Format for Magri, C., AJ, 1994, 108, 896 -- Table 1

KGC Basic Data

Data consist of 492 records, one per galaxy; each record has up to 101 bytes.
A Fortran-77 program which could access these data would include the following
statements:


      CHARACTER NAME2*6, SAMPLE*1, DEC_SIGN*1, RSA_TYPE*14, RC2_TYPE*15,
     :          UGC_HUB_TYPE*8, UGC_REV_TYPE*12
      INTEGER UGC, RA_HR, RA_MIN, DEC_DEG, DEC_MIN, DEC_SEC
      REAL RA_SEC, A, B, MAG

      READ(10,100) UGC, NAME2, SAMPLE, RA_HR, RA_MIN, RA_SEC,
     :             DEC_SIGN, DEC_DEG, DEC_MIN, DEC_SEC, A, B, MAG,
     :             RSA_TYPE, RC2_TYPE, UGC_HUB_TYPE, UGC_REV_TYPE
  100 FORMAT(I5,1X,A6,1X,A1,1X,2I2,F4.1,1X,A1,3I2,1X,F5.2,1X,
     :       F5.2,1X,F4.1,1X,A14,1X,A15,1X,A8,1X,A12)


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

     UGC number; other name; sample flag (see below); RA and dec (epoch 1950);
     major diameter, minor diameter, and magnitude, as given in UGC;
     morphological types as given by RSA, RC2, and UGC (both on Hubble and
     revised Hubble systems), respectively.


The "sample flag" SAMPLE is 'V' for galaxies with m = 13.2 or brighter which
are in the Virgo core (within six degrees of M87); it is 'X' for galaxies
which are within ten degrees of M87 but which are fainter than m = 13.2; and
it is blank otherwise.

Format for Magri, C., AJ, 1994, 108, 896 -- Table 7

Raw and Corrected Diameters and Magnitudes

Data consist of 492 records, one per galaxy; each record has up to 50 bytes.
A Fortran-77 program which could access these data would include the following
statements:


      CHARACTER D_25_FLAG*1, R_25_FLAG*1, B_T_FLAG*1
      INTEGER UGC
      REAL A, B, Z_MAG, D_25, R_25, B_T, D_0, B_T_0

      READ(10,100) UGC, A, B, Z_MAG, D_25, D_25_FLAG, R_25,
     :             R_25_FLAG, B_T, B_T_FLAG, D_0, B_T_0
  100 FORMAT(I5,1X,F5.2,1X,F5.2,1X,F4.1,1X,F4.1,A1,1X,F4.2,A1,
     :       1X,F4.1,A1,1X,F4.1,1X,F4.1)


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

     UGC number; major diameter, minor diameter, and magnitude, as given in UGC;
     major diameter at 25 blue mags per square arcsec (25 uB); diameter flag
     (see below); axial ratio at 25 uB; ratio flag (see below); total blue
     magnitude within 25 uB; magnitude flag (see below); corrected blue
     diameter; corrected total blue magnitude.


The "flag" for any of the three RC2 photometric parameters is set equal to '*'
when that parameter has been directly measured on the RC2 system for a given
galaxy. If, instead, the parameter has been estimated based on statistical
relationships between UGC and RC2 quantities, then the flag is left blank.

Format for Magri, C., AJ, 1994, 108, 896 -- Table 8

Raw IRAS Data

Data consist of 492 records, one per galaxy; each record has up to 80 bytes.
A Fortran-77 program which could access these data would include the following
statements:


      CHARACTER UPPER_12*1
      INTEGER UGC, RMS_12, RMS_25, RMS_60, RMS_100, CODE_12, CODE_25,
     :        CODE_60, CODE_100
      REAL FLUX_12, FLUX_25, FLUX_60, FLUX_100, FWHM_12, FWHM_25,
     :     FWHM_60, FWHM_100

      READ(10,100) UGC, UPPER_12, FLUX_12, RMS_12, FWHM_12, CODE_12,
     :             FLUX_25, RMS_25, FWHM_25, CODE_25, FLUX_60, RMS_60,
     :             FWHM_60, CODE_60, FLUX_100, RMS_100, FWHM_100, CODE_100
  100 FORMAT(I5,1X,A1,F5.2,1X,I2,1X,F4.2,1X,I2,1X,F5.2,1X,I3,1X,F4.2,1X,I2,
     :       1X,F6.2,1X,I3,1X,F4.2,1X,I2,1X,F7.2,1X,I3,1X,F4.2,1X,I2)


UGC is simply the UGC number of each galaxy. For each of four wavelengths
(12, 25, 60, and 100 microns), the FLUX density (in Jy), the RMS baseline
noise (in mJy), and the FWHM angular diameter (in arcmin) are given.

