Photometric follow-up observations of GJ 436b Virtual Observatory Resource

Authors
  1. Shporer A.
  2. Mazeh T.
  3. Pont F.
  4. Winn J.N.
  5. Holman M.J.
  6. Latham D.W.,Esquerdo G.A.
  7. Published by
    CDS
Abstract

This paper presents multiband photometric follow-up observations of the Neptune-mass transiting planet GJ 436b, consisting of five new ground-based transit light curves obtained in 2007 May. Together with one already published light curve, we have at hand a total of six light curves, spanning 29 days. The analysis of the data yields an orbital period P=2.64386+/-0.00003 days, midtransit time T_c_[HJD]=2454235.8355+/-0.0001, planet mass M_p_=23.1+/-0.9M_{earth}_=0.073+/-0.003M_Jup_, planet radius R_p_=4.2+/-0.2R_{earth}_=0.37+/-0.01R_Jup_, and stellar radius R_s_=0.45+/-0.02R_{sun}_. Our typical precision for the midtransit timing for each transit is about 30s. We searched the data for a possible signature of a second planet in the system through transit timing variations (TTV) and variation of the impact parameter. The analysis could not rule out a small, of the order of a minute, TTV and a long-term modulation of the impact parameter, of the order of +0.2yr^-1^.

Keywords
  1. multiple-stars
  2. solar-system-planets
  3. infrared-photometry
  4. visible-astronomy
  5. photometry
Bibliographic source Bibcode
2009ApJ...694.1559S
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/694/1559
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/694/1559
Document Object Identifer DOI
doi:10.26093/cds/vizier.16941559

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History

2011-04-01T15:38:50Z
Resource record created
2011-04-01T15:38:50Z
Created
2017-06-30T05:48:03Z
Updated

Contact

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