmetry breaking terms. Journal
of Physics: Condensed Matter. IOP Publishing Ltd. https://doi.org/10.1088/1361-648X/aa532f'
chicago: 'Wysokiński, Marcin, and Jan Kaczmarczyk. “Unconventional Superconductivity
in Generalized Hubbard Model Role of Electron–Hole Symmetry Breaking Terms.” Journal
of Physics: Condensed Matter. IOP Publishing Ltd., 2017. https://doi.org/10.1088/1361-648X/aa532f.'
ieee: 'M. Wysokiński and J. Kaczmarczyk, “Unconventional superconductivity in generalized
Hubbard model role of electron–hole symmetry breaking terms,” Journal of Physics:
Condensed Matter, vol. 29, no. 8. IOP Publishing Ltd., 2017.'
ista: 'Wysokiński M, Kaczmarczyk J. 2017. Unconventional superconductivity in generalized
Hubbard model role of electron–hole symmetry breaking terms. Journal of Physics:
Condensed Matter. 29(8), 085604.'
mla: 'Wysokiński, Marcin, and Jan Kaczmarczyk. “Unconventional Superconductivity
in Generalized Hubbard Model Role of Electron–Hole Symmetry Breaking Terms.” Journal
of Physics: Condensed Matter, vol. 29, no. 8, 085604, IOP Publishing Ltd.,
2017, doi:10.1088/1361-648X/aa532f.'
short: 'M. Wysokiński, J. Kaczmarczyk, Journal of Physics: Condensed Matter 29 (2017).'
date_created: 2018-12-11T11:50:29Z
date_published: 2017-01-16T00:00:00Z
date_updated: 2023-09-20T11:25:32Z
day: '16'
department:
- _id: MiLe
doi: 10.1088/1361-648X/aa532f
ec_funded: 1
external_id:
isi:
- '000393955500001'
intvolume: ' 29'
isi: 1
issue: '8'
language:
- iso: eng
month: '01'
oa_version: None
project:
- _id: 25681D80-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '291734'
name: International IST Postdoc Fellowship Programme
publication: 'Journal of Physics: Condensed Matter'
publication_identifier:
issn:
- '09538984'
publication_status: published
publisher: IOP Publishing Ltd.
publist_id: '6194'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Unconventional superconductivity in generalized Hubbard model role of electron–hole
symmetry breaking terms
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 29
year: '2017'
...
---
_id: '11633'
abstract:
- lang: eng
text: Our understanding of stars through asteroseismic data analysis is limited
by our ability to take advantage of the huge amount of observed stars provided
by space missions such as CoRoT, Kepler , K2, and soon TESS and PLATO. Global
seismic pipelines provide global stellar parameters such as mass and radius using
the mean seismic parameters, as well as the effective temperature. These pipelines
are commonly used automatically on thousands of stars observed by K2 for 3 months
(and soon TESS for at least ∼ 1 month). However, pipelines are not immune from
misidentifying noise peaks and stellar oscillations. Therefore, new validation
techniques are required to assess the quality of these results. We present a new
metric called FliPer (Flicker in Power), which takes into account the average
variability at all measured time scales. The proper calibration of FliPer enables
us to obtain good estimations of global stellar parameters such as surface gravity
that are robust against the influence of noise peaks and hence are an excellent
way to find faults in asteroseismic pipelines.
article_number: '1711.02890'
article_processing_charge: No
arxiv: 1
author:
- first_name: Lisa Annabelle
full_name: Bugnet, Lisa Annabelle
id: d9edb345-f866-11ec-9b37-d119b5234501
last_name: Bugnet
orcid: 0000-0003-0142-4000
- first_name: R. A.
full_name: Garcia, R. A.
last_name: Garcia
- first_name: G. R.
full_name: Davies, G. R.
last_name: Davies
- first_name: S.
full_name: Mathur, S.
last_name: Mathur
- first_name: E.
full_name: Corsaro, E.
last_name: Corsaro
citation:
ama: 'Bugnet LA, Garcia RA, Davies GR, Mathur S, Corsaro E. FliPer: Checking the
reliability of global seismic parameters from automatic pipelines. arXiv.
doi:10.48550/arXiv.1711.02890'
apa: 'Bugnet, L. A., Garcia, R. A., Davies, G. R., Mathur, S., & Corsaro, E.
