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J/A+A/527/L11       HAT-P-6 radial velocity curve             (Hebrard+, 2011)

The retrograde orbit of the HAT-P-6b exoplanet. Hebrard G., Ehrenreich D., Bouchy F., Delfosse X., Moutou C., Arnold L., Boisse I., Bonfils X., Diaz R.F., Eggenberger A., Forveille T., Lagrange A.-M., Lovis C., Pepe F., Perrier C., Queloz D., Santerne A., Santos N.C., Segransan D., Udry S., Vidal-Madjar A. <Astron. Astrophys. 527, L11 (2011)> =2011A&A...527L..11H
ADC_Keywords: Stars, double and multiple ; Planets ; Radial velocities Keywords: planets and satellites: dynamical evolution and stability - techniques: radial velocities - planetary systems - stars: individual: HAT-P-6 Abstract: We observed with the SOPHIE spectrograph (OHP, France) the transit of the HAT-P-6b exoplanet across its host star. The resulting stellar radial velocities display the Rossiter-McLaughlin anomaly and reveal a retrograde orbit: the planetary orbital spin and the stellar rotational spin point towards approximately opposite directions. Description: OHP/SOPHIE radial velocity measurements of the star HAT-P-6 and uncertainties as plotted in Fig. 1. Objects: --------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------- 23 39 05.8 +42 27 58 HAT-P-6 = TYC 3239-992-1 --------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file hat6.dat 29 41 SOPHIE radial velocities of HAT-P-6
See also: J/AJ/134/1707 : Six transits of exoplanet HAT-P-1b (Winn+, 2007) J/A+A/523/A84 : Transit light curves of HAT-P-13b (Szabo+, 2010) J/A+A/527/A85 : Light curves of HAT-P-3b and HAT-P-14b (Nascimbeni+, 2011) Byte-by-byte Description of file: hat6.dat
Bytes Format Units Label Explanations
1- 14 F14.6 d BJD Barycentric Julian Day of the observations 15- 22 F8.4 km/s RV Radial velocity 24- 29 F6.4 km/s e_RV rms uncertainty on RV
Acknowledgements: Guillaume Hebrard, hebrard(at)iap.fr
(End) Patricia Vannier [CDS] 31-Jan-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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