Access to Astronomical Catalogues

J/MNRAS/358/149     HDFN SCUBA Super-map. III                (Pope+, 2005)
The Hubble Deep Field North SCUBA Super-map.
III. Optical and near-infrared properties of submillimetre galaxies.
    Pope A., Borys C., Scott D., Conselice C., Dickinson M., Mobasher B.
   <Mon. Not. R. Astron. Soc., 358, 149-167 (2005)>
   =2005MNRAS.358..149P
ADC_Keywords: Surveys ; Millimetric/submm sources

Keywords: methods: statistical - galaxies: evolution - galaxies: formation -
          galaxies: starburst - submillimetre

Abstract:
    We present a new submillimetre (submm) super-map in the Hubble Deep
    Field North (HDF-N) region (Great Observatories Origins Deep Survey
    North, GOODS-N, field), containing 40 statistically robust sources at
    850um. This map contains additional data, and several new sources,
    including one of the brightest blank-sky extragalactic submm sources
    ever detected. We have used the Advanced Camera for Surveys (ACS)
    Hubble Space Telescope (HST) images and ground-based near-infrared
    (IR) observations from the Great Observatories Origins Deep Survey
    (GOODS), along with deep radio observations, to develop a systematic
    approach for counterpart identification. With the depth achieved by
    this survey, optical counterparts have been found for all the
    radio-detected (RD) submm sources.

Description:
    As part of the ground-based follow-up to GOODS, near-IR data were
    obtained using Flamingos at the Kitt Peak National Observatory. These
    images provide coverage with more uniform sensitivity over the GOODS-N
    region than the Capak et al. (2004, Cat. J/AJ/127/180) HK' data, and
    in the standard J and Ks filters.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
tablea1.dat       73       40  *Updated list of 850um sources in GOODS-N region
                             (Great Observatories Origins Deep Survey North)
tablea2.dat       95        7  *450-um source list.

Note on tablea1.dat: The table lists the 21 sources detected at a level
    of 4σ, followed by 17 sources detected initially at the level
    3.5-4.0σ. The two extra sources found by cleaning our map are
    listed at the bottom of the table.
Note on tablea2.dat: There are seven candidate sources detected at a level
    of 4σ; however none of them is detected at >5σ.


See also:
         II/261 : GOODS initial results (Giavalisco+, 2004)
   J/ApJ/616/71 : Optical properties of SCUBA galaxies (Smail+, 2004)
   J/AJ/127/180 : The Hawaii Hubble Deep Field North (Capak+, 2004)


Byte-by-byte Description of file: tablea1.dat

   Bytes Format Units   Label     Explanations

   1-  6  A6    ---    [PBS2005]  GOODS-N (prefix GN) ID number
   8- 10  A3    ---     ---       [SMM]
  11- 24  A14   ---     SMM       SMM designation (JHHMMSS+DDMMSS) (G1)
  26- 27  I2    h       RAh       Right ascension (J2000.0)
  29- 30  I2    min     RAm       Right ascension (J2000.0)
  32- 35  F4.1  s       RAs       Right ascension (J2000.0)
      37  A1    ---     DE-       Declination sign (J2000.0)
  38- 39  I2    deg     DEd       Declination (J2000.0)
  41- 42  I2    arcmin  DEm       Declination (J2000.0)
  44- 45  I2    arcsec  DEs       Declination (J2000.0)
  47- 50  F4.1  mJy     S850um    Flux density at 850um
  52- 54  F3.1  mJy     e_S850um  rms uncertainty on S850um
  56- 59  F4.1  ---     S/N       Signal-to-noise ratio
  61- 70  A10   ---     Com       Comments (1)
      71  A1    ---     n_Com     Note on Com (2)
      73  A1    ---     OID       Optical ID code (3)

Note (1): Sources that are new since Paper II (Borys et al.,
          2004MNRAS.355..485B) are listed as New
Note (2): Note as follows:
      a = See Dunlop et al. (2004MNRAS.350..769D) for detailed counterpart
          analysis of this source. Our cleaning procedure finds a
          companion source approximately 25 arcsec to the south-west.
          However a simultaneous fit places it at an signal-to-noise ratio
          of slightly less than 3.5.
      b = There are several minor changes compared with the table 4 of
          Paper II, which we discuss in the text. Note that GN38 is just
          outside the GOODS-N region.
Note (3): Status of the optical counterpart for each submillimetre (submm)
          source as follows:
      S = secure
      T = tentative
      M = multiple possible counterparts that meet our counterpart
          selection criteria
      N = no counterpart


Byte-by-byte Description of file: tablea2.dat

   Bytes Format Units   Label     Explanations

   1-  3  A3    ---     ---       [SMM]
   4- 17  A14   ---     SMM       SMM designation (JHHMMSS+DDMMSS) (G1)
  19- 20  I2    h       RAh       Right ascension (J2000.0)
  22- 23  I2    min     RAm       Right ascension (J2000.0)
  25- 28  F4.1  s       RAs       Right ascension (J2000.0)
      30  A1    ---     DE-       Declination sign (J2000.0)
  31- 32  I2    deg     DEd       Declination (J2000.0)
  34- 35  I2    arcmin  DEm       Declination (J2000.0)
  37- 38  I2    arcsec  DEs       Declination (J2000.0)
  40- 42  I3    mJy     S450um    Flux density at 450um
  44- 45  I2    mJy     e_S450um  rms uncertainty on S450um
      47  A1    ---     l_S850um  Limit flag on S850um
  48- 51  F4.1  mJy     S850um    3σ upper limits of Flux density at 850um
  53- 95  A43   ---     Com       Comment


Global notes:

Note (G1):
    Identified as [PBS2005] SMM JHHMMSS+DDMMSS in Simbad


History:
    From electronic version of the journal

References:
    Borys et al., Paper I    2003MNRAS.344..385B
    Borys et al., Paper II   2004MNRAS.355..485B
(End)                                      Patricia Vannier [CDS]    27-Mar-2006