J/AJ/132/2187  MCT1 photometry of NGC 5128 globular clusters (Harris+, 2006)
Structural parameters for globular clusters in NGC 5128.
II. Hubble Space Telescope ACS imaging and new clusters.
    Harris W.E., Harris G.L.H., Barmby P., McLaughlin D.E., Forbes D.A.
   <Astron. J., 132, 2187-2197 (2006)>
   =2006AJ....132.2187H 2006AJ....132.2187H
ADC_Keywords: Galaxies, nearby ; Clusters, globular ; Photometry, CMT1T2V
Keywords: galaxies: elliptical and lenticular, cD -
          galaxies: individual (NGC 5128) - galaxies: star clusters
Abstract:
    We report the first results from an imaging program with the ACS
    on the Hubble Space Telescope designed to measure the structural
    characteristics of a wide range of globular clusters in NGC 5128,
    the nearest giant elliptical galaxy. From 12 ACS WFC fields we have
    measured a total of 62 previously known globular clusters and have
    discovered 69 new high-probability cluster candidates not found in
    any previous work. We present magnitudes and color indices for all of
    these, along with rough measurements of their effective diameters and
    ellipticities.
Description:
    Our HST program 10260 was targeted at imaging many of the most massive
    known GCs in both M31 and NGC 5128. The M31 material will be presented
    in a later paper (P. Barmby et al. 2006, in preparation). In NGC 5128,
    12 fields were imaged, centered on the clusters C3, C6, C7, C12, C14,
    C18, C19, C25, C29, C30, C32, and C37 (Harris et al.,
    1992AJ....104..613). We used the ACS in its Wide Field Channel (field
    size 3.3" and scale 0.05"/pix), and with a total exposure time on each
    field of one full orbit of 2500s divided into three equal
    subexposures, in the F606W ("Wide V") filter.
File Summary:
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 FileName  Lrecl  Records   Explanations
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ReadMe        80        .   This file
table1.dat    88       62   ACS/WFC data for previously known NGC 5128 clusters
table2.dat    80       69   ACS/WFC data for new NGC 5128 clusters
table3.dat    47       27   Revised coordinates for clusters from paper I,
                             Harris et al., 2002AJ....124.1435H 2002AJ....124.1435H
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See also:
 J/ApJS/150/367 : Globular clusters in NGC 5128 (Peng+, 2004)
 J/A+A/369/812  : UVKs photometry of NGC 5128 globular clusters (Rejkuba, 2001)
 J/ApJ/560/675  : Chandra X-ray point sources in Cen A (Kraft+, 2001)
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label     Explanations
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   1- 14  A14   ---     Cluster   Cluster name (1)
  16- 17  I2    h       RAh       Hour of Right Ascension (J2000)
  19- 20  I2    min     RAm       Minute of Right Ascension (J2000)
  22- 26  F5.2  s       RAs       Second of Right Ascension (J2000)
      28  A1    ---     DE-       Sign of the Declination (J2000)
  29- 30  I2    deg     DEd       Degree of Declination (J2000)
  32- 33  I2    arcmin  DEm       Arcminute of Declination (J2000)
  35- 38  F4.1  arcsec  DEs       Arcsecond of Declination (J2000)
  40- 44  F5.2  arcmin  R         Radius from NGC 5128 center
  46- 50  F5.1  deg     PA        Azimuthal angle measured East of North
  52- 57  F6.3  mag     T1mag     Washington system T1 (red ∼633nm) magnitude
  59- 63  F5.3  mag     M-T1      Washington system M-T1 color index
  65- 69  F5.3  mag     C-T1      ? Washington system C-T1 color index
  71- 74  F4.2  ---     ell       The imexamine ellipticity
  76- 80  F5.2  pix     FWHM      The imexamine Moffat-profile FWHM (2)
  82- 88  A7    ---     Field     ACS field(s)
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Note (1): For the cluster identification numbers:
       CNNN = [VHH81] NN, Harris et al. (1992AJ....104..613H 1992AJ....104..613H)
       GNNN = [HGH92] GNNN, Harris et al. (1992AJ....104..613H 1992AJ....104..613H)
      PFFNN = [PFF2004] gc NNN, Peng et al., (2004, Cat. J/ApJS/150/367)
     WHHNNN = [WHH2005] NNN, Woodley et al. (2005AJ....129.2654W 2005AJ....129.2654W)
   fN-.GCNN = [R2001b] fN.GC-NN, Rejkuba (2001, Cat. J/A+A/369/812)
   AATNNNNN = [BBP2008] AATNNNNN, Beasley et al. (2006AJ....131..814B 2006AJ....131..814B) and
                                  2008, Cat. J/MNRAS/386/1443
       KNNN = [KKF2001] NNN, Kraft et al. (2001, Cat. J/ApJ/560/675)
Note (2): Conveniently, at the 3.9Mpc distance of NGC 5128, one pixel
     of 0.05" corresponds to a linear scale of very close to 1pc.
