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J/A+A/532/A24       Light curves of HAT-P-13b                (Nascimbeni+, 2011)

TASTE: The Asiago Search for Transit timing variations of Exoplanets II. A new observational study of transit time variations in HAT-P-13b. Nascimbeni V., Piotto G., Bedin L.R., Damasso M., Malavolta L., Borsato L. <Astron. Astrophys. 532, A24 (2011)> =2011A&A...532A..24N
ADC_Keywords: Stars, double and multiple ; Planets ; Photometry Keywords: techniques: photometric - planetary systems - stars: individual: HAT-P-13 Abstract: TASTE (The Asiago Search for Transit timing variations of Exoplanets) project is collecting high-precision, short-cadence light curves for a selected sample of transiting exoplanets. It has been claimed that the hot jupiter HAT-P-13b suddenly deviated from a linear ephemeris by ∼20min, implying that there is a perturber in the system. Using five new transits, we discuss the plausibility of this transit time variation (TTV), and show that a periodic signal should not be excluded. More follow-up observations are required to constrain the mass and the orbit of the hypothetical perturber. Objects: --------------------------------------------------------- RA (2000) DE Designation(s) (Per) --------------------------------------------------------- 08 39 32.0 +47 21 07 HAT-P-13 = TYC 3416-543-1 (2.91) --------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file hat13.dat 31 12585 Five light curves of HAT-P-13b
See also: J/A+A/527/A85 : Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011) Byte-by-byte Description of file: hat13.dat
Bytes Format Units Label Explanations
1- 14 F14.6 d BJD Barycentric Julian Day (UTC-based) 16- 23 F8.5 mag mag Normalized magnitude 25- 31 F7.5 mag e_mag Error on magnitude
Acknowledgements: Valerio Nascimbeni, valerio.nascimbeni(at)unipd.it References: Nascimbeni et al., Paper I 2011A&A...527A..85N, Cat. J/A+A/527/A85
(End) Valerio Nascimbeni [UNIPD, Italy], Patricia Vannier [CDS] 14-Jul-2011
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

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