(n.d.). FliPer: Checking the reliability of global seismic parameters from automatic
pipelines. arXiv. https://doi.org/10.48550/arXiv.1711.02890'
chicago: 'Bugnet, Lisa Annabelle, R. A. Garcia, G. R. Davies, S. Mathur, and E.
Corsaro. “FliPer: Checking the Reliability of Global Seismic Parameters from Automatic
Pipelines.” ArXiv, n.d. https://doi.org/10.48550/arXiv.1711.02890.'
ieee: 'L. A. Bugnet, R. A. Garcia, G. R. Davies, S. Mathur, and E. Corsaro, “FliPer:
Checking the reliability of global seismic parameters from automatic pipelines,”
arXiv. .'
ista: 'Bugnet LA, Garcia RA, Davies GR, Mathur S, Corsaro E. FliPer: Checking the
reliability of global seismic parameters from automatic pipelines. arXiv, 1711.02890.'
mla: 'Bugnet, Lisa Annabelle, et al. “FliPer: Checking the Reliability of Global
Seismic Parameters from Automatic Pipelines.” ArXiv, 1711.02890, doi:10.48550/arXiv.1711.02890.'
short: L.A. Bugnet, R.A. Garcia, G.R. Davies, S. Mathur, E. Corsaro, ArXiv (n.d.).
date_created: 2022-07-21T07:13:13Z
date_published: 2017-11-08T00:00:00Z
date_updated: 2022-08-22T08:45:42Z
day: '08'
doi: 10.48550/arXiv.1711.02890
extern: '1'
external_id:
arxiv:
- '1711.02890'
keyword:
- asteroseismology - methods
- data analysis - stars
- oscillations
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://doi.org/10.48550/arXiv.1711.02890
month: '11'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: 'FliPer: Checking the reliability of global seismic parameters from automatic
pipelines'
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2017'
...
---
_id: '11651'
abstract:
- lang: eng
text: Diffusions and related random walk procedures are of central importance in
many areas of machine learning, data analysis, and applied mathematics. Because
they spread mass agnostically at each step in an iterative manner, they can sometimes
spread mass “too aggressively,” thereby failing to find the “right” clusters.
We introduce a novel Capacity Releasing Diffusion (CRD) Process, which is both
faster and stays more local than the classical spectral diffusion process. As
an application, we use our CRD Process to develop an improved local algorithm
for graph clustering. Our local graph clustering method can find local clusters
in a model of clustering where one begins the CRD Process in a cluster whose vertices
are connected better internally than externally by an O(log2n) factor, where n
is the number of nodes in the cluster. Thus, our CRD Process is the first local
graph clustering algorithm that is not subject to the well-known quadratic Cheeger
barrier. Our result requires a certain smoothness condition, which we expect to
be an artifact of our analysis. Our empirical evaluation demonstrates improved
results, in particular for realistic social graphs where there are moderately
good—but not very good—clusters.
alternative_title:
- PMLR
article_processing_charge: No
arxiv: 1
author:
- first_name: Di
full_name: Wang, Di
last_name: Wang
- first_name: Kimon
full_name: Fountoulakis, Kimon
last_name: Fountoulakis
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: Michael W.
full_name: Mahoney, Michael W.
last_name: Mahoney
- first_name: ' Satish'
full_name: Rao , Satish
last_name: 'Rao '
citation:
ama: 'Wang D, Fountoulakis K, Henzinger MH, Mahoney MW, Rao Satish. Capacity releasing
diffusion for speed and locality. In: Proceedings of the 34th International
Conference on Machine Learning. Vol 70. ML Research Press; 2017:3598-3607.'
apa: 'Wang, D., Fountoulakis, K., Henzinger, M. H., Mahoney, M. W., & Rao , Satish.
(2017). Capacity releasing diffusion for speed and locality. In Proceedings
of the 34th International Conference on Machine Learning (Vol. 70, pp. 3598–3607).
