2019PASP..131c4501Z


Query : 2019PASP..131c4501Z

2019PASP..131c4501Z - Publ. Astron. Soc. Pac., 131, part no 3, 4501-34501 (2019/March-0)

Forward modeling and retrievals with PLATON, a fast open-source tool.

ZHANG M., CHACHAN Y., KEMPTON E.M.-R. and KNUTSON H.A.

Abstract (from CDS):

We introduce PLanetary Atmospheric Transmission for Observer Noobs (PLATON), a Python package that calculates transmission spectra for exoplanets and retrieves atmospheric characteristics based on observed spectra. PLATON is easy to install and use, with common use cases taking no more than a few lines of code. It is also fast, with the forward model taking much less than one second, and a typical retrieval finishing in minutes on an ordinary desktop. PLATON supports the most common atmospheric parameters, such as temperature, metallicity, C/O ratio, cloud-top pressure, and scattering slope. It also has less commonly included features, such as a Mie scattering cloud model and unocculted starspot corrections. The code is available online at https://github.com/ideasrule/platon under the open-source GPL-3.0 license.

Abstract Copyright: © 2019. The Astronomical Society of the Pacific. All rights reserved.

Journal keyword(s):

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 HAT-P-26b Pl 14 12 37.5331103311 +04 03 36.116569918           ~ 200 1
2 WASP-39b Pl 14 29 18.4151689656 -03 26 40.204480380           ~ 345 1
3 HD 209458b Pl 22 03 10.7727465312 +18 53 03.549393384           ~ 2037 1

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