Consequences of parameterization choice on eclipsing binary light curve solutions
(2021) In Contributions of the Astronomical Observatory Skalnate Pleso 51(1). p.58-67- Abstract
Eclipsing Binaries (EBs) are known to be the source of most ac- curate stellar parameters, which are important for testing theories of stellar evolution. With improved quality and quantity of observations using space tele- scopes like TESS, there is an urgent need for accuracy in modeling to obtain precise parameters. We use the soon to be released PHOEBE 2.3 EB modeling package to test the robustness and accuracy of parameters and their depen- dency on choice of parameters for optimization.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/318d5c80-f915-4bed-a481-8cf64f3849f8
- author
- Korth, J. LU ; Moharana, A. ; Pesta, M. ; Czavalinga, D. R. and Conroy, K. E.
- publishing date
- 2021
- type
- Contribution to journal
- publication status
- published
- keywords
- binaries, eclipsing, fundamental parameters, methods, numerical, stars, Stars
- in
- Contributions of the Astronomical Observatory Skalnate Pleso
- volume
- 51
- issue
- 1
- pages
- 10 pages
- publisher
- Astronomický ústav SAV
- external identifiers
-
- scopus:85101076518
- ISSN
- 1335-1842
- DOI
- 10.31577/caosp.2021.51.1.58
- language
- English
- LU publication?
- no
- additional info
- Funding Information: The work presented here was part of the GATE Summer School, hosted (virtually) by Masaryk University Brno and sponsored by ERASMUS+ under grant number 2017-1-CZ01-KA203-035562. The authors would like to thank all involved and Marek Skarka for his organization. A.M. would like to acknowledge the support provided by the Polish National Science Center (NCN) through the grant number 2017/27/B/ST9/02727. Publisher Copyright: © 2021. All Rights Reserved.
- id
- 318d5c80-f915-4bed-a481-8cf64f3849f8
- date added to LUP
- 2023-02-01 10:30:52
- date last changed
- 2023-02-14 16:38:55
@article{318d5c80-f915-4bed-a481-8cf64f3849f8, abstract = {{<p>Eclipsing Binaries (EBs) are known to be the source of most ac- curate stellar parameters, which are important for testing theories of stellar evolution. With improved quality and quantity of observations using space tele- scopes like TESS, there is an urgent need for accuracy in modeling to obtain precise parameters. We use the soon to be released PHOEBE 2.3 EB modeling package to test the robustness and accuracy of parameters and their depen- dency on choice of parameters for optimization.</p>}}, author = {{Korth, J. and Moharana, A. and Pesta, M. and Czavalinga, D. R. and Conroy, K. E.}}, issn = {{1335-1842}}, keywords = {{binaries; eclipsing; fundamental parameters; methods; numerical; stars; Stars}}, language = {{eng}}, number = {{1}}, pages = {{58--67}}, publisher = {{Astronomický ústav SAV}}, series = {{Contributions of the Astronomical Observatory Skalnate Pleso}}, title = {{Consequences of parameterization choice on eclipsing binary light curve solutions}}, url = {{http://dx.doi.org/10.31577/caosp.2021.51.1.58}}, doi = {{10.31577/caosp.2021.51.1.58}}, volume = {{51}}, year = {{2021}}, }