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/journal_tables/ApJ/473/822/

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J/ApJ/473/822         APS Catalog of Galaxies behind Virgo  (Hoffman+ 1996)
================================================================================
A Minnesota automated plate scanner catalog of galaxies behind the Virgo
cluster and toward its antipode
      Hoffman G.L., Dickey J.M., Lu N.Y., Fromhold-Treu R.
     <Astrophys. J. 473, 822 (1996)>
     =1996ApJ...473..822H      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Galaxies, photometry
Keywords: Galaxies: spiral - Galaxies: irregular - Galaxies: photometry -
          Galaxies: clustering
Abstract:
    We present a catalog of 1268 galaxies, essentially complete to
    B<=17.0, found by scanning glass copies of several fields of the
    original Palomar Sky Survey using the Minnesota Automated Plate
    Scanner in its isodensitometric mode (as opposed to the threshold
    densitometric mode used in the APS Catalog of the POSS I). In addition
    to the different scanning mode, we have employed a different
    star-galaxy separation method and have visually inspected POSS prints
    to verify that each image remaining in the catalog is non-stellar. The
    scanned fields are distributed generally in two areas, one around the
    outskirts of the Virgo Cluster, the other toward the antipode of the
    cluster (but still in the northern celestial hemisphere). The catalog
    gives the position of the center of each galaxy; estimates of the blue
    and red magnitudes within the outermost threshold crossing and of the
    blue magnitude extrapolated to zero surface brightness; blue and red
    diameters of four ellipses fit to the four threshold crossings
    (approximately 23.8, 23.6, 23.2, and 22.7 mag per square arcsec in
    blue, and 22.5, 22.4, 21.5 and 21.2 mag per square arcsec in red), and
    the ellipticities of those four ellipses. The catalog has served as a
    base from which to draw targets for a Tully-Fisher study of the
    Virgocentric infall velocity of the Local Group.

Description:
    Table 3 lists the galaxies found by the scanner in each of the 17
    fields. The table is organized by CGCG (see Cat. <VII/49>) field, with
    a local running reference number ordered by increasing right ascension
    within that field. B24 is our estimate of the faintest B magnitude
    consistent with the four threshold crossings for each galaxy, and Btot
    is our attempt to estimate the total B magnitude extrapolated to zero
    surface brightness. The diameters of circles with areas equal to the
    ellipses fit to the four threshold crossings are given, along with the
    ellipticities of those ellipses. For broken images ("clumps"), only
    the ellipticity of the outermost ellipse is given. On the second line
    for each galaxy, we give corresponding measurements of R24, diameters
    and ellipticities from the E plate.

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
table3.dat        127     1268   Galaxies found by MAPS
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---     Field     CGCG (Cat. <VII/4>) field number
   5-  7  I3    ---     No        Running index for each field
   9- 17  A9    ---     Name      Name from another catalog
  19- 20  I2    h       RAh       Right ascension (1950) (hours)
  22- 23  I2    min     RAm       Right ascension (1950) (minutes)
  25- 28  F4.1  s       RAs       Right ascension (1950) (seconds)
  30- 31  I2    deg     DEd       Declination (1950) (degrees)
  33- 34  I2    arcmin  DEm       Declination (1950) (arcminutes)
  36- 39  F4.1  arcsec  DEs       Declination (1950) (arcseconds)
  41- 44  F4.1  mag     B24       B magnitude to lowest threshold (1)
  46- 49  F4.1  mag     Btot      B magnitude extrapolated
  51- 53  I3    arcsec  diamB1    B diameter to lowest threshold
  55- 57  I3    arcsec  diamB2    B diameter to second threshold
  59- 61  I3    arcsec  diamB3    B diameter to third threshold
  63- 65  I3    arcsec  diamB4    B diameter to highest threshold
  67- 70  F4.2  ---     eB1       Ellipticity, lowest B threshold
  72- 75  F4.2  ---     eB2       ? Ellipticity, second B threshold
  77- 80  F4.2  ---     eB3       ? Ellipticity, third B threshold
  82- 85  F4.2  ---     eB4       ? Ellipticity, highest B threshold
  87- 90  F4.1  mag     R24       R magnitude to lowest threshold (1)
  92- 94  I3    arcsec  diamR1    R diameter to lowest threshold
  96- 98  I3    arcsec  diamR2    R diameter to second threshold
 100-102  I3    arcsec  diamR3    R diameter to third threshold
 104-106  I3    arcsec  diamR4    R diameter to highest threshold
 108-111  F4.2  ---     eR1       Ellipticity, lowest R threshold
 113-116  F4.2  ---     eR2       ? Ellipticity, second R threshold
 118-121  F4.2  ---     eR3       ? Ellipticity, third R threshold
 123-126  F4.2  ---     eR4       ? Ellipticity, highest Rthreshold
--------------------------------------------------------------------------------
Note (1): Throughout, B refers to quantities measured on the POSS O plate,
           R to quantities measured on the POSS E plate.
--------------------------------------------------------------------------------

Acknowledgements: Lyle Hoffman <hoffmang@nova.phys.lafayette.edu>

History:
  * 14-Apr-1997: Error signaled by Marion Schmitz [NED]
    (zb4ms@ipac.caltech.edu):
    Misprint in the field 097, Z979-022 instead of Z097-022.
================================================================================
(End)                                          Patricia Bauer [CDS] 11-Feb-1997

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