Sydney, Australia: ML Research Press.'
chicago: Wang, Di, Kimon Fountoulakis, Monika H Henzinger, Michael W. Mahoney, and Satish
Rao . “Capacity Releasing Diffusion for Speed and Locality.” In Proceedings
of the 34th International Conference on Machine Learning, 70:3598–3607. ML
Research Press, 2017.
ieee: D. Wang, K. Fountoulakis, M. H. Henzinger, M. W. Mahoney, and Satish Rao
, “Capacity releasing diffusion for speed and locality,” in Proceedings of
the 34th International Conference on Machine Learning, Sydney, Australia,
2017, vol. 70, pp. 3598–3607.
ista: Wang D, Fountoulakis K, Henzinger MH, Mahoney MW, Rao Satish. 2017. Capacity
releasing diffusion for speed and locality. Proceedings of the 34th International
Conference on Machine Learning. International Conference on Machine Learning,
PMLR, vol. 70, 3598–3607.
mla: Wang, Di, et al. “Capacity Releasing Diffusion for Speed and Locality.” Proceedings
of the 34th International Conference on Machine Learning, vol. 70, ML Research
Press, 2017, pp. 3598–607.
short: D. Wang, K. Fountoulakis, M.H. Henzinger, M.W. Mahoney, Satish Rao , in:,
Proceedings of the 34th International Conference on Machine Learning, ML Research
Press, 2017, pp. 3598–3607.
conference:
end_date: 2017-08-11
location: Sydney, Australia
name: International Conference on Machine Learning
start_date: 2017-08-06
date_created: 2022-07-25T13:59:21Z
date_published: 2017-09-01T00:00:00Z
date_updated: 2023-02-09T09:15:31Z
day: '01'
extern: '1'
external_id:
arxiv:
- '1706.05826'
intvolume: ' 70'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://proceedings.mlr.press/v70/wang17b/wang17b.pdf
month: '09'
oa: 1
oa_version: Published Version
page: 3598-3607
publication: Proceedings of the 34th International Conference on Machine Learning
publication_identifier:
eissn:
- 2640-3498
publication_status: published
publisher: ML Research Press
quality_controlled: '1'
status: public
title: Capacity releasing diffusion for speed and locality
type: conference
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 70
year: '2017'
...
---
_id: '11665'
abstract:
- lang: eng
text: "We study the problem of maintaining a breadth-first spanning tree (BFS tree)
in partially dynamic distributed networks modeling a sequence of either failures
or additions of communication links (but not both). We present deterministic (1+ϵ)-approximation
algorithms whose amortized time (over some number of link changes) is sublinear
in D, the maximum diameter of the network.\r\n\r\nOur technique also leads to
a deterministic (1+ϵ)-approximate incremental algorithm for single-source shortest
paths in the sequential (usual RAM) model. Prior to our work, the state of the
art was the classic exact algorithm of Even and Shiloach (1981), which is optimal
under some assumptions (Roditty and Zwick 2011; Henzinger et al. 2015). Our result
is the first to show that, in the incremental setting, this bound can be beaten
in certain cases if some approximation is allowed."
acknowledgement: "We thank the reviewers of ICALP 2013 for pointing to related articles
and to an error in an example\r\ngiven in a previous version of this article. We
also thank one of the reviewers of Transactions on\r\nAlgorithms for very detailed
comments."
article_number: '51'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: Sebastian
full_name: Krinninger, Sebastian
last_name: Krinninger
- first_name: Danupon
full_name: Nanongkai, Danupon
last_name: Nanongkai
citation:
ama: Henzinger MH, Krinninger S, Nanongkai D. Sublinear-time maintenance of breadth-first
spanning trees in partially dynamic networks. ACM Transactions on Algorithms.
2017;13(4). doi:10.1145/3146550
apa: Henzinger, M. H., Krinninger, S., & Nanongkai, D. (2017). Sublinear-time
maintenance of breadth-first spanning trees in partially dynamic networks. ACM
Transactions on Algorithms. Association for Computing Machinery. https://doi.org/10.1145/3146550
chicago: Henzinger, Monika H, Sebastian Krinninger, and Danupon Nanongkai. “Sublinear-Time
Maintenance of Breadth-First Spanning Trees in Partially Dynamic Networks.” ACM
Transactions on Algorithms. Association for Computing Machinery, 2017. https://doi.org/10.1145/3146550.
ieee: M. H. Henzinger, S. Krinninger, and D. Nanongkai, “Sublinear-time maintenance
of breadth-first spanning trees in partially dynamic networks,” ACM Transactions
on Algorithms, vol. 13, no. 4. Association for Computing Machinery, 2017.
ista: Henzinger MH, Krinninger S, Nanongkai D. 2017. Sublinear-time maintenance
of breadth-first spanning trees in partially dynamic networks. ACM Transactions
on Algorithms. 13(4), 51.
mla: Henzinger, Monika H., et al. “Sublinear-Time Maintenance of Breadth-First Spanning
Trees in Partially Dynamic Networks.” ACM Transactions on Algorithms, vol.
