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:
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 FileName  Lrecl Records   Explanations
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ReadMe        80       .   This file
catalog.dat  396   55470   Southern sky survey data
software.for  80     459   Two Fortran main codes and several subroutines
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Byte-by-byte Description of file: catalog.dat
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 Bytes  Format Units   Label    Explanations
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  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
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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
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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