HAT-P-32b differential photometry time series Virtual Observatory Resource

Authors

1. Mallonn M.
2. Koehler J.
3. Alexoudi X.
4. von Essen C.
5. Granzer T.,Poppenhaeger K.
6. Strassmeier K.G.

Published by

CDS

Abstract

We obtained 11 photometric time series of secondary eclipse events of the hot Jupiter HAT-P-32b in the Sloan z' band. We inferred the eclipse depth and employed this value to derive an upper limit on the planetary geometric albedo.

Keywords

1. Multiple stars
2. Exoplanets
3. Photometry

Bibliographic source Bibcode

2019A&A...624A..62M

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/624/A62

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/624/A62

Document Object Identifer DOI

doi:10.26093/cds/vizier.36240062

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/624/A62
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/624/A62
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/624/A62

IVOA Table Access TAP

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