13, no. 4, 51, Association for Computing Machinery, 2017, doi:10.1145/3146550.
short: M.H. Henzinger, S. Krinninger, D. Nanongkai, ACM Transactions on Algorithms
13 (2017).
date_created: 2022-07-27T11:37:23Z
date_published: 2017-10-01T00:00:00Z
date_updated: 2022-09-09T11:57:42Z
day: '01'
doi: 10.1145/3146550
extern: '1'
external_id:
arxiv:
- '1512.08147'
intvolume: ' 13'
issue: '4'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1512.08147
month: '10'
oa: 1
oa_version: Preprint
publication: ACM Transactions on Algorithms
publication_identifier:
eissn:
- 1549-6333
issn:
- 1549-6325
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
scopus_import: '1'
status: public
title: Sublinear-time maintenance of breadth-first spanning trees in partially dynamic
networks
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 13
year: '2017'
...
---
_id: '11676'
abstract:
- lang: eng
text: We study the problem of maximizing a monotone submodular function with viability
constraints. This problem originates from computational biology, where we are
given a phylogenetic tree over a set of species and a directed graph, the so-called
food web, encoding viability constraints between these species. These food webs
usually have constant depth. The goal is to select a subset of k species that
satisfies the viability constraints and has maximal phylogenetic diversity. As
this problem is known to be NP-hard, we investigate approximation algorithms.
We present the first constant factor approximation algorithm if the depth is constant.
Its approximation ratio is (1−1e√). This algorithm not only applies to phylogenetic
trees with viability constraints but for arbitrary monotone submodular set functions
with viability constraints. Second, we show that there is no (1−1/e+ϵ)-approximation
algorithm for our problem setting (even for additive functions) and that there
is no approximation algorithm for a slight extension of this setting.
acknowledgement: "The research leading to these results has received funding from
the European Research\r\nCouncil under the European Union’s Seventh Framework Programme
(FP/2007-2013)/ERC Grant Agreement No. 340506."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Wolfgang
full_name: Dvořák, Wolfgang
last_name: Dvořák
- first_name: Monika H
full_name: Henzinger, Monika H
id: 540c9bbd-f2de-11ec-812d-d04a5be85630
last_name: Henzinger
orcid: 0000-0002-5008-6530
- first_name: David P.
full_name: Williamson, David P.
last_name: Williamson
citation:
ama: Dvořák W, Henzinger MH, Williamson DP. Maximizing a submodular function with
viability constraints. Algorithmica. 2017;77(1):152-172. doi:10.1007/s00453-015-0066-y
apa: Dvořák, W., Henzinger, M. H., & Williamson, D. P. (2017). Maximizing a
submodular function with viability constraints. Algorithmica. Springer
Nature. https://doi.org/10.1007/s00453-015-0066-y
chicago: Dvořák, Wolfgang, Monika H Henzinger, and David P. Williamson. “Maximizing
a Submodular Function with Viability Constraints.” Algorithmica. Springer
Nature, 2017. https://doi.org/10.1007/s00453-015-0066-y.
ieee: W. Dvořák, M. H. Henzinger, and D. P. Williamson, “Maximizing a submodular
function with viability constraints,” Algorithmica, vol. 77, no. 1. Springer
Nature, pp. 152–172, 2017.
ista: Dvořák W, Henzinger MH, Williamson DP. 2017. Maximizing a submodular function
with viability constraints. Algorithmica. 77(1), 152–172.
mla: Dvořák, Wolfgang, et al. “Maximizing a Submodular Function with Viability Constraints.”
Algorithmica, vol. 77, no. 1, Springer Nature, 2017, pp. 152–72, doi:10.1007/s00453-015-0066-y.
short: W. Dvořák, M.H. Henzinger, D.P. Williamson, Algorithmica 77 (2017) 152–172.
date_created: 2022-07-27T14:37:24Z
date_published: 2017-01-01T00:00:00Z
date_updated: 2022-09-12T08:58:16Z
day: '01'
doi: 10.1007/s00453-015-0066-y
extern: '1'
external_id:
arxiv:
- '1611.05753'
intvolume: ' 77'
issue: '1'
keyword:
- Approximation algorithms
- Submodular functions
- Phylogenetic diversity
- Viability constraints
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1611.05753
month: '01'
oa: 1
oa_version: Preprint
page: 152-172
publication: Algorithmica
publication_identifier:
eissn:
- 1432-0541
issn:
- 0178-4617
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
scopus_import: '1'
status: public
title: Maximizing a submodular function with viability constraints
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 77
year: '2017'
...
