J/ApJ/721/1829      High-precision transits of OGLE-TR-113b       (Adams+, 2010)

Six high-precision transits of OGLE-TR-113b. Adams E.R., Lopez-Morales M., Elliot J.L., Seager S., Osip D.J. <Astrophys. J., 721, 1829-1834 (2010)> =2010ApJ...721.1829A 2010ApJ...721.1829A
ADC_Keywords: Planets ; Photometry, SDSS ; Stars, double and multiple Keywords: planetary systems - stars: individual (OGLE-TR-113) Abstract: We present six new transits of the hot Jupiter OGLE-TR-113b observed with MagIC on the Magellan Telescopes between 2007 January and 2009 May. We update the system parameters and revise the planetary radius to Rp=1.084±0.029RJ, where the error is dominated by stellar radius uncertainties. The new transit midtimes reveal no transit timing variations from a constant ephemeris of greater than 13±28s over two years, placing an upper limit of 1-2M{earth} on the mass of any perturber in a 1:2 or 2:1 mean-motion resonance with OGLE-TR-113b. Combining the new transit epochs with five epochs published between 2002 and 2006, we find hints that the orbital period of the planet may not be constant, with the best fit indicating a decrease of dP/dt=-60±15ms/yr. If real, this change in period could result from either a long-period (more than eight years) timing variation due to a massive external perturber or more intriguingly from the orbital decay of the planet. The detection of a changing period is still tentative and requires additional observations, but if confirmed it would enable direct tests of tidal stability and dynamical models of close-in planets. Description: OGLE-TR-113b was reported by Udalski et al. (2002, Cat. II/278) as a planet candidate transiting a K dwarf (I=14.4; RA(J2000)=10:52:24.40, DE(J2000)=-61:26:48.5). We observed six transits of OGLE-TR-113b as part of a larger campaign to detect transit timing variations of OGLE planets (Adams 2010, PhD thesis, Massachusetts Institute of Technology). All transits were observed in the Sloan i' band with the dual-CCD instrument MagIC on the Magellan Telescopes, located at Las Campanas Observatory in Chile. We used MagIC-SITe for two transits in 2007 January and 2008 February, henceforth denoted by their UT dates as 20070130 and 20080225. MagIC-e2v was used for four additional transits between 2008 April and 2009 May (20080424, 20080514, 20090315, and 20090510). Our analysis also includes four literature light curves: 20050404 and 20050414 in R band (Gillon et al. 2006A&A...459..249G 2006A&A...459..249G), 20050411 in V band (Pietrukowicz et al. 2010, Cat. J/A+A/509/A4; Diaz et al. 2007ApJ...660..850D 2007ApJ...660..850D), and 20060318 in K band (Snellen & Covino 2007MNRAS.375..307S 2007MNRAS.375..307S). Objects: ------------------------------------------------------------------------- RA (2000) DE Designation(s) (Period) ------------------------------------------------------------------------- 10 52 24.40 -61 26 48.5 OGLE-TR-113b = NAME OGLE-TR-113b (P=1.43248) ------------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 48 2697 New transit flux values -------------------------------------------------------------------------------- See also: II/278 : Transits observed in OGLE 2001-2003 (Udalski+, 2002-2004) J/MNRAS/422/2024 : Exoplanet evaporation (Jackson+, 2012) J/MNRAS/414/108 : Calibrator of exoplanet-host stars (Beust+, 2011) J/MNRAS/411/L46 : Exoplanet magnetic fields (Vidotto+, 2011) J/A+A/509/A4 : Transits of 12 exoplanet candidates (Pietrukowicz+, 2010) J/ApJ/692/L9 : Tidal evolution of transiting extrasolar planets (Levrard+, 2009) J/ApJ/666/475 : Extrasolar planet taxonomy (Marchi+, 2007) J/A+A/475/359 : Predicting radio fluxes of extrasolar planets (Griessmeier+, 2007) J/ApJ/649/1010 : Habitability of known exoplanetary systems (Jones+, 2006) J/A+A/458/997 : Abundances for transiting planet host stars (Santos+, 2006) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.6 d UTC UTC mid-exposure date 16- 29 F14.6 d BJD BJDTDB mid-exposure date 31- 39 F9.7 --- Flux Magellan/MagIC relative flux in Sloan i'-band 41- 48 F8.6 --- e_Flux Error in Flux -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 10-Jul-2012
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