---
_id: '9781'
abstract:
- lang: eng
  text: We consider the Pekar functional on a ball in ℝ3. We prove uniqueness of minimizers,
    and a quadratic lower bound in terms of the distance to the minimizer. The latter
    follows from nondegeneracy of the Hessian at the minimum.
acknowledgement: We are grateful for the hospitality at the Mittag-Leffler Institute,
  where part of this work has been done. The work of the authors was supported by
  the European Research Council (ERC)under the European Union's Horizon 2020 research
  and innovation programme grant 694227.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Dario
  full_name: Feliciangeli, Dario
  id: 41A639AA-F248-11E8-B48F-1D18A9856A87
  last_name: Feliciangeli
  orcid: 0000-0003-0754-8530
- first_name: Robert
  full_name: Seiringer, Robert
  id: 4AFD0470-F248-11E8-B48F-1D18A9856A87
  last_name: Seiringer
  orcid: 0000-0002-6781-0521
citation:
  ama: Feliciangeli D, Seiringer R. Uniqueness and nondegeneracy of minimizers of
    the Pekar functional on a ball. <i>SIAM Journal on Mathematical Analysis</i>.
    2020;52(1):605-622. doi:<a href="https://doi.org/10.1137/19m126284x">10.1137/19m126284x</a>
  apa: Feliciangeli, D., &#38; Seiringer, R. (2020). Uniqueness and nondegeneracy
    of minimizers of the Pekar functional on a ball. <i>SIAM Journal on Mathematical
    Analysis</i>. Society for Industrial &#38; Applied Mathematics . <a href="https://doi.org/10.1137/19m126284x">https://doi.org/10.1137/19m126284x</a>
  chicago: Feliciangeli, Dario, and Robert Seiringer. “Uniqueness and Nondegeneracy
    of Minimizers of the Pekar Functional on a Ball.” <i>SIAM Journal on Mathematical
    Analysis</i>. Society for Industrial &#38; Applied Mathematics , 2020. <a href="https://doi.org/10.1137/19m126284x">https://doi.org/10.1137/19m126284x</a>.
  ieee: D. Feliciangeli and R. Seiringer, “Uniqueness and nondegeneracy of minimizers
    of the Pekar functional on a ball,” <i>SIAM Journal on Mathematical Analysis</i>,
    vol. 52, no. 1. Society for Industrial &#38; Applied Mathematics , pp. 605–622,
    2020.
  ista: Feliciangeli D, Seiringer R. 2020. Uniqueness and nondegeneracy of minimizers
    of the Pekar functional on a ball. SIAM Journal on Mathematical Analysis. 52(1),
    605–622.
  mla: Feliciangeli, Dario, and Robert Seiringer. “Uniqueness and Nondegeneracy of
    Minimizers of the Pekar Functional on a Ball.” <i>SIAM Journal on Mathematical
    Analysis</i>, vol. 52, no. 1, Society for Industrial &#38; Applied Mathematics
    , 2020, pp. 605–22, doi:<a href="https://doi.org/10.1137/19m126284x">10.1137/19m126284x</a>.
  short: D. Feliciangeli, R. Seiringer, SIAM Journal on Mathematical Analysis 52 (2020)
    605–622.
date_created: 2021-08-06T07:34:16Z
date_published: 2020-02-12T00:00:00Z
date_updated: 2023-09-07T13:30:11Z
day: '12'
ddc:
- '510'
department:
- _id: RoSe
doi: 10.1137/19m126284x
ec_funded: 1
external_id:
  arxiv:
  - '1904.08647 '
  isi:
  - '000546967700022'
has_accepted_license: '1'
intvolume: '        52'
isi: 1
issue: '1'
keyword:
- Applied Mathematics
- Computational Mathematics
- Analysis
language:
- iso: eng
license: https://creativecommons.org/licenses/by-nc-nd/4.0/
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1904.08647
month: '02'
oa: 1
oa_version: Preprint
page: 605-622
project:
- _id: 25C6DC12-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '694227'
  name: Analysis of quantum many-body systems
publication: SIAM Journal on Mathematical Analysis
publication_identifier:
  eissn:
  - 1095-7154
  issn:
  - 0036-1410
publication_status: published
publisher: 'Society for Industrial & Applied Mathematics '
quality_controlled: '1'
related_material:
  record:
  - id: '9733'
    relation: dissertation_contains
    status: public
scopus_import: '1'
status: public
title: Uniqueness and nondegeneracy of minimizers of the Pekar functional on a ball
tmp:
  image: /images/cc_by_nc_nd.png
  legal_code_url: https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode
  name: Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
    (CC BY-NC-ND 4.0)
  short: CC BY-NC-ND (4.0)
type: journal_article
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 52
year: '2020'
...
---
_id: '10878'
abstract:
- lang: eng
  text: Starting from a microscopic model for a system of neurons evolving in time
    which individually follow a stochastic integrate-and-fire type model, we study
    a mean-field limit of the system. Our model is described by a system of SDEs with
    discontinuous coefficients for the action potential of each neuron and takes into
    account the (random) spatial configuration of neurons allowing the interaction
    to depend on it. In the limit as the number of particles tends to infinity, we
    obtain a nonlinear Fokker-Planck type PDE in two variables, with derivatives only
    with respect to one variable and discontinuous coefficients. We also study strong
    well-posedness of the system of SDEs and prove the existence and uniqueness of
    a weak measure-valued solution to the PDE, obtained as the limit of the laws of
    the empirical measures for the system of particles.
acknowledgement: "The second author has been partially supported by INdAM through
  the GNAMPA Research\r\nProject (2017) “Sistemi stocastici singolari: buona posizione
  e problemi di controllo”. The third\r\nauthor was partly funded by the Austrian
  Science Fund (FWF) project F 65."
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Franco
  full_name: Flandoli, Franco
  last_name: Flandoli
- first_name: Enrico
  full_name: Priola, Enrico
  last_name: Priola
- first_name: Giovanni A
  full_name: Zanco, Giovanni A
  id: 47491882-F248-11E8-B48F-1D18A9856A87
  last_name: Zanco
citation:
  ama: Flandoli F, Priola E, Zanco GA. A mean-field model with discontinuous coefficients
    for neurons with spatial interaction. <i>Discrete and Continuous Dynamical Systems</i>.
    2019;39(6):3037-3067. doi:<a href="https://doi.org/10.3934/dcds.2019126">10.3934/dcds.2019126</a>
  apa: Flandoli, F., Priola, E., &#38; Zanco, G. A. (2019). A mean-field model with
    discontinuous coefficients for neurons with spatial interaction. <i>Discrete and
    Continuous Dynamical Systems</i>. American Institute of Mathematical Sciences.
    <a href="https://doi.org/10.3934/dcds.2019126">https://doi.org/10.3934/dcds.2019126</a>
  chicago: Flandoli, Franco, Enrico Priola, and Giovanni A Zanco. “A Mean-Field Model
    with Discontinuous Coefficients for Neurons with Spatial Interaction.” <i>Discrete
    and Continuous Dynamical Systems</i>. American Institute of Mathematical Sciences,
    2019. <a href="https://doi.org/10.3934/dcds.2019126">https://doi.org/10.3934/dcds.2019126</a>.
  ieee: F. Flandoli, E. Priola, and G. A. Zanco, “A mean-field model with discontinuous
    coefficients for neurons with spatial interaction,” <i>Discrete and Continuous
    Dynamical Systems</i>, vol. 39, no. 6. American Institute of Mathematical Sciences,
    pp. 3037–3067, 2019.
  ista: Flandoli F, Priola E, Zanco GA. 2019. A mean-field model with discontinuous
    coefficients for neurons with spatial interaction. Discrete and Continuous Dynamical
    Systems. 39(6), 3037–3067.
  mla: Flandoli, Franco, et al. “A Mean-Field Model with Discontinuous Coefficients
    for Neurons with Spatial Interaction.” <i>Discrete and Continuous Dynamical Systems</i>,
    vol. 39, no. 6, American Institute of Mathematical Sciences, 2019, pp. 3037–67,
    doi:<a href="https://doi.org/10.3934/dcds.2019126">10.3934/dcds.2019126</a>.
  short: F. Flandoli, E. Priola, G.A. Zanco, Discrete and Continuous Dynamical Systems
    39 (2019) 3037–3067.
date_created: 2022-03-18T12:33:34Z
date_published: 2019-06-01T00:00:00Z
date_updated: 2023-09-08T11:34:45Z
day: '01'
department:
- _id: JaMa
doi: 10.3934/dcds.2019126
external_id:
  arxiv:
  - '1708.04156'
  isi:
  - '000459954800003'
intvolume: '        39'
isi: 1
issue: '6'
keyword:
- Applied Mathematics
- Discrete Mathematics and Combinatorics
- Analysis
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1708.04156
month: '06'
oa: 1
oa_version: Preprint
page: 3037-3067
project:
- _id: fc31cba2-9c52-11eb-aca3-ff467d239cd2
  grant_number: F6504
  name: Taming Complexity in Partial Differential Systems
publication: Discrete and Continuous Dynamical Systems
publication_identifier:
  issn:
  - 1553-5231
publication_status: published
publisher: American Institute of Mathematical Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: A mean-field model with discontinuous coefficients for neurons with spatial
  interaction
type: journal_article
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
volume: 39
year: '2019'
...