---
_id: '1168'
abstract:
- lang: eng
text: Optimum experimental design theory has recently been extended for parameter
estimation in copula models. The use of these models allows one to gain in flexibility
by considering the model parameter set split into marginal and dependence parameters.
However, this separation also leads to the natural issue of estimating only a
subset of all model parameters. In this work, we treat this problem with the application
of the (Formula presented.)-optimality to copula models. First, we provide an
extension of the corresponding equivalence theory. Then, we analyze a wide range
of flexible copula models to highlight the usefulness of (Formula presented.)-optimality
in many possible scenarios. Finally, we discuss how the usage of the introduced
design criterion also relates to the more general issue of copula selection and
optimal design for model discrimination.
acknowledgement: 'This work has been supported by the project ANR-2011-IS01-001-01
“DESIRE” and Austrian Science Fund (FWF) I833-N18. Open access funding is provided
by the Austrian Science Fund (FWF). '
article_processing_charge: No
author:
- first_name: Elisa
full_name: Perrone, Elisa
id: 2A5F8724-F248-11E8-B48F-1D18A9856A87
last_name: Perrone
orcid: 0000-0003-0370-9835
- first_name: Andreas
full_name: Rappold, Andreas
last_name: Rappold
- first_name: Werner
full_name: Müller, Werner
last_name: Müller
citation:
ama: Perrone E, Rappold A, Müller W. D inf s optimality in copula models. Statistical
Methods and Applications. 2017;26(3):403-418. doi:10.1007/s10260-016-0375-6
apa: Perrone, E., Rappold, A., & Müller, W. (2017). D inf s optimality in copula
models. Statistical Methods and Applications. Springer. https://doi.org/10.1007/s10260-016-0375-6
chicago: Perrone, Elisa, Andreas Rappold, and Werner Müller. “D Inf s Optimality
in Copula Models.” Statistical Methods and Applications. Springer, 2017.
https://doi.org/10.1007/s10260-016-0375-6.
ieee: E. Perrone, A. Rappold, and W. Müller, “D inf s optimality in copula models,”
Statistical Methods and Applications, vol. 26, no. 3. Springer, pp. 403–418,
2017.
ista: Perrone E, Rappold A, Müller W. 2017. D inf s optimality in copula models.
Statistical Methods and Applications. 26(3), 403–418.
mla: Perrone, Elisa, et al. “D Inf s Optimality in Copula Models.” Statistical
Methods and Applications, vol. 26, no. 3, Springer, 2017, pp. 403–18, doi:10.1007/s10260-016-0375-6.
short: E. Perrone, A. Rappold, W. Müller, Statistical Methods and Applications 26
(2017) 403–418.
date_created: 2018-12-11T11:50:31Z
date_published: 2017-08-01T00:00:00Z
date_updated: 2023-09-20T11:25:09Z
day: '01'
ddc:
- '519'
department:
- _id: CaUh
doi: 10.1007/s10260-016-0375-6
external_id:
isi:
- '000407973200004'
file:
- access_level: open_access
checksum: 0b2d1b647ca96e9ef13a14b8b6775e0f
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:16:13Z
date_updated: 2020-07-14T12:44:37Z
file_id: '5199'
file_name: IST-2017-739-v1+2_10260_2016_375_MOESM1_ESM.pdf
file_size: 56664
relation: main_file
- access_level: open_access
checksum: 3321ef34e02e28acfc427f77cf32812a
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:16:14Z
date_updated: 2020-07-14T12:44:37Z
file_id: '5200'
file_name: IST-2017-739-v1+3_s10260-016-0375-6.pdf
file_size: 688953
relation: main_file
file_date_updated: 2020-07-14T12:44:37Z
has_accepted_license: '1'
intvolume: ' 26'
isi: 1
issue: '3'
language:
- iso: eng
month: '08'
oa: 1
oa_version: Submitted Version
page: 403 - 418
publication: Statistical Methods and Applications
publication_status: published
publisher: Springer
publist_id: '6189'
pubrep_id: '739'
quality_controlled: '1'
scopus_import: '1'
status: public
title: D inf s optimality in copula models
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: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 26
year: '2017'
...
