Sloan i-band light curve of HAT-P-24 Virtual Observatory Resource

Authors

1. Kipping D.M.
2. Bakos G.A.
3. Hartman J.
4. Torres G.
5. Shporer A.
6. Latham D.W.,Kovacs G.
7. Noyes R.W.
8. Howard A.W.
9. Fischer D.A.
10. Johnson J.A.
11. Marcy G.W.,Beky B.
12. Perumpilly G.
13. Esquerdo G.A.
14. Sasselov D.D.
15. Stefanik R.P.,Lazar J.
16. Papp I.
17. Sari P.

Published by

CDS

Abstract

We report the discovery of HAT-P-24b, a transiting extrasolar planet orbiting the moderately bright V=11.818 F8 dwarf star GSC 0774-01441, with a period P=3.3552464+/-0.0000071 days, transit epoch T_c_=2455216.97669+/-0.00024(BJD), and transit duration 3.653+/-0.025hr. The host star has a mass of 1.191+/-0.042M_{sun}_, radius of 1.317+/-0.068R_{sun}_, effective temperature 6373+/-80K, and a low metallicity of [Fe/H]=-0.16+/-0.08. The planetary companion has a mass of 0.681+/-0.031M_J_ and radius of 1.243+/-0.072R_J_ yielding a mean density of 0.439+/-0.069g/cm^3^. By repeating our global fits with different parameter sets, we have performed a critical investigation of the fitting techniques used for previous Hungarian-made Automated Telescope planetary discoveries. We find that the system properties are robust against the choice of priors.

Keywords

1. photometry
2. solar-system-planets
3. multiple-stars
4. f-stars

Bibliographic source Bibcode

2010ApJ...725.2017K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/725/2017

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJ/725/2017

Document Object Identifer DOI

doi:10.26093/cds/vizier.17252017

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/725/2017
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/725/2017
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/725/2017

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
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