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J/A+A/542/A18 βPic Harps radial velocity data (Lagrange+, 2012)
Constraints on planets around β Pic with Harps radial velocity data. Lagrange A.-M., De Bondt K., Meunier N., Sterzik M., Beust H., Galland F. <Astron. Astrophys., 542, A18-18 (2012)> =2012A&A...542A..18L
ADC_Keywords: Stars, double and multiple ; Planets ; Radial velocities Keywords: planets and satellites: detection - planets and satellites: individual: β Pic - techniques: radial velocities Abstract: The β Pictoris system with its debris disk and a massive giant planet orbiting at ~=9AU represents an ideal laboratory for studying giant planet formation and evolution as well as planet-disk interactions. β Pic b can also help in testing brightness-mass relations at young ages. Other planets, yet undetected, may of course be present in the system. We aim at directly constraining the mass of β Pic b and at searching for additional jovian planets on orbits closer than typically 2AU. Description: We used high-precision Harps data collected over eight years since 2003 to measure and analyse β Pic radial velocities. Objects: ----------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------- 05 47 17.09 -51 03 59.4 beta Pic = HD 39060 ----------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file rvbpic.dat 29 1049 β Pic radial velocities
See also: J/A+A/299/557 : Light variations on Beta Pic (Lecavelier des Etangs+, 1995) Byte-by-byte Description of file: rvbpic.dat
Bytes Format Units Label Explanations
1- 14 F14.6 d JD Julian date 16- 22 F7.4 km/s RV Radial velocity 24- 29 F6.4 km/s e_RV rms uncertainty on RV
Acknowledgements: Anne-Marie Lagrange, Anne-Marie.Lagrange(at)obs.ujf-grenoble.fr
(End) Patricia Vannier [CDS] 17-Jul-2012
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