Spectroscopy and photometry of HATS-17 Virtual Observatory Resource

Authors

1. Brahm R.
2. Jordan A.
3. Bakos G.A.
4. Penev K.
5. Espinoza N.
6. Rabus M.,Hartman J.D.
7. Bayliss D.
8. Ciceri S.
9. Zhou G.
10. Mancini L.
11. Tan T.G.,De Val-Borro M.
12. Bhatti W.
13. Csubry Z.
14. Bento J.
15. Henning T.
16. Schmidt B.,Rojas F.
17. Suc V.
18. Lazar J.
19. Papp I.
20. Sari P.

Published by

CDS

Abstract

We report the discovery of HATS-17b, the first transiting warm Jupiter of the HATSouth network. HATS-17b transits its bright (V=12.4) G-type (M_{star}_=1.131+/-0.030M_{sun}_, R_{star}_=1.090_-0.046_^+0.070^) metal-rich ([Fe/H]=+0.3dex) host star in a circular orbit with a period of P=16.2546days. HATS-17b has a very compact radius of 0.777+/-0.056R_J_ given its Jupiter-like mass of 1.338+/-0.065M_J_. Up to 50% of the mass of HATS-17b may be composed of heavy elements in order to explain its high density with current models of planetary structure. HATS-17b is the longest period transiting planet discovered to date by a ground-based photometric survey, and is one of the brightest transiting warm Jupiter systems known. The brightness of HATS-17 will allow detailed follow-up observations to characterize the orbital geometry of the system and the atmosphere of the planet.

Keywords

1. Multiple stars
2. G stars
3. Solar system planets
4. Radial velocity
5. Photometry

Bibliographic source Bibcode

2016AJ....151...89B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/151/89

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/151/89

Document Object Identifer DOI

doi:10.26093/cds/vizier.51510089

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/151/89
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/151/89
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/151/89

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).