The flag UPPER_12 is set to '<' when FLUX_12 represents an upper limit taken
from PSC; otherwise it is left blank. (Note that it is left blank for upper
limits NOT taken from PSC.)

The four detection CODEs are 0 for nondetections; 1 for good detections; 2
for marginal detections; 3 for improbable detections; 4 for PSC/SSSC
detections which are probably confused; 5 for spirals mapped by Rice et al.
(1988); 6 for unconfused PSC data; 7 for unconfused SSSC data; 8 for one
galaxy (UGC 6962) for which existing IRAS data were not coadded; and -1 for
objects not observed by IRAS. See printed article for details.

Format for Magri, C., AJ, 1994, 108, 896 -- Table 10

New HI parameters for KGC spirals

Data consist of 223 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 M_HI_LIMIT*1, DEF_LIMIT*1
      INTEGER UGC, V_HEL, V_LG, WIDTH, V_ROT, TEL_CODE, DET_CODE
      REAL RMS, FLUX, CORR_FLUX, DIST, M_HI, DEF

      READ(10,100) UGC, V_HEL, V_LG, RMS, WIDTH, V_ROT, FLUX,
     :             CORR_FLUX, TEL_CODE, DET_CODE, DIST, M_HI_LIMIT,
     :             M_HI, DEF_LIMIT, DEF
  100 FORMAT(I5,1X,I4,1X,I4,1X,F4.2,1X,I3,1X,I3,1X,F6.2,1X,F6.2,1X,
     :       I1,1X,I1,1X,F4.1,1X,A1,F5.2,1X,A1,F5.2)


In the order given in the READ statement above, the data for each galaxy are:
     UGC number; heliocentric velocity (km/s); velocity relative to the
     Local Group barycenter (km/s); rms baseline noise (mJy); HI profile
     width at 50% of the mean signal strength (km/s); computed rotation
     velocity (km/s); raw HI flux (Jy km/s); corrected HI flux (Jy km/s);
     telescope code (see below); detection code (see below); distance (Mpc);
     HI mass flag (see below); logarithm of the HI mass (solar units);
     HI deficiency flag (see below); HI deficiency.

The telescope code TEL_CODE (code "C" in the printed article) is 0 for spirals 
observed with either of the two dual-circular feeds at Arecibo; 1 for those 
observed with the 91 m Green Bank dish; and 2 for those observed with the
Arecibo flat feed.

The detection code DET_CODE (code "D" in the printed article) is 0 for 
nondetections; 1 for good detections; 2 for marginal detections; 3 for confused 
detections; 4 for spirals whose spectra show HI absorption; and 9 for objects 
of unknown redshift for which a search in velocity space was unsuccessful.

The flag M_HI_LIMIT is set to '<' when the HI mass which follows is an upper 
limit; otherwise it is left blank. Similarly, DEF_LIMIT is set to '>' when the 
HI deficiency which follows it is a lower limit, and is left blank otherwise.

Format for Magri, C., AJ, 1994, 108, 896 -- Table 11

New HI Parameters for Non-KGC Galaxies

Data consist of 42 records, one per galaxy; each record has up to 104 bytes.
A Fortran-77 program which could access these data would include the following
statements:


      CHARACTER NAME2*5, DEC_SIGN*1, TYPE*3, M_HI_LIMIT*1, DEF_LIMIT*1
      INTEGER UGC, RA_HR, RA_MIN, DEC_DEG, DEC_MIN, DEC_SEC, V_HEL,
     :        V_LG, WIDTH, V_ROT, TEL_CODE, DET_CODE
      REAL RA_SEC, A, B, MAG, RMS, FLUX, CORR_FLUX, DIST, M_HI, DEF

      READ(10,100) UGC, NAME2, RA_HR, RA_MIN, RA_SEC, DEC_SIGN, DEC_DEG,
     :             DEC_MIN, DEC_SEC, A, B, MAG, TYPE, V_HEL, V_LG, RMS,
     :             WIDTH, V_ROT, FLUX, CORR_FLUX, TEL_CODE, DET_CODE,
     :             DIST, M_HI_LIMIT, M_HI, DEF_LIMIT, DEF
  100 FORMAT(I5,1X,A5,1X,2I2,F4.1,1X,A1,3I2,1X,F3.1,1X,F4.2,1X,F4.1,1X,
     :       A3,1X,I4,1X,I4,1X,F4.2,1X,I3,1X,I3,1X,F5.2,1X,F5.2,1X,I1,
     :       1X,I1,1X,F4.1,1X,A1,F5.2,1X,A1,F5.2)


In the order given in the READ statement above, the data for each galaxy are:
     UGC number; other name; RA and dec (epoch 1950); major diameter, minor
     diameter, and magnitude, taken from UGC; RC2-style morphological type;
     heliocentric velocity (km/s); velocity relative to the Local Group
     barycenter (km/s); rms baseline noise (mJy); HI profile width at 50% of
     the mean signal strength (km/s); computed rotation velocity (km/s); raw HI
     flux (Jy km/s); corrected HI flux (Jy km/s); telescope code (see below);
     detection code (see below); distance (Mpc); HI mass flag (see below);
     logarithm of the HI mass (solar units); HI deficiency flag (see below);
     HI deficiency.

