VIII/9      Argentina High-Latitude H I Survey     (Colomb 1980)

The Argentina High-Latitude H I Survey Colomb F.R., Poppel W.G.L., Heiles C. <Astron. & Astrophys. Suppl., 40, 47 (1980)> =1980A&AS...40...47C 1980A&AS...40...47C
ADC_Keywords: Radio sources ; Surveys ; Radio lines ; H I data Description: This survey consists of H I 21-cm spectra covering the southern sky with absolute galactic latitude |b|>10 degrees and a declination dec←25 degrees. The observations were made with the 30m telescope of the Instituto Argentino de Radioastronomia during 1973 to 1977 and were described in Colomb et al. (1977A&AS...29...89C 1977A&AS...29...89C). The data were obtained by keeping the telescope fixed on the meridian at the desired declination and letting the sky drift through the field. The individual spectra were obtained with a 56-channel filterbank and covering the velocity range from about -40 to +40km/s. The velocity resolution is 2km/s, and the beamwidth is 30arcmin. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 396 55470 Southern sky survey data software.for 80 459 Two Fortran main codes and several subroutines -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 mdeg mGLON Galactic longitude in units of 0.001 degrees 7- 12 I6 mdeg mGLAT Galactic latitude in units of 0.001 degrees 13- 14 I2 h RAh Right ascension (1950) 15- 16 I2 min RAm RA in minutes (1950) 17- 18 I2 s RAs RA in seconds (1950) 19 A1 --- DE- Sign of declination 20- 21 I2 deg DEd [0,90] DEC in degree (1950) 22- 23 I2 arcmin DEm DEC in arcminutes (1950) 24- 25 I2 arcsec DEs DEC in arcseconds (1950) 26- 27 I2 h LST.h Local Standard Time (LST) in hours 28- 29 I2 min LST.m LST in minutes 30- 31 I2 s LST.s LST in seconds 32- 37 A6 "YYMMDD" ObsDate Date of observation in yymmdd (year month day) 38- 47 5I2 --- Bscan Bad scan numbers (always 0) 48- 53 I6 dam/s Vmin *Central velocity at channel 1 54- 59 I6 dam/s Vmax *Central velocity at channel 56 60 I1 --- Qual Quality factor (always 0) 61-396 56I6 0.01K TA *Antenna temperature in units of 0.01K -------------------------------------------------------------------------------- Note on Vmin, Vmax, TA: The VLSRs of the 56 channels corresponding to the measured antenna temperatures can be obtained by the following FORTRAN statements: V1 = Vmin * 0.01 ! in units of km/s V56= Vmax * 0.01 dv = (V56-V1)/55. do i = 1, 56 VLSR(i)= V1 + (i-1)* dv 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), this catalog (VIII/9), Bell Labs (VIII/10), and Weaver and Williams (VIII/11) History: * The catalog was received at ADC in 1992; a brief introduction was added at CDS (Francois Ochsenbein). * The documentation was added in December 1995 at ADC (C.-H. Joseph Lyu) * The documentation was revised in November 2003 at CDS (F. Ochsenbein) Acknowledgements: The General Information on High-latitude 21-cm Line Surveys by Carl Heiles (1988), University of California, Berkeley was used to create this ReadMe file.
(End) C.-H. Joseph Lyu [Hughes STX/NASA] 12-Dec-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