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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-  4  A4    ---     Cluster   Cluster name (CNNN) (1)
   6-  7  I2    h       RAh       Hour of Right Ascension (J2000)
   9- 10  I2    min     RAm       Minute of Right Ascension (J2000)
  12- 16  F5.2  s       RAs       Second of Right Ascension (J2000)
      18  A1    ---     DE-       Sign of the Declination (J2000)
  19- 20  I2    deg     DEd       Degree of Declination (J2000)
  22- 23  I2    arcmin  DEm       Arcminute of Declination (J2000)
  25- 28  F4.1  arcsec  DEs       Arcsecond of Declination (J2000)
  30- 34  F5.2  arcmin  R         Radius from NGC 5128 center
  36- 40  F5.1  deg     PA        Azimuthal angle measured East of North
  42- 47  F6.3  mag     T1mag     Washington system T1 (red ∼633nm) magnitude
  49- 53  F5.3  mag     M-T1      ? Washington system M-T1 color index
  55- 59  F5.3  mag     C-T1      ? Washington system C-T1 color index
  61- 64  F4.2  ---     ell       The imexamine ellipticity
  66- 70  F5.2  pix     FWHM      The imexamine Moffat-profile FWHM (2)
  72- 78  A7    ---     Field     ACS field(s)
      80  I1    ---     Note      ? Additional note (3)
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Note (1): Labelled continuing with the C-numbers from Harris et al.
     (1992AJ....104..613H 1992AJ....104..613H) and Paper I (2002AJ....124.1435H 2002AJ....124.1435H), 
     starting at C111. [VHH81] NNN in Simbad
Note (2): Conveniently, at the 3.9 Mpc distance of NGC 5128, one pixel of
     0.05 arcsecond corresponds to a linear scale of very close to 1 pc.
Note (3): Note ad follows:
      1 = Faint globular?
      2 = Very crowded, in inner bulge region
      3 = Very compact globular or possible star
      4 = Possible globular, slightly elliptical
      5 = Globular next to very bright star
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Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label     Explanations
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   1-  4  A4    ---     Cluster   Cluster name (GNNN, CNNN) (1)
   6-  7  I2    h       RAh       right ascension (J2000.0)
   9- 10  I2    min     RAm       right ascension (J2000.0)
  12- 16  F5.2  s       RAs       right ascension (J2000.0)
      18  A1    ---     DE-       Declination sign (J2000.0)
  19- 20  I2    deg     DEd       Declination (J2000.0)
  22- 23  I2    arcmin  DEm       Declination (J2000.0)
  25- 28  F4.1  arcsec  DEs       Declination (J2000.0)
  30- 35  F6.3  mag     T1mag     Washington system T1 (red ∼633nm) magnitude
  37- 41  F5.3  mag     M-T1      Washington system M-T1 colour index
  43- 47  F5.3  mag     C-T1      Washington system C-T1 colour index
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Note (1): CNNN are [VHH81] NNN in Simbad, GNNN are [HGH92] GNNN in Simbad
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History:
    From electronic version of the journal
References:
   Harris et al.,     Paper I       2002AJ....124.1435H 2002AJ....124.1435H
   McLaughlin et al., Paper III     2008MNRAS.384..563M 2008MNRAS.384..563M
(End)                  Greg Schwarz [AAS], Patricia Vannier [CDS]    24-Jul-2008