---
_id: '1169'
abstract:
- lang: eng
text: Dispersal is a crucial factor in natural evolution, since it determines the
habitat experienced by any population and defines the spatial scale of interactions
between individuals. There is compelling evidence for systematic differences in
dispersal characteristics within the same population, i.e., genotype-dependent
dispersal. The consequences of genotype-dependent dispersal on other evolutionary
phenomena, however, are poorly understood. In this article we investigate the
effect of genotype-dependent dispersal on spatial gene frequency patterns, using
a generalization of the classical diffusion model of selection and dispersal.
Dispersal is characterized by the variance of dispersal (diffusion coefficient)
and the mean displacement (directional advection term). We demonstrate that genotype-dependent
dispersal may change the qualitative behavior of Fisher waves, which change from
being “pulled” to being “pushed” wave fronts as the discrepancy in dispersal between
genotypes increases. The speed of any wave is partitioned into components due
to selection, genotype-dependent variance of dispersal, and genotype-dependent
mean displacement. We apply our findings to wave fronts maintained by selection
against heterozygotes. Furthermore, we identify a benefit of increased variance
of dispersal, quantify its effect on the speed of the wave, and discuss the implications
for the evolution of dispersal strategies.
article_processing_charge: No
author:
- first_name: Sebastian
full_name: Novak, Sebastian
id: 461468AE-F248-11E8-B48F-1D18A9856A87
last_name: Novak
orcid: 0000-0002-2519-824X
- first_name: Richard
full_name: Kollár, Richard
last_name: Kollár
citation:
ama: Novak S, Kollár R. Spatial gene frequency waves under genotype dependent dispersal.
Genetics. 2017;205(1):367-374. doi:10.1534/genetics.116.193946
apa: Novak, S., & Kollár, R. (2017). Spatial gene frequency waves under genotype
dependent dispersal. Genetics. Genetics Society of America. https://doi.org/10.1534/genetics.116.193946
chicago: Novak, Sebastian, and Richard Kollár. “Spatial Gene Frequency Waves under
Genotype Dependent Dispersal.” Genetics. Genetics Society of America, 2017.
https://doi.org/10.1534/genetics.116.193946.
ieee: S. Novak and R. Kollár, “Spatial gene frequency waves under genotype dependent
dispersal,” Genetics, vol. 205, no. 1. Genetics Society of America, pp.
367–374, 2017.
ista: Novak S, Kollár R. 2017. Spatial gene frequency waves under genotype dependent
dispersal. Genetics. 205(1), 367–374.
mla: Novak, Sebastian, and Richard Kollár. “Spatial Gene Frequency Waves under Genotype
Dependent Dispersal.” Genetics, vol. 205, no. 1, Genetics Society of America,
2017, pp. 367–74, doi:10.1534/genetics.116.193946.
short: S. Novak, R. Kollár, Genetics 205 (2017) 367–374.
date_created: 2018-12-11T11:50:31Z
date_published: 2017-01-01T00:00:00Z
date_updated: 2025-05-28T11:42:46Z
day: '01'
ddc:
- '576'
department:
- _id: NiBa
doi: 10.1534/genetics.116.193946
ec_funded: 1
external_id:
isi:
- '000393677300025'
file:
- access_level: open_access
checksum: 7c8ab79cda1f92760bbbbe0f53175bfc
content_type: application/pdf
creator: system
date_created: 2018-12-12T10:10:43Z
date_updated: 2020-07-14T12:44:37Z
file_id: '4833'
file_name: IST-2016-727-v1+1_SFC_Genetics_final.pdf
file_size: 361500
relation: main_file
file_date_updated: 2020-07-14T12:44:37Z
has_accepted_license: '1'
intvolume: ' 205'
isi: 1
issue: '1'
language:
- iso: eng
month: '01'
oa: 1
oa_version: Submitted Version
page: 367 - 374
project:
- _id: 25B1EC9E-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '618091'
name: Speed of Adaptation in Population Genetics and Evolutionary Computation
- _id: 25B07788-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '250152'
name: Limits to selection in biology and in evolutionary computation
publication: Genetics
publication_identifier:
issn:
- '00166731'
publication_status: published
publisher: Genetics Society of America
publist_id: '6188'
pubrep_id: '727'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Spatial gene frequency waves under genotype dependent dispersal
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 205
year: '2017'
...