---
_id: '11615'
abstract:
- lang: eng
  text: The recently published Kepler mission Data Release 25 (DR25) reported on ∼197 000
    targets observed during the mission. Despite this, no wide search for red giants
    showing solar-like oscillations have been made across all stars observed in Kepler’s
    long-cadence mode. In this work, we perform this task using custom apertures on
    the Kepler pixel files and detect oscillations in 21 914 stars, representing the
    largest sample of solar-like oscillating stars to date. We measure their frequency
    at maximum power, νmax, down to νmax≃4μHz and obtain log (g) estimates with a
    typical uncertainty below 0.05 dex, which is superior to typical measurements
    from spectroscopy. Additionally, the νmax distribution of our detections show
    good agreement with results from a simulated model of the Milky Way, with a ratio
    of observed to predicted stars of 0.992 for stars with 10<νmax<270μHz. Among our
    red giant detections, we find 909 to be dwarf/subgiant stars whose flux signal
    is polluted by a neighbouring giant as a result of using larger photometric apertures
    than those used by the NASA Kepler science processing pipeline. We further find
    that only 293 of the polluting giants are known Kepler targets. The remainder
    comprises over 600 newly identified oscillating red giants, with many expected
    to belong to the Galactic halo, serendipitously falling within the Kepler pixel
    files of targeted stars.
acknowledgement: Funding for this Discovery mission is provided by NASA’s Science
  mission Directorate. We thank the entire Kepler team without whom this investigation
  would not be possible. DS is the recipient of an Australian Research Council Future
  Fellowship (project number FT1400147). RAG acknowledges the support from CNES. SM
  acknowledges support from NASA grant NNX15AF13G, NSF grant AST-1411685, and the
  Ramon y Cajal fellowship number RYC-2015-17697. ILC acknowledges scholarship support
  from the University of Sydney. We would like to thank Nicholas Barbara and Timothy
  Bedding for providing us with a list of variable stars that helped to validate a
  number of detections in this study. We also thank the group at the University of
  Sydney for fruitful discussions. Finally, we gratefully acknowledge the support
  of NVIDIA Corporation with the donation of the Titan Xp GPU used for this research.
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Marc
  full_name: Hon, Marc
  last_name: Hon
- first_name: Dennis
  full_name: Stello, Dennis
  last_name: Stello
- first_name: Rafael A
  full_name: García, Rafael A
  last_name: García
- first_name: Savita
  full_name: Mathur, Savita
  last_name: Mathur
- first_name: Sanjib
  full_name: Sharma, Sanjib
  last_name: Sharma
- first_name: Isabel L
  full_name: Colman, Isabel L
  last_name: Colman
- first_name: Lisa Annabelle
  full_name: Bugnet, Lisa Annabelle
  id: d9edb345-f866-11ec-9b37-d119b5234501
  last_name: Bugnet
  orcid: 0000-0003-0142-4000
citation:
  ama: Hon M, Stello D, García RA, et al. A search for red giant solar-like oscillations
    in all Kepler data. <i>Monthly Notices of the Royal Astronomical Society</i>.
    2019;485(4):5616-5630. doi:<a href="https://doi.org/10.1093/mnras/stz622">10.1093/mnras/stz622</a>
  apa: Hon, M., Stello, D., García, R. A., Mathur, S., Sharma, S., Colman, I. L.,
    &#38; Bugnet, L. A. (2019). A search for red giant solar-like oscillations in
    all Kepler data. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford
    University Press. <a href="https://doi.org/10.1093/mnras/stz622">https://doi.org/10.1093/mnras/stz622</a>
  chicago: Hon, Marc, Dennis Stello, Rafael A García, Savita Mathur, Sanjib Sharma,
    Isabel L Colman, and Lisa Annabelle Bugnet. “A Search for Red Giant Solar-like
    Oscillations in All Kepler Data.” <i>Monthly Notices of the Royal Astronomical
    Society</i>. Oxford University Press, 2019. <a href="https://doi.org/10.1093/mnras/stz622">https://doi.org/10.1093/mnras/stz622</a>.
  ieee: M. Hon <i>et al.</i>, “A search for red giant solar-like oscillations in all
    Kepler data,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 485,
    no. 4. Oxford University Press, pp. 5616–5630, 2019.
  ista: Hon M, Stello D, García RA, Mathur S, Sharma S, Colman IL, Bugnet LA. 2019.
    A search for red giant solar-like oscillations in all Kepler data. Monthly Notices
    of the Royal Astronomical Society. 485(4), 5616–5630.
  mla: Hon, Marc, et al. “A Search for Red Giant Solar-like Oscillations in All Kepler
    Data.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 485, no.
    4, Oxford University Press, 2019, pp. 5616–30, doi:<a href="https://doi.org/10.1093/mnras/stz622">10.1093/mnras/stz622</a>.
  short: M. Hon, D. Stello, R.A. García, S. Mathur, S. Sharma, I.L. Colman, L.A. Bugnet,
    Monthly Notices of the Royal Astronomical Society 485 (2019) 5616–5630.
date_created: 2022-07-18T14:26:03Z
date_published: 2019-06-01T00:00:00Z
date_updated: 2022-08-22T07:35:19Z
day: '01'
doi: 10.1093/mnras/stz622
extern: '1'
external_id:
  arxiv:
  - '1903.00115'
intvolume: '       485'
issue: '4'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- asteroseismology
- 'methods: data analysis'
- 'techniques: image processing'
- 'stars: oscillations'
- 'stars: statistics'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1903.00115
month: '06'
oa: 1
oa_version: Preprint
page: 5616-5630
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 search for red giant solar-like oscillations in all Kepler data
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 485
year: '2019'
...
---
_id: '11623'
abstract:
- lang: eng
  text: Brightness variations due to dark spots on the stellar surface encode information
    about stellar surface rotation and magnetic activity. In this work, we analyze
    the Kepler long-cadence data of 26,521 main-sequence stars of spectral types M
    and K in order to measure their surface rotation and photometric activity level.
    Rotation-period estimates are obtained by the combination of a wavelet analysis
    and autocorrelation function of the light curves. Reliable rotation estimates
    are determined by comparing the results from the different rotation diagnostics
    and four data sets. We also measure the photometric activity proxy Sph using the
    amplitude of the flux variations on an appropriate timescale. We report rotation
    periods and photometric activity proxies for about 60% of the sample, including
    4431 targets for which McQuillan et al. did not report a rotation period. For
    the common targets with rotation estimates in this study and in McQuillan et al.,
    our rotation periods agree within 99%. In this work, we also identify potential
    polluters, such as misclassified red giants and classical pulsator candidates.
    Within the parameter range we study, there is a mild tendency for hotter stars
    to have shorter rotation periods. The photometric activity proxy spans a wider
    range of values with increasing effective temperature. The rotation period and
    photometric activity proxy are also related, with Sph being larger for fast rotators.
    Similar to McQuillan et al., we find a bimodal distribution of rotation periods.
acknowledgement: "The authors thank Róbert Szabó Paul G. Beck, Katrien Kolenberg,
  and Isabel L. Colman for helping on the classification of stars. This paper includes
  data collected by the Kepler mission and obtained from the MAST data archive at
  the Space Telescope Science Institute (STScI). Funding for the Kepler mission is
  provided by the National Aeronautics and Space Administration (NASA) Science Mission
  Directorate. STScI is operated by the Association of Universities for Research in
  Astronomy, Inc., under NASA contract NAS 5–26555. A.R.G.S. acknowledges the support
  from NASA under grant NNX17AF27G. R.A.G. and L.B. acknowledge the support from PLATO
  and GOLF CNES grants. S.M. acknowledges the support from the Ramon y Cajal fellowship
  number RYC-2015-17697. T.S.M. acknowledges support from a Visiting Fellowship at
  the Max Planck Institute for Solar System Research. This research has made use of
  the NASA Exoplanet Archive, which is operated by the California Institute of Technology,
  under contract with the National Aeronautics and Space Administration under the
  Exoplanet Exploration Program.\r\n\r\nSoftware: KADACS (García et al. 2011), NumPy
  (van der Walt et al. 2011), SciPy (Jones et al. 2001), Matplotlib (Hunter 2007).\r\n\r\nFacilities:
  MAST - , Kepler Eclipsing Binary Catalog - , Exoplanet Archive. -"
article_number: '21'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: A. R. G.
  full_name: Santos, A. R. G.
  last_name: Santos
- first_name: R. A.
  full_name: García, R. A.
  last_name: García
- first_name: S.
  full_name: Mathur, S.
  last_name: Mathur
- 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: J. L.
  full_name: van Saders, J. L.
  last_name: van Saders
- first_name: T. S.
  full_name: Metcalfe, T. S.
  last_name: Metcalfe
- first_name: G. V. A.
  full_name: Simonian, G. V. A.
  last_name: Simonian
- first_name: M. H.
  full_name: Pinsonneault, M. H.
  last_name: Pinsonneault
citation:
  ama: Santos ARG, García RA, Mathur S, et al. Surface rotation and photometric activity
    for Kepler targets. I. M and K main-sequence stars. <i>The Astrophysical Journal
    Supplement Series</i>. 2019;244(1). doi:<a href="https://doi.org/10.3847/1538-4365/ab3b56">10.3847/1538-4365/ab3b56</a>
  apa: Santos, A. R. G., García, R. A., Mathur, S., Bugnet, L. A., van Saders, J.
