Transit of TrES-1 Virtual Observatory Resource

Authors
  1. Winn J.N.
  2. Holman M.J.
  3. Roussanova A.
  4. Published by
    CDS
Abstract

We present z-band photometry of three consecutive transits of the exoplanet TrES-1, with an accuracy of 0.15% and a cadence of 40s. We improve on estimates of the system parameters, finding in particular that the planetary radius is 1.081+/-0.029R_Jup_ and the stellar radius is 0.011+/-0.020R_{sun}_. The uncertainties include both the statistical error and the systematic error arising from the uncertainty in the stellar mass. The transit times are determined to within about 15s and allow us to refine the estimate of the mean orbital period: P=3.0300737+/-0.0000026days. We find no evidence for starspots or other irregularities that have been previously reported.

Keywords
  1. multiple-stars
  2. solar-system-planets
Bibliographic source Bibcode
2007ApJ...657.1098W
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/657/1098
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/657/1098
Document Object Identifer DOI
doi:10.26093/cds/vizier.16571098

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/657/1098
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/657/1098
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/657/1098
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2009-02-28T13:55:17Z
Resource record created
2009-02-28T13:55:17Z
Created
2017-06-19T07:57:50Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr