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J/A+A/382/513      Galaxy warps in the HDF North and South  (Reshetnikov+, 2002)
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Statistics of galaxy warps in the HDF North and South.
    Reshetnikov V., Battaner E., Combes F., Jimenez-Vicente J.
      <Astron. Astrophys. 382, 513 (2002)>
      =2002A&A...382..513R      (SIMBAD/NED BibCode)
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ADC_Keywords: Galaxies, photometry ; Morphology ; Redshifts
Keywords: galaxies: evolution - galaxies: formation -
          general; interactions; peculiar; photometry

Abstract:
    We present a statistical study of the presence of galaxy warps in the
    Hubble deep fields. Among a complete sample of 45 edge-on galaxies
    above a diameter of 1.3", we find 5 galaxies to be certainly warped
    and 6 galaxies as good candidates. In addition, 4 galaxies reveal a
    characteristic U-warp. Compared to statistical studies of local warps,
    and taking into account the strong bias against observing the outer
    parts of galaxies at high redshift, these numbers point towards a very
    high frequency of warps at z~1: almost all galaxy discs might be
    warped. Furthermore, the amplitude of warps are stronger than for
    local warps. This is easily interpreted in terms of higher galaxy
    interactions and matter accretion in the past. This result supports
    these two mechanisms as the best candidates for the origin of early
    warps. The mean observed axis ratio of our sample of edge-on galaxies
    is significantly larger in the high-z sample than is found for samples
    of local spiral galaxies. This might be due to disk thickening due to
    more frequent galaxy interactions. Description:

File Summary:
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 FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
table1.dat        61       32   Edge-on galaxies in the HDF-N
table2.dat        37       18   Edge-on galaxies in the HDF-S
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See also:
   J/ApJ/513/34  : HDF photometric redshifts catalog (Fernandez-Soto+, 1999)
   J/AJ/120/2206 : NTT, HDF-S and HDF-N photometric redshifts (Fontana+, 2000)
   J/ApJ/538/29  : HDF-N Caltech faint galaxy redshift survey. X. (Cohen+, 2000)
   J/ApJS/127/1  : UGRK Photometry in the Hubble Deep field region (Hogg+, 2000)

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Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label   Explanations
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   1-  4  I4    ---     [FLY99] Number according to the catalogue of
                                Fernandez-Soto et al., 1999, Cat. <J/ApJ/513/34>
   6- 11  F6.1  pix     Xpos    X position
  13- 18  F6.1  pix     Ypos    Y position
  20- 29  A10   ---     [WBD96] Williams et al. (1996, Cat. <J/AJ/112/1335>)
                                 identification number
  31- 35  F5.2  mag     Imag    I814 magnitude in AB photometric system
  37- 41  F5.3  ---     z       ? Spectroscopic redshift
                                  (Cohen et al. 2000, Cat. <J/ApJ/538/29>;
                                   Hogg et al. 2000, Cat. <J/ApJS/127/1>)
  43- 47  F5.3  ---     z1      Photometric redshift from Fernandez-Soto et al.
                                 (1999, Cat. <J/ApJ/513/34>)
  49- 52  F4.2  ---     z2      Photometric redshift according to Fontana et al.
                                 (2000, Cat. <J/AJ/120/2206>)
  54- 56  A3    ---     Type    Best-fit spectral type of galaxy,
                                 Fernandez-Soto et al. 1999, Cat. <J/ApJ/513/34>
      58  A1    ---     Warp    [456U] Index of warp (G1)
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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- 15  A15   ---     Name   Name according to the Stony Brook catalogue,
                               (Yahata et al., 2000ApJ...538..493Y) (1)
  17- 21  F5.2  mag     Imag   I814 magnitude in AB photometric system
  23- 26  F4.2  ---     z1     Photometric redshift from Fernandez-Soto
                                et al. 1999, Cat. <J/ApJ/513/34>
  28- 31  F4.2  ---     z2     Photometric redshift according to Fontana et al.
                                (2000, Cat. <J/AJ/120/2206>)
  33- 35  A3    ---     Type   Best-fit spectral type of galaxy
                               (Fernandez-Soto et al. 1999, Cat. <J/ApJ/513/34>)
      37  I1    ---     Warp   [4-6]? Index of warp (G1)
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Note (1): The numbers mean coordinates in pixels
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Global notes:
Note (G1): Index of warp:
            The original I814-band images and contour maps of all the sample
             galaxies were examined independently by three of us (E.B., F.C. and
             V.R.). On the basis of eyeball classification, they assigned an
             "index of warp" (IW) for each object: 0 - no warp, 2 - a certain
             integral-shaped warp, and 1 - intermediate case. We also marked
             U-shaped warps, when the plane bends towards the same direction on
             both sides (Reshetnikov & Combes, 1998A&A...337....9R) like the
             letter "U". Then, we summed the personal indices for each object
             and decided to consider those galaxies with total IW=6 (index 2 for
             each observer) as true warps and IW=4-5 as good candidates for
             warped disks.
             So:
              6: a certain integral-shaped warp
            4,5: good candidates to be warped
              U:  U-shaped warps
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History:
    From electronic version of the journal

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(End)                                        Patricia Bauer [CDS]    15-Mar-2002

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