The telescope code TEL_CODE (code "C" in the printed article) is 0 for spirals 
observed with either of the two dual-circular feeds at Arecibo; 1 for those 
observed with the 91 m Green Bank dish; and 2 for those observed with the
Arecibo flat feed.

The detection code DET_CODE (code "D" in the printed article) is 0 for 
nondetections; 1 for good detections; 2 for marginal detections; 3 for confused 
detections; 4 for spirals whose spectra show HI absorption; and 9 for objects 
of unknown redshift for which a search in velocity space was unsuccessful.

The flag M_HI_LIMIT is set to '<' when the HI mass which follows is an upper 
limit; otherwise it is left blank. Similarly, DEF_LIMIT is set to '>' when the 
HI deficiency which follows it is a lower limit, and is left blank otherwise.

Format for Magri, C., AJ, 1994, 108, 896 -- Table 12

Compiled Data on KGC Spirals

Data consist of 492 records, one per galaxy; each record has up to 110 bytes.
A Fortran-77 program which could access these data would include the following
statements:


      CHARACTER TYPE*2, NR*2, B_D_SIGN*1, M_HI_SIGN*1, DEF_SIGN*1,
     :          L_RAD_SIGN*1, L_FIR_SIGN*1, L_WARM_SIGN*1,
     :          M_DUST_SIGN*1, W_MINUS_C_SIGN*1
      INTEGER UGC
      REAL LC, B_D, DIST, DIAM, L_B, B_MINUS_V, U_MINUS_B, B_MINUS_H,
     :     M_HI, DEF, V_ROT, L_RAD, L_FIR, L_WARM, M_DUST, W_MINUS_C,
     :     ENV

      READ(10,100) UGC, TYPE, LC, NR, B_D_SIGN, B_D, DIST,
     :             DIAM, L_B, B_MINUS_V, U_MINUS_B, B_MINUS_H,
     :             M_HI_SIGN, M_HI, DEF_SIGN, DEF, V_ROT,
     :             L_RAD_SIGN, L_RAD, L_FIR_SIGN, L_FIR,
     :             L_WARM_SIGN, L_WARM, M_DUST_SIGN, M_DUST,
     :             W_MINUS_C_SIGN, W_MINUS_C, ENV
  100 FORMAT(I5,1X,A2,1X,F3.1,1X,A2,1X,A1,F3.2,1X,F5.1,1X,F4.2,1X,
     :       F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,A1,F5.2,1X,A1,F4.2,1X,
     :       F4.2,1X,A1,F5.2,1X,A1,F5.2,1X,A1,F5.2,1X,A1,F4.2,1X,
     :       A1,F5.2,1X,F5.2)


In the order given in the READ statement above, the data for each galaxy are:

      UGC (I5): UGC number
      TYPE (A2): morphological type (including bar status) on RC2 system
      LC (F3.1): luminosity class
      NR (A2): non-randomness (see printed text)
      B_D_SIGN, B_D (A1,F3.2): bulge-to-disk diameter ratio
      DIST (F5.1): distance (Mpc)
      DIAM (F4.2): logarithm of blue diameter (kpc)
      L_B (F5.2): logarithm of blue luminosity (solar units)
      B_MINUS_V, U_MINUS_B, B_MINUS_H (all F4.2): optical/NIR colors
      M_HI_SIGN, M_HI (A1,F5.2): logarithm of H I mass (solar units)
      DEF_SIGN, DEF (A1,F4.2): H I deficiency
      V_ROT (F4.2): logarithm of rotation velocity (km/s)
      L_RAD_SIGN, L_RAD (A1,F5.2): logarithm of 20 cm luminosity (solar units)
      L_FIR_SIGN, L_FIR (A1,F5.2): logarithm of far-IR luminosity (solar units)
      L_WARM_SIGN, L_WARM (A1,F5.2): log of warm-dust luminosity (solar units)
      M_DUST_SIGN, M_DUST (A1,F4.2): logarithm of dust mass (solar units)
      W_MINUS_C_SIGN, W_MINUS_C (A1,F5.2): warm/cool dust "color" (see text)
      ENV (F5.2): local environmental harshness (see text)

The SIGNs placed before several quantities are '<' for upper limits,
'>' for lower limits, ':' for marginal detections, and blank otherwise.