Format for Haynes et al. AJ, April 97

"21 cm HI Line Spectra of Galaxies in Nearby Clusters"
Haynes, M.P., Giovanelli, R., Herter, T., Vogt, N., Freudling, W., 
Maia, M.A.G., Salzer, J.J. and Wegner, G. 1997, AJ (Apr 97). 

Table 2: Properties of Detected Galaxies

Data consist of 840 records, one per galaxy; each record has up
to 97 bytes.

A Fortran-77 program which could access these data would include the 
following statements:

      CHARACTER Name*8, SIGN*1, TIMES*1, 
     *   ACMode*1,SmoCode*1,TFQualCode*1,
     *   ClusterNote*1,TableNote*1

      INTEGER RAh,RAm,DECD,DECm,DECs,AGCNumber,
     *   TYPE,VHel21,ObsWidth
      REAL RAs,Dmaj,Dmin,ObsFlux,CorrFlux,RMS,SNR,
     *   CorrWidth,WidthError

      READ(10,100) AGCNumber,Name,RAh,RAm,RAS,
     *   SIGN,DECD,DECm,DECS,Dmaj,TIMES,Dmin,TYPE,
     *   ObsFlux,CorrFlux,RMS,SNR,VHel21,
     *   ObsWidth,CorrWidth,WidthError,
     *   ACMode,SmoCode,TFQualCode,ClusterNote,TableNote
  100 format(i6,1x,a8,1x,2i2.2,f4.1,1x,a1,3i2.2,
     *   1x,f3.1,a1,f3.1,1x,i2,1x,f6.2,1x,f6.2,1x,
     *   f5.2,1x,f6.1,1x,i5,1x,i3,1x,f5.1,1x,
     *   f4.1,1x,5a1)

In the order given in the READ statement, the variables are:

   AGC Number, Name, RA and Dec (1950), major diameter, minor diameter,
   morphological type, observed HI line flux, HI line flux corrected
   for source extent and pointing errors, RMS noise per channel,
   peak signal-to-RMS noise ratio, heliocentric systemic velocity,
   observed HI line width, HI line width corrected for instrumental
   broadening and smoothing, error on the corrected HI line width,
   autocorrelator configuration code, smoothing code, quality code for
   Tully-Fisher method applications, flag set if included in the cluster
   sample of Giovanelli et al. 1997a (AJ 113, 22), flag set if a note
   is included for galaxy in the Notes to Table 2.

The "autocorrelator code" refers to the configuration of the final spectrum:
a = 20 MHz/512 channels; o = 10 MHz/252 channels; g = 10 MHz/192 channels.

The "smoothing code" describes the degree of smoothing applied to the
final spectrum: H = single hanning only; B = hanning plus 3 channel boxcar.

The "TF quality code" is a qualitative assessment of the quality of the profile
for TF applications: G = good; F = fair; S = single peak;
M = marginal detection; C = confused. "F" should be used with caution. Because
the width measuring algorithm is designed for application to two--horned
profiles, the widths measured on single peaked profiles should also be
used with caution, as they may underestimate the true rotation width.
Widths in the latter two categories cannot be used for TF purposes.
A designation of marginal detection is given to those cases in which 
the signal has not been verified through adequate reobservation.
Confusion is identified only when contamination from another galaxy
in the beam is certain.  

The "cluster note" flag denoted by "c" indicates that the galaxy is also
included in the tabulation by Giovanelli et al. 1997a. 

The "table note" flag  indicates the presence of a comment for the object
in the notes to Table 2.


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Table 3: Observational Results for Non--detections

Data consist of 246 records, one per galaxy; each record has up
to 65 bytes.

A Fortran-77 program which could access these data would include the 
following statements:

      CHARACTER Name*8,SIGN*1,TIMES*1,DASH*1,
     *   ACMode*1,TableNote*1
      INTEGER AGCNumber,RAh,RAm,DECD,DECm,DECs,
     *   Type,VelMin,VelMax
      REAL RAs,Dmaj,Dmin,RMS

      READ(10,100) AGCNumber,Name,RAh,RAm,RAS,
     *   SIGN,DECD,DECm,DECS,Dmaj,TIMES,Dmin,Type,
     *   VelMin,DASH,VelMax,ACMode,RMS,TableNote
  100 format(i6,1x,a8,1x,2i2.2,f4.1,1x,a1,3i2.2,
     *   1x,f3.1,a1,f3.1,1x,i2,1x,I5,A1,I5,
     *   1x,a1,1x,f5.2,1x,a1)
      write(14,100) AGCNumber,Name,RAh,RAm,RAS,
     *   SIGN,DECD,DECm,DECS,Dmaj,TIMES,Dmin,Type,
     *   VelMin,DASH,VelMax,ACMode,RMS,TableNote

In the order given in the READ statement, the variables are:

   AGC Number, Name, RA and Dec (1950), major diameter, minor diameter,
   morphological type, minimum velocity covered by the spectral observations,
   maximum velocity covered by the spectral observations, autocorrelation
   configuration code, the RMS noise per channel and a flag set if a note
   is included for galaxy in the Notes to Table 2.


The "autocorrelator code" refers to the configuration of the spectral
observations: "A" indicates that all correlator quadrants were centered on the
same frequency. "S" indicates that the search mode was employed. 

The "table note" flag  indicates the presence of a comment for the object
in the notes to Table 3.