---
_id: '1173'
abstract:
- lang: eng
text: We introduce the Voronoi functional of a triangulation of a finite set of
points in the Euclidean plane and prove that among all geometric triangulations
of the point set, the Delaunay triangulation maximizes the functional. This result
neither extends to topological triangulations in the plane nor to geometric triangulations
in three and higher dimensions.
acknowledgement: This research is partially supported by the Russian Government under
the Mega Project 11.G34.31.0053, by the Toposys project FP7-ICT-318493-STREP, by
ESF under the ACAT Research Network Programme, by RFBR grant 11-01-00735, and by
NSF grants DMS-1101688, DMS-1400876.
article_processing_charge: No
author:
- first_name: Herbert
full_name: Edelsbrunner, Herbert
id: 3FB178DA-F248-11E8-B48F-1D18A9856A87
last_name: Edelsbrunner
orcid: 0000-0002-9823-6833
- first_name: Alexey
full_name: Glazyrin, Alexey
last_name: Glazyrin
- first_name: Oleg
full_name: Musin, Oleg
last_name: Musin
- first_name: Anton
full_name: Nikitenko, Anton
id: 3E4FF1BA-F248-11E8-B48F-1D18A9856A87
last_name: Nikitenko
orcid: 0000-0002-0659-3201
citation:
ama: Edelsbrunner H, Glazyrin A, Musin O, Nikitenko A. The Voronoi functional is
maximized by the Delaunay triangulation in the plane. Combinatorica. 2017;37(5):887-910.
doi:10.1007/s00493-016-3308-y
apa: Edelsbrunner, H., Glazyrin, A., Musin, O., & Nikitenko, A. (2017). The
Voronoi functional is maximized by the Delaunay triangulation in the plane. Combinatorica.
Springer. https://doi.org/10.1007/s00493-016-3308-y
chicago: Edelsbrunner, Herbert, Alexey Glazyrin, Oleg Musin, and Anton Nikitenko.
“The Voronoi Functional Is Maximized by the Delaunay Triangulation in the Plane.”
Combinatorica. Springer, 2017. https://doi.org/10.1007/s00493-016-3308-y.
ieee: H. Edelsbrunner, A. Glazyrin, O. Musin, and A. Nikitenko, “The Voronoi functional
is maximized by the Delaunay triangulation in the plane,” Combinatorica,
vol. 37, no. 5. Springer, pp. 887–910, 2017.
ista: Edelsbrunner H, Glazyrin A, Musin O, Nikitenko A. 2017. The Voronoi functional
is maximized by the Delaunay triangulation in the plane. Combinatorica. 37(5),
887–910.
mla: Edelsbrunner, Herbert, et al. “The Voronoi Functional Is Maximized by the Delaunay
Triangulation in the Plane.” Combinatorica, vol. 37, no. 5, Springer, 2017,
pp. 887–910, doi:10.1007/s00493-016-3308-y.
short: H. Edelsbrunner, A. Glazyrin, O. Musin, A. Nikitenko, Combinatorica 37 (2017)
887–910.
date_created: 2018-12-11T11:50:32Z
date_published: 2017-10-01T00:00:00Z
date_updated: 2023-09-20T11:23:53Z
day: '01'
department:
- _id: HeEd
doi: 10.1007/s00493-016-3308-y
ec_funded: 1
external_id:
isi:
- '000418056000005'
intvolume: ' 37'
isi: 1
issue: '5'
language:
- iso: eng
main_file_link:
- open_access: '1'
url: https://arxiv.org/abs/1411.6337
month: '10'
oa: 1
oa_version: Submitted Version
page: 887 - 910
project:
- _id: 255D761E-B435-11E9-9278-68D0E5697425
call_identifier: FP7
grant_number: '318493'
name: Topological Complex Systems
publication: Combinatorica
publication_identifier:
issn:
- '02099683'
publication_status: published
publisher: Springer
publist_id: '6182'
quality_controlled: '1'
scopus_import: '1'
status: public
title: The Voronoi functional is maximized by the Delaunay triangulation in the plane
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 37
year: '2017'
...
---
_id: '1174'
abstract:
- lang: eng
text: Security of cryptographic applications is typically defined by security games.