    L., Metcalfe, T. S., … Pinsonneault, M. H. (2019). Surface rotation and photometric
    activity for Kepler targets. I. M and K main-sequence stars. <i>The Astrophysical
    Journal Supplement Series</i>. IOP Publishing. <a href="https://doi.org/10.3847/1538-4365/ab3b56">https://doi.org/10.3847/1538-4365/ab3b56</a>
  chicago: Santos, A. R. G., R. A. García, S. Mathur, Lisa Annabelle Bugnet, J. L.
    van Saders, T. S. Metcalfe, G. V. A. Simonian, and M. H. Pinsonneault. “Surface
    Rotation and Photometric Activity for Kepler Targets. I. M and K Main-Sequence
    Stars.” <i>The Astrophysical Journal Supplement Series</i>. IOP Publishing, 2019.
    <a href="https://doi.org/10.3847/1538-4365/ab3b56">https://doi.org/10.3847/1538-4365/ab3b56</a>.
  ieee: A. R. G. Santos <i>et al.</i>, “Surface rotation and photometric activity
    for Kepler targets. I. M and K main-sequence stars,” <i>The Astrophysical Journal
    Supplement Series</i>, vol. 244, no. 1. IOP Publishing, 2019.
  ista: Santos ARG, García RA, Mathur S, Bugnet LA, van Saders JL, Metcalfe TS, Simonian
    GVA, Pinsonneault MH. 2019. Surface rotation and photometric activity for Kepler
    targets. I. M and K main-sequence stars. The Astrophysical Journal Supplement
    Series. 244(1), 21.
  mla: Santos, A. R. G., et al. “Surface Rotation and Photometric Activity for Kepler
    Targets. I. M and K Main-Sequence Stars.” <i>The Astrophysical Journal Supplement
    Series</i>, vol. 244, no. 1, 21, IOP Publishing, 2019, doi:<a href="https://doi.org/10.3847/1538-4365/ab3b56">10.3847/1538-4365/ab3b56</a>.
  short: A.R.G. Santos, R.A. García, S. Mathur, L.A. Bugnet, J.L. van Saders, T.S.
    Metcalfe, G.V.A. Simonian, M.H. Pinsonneault, The Astrophysical Journal Supplement
    Series 244 (2019).
date_created: 2022-07-19T09:21:58Z
date_published: 2019-09-19T00:00:00Z
date_updated: 2022-08-22T08:10:38Z
day: '19'
doi: 10.3847/1538-4365/ab3b56
extern: '1'
external_id:
  arxiv:
  - '1908.05222'
intvolume: '       244'
issue: '1'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- 'methods: data analysis'
- 'stars: activity'
- 'stars: low-mass'
- 'stars: rotation'
- starspots
- 'techniques: photometric'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1908.05222
month: '09'
oa: 1
oa_version: Preprint
publication: The Astrophysical Journal Supplement Series
publication_identifier:
  issn:
  - 0067-0049
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: Surface rotation and photometric activity for Kepler targets. I. M and K main-sequence
  stars
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 244
year: '2019'
...
---
_id: '11630'
abstract:
- lang: eng
  text: 'The second mission of NASA’s Kepler satellite, K2, has collected hundreds
    of thousands of lightcurves for stars close to the ecliptic plane. This new sample
    could increase the number of known pulsating stars and then improve our understanding
    of those stars. For the moment only a few stars have been properly classified
    and published. In this work, we present a method to automaticly classify K2 pulsating
    stars using a Machine Learning technique called Random Forest. The objective is
    to sort out the stars in four classes: red giant (RG), main-sequence Solar-like
    stars (SL), classical pulsators (PULS) and Other. To do this we use the effective
    temperatures and the luminosities of the stars as well as the FliPer features,
    that measures the amount of power contained in the power spectral density. The
    classifier now retrieves the right classification for more than 80% of the stars.'
article_number: '1906.09611'
article_processing_charge: No
arxiv: 1
author:
- first_name: A. Le
  full_name: Saux, A. Le
  last_name: Saux
- 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: S.
  full_name: Mathur, S.
  last_name: Mathur
- first_name: S. N.
  full_name: Breton, S. N.
  last_name: Breton
- first_name: R. A.
  full_name: Garcia, R. A.
  last_name: Garcia
citation:
  ama: Saux AL, Bugnet LA, Mathur S, Breton SN, Garcia RA. Automatic classification
    of K2 pulsating stars using machine learning techniques. <i>arXiv</i>. doi:<a
    href="https://doi.org/10.48550/arXiv.1906.09611">10.48550/arXiv.1906.09611</a>
  apa: Saux, A. L., Bugnet, L. A., Mathur, S., Breton, S. N., &#38; Garcia, R. A.
    (n.d.). Automatic classification of K2 pulsating stars using machine learning
    techniques. <i>arXiv</i>. <a href="https://doi.org/10.48550/arXiv.1906.09611">https://doi.org/10.48550/arXiv.1906.09611</a>
  chicago: Saux, A. Le, Lisa Annabelle Bugnet, S. Mathur, S. N. Breton, and R. A.
    Garcia. “Automatic Classification of K2 Pulsating Stars Using Machine Learning
    Techniques.” <i>ArXiv</i>, n.d. <a href="https://doi.org/10.48550/arXiv.1906.09611">https://doi.org/10.48550/arXiv.1906.09611</a>.
  ieee: A. L. Saux, L. A. Bugnet, S. Mathur, S. N. Breton, and R. A. Garcia, “Automatic
    classification of K2 pulsating stars using machine learning techniques,” <i>arXiv</i>.
    .
  ista: Saux AL, Bugnet LA, Mathur S, Breton SN, Garcia RA. Automatic classification
    of K2 pulsating stars using machine learning techniques. arXiv, 1906.09611.
  mla: Saux, A. Le, et al. “Automatic Classification of K2 Pulsating Stars Using Machine
    Learning Techniques.” <i>ArXiv</i>, 1906.09611, doi:<a href="https://doi.org/10.48550/arXiv.1906.09611">10.48550/arXiv.1906.09611</a>.
  short: A.L. Saux, L.A. Bugnet, S. Mathur, S.N. Breton, R.A. Garcia, ArXiv (n.d.).
date_created: 2022-07-21T06:57:10Z
date_published: 2019-06-23T00:00:00Z
date_updated: 2022-08-22T08:20:29Z
day: '23'
doi: 10.48550/arXiv.1906.09611
extern: '1'
external_id:
  arxiv:
  - '1906.09611'
keyword:
- asteroseismology - methods
- data analysis - thecniques
- machine learning - stars
- oscillations
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.48550/arXiv.1906.09611
month: '06'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: Automatic classification of K2 pulsating stars using machine learning techniques
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2019'
...
---
_id: '8418'
abstract:
- lang: eng
  text: For the Restricted Circular Planar 3 Body Problem, we show that there exists
    an open set U in phase space of fixed measure, where the set of initial points
    which lead to collision is O(μ120) dense as μ→0.
article_processing_charge: No
article_type: original
author:
- first_name: Marcel
  full_name: Guardia, Marcel
  last_name: Guardia
- first_name: Vadim
  full_name: Kaloshin, Vadim
  id: FE553552-CDE8-11E9-B324-C0EBE5697425
  last_name: Kaloshin
  orcid: 0000-0002-6051-2628
- first_name: Jianlu
  full_name: Zhang, Jianlu
  last_name: Zhang
citation:
  ama: Guardia M, Kaloshin V, Zhang J. Asymptotic density of collision orbits in the
    Restricted Circular Planar 3 Body Problem. <i>Archive for Rational Mechanics and
    Analysis</i>. 2019;233(2):799-836. doi:<a href="https://doi.org/10.1007/s00205-019-01368-7">10.1007/s00205-019-01368-7</a>
  apa: Guardia, M., Kaloshin, V., &#38; Zhang, J. (2019). Asymptotic density of collision
    orbits in the Restricted Circular Planar 3 Body Problem. <i>Archive for Rational
    Mechanics and Analysis</i>. Springer Nature. <a href="https://doi.org/10.1007/s00205-019-01368-7">https://doi.org/10.1007/s00205-019-01368-7</a>
  chicago: Guardia, Marcel, Vadim Kaloshin, and Jianlu Zhang. “Asymptotic Density
    of Collision Orbits in the Restricted Circular Planar 3 Body Problem.” <i>Archive
    for Rational Mechanics and Analysis</i>. Springer Nature, 2019. <a href="https://doi.org/10.1007/s00205-019-01368-7">https://doi.org/10.1007/s00205-019-01368-7</a>.
