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J/A+AS/134/59    The central Fornax Cluster. I. Galaxy photometry (Hilker+ 1999)
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The central region of the Fornax cluster. I. A catalog and photometric
properties of galaxies in selected CCD fields
       Hilker M., Kissler-Patig M., Richtler T., Infante L., Quintana H.
      <Astron. Astrophys. Suppl. Ser. 134, 59 (1999)>
      =1999A&AS..134...59H      (SIMBAD/NED BibCode)
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ADC_Keywords: Clusters, galaxy ; Galaxies, photometry
Keywords: galaxies: clusters: individual: Fornax cluster -
          galaxies: fundamental parameters - galaxies: photometry - catalogs -
          galaxies: dwarf

Description:
    In this paper, a photometric catalog is presented of V and I
    photometry of galaxies in the central regions of the Fornax galaxy
    cluster. Our 11 CCD fields cover 0.17 square degrees in total. The
    limiting surface brightness is around 24mag/arcsec^2^, similar to that
    of Ferguson's (1989, Cat. <VII/180>) catalog, whereas our limiting
    total magnitude is around V=22mag, about two magnitudes fainter. The
    photometric properties of more than 870 objects are presented as a
    catalog (Appendix A). The properties and fit parameters of the surface
    brightness profiles for a sub-sample are presented in a second catalog
    (Appendix B). Four new dwarf galaxies are added to Ferguson's catalog.
    However, we confirm that the dwarf galaxies in Fornax follow a similar
    surface brightness -- magnitude relation as the Local Group dwarfs.
    They also follow the color (metallicity) -- magnitude relation seen in
    other galaxy clusters. A formerly suspected excess of dwarf galaxies
    surrounding the central giant cD galaxy NGC 1399 can be explained by
    the superposition of a background cluster at z=0.11 (Hilker et al.
    1998, Cat. <J/A+AS/134/75>, Paper II in this series).

File Summary:
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 FileName    Lrecl  Records   Explanations
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ReadMe          80        .   This file
appendxa.dat    96      873   Photometric catalog
appendxb.dat   119      192   Catalog of profile fit parameters
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See also:
       VII/180 : Galaxies in 3.5 degs of Fornax cluster (Ferguson+ 1989)
 J/A+AS/134/75 : Paper II. Galaxy spectroscopy (Hilker+ 1999)

Byte-by-byte Description of file: appendxa.dat
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   Bytes Format Units       Label  Explanations
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   1-  9  A9    ---         CGF    Catalog name of the object (1)
      10  A1    ---       n_CGF    [*] *: objects that are also listed in
                                           appendb.dat file
      13  I1    h           RAh    Right ascension (J2000)
  15- 16  I2    min         RAm    Right ascension (J2000)
  18- 22  F5.2  s           RAs    Right ascension (J2000)
      25  A1    ---         DE-    Declination sign
  26- 27  I2    deg         DEd    Declination (J2000)
  29- 30  I2    arcmin      DEm    Declination (J2000)
  32- 35  F4.1  arcsec      DEs    Declination (J2000)
  38- 42  F5.2  mag         Vtot   Total V apparent magnitude
      44  A1    ---         nbo    [n] Neighbouring object (2)
  47- 51  F5.2  mag/arcsec2 sbVp   V peak surface brightness
  54- 58  F5.2  mag         V-I    ? (V-I) color within 3 arcsec aperture
  61- 64  F4.2  ---         ell    ? Ellipticity, ell = 1 - b/a
  67- 71  F5.1  deg         PA     [-90/90] Position angle of the major axis (3)
  74- 77  F4.1  arcsec      aphot  Size of the major axis
  80- 83  F4.1  arcsec      d26    ? Size of major axis at sbV = 26 mag/arcsec2
  86- 89  F4.1  arcsec      aeff   ? Effective semi-major axis
  92- 96  F5.2  mag/arcsec2 sbVeff V effective surface brightness
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Note (1): 
    The catalog names are prefixed by the acronym CGF (Catalog of
    Galaxies in Fornax) followed by a sequence number of the field and the
    sequence number of the galaxy in this field (ordered with decreasing
    magnitude). In the catalog the galaxies are ordered by increasing
    right ascension.

Note (2): 
    The letter "n" indicates that a neighbouring object is present within
    two isophotal radii.

Note (3): 
    0 degree is in east direction, positive angles towards the south,
    and negative angles towards the north direction

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Byte-by-byte Description of file: appendxb.dat
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   Bytes Format Units       Label  Explanations
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   1-  9  A9    ---         CGF    Catalog name of the object (see Appendix A)
      12  I1    h           RAh    Right ascension (J2000)
  14- 15  I2    min         RAm    Right ascension (J2000)
  17- 21  F5.2  s           RAs    Right ascension (J2000)
      24  A1    ---         DE-    Declination sign
  25- 26  I2    deg         DEd    Declination (J2000)
  28- 29  I2    arcmin      DEm    Declination (J2000)
  31- 34  F4.1  arcsec      DEs    Declination (J2000)
  37- 44  A8    ---         MType  Morphological Type
  47- 51  F5.2  mag         Vtot   Total V apparent magnitude
      53  A1    ---         nbo    Neighboring object (see Appendix A)
  56- 58  F3.1  arcsec      rcap   Apparent core radius (1)
  61- 63  F3.1  arcsec      rccor  ? Corrected core radius (using
                                      Kormendy 1985ApJ...295...73K)
  66- 70  F5.2  mag/arcsec2 sbVcor ? Corrected central surface brightness (sb)
  73- 76  F4.2  ---         nsers  ? Exponent of Sersic (1968, Atlas de galaxias
                                      australes) profile fit
  79- 83  F5.2  mag/arcsec2 sbVser ? Central surface brightness of Sersic fit
  86- 89  F4.2  arcsec      r0sers ? Scale length of Sersic profile fit
  92- 96  F5.2  mag/arcsec2 sbVdV  ? Central sb of de Vaucouleurs profile fit
  99-103  F5.2  arcsec      refdV  ? Effective radius of de Vaucouleurs profile
 106-110  F5.2  mag/arcsec2 sbVexp ? Central sb of exponential profile fit
 112-116  F5.2  arcsec      alpha  ? Scale length of exponential profile fit
     119  A1    ---         flag   [bdne] Exponential profile fit flag (2)
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Note (1): 
    Radius where the apparent central surface intensity has its half
    value

Note (2): the meaning of the flag is:
       b: bulge is present
       d: light deficiency in the center
       n: nucleus present
       e: exponential law at all radii
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References:
  Sersic J.-L., 1968, Atlas de galaxias australes, Observatorio Astronomica,
    Cordoba
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(End)      M. Hilker [Pontifica Universidad Catolica, Santiago]      30-Jun-1998

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