The adversary, within certain resources, cannot win with probability much better
than 0 (for unpredictability applications, like one-way functions) or much better
than 1/2 (indistinguishability applications for instance encryption schemes).
In so called squared-friendly applications the winning probability of the adversary,
for different values of the application secret randomness, is not only close to
0 or 1/2 on average, but also concentrated in the sense that its second central
moment is small. The class of squared-friendly applications, which contains all
unpredictability applications and many indistinguishability applications, is particularly
important for key derivation. Barak et al. observed that for square-friendly applications
one can beat the "RT-bound", extracting secure keys with significantly
smaller entropy loss. In turn Dodis and Yu showed that in squared-friendly applications
one can directly use a "weak" key, which has only high entropy, as a
secure key. In this paper we give sharp lower bounds on square security assuming
security for "weak" keys. We show that any application which is either
(a) secure with weak keys or (b) allows for entropy savings for keys derived by
universal hashing, must be square-friendly. Quantitatively, our lower bounds match
the positive results of Dodis and Yu and Barak et al. (TCC\'13, CRYPTO\'11) Hence,
they can be understood as a general characterization of squared-friendly applications.
While the positive results on squared-friendly applications where derived by one
clever application of the Cauchy-Schwarz Inequality, for tight lower bounds we
need more machinery. In our approach we use convex optimization techniques and
some theory of circular matrices.
alternative_title:
- LIPIcs
article_number: '57'
article_processing_charge: No
author:
- first_name: Maciej
full_name: Skórski, Maciej
id: EC09FA6A-02D0-11E9-8223-86B7C91467DD
last_name: Skórski
citation:
ama: 'Skórski M. Lower bounds on key derivation for square-friendly applications.
In: Vol 66. Schloss Dagstuhl - Leibniz-Zentrum für Informatik; 2017. doi:10.4230/LIPIcs.STACS.2017.57'
apa: 'Skórski, M. (2017). Lower bounds on key derivation for square-friendly applications
(Vol. 66). Presented at the STACS: Symposium on Theoretical Aspects of Computer
Science, Hannover, Germany: Schloss Dagstuhl - Leibniz-Zentrum für Informatik.
https://doi.org/10.4230/LIPIcs.STACS.2017.57'
chicago: Skórski, Maciej. “Lower Bounds on Key Derivation for Square-Friendly Applications,”
Vol. 66. Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017. https://doi.org/10.4230/LIPIcs.STACS.2017.57.
ieee: 'M. Skórski, “Lower bounds on key derivation for square-friendly applications,”
presented at the STACS: Symposium on Theoretical Aspects of Computer Science,
Hannover, Germany, 2017, vol. 66.'
ista: 'Skórski M. 2017. Lower bounds on key derivation for square-friendly applications.
STACS: Symposium on Theoretical Aspects of Computer Science, LIPIcs, vol. 66,
57.'
mla: Skórski, Maciej. Lower Bounds on Key Derivation for Square-Friendly Applications.
Vol. 66, 57, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017, doi:10.4230/LIPIcs.STACS.2017.57.
short: M. Skórski, in:, Schloss Dagstuhl - Leibniz-Zentrum für Informatik, 2017.
conference:
end_date: 2017-03-11
location: Hannover, Germany
name: 'STACS: Symposium on Theoretical Aspects of Computer Science'
start_date: 2017-03-08
date_created: 2018-12-11T11:50:32Z
date_published: 2017-03-01T00:00:00Z
date_updated: 2023-09-20T11:23:15Z
day: '01'
department:
- _id: KrPi
doi: 10.4230/LIPIcs.STACS.2017.57
ec_funded: 1
external_id:
isi:
- '000521077300057'
intvolume: ' 66'
isi: 1
language:
- iso: eng
main_file_link:
- open_access: '1'
url: http://drops.dagstuhl.de/opus/volltexte/2017/6976
month: '03'
oa: 1
oa_version: Submitted Version
project:
- _id: 258AA5B2-B435-11E9-9278-68D0E5697425
call_identifier: H2020
grant_number: '682815'
name: Teaching Old Crypto New Tricks
publication_identifier:
issn:
- '18688969'
publication_status: published
publisher: Schloss Dagstuhl - Leibniz-Zentrum für Informatik
publist_id: '6180'
quality_controlled: '1'
scopus_import: '1'
status: public
title: Lower bounds on key derivation for square-friendly applications
type: conference
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 66
year: '2017'
...