  ieee: M. Guardia, V. Kaloshin, and J. Zhang, “Asymptotic density of collision orbits
    in the Restricted Circular Planar 3 Body Problem,” <i>Archive for Rational Mechanics
    and Analysis</i>, vol. 233, no. 2. Springer Nature, pp. 799–836, 2019.
  ista: Guardia M, Kaloshin V, Zhang J. 2019. Asymptotic density of collision orbits
    in the Restricted Circular Planar 3 Body Problem. Archive for Rational Mechanics
    and Analysis. 233(2), 799–836.
  mla: Guardia, Marcel, et al. “Asymptotic Density of Collision Orbits in the Restricted
    Circular Planar 3 Body Problem.” <i>Archive for Rational Mechanics and Analysis</i>,
    vol. 233, no. 2, Springer Nature, 2019, pp. 799–836, doi:<a href="https://doi.org/10.1007/s00205-019-01368-7">10.1007/s00205-019-01368-7</a>.
  short: M. Guardia, V. Kaloshin, J. Zhang, Archive for Rational Mechanics and Analysis
    233 (2019) 799–836.
date_created: 2020-09-17T10:41:51Z
date_published: 2019-03-12T00:00:00Z
date_updated: 2021-01-12T08:19:09Z
day: '12'
doi: 10.1007/s00205-019-01368-7
extern: '1'
intvolume: '       233'
issue: '2'
keyword:
- Mechanical Engineering
- Mathematics (miscellaneous)
- Analysis
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://doi.org/10.1007/s00205-019-01368-7
month: '03'
oa: 1
oa_version: Published Version
page: 799-836
publication: Archive for Rational Mechanics and Analysis
publication_identifier:
  issn:
  - 0003-9527
  - 1432-0673
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
status: public
title: Asymptotic density of collision orbits in the Restricted Circular Planar 3
  Body Problem
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 233
year: '2019'
...
---
_id: '6035'
abstract:
- lang: eng
  text: 'We present JuliaReach, a toolbox for set-based reachability analysis of dynamical
    systems. JuliaReach consists of two main packages: Reachability, containing implementations
    of reachability algorithms for continuous and hybrid systems, and LazySets, a
    standalone library that implements state-of-the-art algorithms for calculus with
    convex sets. The library offers both concrete and lazy set representations, where
    the latter stands for the ability to delay set computations until they are needed.
    The choice of the programming language Julia and the accompanying documentation
    of our toolbox allow researchers to easily translate set-based algorithms from
    mathematics to software in a platform-independent way, while achieving runtime
    performance that is comparable to statically compiled languages. Combining lazy
    operations in high dimensions and explicit computations in low dimensions, JuliaReach
    can be applied to solve complex, large-scale problems.'
article_processing_charge: No
arxiv: 1
author:
- first_name: Sergiy
  full_name: Bogomolov, Sergiy
  id: 369D9A44-F248-11E8-B48F-1D18A9856A87
  last_name: Bogomolov
  orcid: 0000-0002-0686-0365
- first_name: Marcelo
  full_name: Forets, Marcelo
  last_name: Forets
- first_name: Goran
  full_name: Frehse, Goran
  last_name: Frehse
- first_name: Kostiantyn
  full_name: Potomkin, Kostiantyn
  last_name: Potomkin
- first_name: Christian
  full_name: Schilling, Christian
  id: 3A2F4DCE-F248-11E8-B48F-1D18A9856A87
  last_name: Schilling
  orcid: 0000-0003-3658-1065
citation:
  ama: 'Bogomolov S, Forets M, Frehse G, Potomkin K, Schilling C. JuliaReach: A toolbox
    for set-based reachability. In: <i>Proceedings of the 22nd International Conference
    on Hybrid Systems: Computation and Control</i>. Vol 22. ACM; 2019:39-44. doi:<a
    href="https://doi.org/10.1145/3302504.3311804">10.1145/3302504.3311804</a>'
  apa: 'Bogomolov, S., Forets, M., Frehse, G., Potomkin, K., &#38; Schilling, C. (2019).
    JuliaReach: A toolbox for set-based reachability. In <i>Proceedings of the 22nd
    International Conference on Hybrid Systems: Computation and Control</i> (Vol.
    22, pp. 39–44). Montreal, QC, Canada: ACM. <a href="https://doi.org/10.1145/3302504.3311804">https://doi.org/10.1145/3302504.3311804</a>'
  chicago: 'Bogomolov, Sergiy, Marcelo Forets, Goran Frehse, Kostiantyn Potomkin,
    and Christian Schilling. “JuliaReach: A Toolbox for Set-Based Reachability.” In
    <i>Proceedings of the 22nd International Conference on Hybrid Systems: Computation
    and Control</i>, 22:39–44. ACM, 2019. <a href="https://doi.org/10.1145/3302504.3311804">https://doi.org/10.1145/3302504.3311804</a>.'
  ieee: 'S. Bogomolov, M. Forets, G. Frehse, K. Potomkin, and C. Schilling, “JuliaReach:
    A toolbox for set-based reachability,” in <i>Proceedings of the 22nd International
    Conference on Hybrid Systems: Computation and Control</i>, Montreal, QC, Canada,
    2019, vol. 22, pp. 39–44.'
  ista: 'Bogomolov S, Forets M, Frehse G, Potomkin K, Schilling C. 2019. JuliaReach:
    A toolbox for set-based reachability. Proceedings of the 22nd International Conference
    on Hybrid Systems: Computation and Control. HSCC: Hybrid Systems Computation and
    Control vol. 22, 39–44.'
  mla: 'Bogomolov, Sergiy, et al. “JuliaReach: A Toolbox for Set-Based Reachability.”
    <i>Proceedings of the 22nd International Conference on Hybrid Systems: Computation
    and Control</i>, vol. 22, ACM, 2019, pp. 39–44, doi:<a href="https://doi.org/10.1145/3302504.3311804">10.1145/3302504.3311804</a>.'
  short: 'S. Bogomolov, M. Forets, G. Frehse, K. Potomkin, C. Schilling, in:, Proceedings
    of the 22nd International Conference on Hybrid Systems: Computation and Control,
    ACM, 2019, pp. 39–44.'
conference:
  end_date: 2019-04-18
  location: Montreal, QC, Canada
  name: 'HSCC: Hybrid Systems Computation and Control'
  start_date: 2019-04-16
date_created: 2019-02-18T14:43:28Z
date_published: 2019-04-16T00:00:00Z
date_updated: 2023-08-24T14:47:21Z
day: '16'
ddc:
- '000'
department:
- _id: ToHe
doi: 10.1145/3302504.3311804
ec_funded: 1
external_id:
  arxiv:
  - '1901.10736'
  isi:
  - '000516713900005'
file:
- access_level: open_access
  checksum: 28ed56439aea5991c3122d4730fd828f
  content_type: application/pdf
  creator: cschilli
  date_created: 2019-03-05T09:27:18Z
  date_updated: 2020-07-14T12:47:17Z
  file_id: '6067'
  file_name: hscc19.pdf
  file_size: 3784414
  relation: main_file
file_date_updated: 2020-07-14T12:47:17Z
has_accepted_license: '1'
intvolume: '        22'
isi: 1
keyword:
- reachability analysis
- hybrid systems
- lazy computation
language:
- iso: eng
month: '04'
oa: 1
oa_version: Submitted Version
page: 39-44
project:
- _id: 25F42A32-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: Z211
  name: The Wittgenstein Prize
- _id: 25832EC2-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: S 11407_N23
  name: Rigorous Systems Engineering
- _id: 260C2330-B435-11E9-9278-68D0E5697425
  call_identifier: H2020
  grant_number: '754411'
  name: ISTplus - Postdoctoral Fellowships
publication: 'Proceedings of the 22nd International Conference on Hybrid Systems:
  Computation and Control'
publication_identifier:
  isbn:
  - '9781450362825'
publication_status: published
publisher: ACM
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'JuliaReach: A toolbox for set-based reachability'
type: conference
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
volume: 22
year: '2019'
...
