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CITATION.txt
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Citation
========
Hannah Wakeford, & David Grant. (2022). Exo-TiC/ExoTiC-LD: ExoTiC-LD v2.1 Zenodo Release (v2.1.0). Zenodo. https://doi.org/10.5281/zenodo.6809899
**Additional notes:**
ExoTic-LD was developed and packaged from ExoTiC-ISM (Laginja and Wakeford, 2020 [1]) \citep{Laginja2020}.
If you used ExoTiC-LD in your work, if appropriate please additionally cite the software paper Laginja
and Wakeford, 2020 [1] and the software version [2].
"This research made use of packages associated with the software package
ExoTiC-ISM \citep{Laginja2020}"
To cite the scientific methods, please cite Claret et al. 2000 [3], Sing et al. 2010 [4].
If you make use of the 3D stellar models please cite Magic et al. 2015 [5]
We provide the following LaTeX/BibTeX acknowledgment if there is no specific place to cite the above:
[1] Laginja and Wakeford 2020, software paper
@article{Laginja2020,
doi = {10.21105/joss.02281},
url = {https://doi.org/10.21105/joss.02281},
year = {2020},
publisher = {The Open Journal},
volume = {5},
number = {51},
pages = {2281},
author = {Iva Laginja and Hannah R. Wakeford},
title = {{ExoTiC-ISM}: A {P}ython package for marginalised exoplanet transit parameters across a grid of systematic instrument models},
journal = {Journal of Open Source Software}
}
[2] Software version
@software{iva_laginja_2020_3923986,
author = {Iva Laginja and
Hannah R. Wakeford},
title = {ExoTiC-ISM v2.0.0},
month = jun,
year = 2020,
publisher = {Zenodo},
version = {v2.0.0},
doi = {10.5281/zenodo.3923986},
url = {https://doi.org/10.5281/zenodo.3923986}
}
[3] Claret (2000) - Limb-darkening laws
@article{claret2000,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...363.1081C},
author = {{Claret}, A.},
date-added = {2015-02-18 15:55:15 +0000},
date-modified = {2015-02-18 15:55:26 +0000},
journal = {\aap},
keywords = {STARS: ATMOSPHERES, STARS: BINARIES: ECLIPSING},
month = nov,
pages = {1081-1190},
title = {{A new non-linear limb-darkening law for LTE stellar atmosphere models. Calculations for -5.0 {\lt}= log[M/H] {\lt}= +1, 2000 K {\lt}= T$_{eff}$ {\lt}= 50000 K at several surface gravities}},
volume = 363,
year = 2000}
[4] Sing (2010) - Limb-darkening coefficients
@article{sing2010,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...510A..21S},
archiveprefix = {arXiv},
author = {{Sing}, D.~K.},
date-added = {2013-04-25 14:25:26 +0000},
date-modified = {2013-04-25 14:25:26 +0000},
doi = {10.1051/0004-6361/200913675},
eid = {A21},
eprint = {0912.2274},
journal = {\aap},
keywords = {stars: atmospheres, planetary systems, binaries: eclipsing},
month = feb,
pages = {A21},
primaryclass = {astro-ph.EP},
title = {{Stellar limb-darkening coefficients for CoRot and Kepler}},
volume = 510,
year = 2010,
Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/200913675}}
[5] Magic et al. (2015) - 3D stellar model grid
@article{Magic2015,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2015A%26A...573A..90M},
archiveprefix = {arXiv},
author = {{Magic}, Z. and {Chiavassa}, A. and {Collet}, R. and {Asplund}, M.},
date-added = {2018-05-14 19:27:43 +0000},
date-modified = {2018-05-14 19:27:49 +0000},
doi = {10.1051/0004-6361/201423804},
eid = {A90},
eprint = {1403.3487},
journal = {\aap},
keywords = {convection, hydrodynamics, radiative transfer, stars: atmospheres, binaries: eclipsing, planetary systems},
month = jan,
pages = {A90},
primaryclass = {astro-ph.SR},
title = {{The Stagger-grid: A grid of 3D stellar atmosphere models. IV. Limb darkening coefficients}},
volume = 573,
year = 2015,
Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201423804}}