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J/A+A/505/1311  Radial velocity curves of 11 UMa and HD 32518 (Dollinger+, 2009)

Planetary companions around the K giant stars 11 Ursae Minoris and HD 32518. Dollinger M.P., Hatzes A.P., Pasquini L., Guenther E.M., Hartmann M. <Astron. Astrophys. 505, 1311 (2009)> =2009A&A...505.1311D
ADC_Keywords: Stars, variable ; Planets ; Radial velocities Keywords: stars: individual: 11 Ursae Minoris - stars: variables: general - stars: individual: HD 32518 - stars: late-type - techniques: radial velocities - stars: planetary systems Abstract: 11 UMi and HD 32518 belong to a sample of 62 K giant stars that has been observed since February 2004 using the 2m Alfred Jensch telescope of the Thueringer Landessternwarte (TLS) to measure precise radial velocities (RVs). The aim of this survey is to investigate the dependence of planet formation on the mass of the host star by searching for planetary companions around intermediate-mass giants. Description: An iodine absorption cell was used to obtain accurate RVs for this study. Objects: ------------------------------------------------------------ RA (2000) DE Designation(s) (files) ------------------------------------------------------------ 15 17 05.9 +71 49 26 11 UMi = HD 136726 (table2.dat) 05 09 36.7 +69 38 22 HD 32518 = HIP 24003 (table5.dat) ------------------------------------------------------------ File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 28 58 Radial velocity measurements for 11 UMi table5.dat 28 58 Radial velocity measurements for HD 32518
See also: J/A+A/499/935 : RV curves of 42 Dra and HD 139357 (Dollinger+, 2009) Byte-by-byte Description of file: table2.dat table5.dat
Bytes Format Units Label Explanations
1- 14 F14.6 d JD Julian date 16- 22 F7.2 m/s RV Radial velocity 24- 28 F5.2 m/s e_RV rms uncertainty on RV
Acknowledgements: Michaela Doellinger, mdoellin(at)eso.org
(End) Patricia Vannier [CDS] 14-Aug-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

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