J/AJ/143/95            Transit light curves of HAT-P-12            (Lee+, 2012)

The sub-Saturn mass transiting planet HAT-P-12b. Lee J.W., Youn J.-H., Kim S.-L., Lee C.-U., Hinse T.C. <Astron. J., 143, 95 (2012)> =2012AJ....143...95L 2012AJ....143...95L
ADC_Keywords: Planets ; Stars, double and multiple ; Photometry, CCD ; Photometry, RI Keywords: planetary systems - stars: individual (HAT-P-12) - techniques: photometric Abstract: We present new photometric data of the transiting planet HAT-P-12b observed in 2011. Our three transit curves are modeled using the JKTEBOP code and adopting the quadratic limb-darkening law. Including our measurements, 18 transit times spanning about 4.2yr were used to determine the improved ephemeris with a transit epoch of 2454187.85560±0.00011BJD and an orbital period of 3.21305961±0.00000035days. The physical properties of the star-planet system are computed using empirical calibrations from eclipsing binary stars and stellar evolutionary models, combined with both our transit parameters and previously known spectroscopic results. We found that the absolute dimensions of the host star are MA=0.73±0.02M☉, RA=0.70±0.01R, log gA=4.61±0.02, pA=2.10±0.09ρ☉, and LA=0.21±0.01L. The planetary companion has Mb=0.21±0.01M{Jup}, Rb=0.94±0.01R{Jup}, log gb=2.77±0.02, ρb=0.24±0.01ρ{Jup}, and Teq=960±14K. Our results agree well with standard models of irradiated gas giants with a core mass of 11.3M{earth}. Description: Observations were carried out between 2011 March and May (March 29, April 14 and May 13), using an ARC 4K CCD camera and a Cousins R filter attached to the 1.0m reflector at the Mt. Lemmon Optical Astronomy Observatory (LOAO) in Arizona, USA. The image field of view is ∼28*28arcmin2 at the f/7.5 Cassegrain focus of the telescope. Transit curves of HAT-P-12b are listed in table 2. Objects: --------------------------------------------------------------------- RA (2000) DE Designation(s) (Period) --------------------------------------------------------------------- 13 57 33.48 +43 29 36.7 HAT-P-12 = GSC 03033-00706 (P=3.213089) --------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 35 811 Rc-band photometry of HAT-P-12 -------------------------------------------------------------------------------- See also: J/A+A/552/A119 : Planet-star and moon-planet interaction (Saur+, 2013) J/MNRAS/420/2580 : Four transits of HAT-P-13 (Southworth+, 2012) J/MNRAS/422/2024 : X-ray-age relation & exoplanet evaporation (Jackson+, 2012) J/MNRAS/411/L46 : Exoplanet magnetic fields (Vidotto+, 2011) J/PASP/123/412 : Exoplanet Orbit Database (Wright+, 2011) J/A+A/532/A24 : Light curves of HAT-P-13b (Nascimbeni+, 2011) J/AJ/142/84 : 10 new transit light curves of HAT-P-13b (Fulton+, 2011) J/A+A/527/A85 : Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011) J/MNRAS/414/1278 : Eccentricities of transiting planets (Pont+, 2011) J/ApJ/726/52 : HAT-P-18 and HAT-P-19 follow-up (Hartman+, 2011) J/A+A/523/A84 : Transit light curves of HAT-P-13b (Szabo+, 2010) J/ApJ/716/1336 : Stability analysis of single-planet (Kopparapu+, 2010) J/ApJ/706/785 : HAT-P-12 light curve (Hartman+, 2009) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d BJD Barycentric Julian Date (1) 15- 21 F7.4 mag DRmag [-0.0067/0.0333] Differential Cousins RC-band magnitude 23- 28 F6.4 mag e_DRmag The 1σ error in DRmag 30- 35 F6.4 --- RFlux Relative flux -------------------------------------------------------------------------------- Note (1): In the Barycentric Dynamical Time (TDB) system (Eastman et al. 2010PASP..122..935E 2010PASP..122..935E). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Sylvain Guehenneux [CDS] 30-May-2013
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line