Photometric follow-up observations of GJ 436b

DOI

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^.

Identifier
DOI http://doi.org/10.26093/cds/vizier.16941559
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/694/1559
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/694/1559
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/694/1559
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/694/1559
Provenance
Creator Shporer A.; Mazeh T.; Pont F.; Winn J.N.; Holman M.J.; Latham D.W.,Esquerdo G.A.
Publisher CDS
Publication Year 2011
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy; Stellar Astronomy