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J/A+A/488/635       HD 203608 radial velocity                 (Mosser+, 2008)

HD 203608, a quiet asteroseismic target in the old galactic disk. Mosser B., Deheuvels S., Michel E,. Thevenin F., Dupret M.A., Samadi R., Barban C., Goupil M.J. <Astron. Astrophys. 488, 635 (2008)> =2008A&A...488..635M
ADC_Keywords: Stars, nearby ; Radial velocities Keywords: techniques: radial velocities - stars: evolution - stars: oscillations Abstract: We conducted a 5-night observing run with the spectrometer HARPS at the ESO 3.6-m telescope in August 2006. We selected the 4th magnitude F8V star HD 203608, a low-metallicity star of the old galactic disk. We reduced the spectra with the on-line data reduction software provided by the instrument. We developed a new statistical approach for extracting the significant peaks in the Fourier domain. Description: Time series of the radial velocities of HD 203608 recorded with the echelle spectrometer HARPS at ESO in August 2006. Objects: ---------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------- 21 26 26.6 -65 21 58 HD 203608 = HR 8181 ---------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 45 2504 Radial velocities
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 11 F11.6 d BJD Barycentric Julian Date from JD=2453948.5 (1) 12- 19 I8 --- Flux Flux (HARPS unit) 20- 31 F12.5 km/s RV Radial velocity 32- 38 F7.2 m/s RVhf Radial velocity after subtraction of 2deg polynomial fit per night 39- 45 F7.2 m/s phnoise Estimated photon noise error (2)
Note (1): JD=2453948.5=2006/08/01 00:00 Note (2): Estimated photon noise error on the stellar spectra, determined by the on-line reduction pipeline
Acknowledgements: Benoit Mosser, benoit.mosser(at)obspm.fr
(End) Benoit Mosser [Paris Obs., France], Patricia Vannier [CDS] 28-Jun-2008
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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