J/MNRAS/399/287     Transiting planetary system WASP-4       (Southworth+, 2009)

High-precision photometry by telescope defocussing. II. The transiting planetary system WASP-4. Southworth J., Hinse T.C., Burgdorf M.J., Dominik M., Hornstrup A., Jorgensen U.G., Liebig C., Ricci D., Thone C.C., Anguita T., Bozza V., Novati S.C., Harpsoe K., Mancini L., Masi G., Mathiasen M., Rahvar S., Scarpetta G., Snodgrass C., Surdej J., Zub M. <Mon. Not. R. Astron. Soc., 399, 287-294 (2009)> =2009MNRAS.399..287S 2009MNRAS.399..287S
ADC_Keywords: Planets ; Photometry Keywords: stars: planetary systems - methods: data analysis - methods: observational - techniques: photometric Abstract: We present and analyse light curves of four transits of the Southern hemisphere extrasolar planetary system WASP-4, obtained with a telescope defocussed so the radius of each point spread function was 17 arcsec (44 pixels). This approach minimises both random and systematic errors, allowing us to achieve scatters of between 0.60 and 0.88mmag per observation over complete transit events. The light curves are augmented by published observations and analysed using the JKTEBOP code. The results of this process are combined with theoretical stellar model predictions to derive the physical properties of the WASP-4 system. WASP-4 is now one of the best-quantified transiting extrasolar planetary systems, and significant further progress requires improvements to our understanding of the physical properties of low-mass stars. Description: Light curves of four transit events of the transiting extrasolar planetary system WASP-4 are presented. The data were obtained using the Danish 1.5m telescope and DFOSC camera at ESO La Silla in 2008, with substantial telescope defocussing in order to improve the photometric precision of the observations. A Cousins R filter and exposure times of 120s were used. Objects: --------------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------------- 23 34 15.1 -42 03 41 WASP-4 = USNO-B1.0 0479-0948995 --------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file wasp4.dat 37 452 Defocussed photometry of WASP-4 (table2) -------------------------------------------------------------------------------- See also: J/MNRAS/396/1023 : Transiting planetary system WASP-5 (Southworth+, 2009) Byte-by-byte Description of file: wasp4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 F14.6 d HJD HJD for the midpoint of observation 17- 26 F10.7 mag Rmag Differential R-band magnitude of WASP-5 29- 37 F9.7 mag e_Rmag Measurement error of the R-band magnitude -------------------------------------------------------------------------------- Acknowledgements: John Southworth, jkt(at)astro.keele.ac.uk References: Southworth et al., Paper I 2009MNRAS.396.1023S 2009MNRAS.396.1023S, Cat. J/MNRAS/396/1023
(End) John Southworth [Keele Univ., UK], Patricia Vannier [CDS] 12-Oct-2009
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