---
_id: '6175'
abstract:
- lang: eng
  text: "We consider the problem of expected cost analysis over nondeterministic probabilistic
    programs,\r\nwhich aims at automated methods for analyzing the resource-usage
    of such programs.\r\nPrevious approaches for this problem could only handle nonnegative
    bounded costs.\r\nHowever, in many scenarios, such as queuing networks or analysis
    of cryptocurrency protocols,\r\nboth positive and negative costs are necessary
    and the costs are unbounded as well.\r\n\r\nIn this work, we present a sound and
    efficient approach to obtain polynomial bounds on the\r\nexpected accumulated
    cost of nondeterministic probabilistic programs.\r\nOur approach can handle (a)
    general positive and negative costs with bounded updates in\r\nvariables; and
    (b) nonnegative costs with general updates to variables.\r\nWe show that several
    natural examples which could not be\r\nhandled by previous approaches are captured
    in our framework.\r\n\r\nMoreover, our approach leads to an efficient polynomial-time
    algorithm, while no\r\nprevious approach for cost analysis of probabilistic programs
    could guarantee polynomial runtime.\r\nFinally, we show the effectiveness of our
    approach using experimental results on a variety of programs for which we efficiently
    synthesize tight resource-usage bounds."
article_processing_charge: No
arxiv: 1
author:
- first_name: Peixin
  full_name: Wang, Peixin
  last_name: Wang
- first_name: Hongfei
  full_name: Fu, Hongfei
  id: 3AAD03D6-F248-11E8-B48F-1D18A9856A87
  last_name: Fu
- first_name: Amir Kafshdar
  full_name: Goharshady, Amir Kafshdar
  id: 391365CE-F248-11E8-B48F-1D18A9856A87
  last_name: Goharshady
  orcid: 0000-0003-1702-6584
- first_name: Krishnendu
  full_name: Chatterjee, Krishnendu
  id: 2E5DCA20-F248-11E8-B48F-1D18A9856A87
  last_name: Chatterjee
  orcid: 0000-0002-4561-241X
- first_name: Xudong
  full_name: Qin, Xudong
  last_name: Qin
- first_name: Wenjun
  full_name: Shi, Wenjun
  last_name: Shi
citation:
  ama: 'Wang P, Fu H, Goharshady AK, Chatterjee K, Qin X, Shi W. Cost analysis of
    nondeterministic probabilistic programs. In: <i>PLDI 2019: Proceedings of the
    40th ACM SIGPLAN Conference on Programming Language Design and Implementation</i>.
    Association for Computing Machinery; 2019:204-220. doi:<a href="https://doi.org/10.1145/3314221.3314581">10.1145/3314221.3314581</a>'
  apa: 'Wang, P., Fu, H., Goharshady, A. K., Chatterjee, K., Qin, X., &#38; Shi, W.
    (2019). Cost analysis of nondeterministic probabilistic programs. In <i>PLDI 2019:
    Proceedings of the 40th ACM SIGPLAN Conference on Programming Language Design
    and Implementation</i> (pp. 204–220). Phoenix, AZ, United States: Association
    for Computing Machinery. <a href="https://doi.org/10.1145/3314221.3314581">https://doi.org/10.1145/3314221.3314581</a>'
  chicago: 'Wang, Peixin, Hongfei Fu, Amir Kafshdar Goharshady, Krishnendu Chatterjee,
    Xudong Qin, and Wenjun Shi. “Cost Analysis of Nondeterministic Probabilistic Programs.”
    In <i>PLDI 2019: Proceedings of the 40th ACM SIGPLAN Conference on Programming
    Language Design and Implementation</i>, 204–20. Association for Computing Machinery,
    2019. <a href="https://doi.org/10.1145/3314221.3314581">https://doi.org/10.1145/3314221.3314581</a>.'
  ieee: 'P. Wang, H. Fu, A. K. Goharshady, K. Chatterjee, X. Qin, and W. Shi, “Cost
    analysis of nondeterministic probabilistic programs,” in <i>PLDI 2019: Proceedings
    of the 40th ACM SIGPLAN Conference on Programming Language Design and Implementation</i>,
    Phoenix, AZ, United States, 2019, pp. 204–220.'
  ista: 'Wang P, Fu H, Goharshady AK, Chatterjee K, Qin X, Shi W. 2019. Cost analysis
    of nondeterministic probabilistic programs. PLDI 2019: Proceedings of the 40th
    ACM SIGPLAN Conference on Programming Language Design and Implementation. PLDI:
    Conference on Programming Language Design and Implementation, 204–220.'
  mla: 'Wang, Peixin, et al. “Cost Analysis of Nondeterministic Probabilistic Programs.”
    <i>PLDI 2019: Proceedings of the 40th ACM SIGPLAN Conference on Programming Language
    Design and Implementation</i>, Association for Computing Machinery, 2019, pp.
    204–20, doi:<a href="https://doi.org/10.1145/3314221.3314581">10.1145/3314221.3314581</a>.'
  short: 'P. Wang, H. Fu, A.K. Goharshady, K. Chatterjee, X. Qin, W. Shi, in:, PLDI
    2019: Proceedings of the 40th ACM SIGPLAN Conference on Programming Language Design
    and Implementation, Association for Computing Machinery, 2019, pp. 204–220.'
conference:
  end_date: 2019-06-26
  location: Phoenix, AZ, United States
  name: 'PLDI: Conference on Programming Language Design and Implementation'
  start_date: 2019-06-22
date_created: 2019-03-25T10:13:25Z
date_published: 2019-06-08T00:00:00Z
date_updated: 2025-06-02T08:53:45Z
day: '08'
ddc:
- '000'
department:
- _id: KrCh
doi: 10.1145/3314221.3314581
ec_funded: 1
external_id:
  arxiv:
  - '1902.04659'
  isi:
  - '000523190300014'
file:
- access_level: open_access
  checksum: 703a5e9b8c8587f2a44085ffd9a4db64
  content_type: application/pdf
  creator: akafshda
  date_created: 2019-03-25T10:11:22Z
  date_updated: 2020-07-14T12:47:20Z
  file_id: '6176'
  file_name: paper.pdf
  file_size: 4051066
  relation: main_file
file_date_updated: 2020-07-14T12:47:20Z
has_accepted_license: '1'
isi: 1
keyword:
- Program Cost Analysis
- Program Termination
- Probabilistic Programs
- Martingales
language:
- iso: eng
month: '06'
oa: 1
oa_version: Submitted Version
page: 204-220
project:
- _id: 25892FC0-B435-11E9-9278-68D0E5697425
  grant_number: ICT15-003
  name: Efficient Algorithms for Computer Aided Verification
- _id: 25863FF4-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: S11407
  name: Game Theory
- _id: 25832EC2-B435-11E9-9278-68D0E5697425
  call_identifier: FWF
  grant_number: S 11407_N23
  name: Rigorous Systems Engineering
- _id: 2581B60A-B435-11E9-9278-68D0E5697425
  call_identifier: FP7
  grant_number: '279307'
  name: 'Quantitative Graph Games: Theory and Applications'
- _id: 266EEEC0-B435-11E9-9278-68D0E5697425
  name: Quantitative Game-theoretic Analysis of Blockchain Applications and Smart
    Contracts
publication: 'PLDI 2019: Proceedings of the 40th ACM SIGPLAN Conference on Programming
  Language Design and Implementation'
publication_status: published
publisher: Association for Computing Machinery
quality_controlled: '1'
related_material:
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  - id: '5457'
    relation: earlier_version
    status: public
  - id: '8934'
    relation: dissertation_contains
    status: public
scopus_import: '1'
status: public
title: Cost analysis of nondeterministic probabilistic programs
type: conference
user_id: 4359f0d1-fa6c-11eb-b949-802e58b17ae8
year: '2019'
...
---
_id: '6473'
abstract:
- lang: eng
  text: "Single cells are constantly interacting with their environment and each other,
    more importantly, the accurate perception of environmental cues is crucial for
    growth, survival, and reproduction. This communication between cells and their
    environment can be formalized in mathematical terms and be quantified as the information
    flow between them, as prescribed by information theory. \r\nThe recent availability
    of real–time dynamical patterns of signaling molecules in single cells has allowed
    us to identify encoding about the identity of the environment in the time–series.
    However, efficient estimation of the information transmitted by these signals
    has been a data–analysis challenge due to the high dimensionality of the trajectories
    and the limited number of samples. In the first part of this thesis, we develop
    and evaluate decoding–based estimation methods to lower bound the mutual information
    and derive model–based precise information estimates for biological reaction networks
    governed by the chemical master equation. This is followed by applying the decoding-based
    methods to study the intracellular representation of extracellular changes in
    budding yeast, by observing the transient dynamics of nuclear translocation of
    10 transcription factors in response to 3 stress conditions. Additionally, we
    apply these estimators to previously published data on ERK and Ca2+ signaling
    and yeast stress response. We argue that this single cell decoding-based measure
    of information provides an unbiased, quantitative and interpretable measure for
    the fidelity of biological signaling processes. \r\nFinally, in the last section,
    we deal with gene regulation which is primarily controlled by transcription factors
    (TFs) that bind to the DNA to activate gene expression. The possibility that non-cognate
    TFs activate transcription diminishes the accuracy of regulation with potentially
    disastrous effects for the cell. This ’crosstalk’ acts as a previously unexplored
    source of noise in biochemical networks and puts a strong constraint on their
    performance. To mitigate erroneous initiation we propose an out of equilibrium
    scheme that implements kinetic proofreading. We show that such architectures are
    favored  over their equilibrium counterparts for complex organisms despite introducing
    noise in gene expression. "
alternative_title:
- ISTA Thesis
article_processing_charge: No
author:
- first_name: Sarah A
  full_name: Cepeda Humerez, Sarah A
  id: 3DEE19A4-F248-11E8-B48F-1D18A9856A87
  last_name: Cepeda Humerez
citation:
  ama: Cepeda Humerez SA. Estimating information flow in single cells. 2019. doi:<a
    href="https://doi.org/10.15479/AT:ISTA:6473">10.15479/AT:ISTA:6473</a>
  apa: Cepeda Humerez, S. A. (2019). <i>Estimating information flow in single cells</i>.
