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/journal_tables/A+AS/130/323/

The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:

1. Use the ADC Data Viewer Suite to visualize the data. [preview
2. Get the data files via anonymous FTP. (See Note.) [ftp


J/A+AS/130/323      ESO Slice Project                           (Vettolani+ 1998)
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The ESO Slice Project (ESP) galaxy redshift survey: III. The Sample
       Vettolani G., Zucca E., Merighi R., Mignoli M., Proust D., Zamorani G.,
       Cappi A., Guzzo L., Maccagni D., Ramella M., Stirpe G.M., Blanchard A.,
       Cayatte V., Collins C., MacGillivray H., Maurogordato S., Scaramella R.,
       Balkowski C., Chincarini G., Felenbok P.
      <Astron. Astrophys. Suppl. Ser. 130, 323 (1998)>
      =1998A&AS..130..323V      (SIMBAD/NED BibCode)
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ADC_Keywords: Galaxy catalogs ; Surveys ; Radial velocities
Keywords: galaxies: distances and redshifts - cosmology: observations ;
          large-scale structure of the Universe

Description:
    The ESO Slice Project (ESP) is a galaxy redshift survey in a region
    near the South Galactic Pole (see Vettolani et al.,
    1997A&A...325..954V; Zucca et al. 1997A&A...326..477Z). It extends
    over a strip 22(RA)x1(DEC) square degrees, plus a nearby area of 5x1
    square degrees, 5 degrees west of the main strip. The right ascension
    limits are 22h30m and 01h20m, at a mean declination of -40{deg}15'
    (B1950). We have covered this region with a regular grid of adjacent
    circular fields, with a diameter of 32arcmin each, corresponding to
    the field of view of the multifiber spectrograph OPTOPUS at the 3.6m
    ESO telescope. The total solid angle of the spectroscopic survey is
    23.2 square degrees. The galaxy catalogue has been extracted from the
    Edinburgh-Durham Southern Galaxy catalogue (Heydon-Dumbleton et al.,
    1989MNRAS.238..379H) which has been obtained from COSMOS (MacGillivray
    & Stobie, 1984VA.....27..433M) scans of SERC J survey plates. The
    number of objects in the photometric ESP sample is 4487. The
    spectroscopic survey is about 85% complete to the limiting magnitude
    bJ=19.4, and consists of 3342 galaxies + 1 QSO with redshift
    determination. The ESP survey is intermediate between shallow, wide
    angle samples and very deep, one--dimensional pencil beams.
    Table 2 lists the fields observed with OPTOPUS and their properties:
    the numbers listed in this table can be used to compute the redshift
    completeness of each fields, following eq.(2) of the paper. Table 3
    provides the catalogue, with galaxies sorted in right ascension.
    The catalogue with additional information and updates can also be
    found at the following URL: http://boas5.bo.astro.it/~cappi/esokp.html

File Summary:
--------------------------------------------------------------------------------
  FileName   Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe          80        .   This file
table2.dat      54      107   OPTOPUS fields
table3.dat      70     4487   Catalogue
--------------------------------------------------------------------------------

See also:
   http://boas5.bo.astro.it/~cappi/esokp.html : the database
   J/A+A/342/1 : ESO Slice Project. VI. Groups  of Galaxies.  (Ramella+ 1999)

Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   2- 4   I3    ---     Field     OPTOPUS field number as in paper
   8- 9   I2    h       RAh       Right ascension (B1950)
  11- 12  I2    min     RAm       Right ascension (B1950)
  14- 17  F4.1  s       RAs       Right ascension (B1950)
      21  A1    ---     DE-       Declination sign
  22- 23  I2    deg     DEd       Declination (B1950)
  25- 26  I2    arcmin  DEm       Declination (B1950)
  28- 29  I2    arcsec  DEs       Declination (B1950)
  33- 34  I2    ---     Nt        No. of objects classified as galaxies in the
                                   photometric catalogue
  38- 39  I2    ---     Nz        No. of measured redshifts
  43- 44  I2    ---     Nno       No. of not observed objects
  48- 49  I2    ---     Nf        No. of failed spectra
  53- 54  I2    ---     Ns        No. of stars
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label    Explanations
--------------------------------------------------------------------------------
   3-  7  I5    ---     ESP      ESP galaxy number as in paper
  10- 12  I3    ---     Field    OPTOPUS field number as in paper
  15- 16  I2    h       RAh      Right ascension (B1950)
  18- 19  I2    min     RAm      Right ascension (B1950)
  21- 24  F4.1  s       RAs      Right ascension (B1950)
      27  A1    ---     DE-      Declination sign
  28- 29  I2    deg     DEd      Declination (B1950)
  31- 32  I2    arcmin  DEm      Declination (B1950)
  34- 35  I2    arcsec  DEs      Declination (B1950)
  38- 42  F5.2  ---     bJmag    bJ magnitude
  45- 49  I5    km/s    HRVa     ?=0 Heliocentric radial velocity from
                                  absorption lines (1)
  51- 53  I3    km/s  e_HRVa     ?=0 Error on absorption line velocity
  55- 59  F5.2  ---     R        ?=0 R parameter value from cross-correlation
  62- 66  I5    km/s    HRVe     ?=0 Heliocentric radial velocity from
                                  emission lines (1)
  68- 70  I3    km/s  e_HRVe     ?=0 Error on emission line velocity
--------------------------------------------------------------------------------
Note (1): Codes in the velocity column:
          -8888 = failed radial velocity measurement
          -9999 = stellar spectrum (hence stars misclassified in the EDSGC)
          99999 = only for the object #31954, a QSO with z=1.174
--------------------------------------------------------------------------------

Acknowledgements: Elena Zucca <ZUCCA@astbo1.bo.cnr.it>

References:
    Vettolani et al., Paper I.  1997A&A...325..954V
    Zucca et al., Paper II.     1997A&A...326..477Z
    Cappi et al., Paper IV.     1998A&A...336..445C
    Scaramella et al. Paper V.  1998A&A...334..404S
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(End)                                         Patricia Bauer [CDS]   26-Mar-1998

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