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J/A+A/513/A6        NOT survey of subdwarf B stars         (Ostensen+, 2010)

A survey for pulsating subdwarf B stars with the Nordic Optical Telescope. Ostensen R.H., Oreiro R., Solheim J.-E., Heber U., Silvotti R., Gonzales-Perez J.M., Ulla A., Perez Hernandez, F., Rodriguez-Lopez C., Telting J.H. <Astron. Astrophys. 513, A6 (2010)> =2010A&A...513A...6O
ADC_Keywords: Surveys ; Stars, subdwarf ; Stars, B-type Keywords: subdwarfs - surveys - stars: oscillations - Abstract: A search programme for pulsating subdwarf B stars was conducted with the Nordic Optical Telescope on La Palma over 59 nights between 1999 and 2009. The purpose of the programme was to significantly extend the number of rapidly pulsating sdB stars to better understand the properties of this new group of variable compact stars. Candidates were selected initially from the HS and HE surveys, but were supplemented with additional objects from other surveys. Short sequences of time-series photometry were made on the candidates to determine the presence of rapid pulsations. Description: The table contains all the sdB stars observed during the NOT survey that were not identified as pulsators. It provides coordinates, details of the photometric sequences, and on the variability for each object. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table5.dat 91 285 Catalog of subdwarf B stars
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 16 A16 --- Name Target star name 18- 33 A16 --- AName Alternative name 35- 36 I2 h RAh Right ascension (J2000) 38- 39 I2 min RAm Right ascension (J2000) 41- 45 F5.2 s RAs Right ascension (J2000) 48 A1 --- DE- Declination sign 49- 50 I2 deg DEd Declination (J2000) 52- 53 I2 arcmin DEm Declination (J2000) 55- 59 F5.2 arcsec DEs Declination (J2000) 61- 64 F4.1 mag pgmag Photographic magnitude 66- 67 A2 --- Run Run identifier 69- 72 I4 --- Np Number of data points in light curve 74- 75 I2 s Dt Sampling interval 77- 81 F5.2 10-3 Sigma Mean noise level, in mma units (1) 83- 87 F5.2 10-3 Amax Amplitude of highest peak in Fourier spectrum, in mma units (1) 89- 91 A3 --- Type [NOV. ] Non-variability flag (2)
Note (1): The mma units are milli-modulation amplitudes, i.e. 1E-3 of the Fourier amplitudes of a light-curve in normalised intensity units. One mma translates to a peak-to-peak amplitude of two millimodulation intensity (mmi) units in the light curve. Note (2): Targets flagged as NOV (not observed to vary) have Amax<3.7xSigma. The remaining targets are discussed individually in the paper.
Acknowledgements: Roy Ostensen, roy(at)ster.kuleuven.be
(End) Roy Ostensen [K.U. Leuven], Patricia Vannier [CDS] 21-Jan-2010
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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