========================================================================== J/A+A/506/359 FORS2 and HAWKI photometry of CoRoT-1 (Gillon+, 2009) The following files can be converted to FITS (extension .fit or fit.gz) fors-r.dat hawki-nb.dat ========================================================================== Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/506/359 ==========================================================================
drwxr-xr-x 30 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 252 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 481 Dec 19 2022 .message -r--r--r-- 1 cats archive 3818 Dec 29 2009 ReadMe -r--r--r-- 1 cats archive 3708 May 29 2009 fors-r.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 10836 May 29 2009 hawki-nb.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/A+A/506/359 FORS2 and HAWKI photometry of CoRoT-1 (Gillon+, 2009) ================================================================================ VLT transit and occultation photometry for the bloated planet CoRoT-1b. Gillon M., Demory B.-O., Triaud A.H.M.J., Barman T., Hebb L., Montalban J., Maxted P.F.L., Queloz D., Deleuil M., Magain P. <Astron. Astrophys. 506, 359 (2009)> =2009A&A...506..359G ================================================================================ ADC_Keywords: Binaries, eclipsing ; Planets ; Photometry Keywords: binaries: eclipsing - planetary systems - stars: individual: CoRoT-1 - infrared: stars - techniques: photometric - techniques: radial velocities Abstract: We present VLT eclipse photometry for the giant planet CoRoT-1b. We observed a transit in the R-band filter and an occultation in a narrow filter centered on 2.09mum. Our analysis of this new photometry and published radial velocities, in combination with stellar-evolutionary modeling, leads to a planetary mass and radius of 1.07^+0.13^_-0.18_M_Jup_ and 1.45^+0.07^_-0.13_R_Jup, confirming the very low density previously deduced from CoRoT photometry. The large occultation depth that we measure at 2.09mum (0.278^0.043^_-0.066_% ) is consistent with thermal emission and is better reproduced by an atmospheric model with no redistribution of the absorbed stellar flux to the night side of the planet. Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 06 48 19.2 -03 06 08 CoRoT-1 = Corot-Exo-1 -----------------------------------------------