VIII/10      Bell Laboratories H I Profiles         (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: Radio sources ; Surveys ; Radio lines ; H I data Description: This survey consists of H I 21-cm spectra covering galactic latitudes |b|>10degrees, North of Declination -40deg, observed with the 20-foot horn reflector at AT&T Bell Laboratories, Crawford Hill. The instrument beam is 2° (FWHM). The data consist of 124-channel profiles sorted in Galactic latitude and longitude; each channel has a width of 5.3km/s. The data were obtained by holding the telescope fixed and letting the sky drift through. Then the natural coordinate system for the data is in equatorial coordinates, so the data are not gridded in Galactic coordinates. Note that this catalog represents the Bell Laboratories H I Survey in a preliminary version; it is superseded by Catalog VIII/28. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 703 22261 The Bell Labs HI Survey software.for 80 459 Two Fortran main codes and several subroutines -------------------------------------------------------------------------------- See also: VIII/28 : Bell Laboratories H I Survey Maps (Stark+ 1992) Byte-per-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 mdeg GLONc Galactic longitude, in 0.001 degrees 7- 12 I6 mdeg GLATc Galactic latitude , in 0.001 degrees 13- 14 I2 h RAh Right ascension (hours) [B1950] 15- 16 I2 min RAm Right ascension (minutes) 17- 18 I2 s RAs Right ascension (seconds) 19 A1 --- DE- Declination sign 20- 21 I2 deg DEd [0,90] Declination (degrees) [B1950] 22- 23 I2 arcmin DEm Declination (minutes) 24- 25 I2 arcsec DEs Declination (seconds) 26- 29 I4 0.1 Ch0 *Central channel 30- 35 I6 dam/s V0 *Velocity of Chan0 in LSR, in 0.01km/s 36- 39 I4 s tInt Integration Time 40- 44 I5 0.01K rms3 3 times rms noise 45- 47 I3 --- Chan Channel Number in base 48- 53 I6 10-4 a1 0.0001 narrow baseline coefficients 54- 59 I6 10-4 a2 0.0001 narrow baseline coefficients 60- 65 I6 10-4 a3 0.0001 narrow baseline coefficients 66- 71 I6 10-4 b1 0.0001 broad baseline coefficients 72- 77 I6 10-4 b2 0.0001 broad baseline coefficients 78- 83 I6 10-4 b3 0.0001 broad baseline coefficients 84-703 124I5 0.01K TA *Antenna temperatures -------------------------------------------------------------------------------- Note on V0, Ch0, TA: V0 represents the LSR velocity corresponding to the Chan0 point. The VLSRs for the measured antenna temperatures can be obtained by the following FORTRAN statements: ch0 = real(ich0)/10. ! "pixel" position cvel = real(icv)/100. ! in km/s do i = 1,124 vlsr(i) = cvel + (real(i)-ch0)*5.2767 enddo -------------------------------------------------------------------------------- Brief description of software.for: FORTRAN codes for use in extracting spectra from the H I surveys of Heiles and Habing (VIII/7), Parkes (VIII/8), Argentina (VIII/9), this catalog (VIII/10), and Weaver and Williams (VIII/11).
(End) Francois Ochsenbein [CDS] 16-Mar-1993
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