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J/ApJ/539/136     Properties of poor groups of galaxies. III. (Zabludoff+, 2000)
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The properties of poor groups of galaxies. III. The galaxy luminosity function.
    Zabludoff A.I., Mulchaey J.S.
   <Astrophys. J. 539, 136 (2000)>
   =2000ApJ...539..136Z
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ADC_Keywords: Clusters, galaxy ; Radial velocities ; Magnitudes
Keywords: cosmology: large - scale structure of Universe -
          galaxies: clusters: general - galaxies: evolution -
          galaxies: luminosity function, mass function

Abstract:
    The form of the galaxy luminosity function (GLF) in poor groups -
    regions of intermediate galaxy density that are common environments
    for galaxies - is not well understood. Multiobject spectroscopy and
    wide-field CCD imaging now allow us to measure the GLF of bound group
    members directly (i.e., without statistical background subtraction)
    and to compare the group GLF with the GLFs of the field and of rich
    clusters. We use R-band images in 1.5x1.5degree^2^ mosaics to obtain
    photometry for galaxies in the fields of six nearby (2800<cz<7700km/s)
    poor groups for which we have extensive spectroscopic data, including
    328 new galaxy velocities.

File Summary:
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 FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
table1.dat        66      742   Galaxy data
table2.dat        77        6   Group properties
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See also:
   J/ApJ/496/39 : Properties of poor groups of galaxies. I. (Zabludoff+ 1998)

Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label     Explanations
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   1- 12  A12   ---     Name      Galaxy name
  14- 15  I2    h       RAh       Right Ascension (J2000)
  18- 19  I2    min     RAm       Right Ascension (J2000)
  22- 25  F4.1  s       RAs       Right Ascension (J2000)
      30  A1    ---     DE-       Sign of the Declination (J2000)
  31- 32  I2    deg     DEd       Declination (J2000)
  35- 36  I2    arcmin  DEm       Declination (J2000)
  39- 40  I2    arcsec  DEs       Declination (J2000)
  47- 51  I5    km/s    HRV       Heliocentric radial velocity from NED
  55- 57  I3    km/s  e_HRV       Uncertainty in HRV
      60  I1    ---   f_HRV       Flag on the type of velocity measurement (1)
  63- 66  F4.1  mag     Rmag      ? Magnitude in the R band
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Note (1): Type of velocity measurement:
       0: Velocity measured from absorption lines
       1: Velocity measured from emission lines
       2: Velocity measured from a combination of absorption and emission lines
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label     Explanations
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   1-  8  A8    ---     Group     Group name (4)
  10- 11  I2    h       RAh       Right ascension of the group optical
                                   projected centroid in J2000
  13- 14  I2    min     RAm       Right ascension of the group optical
                                   projected centroid in J2000
  16- 19  F4.1  s       RAs       Right ascension of the group optical
                                   projected centroid in J2000
      21  A1    ---     DE-       Declination sign
  22- 23  I2    deg     DEd       Declination of the group optical
                                   projected centroid in J2000
  25- 26  I2    arcmin  DEm       Declination of the group optical
                                   projected centroid in J2000
  28- 29  I2    arcsec  DEs       Declination of the group optical
                                   projected centroid in J2000
  31- 32  I2    ---     Ngroup    Number of group members (1)
  34- 37  I4    km/s    <HRV>     Mean heliocentric velocity (1)
  39- 40  I2    km/s  e_<HRV>     rms uncertainty on <HRV>
  42- 44  I3    km/s    sigma     Line-of-sight velocity dispersion
  46- 47  I2    km/s  E_sigma     Error on sigma (upper limit)
  49- 50  I2    km/s  e_sigma     Error on sigma (lower limit)
  52- 55  F4.1 [10-7W]  logLx     X-ray luminosity (2)
  57- 60  F4.2  Mpc     rsample   Sampling radius for the photometry
  62- 63  I2    ---     N'grp     Number of members within rsample (4) (3)
  65- 69  F5.1  Mpc-3   n0,4      Corrected number density of galaxies (5)
  71- 73  F3.1  ---     D/G0.4    Dwarf-to-giant ratio (6)
  75- 77  F3.1  ---   e_D/G0.4    rms uncertainty on D/G0.4
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Note (1): Calculated within r_samp_ except for NGC 4325 (within 1.0h^-1^Mpc)
     and NGC 5129 (within0.9h^-1^Mpc)
Note (2): From Mulchaey & Zabludoff (1998ApJ...496...73M)
     except for NGC 3557 (this paper)
Note (3): Calculated within r_samp_
Note (4): For HGC 42, Ngrp{diff}N'grp  because one member lies outside
       photometric survey boundary.
     For NGC 3557, marginally-detected in X-rays
Note (5): Corrected number density of galaxies  with M_R_<=-17+5logh,
     within 0.4h^-1^Mpc of the group center and assuming spherical symmetry
Note (6): Dwarf-to-giant ratio for galaxies with M_R_<=-17+5logh and
     within 0.4h^-1^Mpc
--------------------------------------------------------------------------------

History: From ApJ electronic version

References:
      Zabudoff & Mulchaey, Paper I    1998ApJ...496...39Z, Cat. <J/ApJ/496/39>
      Mulchaey & Zabudoff, Paper II   1998ApJ...496...73M
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(End)                      Greg Schwartz [AAS], Patricia Bauer [CDS] 29-Aug-2000

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