VIII/28             Bell Laboratories H I Survey         (Stark+ 1992)

The Bell Laboratories H I Survey Stark A.A., Gammie C.F., Wilson R.W., Bally J., Linke R.A. <Astrophys. J. Suppl., 79, 77 (1992)> =1992ApJS...79...77S 1992ApJS...79...77S
ADC_Keywords: H I data; Interstellar medium; Surveys; Radio lines Description: The sky north of declination -40° was observed in the 21cm line of atomic hydrogen with the FWHM=2° beam of the 20 foot horn reflector at AT&T Bell Laboratories, Crawford Hill. The survey covers a velocity range of 654km/s centered on the Galactic standard of rest, with 5.3km/s wide filters. This survey is distinguished by its sensitivity to low surface brightness features (antenna temperature about 50mK) and relative freedom from sidelobe contamination. High-velocity clouds are extracted and catalogued automatically. The data are presented in declination zones in equatorial and polar coordinates, and as R.A. - velocity images. Introduction: Observations were made as drift scans along even declinations between -40° and +90° at the epoch (1981) of the observations. The horn antenna has a FWHM beam size of 2° at 21cm. This large beam made it possible to cover the whole visible sky in 66 constant declination scans. The survey is undersampled in declination (one beam width sampling) and oversampled in right ascension (roughly quarter beamwidth sampling). The average rms noise of spectra taken at all declinations is 0.017K in 5.2km/s wide channels, although in some cases baseline problems make the survey unreliable at this level. The survey contains 19,248 spectra. The data are in FITS format. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This File sky.dat 43 145 List of FITS files with images of the integrated 21cm flux in each velocity channel ravel.dat 17 66 List of FITS files with images of the antenna temperature in declination ranges fits/* . 501 All FITS files described in sky.dat and ravel.dat -------------------------------------------------------------------------------- Byte-by-byte Description of file: sky.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 km/s cVel Central velocity of the channel (limits are cVel±5km/s) 6- 17 A12 --- FITS-Nfile North polar cap image in this channel, in "fits" subdirectory; 19- 30 A12 --- FITS-Wfile Whole sky (outside polar caps) in this channel in "fits" subdirectory; 32- 43 A12 --- FITS-Sfile South polar cap image in this channel, in "fits" subdirectory; -------------------------------------------------------------------------------- Byte-by-byte Description of file: ravel.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 4 I3 deg cDec Central declination 6- 17 A12 --- FITSfile File in "fits" subdirectory fits -------------------------------------------------------------------------------- Modifications: The file names from the tape were renamed to distinguish the different coordinate systems and projections easily. In the notes some information from the HISTORY records in the FITS headers was appended. The data were read with the FITS routines from the IDL ASTRONOMY USER'S LIBRARY maintained by Wayne Landsman (). * 21-Dec-2002: files sky.dat and ravel.dat containing the list of FITS files were added.
(End) N. G. Roman and N.P.M. Kuin [NASA/SSDOO/ADC] 11-Apr-1995
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