    Institute of Science and Technology Austria. <a href="https://doi.org/10.15479/AT:ISTA:6473">https://doi.org/10.15479/AT:ISTA:6473</a>
  chicago: Cepeda Humerez, Sarah A. “Estimating Information Flow in Single Cells.”
    Institute of Science and Technology Austria, 2019. <a href="https://doi.org/10.15479/AT:ISTA:6473">https://doi.org/10.15479/AT:ISTA:6473</a>.
  ieee: S. A. Cepeda Humerez, “Estimating information flow in single cells,” Institute
    of Science and Technology Austria, 2019.
  ista: Cepeda Humerez SA. 2019. Estimating information flow in single cells. Institute
    of Science and Technology Austria.
  mla: Cepeda Humerez, Sarah A. <i>Estimating Information Flow in Single Cells</i>.
    Institute of Science and Technology Austria, 2019, doi:<a href="https://doi.org/10.15479/AT:ISTA:6473">10.15479/AT:ISTA:6473</a>.
  short: S.A. Cepeda Humerez, Estimating Information Flow in Single Cells, Institute
    of Science and Technology Austria, 2019.
date_created: 2019-05-21T00:11:23Z
date_published: 2019-05-23T00:00:00Z
date_updated: 2025-05-28T11:57:00Z
day: '23'
ddc:
- '004'
degree_awarded: PhD
department:
- _id: GaTk
doi: 10.15479/AT:ISTA:6473
file:
- access_level: closed
  checksum: 75f9184c1346e10a5de5f9cc7338309a
  content_type: application/zip
  creator: scepeda
  date_created: 2019-05-23T11:18:16Z
  date_updated: 2020-07-14T12:47:31Z
  file_id: '6480'
  file_name: Thesis_Cepeda.zip
  file_size: 23937464
  relation: source_file
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  checksum: afdc0633ddbd71d5b13550d7fb4f4454
  content_type: application/pdf
  creator: scepeda
  date_created: 2019-05-23T11:18:13Z
  date_updated: 2020-07-14T12:47:31Z
  file_id: '6481'
  file_name: CepedaThesis.pdf
  file_size: 16646985
  relation: main_file
file_date_updated: 2020-07-14T12:47:31Z
has_accepted_license: '1'
keyword:
- Information estimation
- Time-series
- data analysis
language:
- iso: eng
month: '05'
oa: 1
oa_version: Published Version
page: '135'
publication_identifier:
  issn:
  - 2663-337X
publication_status: published
publisher: Institute of Science and Technology Austria
related_material:
  record:
  - id: '6900'
    relation: dissertation_contains
    status: public
  - id: '281'
    relation: dissertation_contains
    status: public
  - id: '2016'
    relation: dissertation_contains
    status: public
  - id: '1576'
    relation: dissertation_contains
    status: public
status: public
supervisor:
- first_name: Gašper
  full_name: Tkačik, Gašper
  id: 3D494DCA-F248-11E8-B48F-1D18A9856A87
  last_name: Tkačik
  orcid: 0000-0002-6699-1455
title: Estimating information flow in single cells
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: dissertation
user_id: c635000d-4b10-11ee-a964-aac5a93f6ac1
year: '2019'
...
---
_id: '11618'
abstract:
- lang: eng
  text: Asteroseismology provides global stellar parameters such as masses, radii,
    or surface gravities using mean global seismic parameters and effective temperature
    for thousands of low-mass stars (0.8 M⊙ < M < 3 M⊙). This methodology has been
    successfully applied to stars in which acoustic modes excited by turbulent convection
    are measured. Other methods such as the Flicker technique can also be used to
    determine stellar surface gravities, but only works for log g above 2.5 dex. In
    this work, we present a new metric called FliPer (Flicker in spectral power density,
    in opposition to the standard Flicker measurement which is computed in the time
    domain); it is able to extend the range for which reliable surface gravities can
    be obtained (0.1 < log g < 4.6 dex) without performing any seismic analysis for
    stars brighter than Kp < 14. FliPer takes into account the average variability
    of a star measured in the power density spectrum in a given range of frequencies.
    However, FliPer values calculated on several ranges of frequency are required
    to better characterize a star. Using a large set of asteroseismic targets it is
    possible to calibrate the behavior of surface gravity with FliPer through machine
    learning. This calibration made with a random forest regressor covers a wide range
    of surface gravities from main-sequence stars to subgiants and red giants, with
    very small uncertainties from 0.04 to 0.1 dex. FliPer values can be inserted in
    automatic global seismic pipelines to either give an estimation of the stellar
    surface gravity or to assess the quality of the seismic results by detecting any
    outliers in the obtained νmax values. FliPer also constrains the surface gravities
    of main-sequence dwarfs using only long-cadence data for which the Nyquist frequency
    is too low to measure the acoustic-mode properties.
acknowledgement: We thank the anonymous referee for the very useful comments. We would
  also like to thank M. Benbakoura for his help in analyzing the light curves of several
  binary systems included in our set of stars. L.B. and R.A.G. acknowledge the support
  from PLATO and GOLF CNES grants. S.M. acknowledges support from the National Aeronautics
  and Space Administration under Grant NNX15AF13G, the National Science Foundation
  grant AST-1411685, and the Ramon y Cajal fellowship no. RYC-2015-17697. E.C. is
  funded by the European Union’s Horizon 2020 research and innovation program under
  the Marie Sklodowska-Curie grant agreement no. 664931. O.J.H and B.M.R. acknowledge
  the support of the UK Science and Technology Facilities Council (STFC). Funding
  for the Stellar Astrophysics Centre is provided by the Danish National Research
  Foundation (Grant DNRF106). This research has made use of NASA’s Astrophysics Data
  System. Data presented in this paper were obtained from the Mikulski Archive for
  Space Telescopes (MAST). STScI is operated by the Association of Universities for
  Research in Astronomy, Inc., under NASA contract NAS5-26555.
article_number: A38
article_processing_charge: No
article_type: original
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: García, R. A.
  last_name: García
- 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
- first_name: O. J.
  full_name: Hall, O. J.
  last_name: Hall
- first_name: B. M.
  full_name: Rendle, B. M.
  last_name: Rendle
citation:
  ama: 'Bugnet LA, García RA, Davies GR, et al. FliPer: A global measure of power
    density to estimate surface gravities of main-sequence solar-like stars and red
    giants. <i>Astronomy &#38; Astrophysics</i>. 2018;620. doi:<a href="https://doi.org/10.1051/0004-6361/201833106">10.1051/0004-6361/201833106</a>'
  apa: 'Bugnet, L. A., García, R. A., Davies, G. R., Mathur, S., Corsaro, E., Hall,
    O. J., &#38; Rendle, B. M. (2018). FliPer: A global measure of power density to
    estimate surface gravities of main-sequence solar-like stars and red giants. <i>Astronomy
    &#38; Astrophysics</i>. EDP Sciences. <a href="https://doi.org/10.1051/0004-6361/201833106">https://doi.org/10.1051/0004-6361/201833106</a>'
  chicago: 'Bugnet, Lisa Annabelle, R. A. García, G. R. Davies, S. Mathur, E. Corsaro,
    O. J. Hall, and B. M. Rendle. “FliPer: A Global Measure of Power Density to Estimate
    Surface Gravities of Main-Sequence Solar-like Stars and Red Giants.” <i>Astronomy
    &#38; Astrophysics</i>. EDP Sciences, 2018. <a href="https://doi.org/10.1051/0004-6361/201833106">https://doi.org/10.1051/0004-6361/201833106</a>.'
  ieee: 'L. A. Bugnet <i>et al.</i>, “FliPer: A global measure of power density to
    estimate surface gravities of main-sequence solar-like stars and red giants,”
    <i>Astronomy &#38; Astrophysics</i>, vol. 620. EDP Sciences, 2018.'
  ista: 'Bugnet LA, García RA, Davies GR, Mathur S, Corsaro E, Hall OJ, Rendle BM.
    2018. FliPer: A global measure of power density to estimate surface gravities
    of main-sequence solar-like stars and red giants. Astronomy &#38; Astrophysics.
    620, A38.'
  mla: 'Bugnet, Lisa Annabelle, et al. “FliPer: A Global Measure of Power Density
    to Estimate Surface Gravities of Main-Sequence Solar-like Stars and Red Giants.”
