J/MNRAS/422/3099    Transit of HAT-P-5                       (Southworth+, 2012)

Physical properties and radius variations in the HAT-P-5 planetary system from simultaneous four-colour photometry. Southworth J., Mancini L., Maxted P.F.L., Bruni I., Tregloan-Reed J., Barbieri M., Ruocco N., Wheatley P.J. <Mon. Not. R. Astron. Soc., 422, 3099-3106 (2012)> =2012MNRAS.422.3099S 2012MNRAS.422.3099S
ADC_Keywords: Stars, double and multiple ; Planets ; Photometry Keywords: stars: fundamental parameters - stars: individual: HAT-P-5 - planetary systems Abstract: The radii of giant planets, as measured from transit observations, may vary with wavelength due to Rayleigh scattering or variations in opacity. Such an effect is predicted to be large enough to detect using ground-based observations at multiple wavelengths. We present the defocused photometry of a transit in the HAT-P-5 system, obtained simultaneously through Stroemgren u, Gunn g and r, and Johnson I filters. Two more transit events were observed through a Gunn r filter. Description: We observed one full transit of HAT-P-5 on the night of 2010 August 23, using the 2.2-m telescope and BUSCA imager at Calar Alto Astronomical Observatory. BUSCA uses dichroics to split the incoming light into four wavelength intervals, which traverse different arms of the instrument and are incident on to four CCDs. We observed two transits of HAT-P-5 in 2011 May and July, using BFOSC mounted on the 1.52-m G.D. Cassini Telescope at Loiano Observatory, Italy. Objects: ------------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------------- 18 17 37.30 +36 37 16.9 HAT-P-5 =TYC 2634-1087-1 ------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file hatp5ca.dat 36 808 Defocussed photometry for transiting extrasolar planetary system HAT-P-5, Stromgren u, Gunn g and r, and Johnson I passbands hatp5lo.dat 36 311 Defocussed photometry for transiting extrasolar planetary system HAT-P-5, Gunn r passband -------------------------------------------------------------------------------- See also: J/ApJ/707/446 : HAT-P-13 photometry follow-up (Bakos+, 2009) J/A+A/523/A84 : Transit light curves of HAT-P-13b (Szabo+, 2010) J/AJ/141/179 : Transits of TrES-4b, HAT-P-3b and WASP-12b (Chan+, 2011) J/MNRAS/420/2580 : Four transits of HAT-P-13 (Southworth+, 2012) Byte-by-byte Description of file: hatp5ca.dat hatp5lo.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Band [ugrI] Band for differential magnitude (1) 3 A1 --- Obs [lc] observatory (2) 5- 15 F11.5 d BJD Barycentric Julian date (BJD-2400000) 18- 26 F9.6 mag dmag Differential magnitude 29- 36 F8.6 mag e_dmag rms uncertainty on dmag -------------------------------------------------------------------------------- Note (1): Bands as follows: u = Stromgren u passband g = Gunn g passband r = Gunn r passband I = Johnson I passband r = Gunn r passband Note (2): Observatory code as follows: c = BUSCA four-channel CCD imager on the 2.2m telescope at Calar Alto Observatory, near Almeria, Spain l = BFOSC CCD imager on the Loiano 1.5m telescope near Bologna, Italy -------------------------------------------------------------------------------- History: Copied at http://www.astro.keele.ac.uk/~jkt/data-teps.html
(End) Patricia Vannier [CDS] 21-Jan-2013
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