J/ApJS/157/228  Catalog of galaxy morphology in four clusters (Saintonge+, 2005)
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Catalog of galaxy morphology in four rich clusters: luminosity evolution of disk
galaxies at 0.33 < z < 0.83.
    Saintonge A., Schade D., Ellingson E., Yee H.K.C., Carlberg R.G.
   <Astrophys. J. Suppl. Ser., 157, 228-250 (2005)>
   =2005ApJS..157..228S
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ADC_Keywords: Clusters, galaxy ; Morphology ; Redshifts
Keywords: catalogs - galaxies: clusters: individual (MS 1358.4+6245,
          MS 0015.9+1609, MS 1621.5+2640, MS 1054.4-0321) -
          galaxies: evolution - galaxies: spiral

Abstract:
    Hubble Space Telescope (HST) imaging of four rich, X-ray-luminous,
    galaxy clusters (0.33<z<0.83) is used to produce quantitative
    morphological measurements for galaxies in their fields. Catalogs of
    these measurements are presented for 1642 galaxies brighter than
    F814W(AB)=23.0. Galaxy luminosity profiles are fitted with three
    models: exponential disk, de Vaucouleurs bulge, and a disk-plus-bulge
    hybrid model. The best fit is selected and produces a quantitative
    assessment of the morphology of each galaxy: the principal parameters
    derived being B/T, the ratio of bulge to total luminosity, the scale
    lengths and half-light radii, axial ratios, position angles, and
    surface brightnesses of each component. Cluster membership is
    determined using a statistical correction for field galaxy
    contamination, and a mass normalization factor (mass within boundaries
    of the observed fields) is derived for each cluster. Morphological
    classes are defined using B/T: disk galaxies have 0<=B/T<=0.4,
    intermediate galaxies 0.4<B/T<0.8, and bulge-dominated galaxies
    have 0.8<=B/T<=1.

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table2.dat    141      331   Catalog of MS 0015.9+1609
table3.dat    141      381   Catalog of MS 1054.4-0321
table4.dat    141      672   Catalog of MS 1358.4+6245
table5.dat    141      258   Catalog of MS 1621.5+2640
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See also:
 VII/174 : Morphological type catalog in 55 rich galaxy clusters (Dressler 1980)
  J/ApJ/644/30  : HST Observations of 2 high-z clusters (Blakeslee+ 2006)
  J/AJ/131/1891 : Photometric survey of MS 1054-03 (Foerster-Schreiber+ 2006)
  J/ApJ/661/750 : Photometry and spectroscopy of MS 1054-03 members (Tran+ 2007)

Byte-by-byte Description of file: table2.dat table3.dat table4.dat table5.dat
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   Bytes Format Units       Label   Explanations
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   1- 13  A13   ---         Name    Source identification (1)
      15  A1    ---       n_Name    [*] Indicates statistically identified
                                     as a field galaxy
  17- 18  I2    h           RAh     Hour of Right Ascension (J2000)
  20- 21  I2    min         RAm     Minute of Right Ascension (J2000)
  23- 26  F4.1  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- 45  F6.3  mag         Imag    HST/ACS F814W band AB system magnitude (2)
  47- 52  F6.3  mag         I-V     ?=29.999 AB system (F814W-F555W) color (2)
  54- 58  F5.3  ---         z       ? Redshift
  60- 63  F4.2  ---         B/T     Bulge to total luminosity ratio (3)
  65- 70  F6.3  mag/arcsec2 muD     ? Disk surface brightness
  72- 77  F6.2  arcsec      H       ? Disk scale length
  79- 85  F7.2  arcsec    e_H       ? Error in H (4)
  87- 90  F4.2  ---         AR-D    ? Disk axial ratio (5)
  92- 96  F5.2  ---       e_AR-D    ? Error in AR-D
  98-102  F5.1  deg         PA-D    ? Disk position angle (6)
 104-109  F6.3  mag/arcsec2 muB     ? Bulge surface brightness
 111-116  F6.2  arcsec      Re      ? Bulge effective radius
 118-124  F7.2  arcsec    e_Re      ? Error in Re (4)
 126-129  F4.2  ---         AR-B    ? Bulge axial ratio (5)
 131-135  F5.2  ---       e_AR-B    ? Error in AR-B
 137-141  F5.1  deg         PA-B    ? Bulge position angle (6)
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Note (1): Identification is the name of the exposure, chip where the 
          galaxy was found, x and y pixel coordinates on that chip.
Note (2): The magnitudes are calculated from the best-fit model parameters
          and are thus effectively integrated to infinite radius.
Note (3): Value is 0 for a pure disk galaxy, and 1 for a pure bulge galaxy.
Note (4): The errors are mostly reliable for the single component models, 
          and are given in the hybrid model case to indicate the average
          precision of the measurements.
Note (5): Ratio of the length of the minor axis to the major axis of the galaxy.
Note (6): Angle between the major axis of the ellipse and the x pixel
          coordinate axis on the original images.
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History:
    From electronic version of the journal
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(End)                   Greg Schwarz [AAS], Marianne Brouty [CDS]    31-Aug-2005