    <i>Astronomy &#38; Astrophysics</i>, vol. 620, A38, EDP Sciences, 2018, doi:<a
    href="https://doi.org/10.1051/0004-6361/201833106">10.1051/0004-6361/201833106</a>.'
  short: L.A. Bugnet, R.A. García, G.R. Davies, S. Mathur, E. Corsaro, O.J. Hall,
    B.M. Rendle, Astronomy &#38; Astrophysics 620 (2018).
date_created: 2022-07-18T14:37:39Z
date_published: 2018-12-01T00:00:00Z
date_updated: 2022-08-22T07:41:07Z
day: '01'
doi: 10.1051/0004-6361/201833106
extern: '1'
external_id:
  arxiv:
  - '1809.05105'
intvolume: '       620'
keyword:
- Space and Planetary Science
- Astronomy and Astrophysics
- asteroseismology / methods
- data analysis / stars
- oscillations
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1809.05105
month: '12'
oa: 1
oa_version: Preprint
publication: Astronomy & Astrophysics
publication_identifier:
  eissn:
  - 1432-0746
  issn:
  - 0004-6361
publication_status: published
publisher: EDP Sciences
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'FliPer: A global measure of power density to estimate surface gravities of
  main-sequence solar-like stars and red giants'
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 620
year: '2018'
...
---
_id: '11631'
abstract:
- lang: eng
  text: "The recently launched NASA Transiting Exoplanet Survey Satellite (TESS) mission
    is going to collect lightcurves for a few hundred million of stars and we expect
    to increase the number of pulsating stars to analyze compared to the few thousand
    stars observed by the CoRoT, Kepler and K2 missions. However, most of the TESS
    targets have not yet been properly classified and characterized. In order to improve
    the analysis of the TESS data, it is crucial to determine the type of stellar
    pulsations in a timely manner. We propose an automatic method to classify stars
    attending to their pulsation properties, in particular, to identify solar-like
    pulsators among all TESS targets. It relies on the use of the global amount of
    power contained in the power spectrum (already known as the FliPer method) as
    a key parameter, along with\r\nthe effective temperature, to feed into a machine
    learning classifier. Our study, based on TESS simulated datasets, shows that we
    are able to classify pulsators with a 98% accuracy."
article_number: '1811.12140'
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: García, R. A.
  last_name: García
- first_name: G. R.
  full_name: Davies, G. R.
  last_name: Davies
- first_name: S.
  full_name: Mathur, S.
  last_name: Mathur
- first_name: O. J.
  full_name: Hall, O. J.
  last_name: Hall
- first_name: B. M.
  full_name: Rendle, B. M.
  last_name: Rendle
citation:
  ama: 'Bugnet LA, García RA, Davies GR, Mathur S, Hall OJ, Rendle BM. FliPer: Classifying
    TESS pulsating stars. <i>arXiv</i>. doi:<a href="https://doi.org/10.48550/arXiv.1811.12140">10.48550/arXiv.1811.12140</a>'
  apa: 'Bugnet, L. A., García, R. A., Davies, G. R., Mathur, S., Hall, O. J., &#38;
    Rendle, B. M. (n.d.). FliPer: Classifying TESS pulsating stars. <i>arXiv</i>.
    <a href="https://doi.org/10.48550/arXiv.1811.12140">https://doi.org/10.48550/arXiv.1811.12140</a>'
  chicago: 'Bugnet, Lisa Annabelle, R. A. García, G. R. Davies, S. Mathur, O. J. Hall,
    and B. M. Rendle. “FliPer: Classifying TESS Pulsating Stars.” <i>ArXiv</i>, n.d.
    <a href="https://doi.org/10.48550/arXiv.1811.12140">https://doi.org/10.48550/arXiv.1811.12140</a>.'
  ieee: 'L. A. Bugnet, R. A. García, G. R. Davies, S. Mathur, O. J. Hall, and B. M.
    Rendle, “FliPer: Classifying TESS pulsating stars,” <i>arXiv</i>. .'
  ista: 'Bugnet LA, García RA, Davies GR, Mathur S, Hall OJ, Rendle BM. FliPer: Classifying
    TESS pulsating stars. arXiv, 1811.12140.'
  mla: 'Bugnet, Lisa Annabelle, et al. “FliPer: Classifying TESS Pulsating Stars.”
    <i>ArXiv</i>, 1811.12140, doi:<a href="https://doi.org/10.48550/arXiv.1811.12140">10.48550/arXiv.1811.12140</a>.'
  short: L.A. Bugnet, R.A. García, G.R. Davies, S. Mathur, O.J. Hall, B.M. Rendle,
    ArXiv (n.d.).
date_created: 2022-07-21T07:05:23Z
date_published: 2018-11-29T00:00:00Z
date_updated: 2022-08-22T08:41:55Z
day: '29'
doi: 10.48550/arXiv.1811.12140
extern: '1'
external_id:
  arxiv:
  - '1811.12140'
keyword:
- asteroseismology - methods
- data analysis - stars
- oscillations
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: ' https://doi.org/10.48550/arXiv.1811.12140'
month: '11'
oa: 1
oa_version: Preprint
publication: arXiv
publication_status: submitted
status: public
title: 'FliPer: Classifying TESS pulsating stars'
type: preprint
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2018'
...
---
_id: '8422'
abstract:
- lang: eng
  text: 'The Birkhoff conjecture says that the boundary of a strictly convex integrable
    billiard table is necessarily an ellipse. In this article, we consider a stronger
    notion of integrability, namely integrability close to the boundary, and prove
    a local version of this conjecture: a small perturbation of an ellipse of small
    eccentricity which preserves integrability near the boundary, is itself an ellipse.
    This extends the result in Avila et al. (Ann Math 184:527–558, ADK16), where integrability
    was assumed on a larger set. In particular, it shows that (local) integrability
    near the boundary implies global integrability. One of the crucial ideas in the
    proof consists in analyzing Taylor expansion of the corresponding action-angle
    coordinates with respect to the eccentricity parameter, deriving and studying
    higher order conditions for the preservation of integrable rational caustics.'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Guan
  full_name: Huang, Guan
  last_name: Huang
- first_name: Vadim
  full_name: Kaloshin, Vadim
  id: FE553552-CDE8-11E9-B324-C0EBE5697425
  last_name: Kaloshin
  orcid: 0000-0002-6051-2628
- first_name: Alfonso
  full_name: Sorrentino, Alfonso
  last_name: Sorrentino
citation:
  ama: Huang G, Kaloshin V, Sorrentino A. Nearly circular domains which are integrable
    close to the boundary are ellipses. <i>Geometric and Functional Analysis</i>.
    2018;28(2):334-392. doi:<a href="https://doi.org/10.1007/s00039-018-0440-4">10.1007/s00039-018-0440-4</a>
  apa: Huang, G., Kaloshin, V., &#38; Sorrentino, A. (2018). Nearly circular domains
    which are integrable close to the boundary are ellipses. <i>Geometric and Functional
    Analysis</i>. Springer Nature. <a href="https://doi.org/10.1007/s00039-018-0440-4">https://doi.org/10.1007/s00039-018-0440-4</a>
  chicago: Huang, Guan, Vadim Kaloshin, and Alfonso Sorrentino. “Nearly Circular Domains
    Which Are Integrable Close to the Boundary Are Ellipses.” <i>Geometric and Functional
    Analysis</i>. Springer Nature, 2018. <a href="https://doi.org/10.1007/s00039-018-0440-4">https://doi.org/10.1007/s00039-018-0440-4</a>.
  ieee: G. Huang, V. Kaloshin, and A. Sorrentino, “Nearly circular domains which are
    integrable close to the boundary are ellipses,” <i>Geometric and Functional Analysis</i>,
    vol. 28, no. 2. Springer Nature, pp. 334–392, 2018.
  ista: Huang G, Kaloshin V, Sorrentino A. 2018. Nearly circular domains which are
    integrable close to the boundary are ellipses. Geometric and Functional Analysis.
    28(2), 334–392.
  mla: Huang, Guan, et al. “Nearly Circular Domains Which Are Integrable Close to
    the Boundary Are Ellipses.” <i>Geometric and Functional Analysis</i>, vol. 28,
    no. 2, Springer Nature, 2018, pp. 334–92, doi:<a href="https://doi.org/10.1007/s00039-018-0440-4">10.1007/s00039-018-0440-4</a>.
  short: G. Huang, V. Kaloshin, A. Sorrentino, Geometric and Functional Analysis 28
    (2018) 334–392.
date_created: 2020-09-17T10:42:30Z
date_published: 2018-03-18T00:00:00Z
date_updated: 2021-01-12T08:19:11Z
day: '18'
doi: 10.1007/s00039-018-0440-4
extern: '1'
external_id:
  arxiv:
  - '1705.10601'
intvolume: '        28'
issue: '2'
keyword:
- Geometry and Topology
- Analysis
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: https://arxiv.org/abs/1705.10601
month: '03'
oa: 1
oa_version: Preprint
page: 334-392
publication: Geometric and Functional Analysis
publication_identifier:
  issn:
  - 1016-443X
  - 1420-8970
publication_status: published
publisher: Springer Nature
quality_controlled: '1'
status: public
title: Nearly circular domains which are integrable close to the boundary are ellipses
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 28
year: '2018'
...
---
_id: '5574'
abstract:
- lang: ger
  text: 'Comparison of Scopus'' and publisher''s data on Austrian publication output
    at IOP. '
article_processing_charge: No
author:
- first_name: Márton
  full_name: Villányi, Márton
  id: 3FFCCD3A-F248-11E8-B48F-1D18A9856A87
  last_name: Villányi
  orcid: 0000-0001-8126-0426
citation:
  ama: Villányi M. Data Check IOP Scopus vs. Publisher. 2018. doi:<a href="https://doi.org/10.15479/AT:ISTA:86">10.15479/AT:ISTA:86</a>
  apa: Villányi, M. (2018). Data Check IOP Scopus vs. Publisher. Institute of Science
    and Technology Austria. <a href="https://doi.org/10.15479/AT:ISTA:86">https://doi.org/10.15479/AT:ISTA:86</a>
  chicago: Villányi, Márton. “Data Check IOP Scopus vs. Publisher.” Institute of Science
    and Technology Austria, 2018. <a href="https://doi.org/10.15479/AT:ISTA:86">https://doi.org/10.15479/AT:ISTA:86</a>.
  ieee: M. Villányi, “Data Check IOP Scopus vs. Publisher.” Institute of Science and
    Technology Austria, 2018.
  ista: Villányi M. 2018. Data Check IOP Scopus vs. Publisher, Institute of Science
    and Technology Austria, <a href="https://doi.org/10.15479/AT:ISTA:86">10.15479/AT:ISTA:86</a>.
  mla: Villányi, Márton. <i>Data Check IOP Scopus vs. Publisher</i>. Institute of
    Science and Technology Austria, 2018, doi:<a href="https://doi.org/10.15479/AT:ISTA:86">10.15479/AT:ISTA:86</a>.
  short: M. Villányi, (2018).
datarep_id: '86'
date_created: 2018-12-12T12:31:37Z
date_published: 2018-01-16T00:00:00Z
date_updated: 2024-02-21T13:42:21Z
day: '16'
ddc:
- '020'
department:
- _id: E-Lib
doi: 10.15479/AT:ISTA:86
file:
- access_level: open_access
  checksum: c7a61147bd15cb4ae45878d270628c06
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  creator: system
  date_created: 2018-12-12T13:05:14Z
  date_updated: 2020-07-14T12:47:05Z
  file_id: '5642'
  file_name: IST-2018-86-v1+1_Data_Check_IOP_Scopus_vs._Publisher.zip
  file_size: 12283857
  relation: main_file
file_date_updated: 2020-07-14T12:47:05Z
has_accepted_license: '1'
keyword:
- Publication analysis
- Bibliography
- Open Access
license: https://creativecommons.org/publicdomain/zero/1.0/
month: '01'
oa: 1
oa_version: Submitted Version
publisher: Institute of Science and Technology Austria
related_material:
  record:
  - id: '278'
    relation: part_of_dissertation
    status: public
status: public
title: Data Check IOP Scopus vs. Publisher
tmp:
  image: /images/cc_0.png
  legal_code_url: https://creativecommons.org/publicdomain/zero/1.0/legalcode
  name: Creative Commons Public Domain Dedication (CC0 1.0)
  short: CC0 (1.0)
type: research_data
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2018'
...
---
_id: '5575'
abstract:
- lang: ger
  text: 'Comparison of Scopus'' and FWF''s data on Austrian publication output at
    RSC. '
article_processing_charge: No
author:
- first_name: Márton
  full_name: Villányi, Márton
  id: 3FFCCD3A-F248-11E8-B48F-1D18A9856A87
  last_name: Villányi
  orcid: 0000-0001-8126-0426
citation:
  ama: Villányi M. Data Check RSC Scopus vs. FWF. 2018. doi:<a href="https://doi.org/10.15479/AT:ISTA:87">10.15479/AT:ISTA:87</a>
  apa: Villányi, M. (2018). Data Check RSC Scopus vs. FWF. Institute of Science and
    Technology Austria. <a href="https://doi.org/10.15479/AT:ISTA:87">https://doi.org/10.15479/AT:ISTA:87</a>
  chicago: Villányi, Márton. “Data Check RSC Scopus vs. FWF.” Institute of Science
    and Technology Austria, 2018. <a href="https://doi.org/10.15479/AT:ISTA:87">https://doi.org/10.15479/AT:ISTA:87</a>.
  ieee: M. Villányi, “Data Check RSC Scopus vs. FWF.” Institute of Science and Technology
    Austria, 2018.
  ista: Villányi M. 2018. Data Check RSC Scopus vs. FWF, Institute of Science and
    Technology Austria, <a href="https://doi.org/10.15479/AT:ISTA:87">10.15479/AT:ISTA:87</a>.
  mla: Villányi, Márton. <i>Data Check RSC Scopus vs. FWF</i>. Institute of Science
    and Technology Austria, 2018, doi:<a href="https://doi.org/10.15479/AT:ISTA:87">10.15479/AT:ISTA:87</a>.
  short: M. Villányi, (2018).
datarep_id: '87'
date_created: 2018-12-12T12:31:37Z
date_published: 2018-01-16T00:00:00Z
date_updated: 2024-02-21T13:43:25Z
day: '16'
ddc:
- '020'
department:
- _id: E-Lib
doi: 10.15479/AT:ISTA:87
file:
- access_level: open_access
  checksum: 563cc5266c0bac354007873c92be777b
  content_type: application/zip
  creator: system
  date_created: 2018-12-12T13:02:44Z
  date_updated: 2020-07-14T12:47:05Z
  file_id: '5610'
  file_name: IST-2018-87-v1+1_Data_Check_RSC_Scopus_vs._FWF.zip
  file_size: 277078
  relation: main_file
file_date_updated: 2020-07-14T12:47:05Z
has_accepted_license: '1'
keyword:
- Publication analysis
- Bibliography
- Open Access
month: '01'
oa: 1
oa_version: Submitted Version
publisher: Institute of Science and Technology Austria
related_material:
  record:
  - id: '278'
    relation: part_of_dissertation
    status: public
status: public
title: Data Check RSC Scopus vs. FWF
tmp:
  image: /images/cc_0.png
  legal_code_url: https://creativecommons.org/publicdomain/zero/1.0/legalcode
  name: Creative Commons Public Domain Dedication (CC0 1.0)
  short: CC0 (1.0)
type: research_data
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
year: '2018'
...
---
_id: '5576'
abstract:
- lang: ger
  text: Comparison of Scopus' and FWF's data on Austrian publication output at T&F.
article_processing_charge: No
author:
- first_name: Márton
  full_name: Villányi, Márton
  id: 3FFCCD3A-F248-11E8-B48F-1D18A9856A87
  last_name: Villányi
  orcid: 0000-0001-8126-0426
citation:
  ama: Villányi M. Data Check T&#38;F Scopus vs. FWF. 2018. doi:<a href="https://doi.org/10.15479/AT:ISTA:88">10.15479/AT:ISTA:88</a>
  apa: Villányi, M. (2018). Data Check T&#38;F Scopus vs. FWF. Institute of Science
    and Technology Austria. <a href="https://doi.org/10.15479/AT:ISTA:88">https://doi.org/10.15479/AT:ISTA:88</a>
  chicago: Villányi, Márton. “Data Check T&#38;F Scopus vs. FWF.” Institute of Science
    and Technology Austria, 2018. <a href="https://doi.org/10.15479/AT:ISTA:88">https://doi.org/10.15479/AT:ISTA:88</a>.
  ieee: M. Villányi, “Data Check T&#38;F Scopus vs. FWF.” Institute of Science and
    Technology Austria, 2018.
  ista: Villányi M. 2018. Data Check T&#38;F Scopus vs. FWF, Institute of Science
    and Technology Austria, <a href="https://doi.org/10.15479/AT:ISTA:88">10.15479/AT:ISTA:88</a>.
  mla: Villányi, Márton. <i>Data Check T&#38;F Scopus vs. FWF</i>. Institute of Science
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  short: M. Villányi, (2018).
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  text: Data on Austrian open access publication output at Emerald from 2013-2017
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  apa: Villányi, M. (2018). Emerald Austrian Publications 2013-2017. Institute of
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  ieee: M. Villányi, “Emerald Austrian Publications 2013-2017.” Institute of Science
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  ista: Villányi M. 2018. Emerald Austrian Publications 2013-2017, Institute of Science
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  mla: Villányi, Márton. <i>Emerald Austrian Publications 2013-2017</i>. Institute
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  short: M. Villányi, (2018).
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  text: Data on Austrian open access publication output at IOP from 2012-2015 including
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  short: M. Villányi, (2018).
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  text: Data on Austrian open access publication output at RSC from 2013-2017 including
    data analysis.
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  full_name: Villányi, Márton
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  text: Data on Austrian open access publication output at SAGE from 2013-2017 including
    data analysis.
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  full_name: Villányi, Márton
  id: 3FFCCD3A-F248-11E8-B48F-1D18A9856A87
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  ista: Villányi M. 2018. SAGE Austrian Publications 2013-2017, Institute of Science
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  text: Data on Austrian open access publication output at Springer from 2013-2016
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  full_name: Villányi, Márton
  id: 3FFCCD3A-F248-11E8-B48F-1D18A9856A87
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  chicago: Villányi, Márton. “Springer Austrian Publications 2013-2016.” Institute
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  ista: Villányi M. 2018. Springer Austrian Publications 2013-2016, Institute of Science
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