J/ApJ/653/1004   Galaxies at 1.4<~z<~3.0 in GOODS-North Field    (Reddy+, 2006)
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A spectroscopic survey of redshift 1.4<~z<~3.0 galaxies in the
GOODS-North Field: survey description, catalogs, and properties.
    Reddy N.A., Steidel C.C., Erb D.K., Shapley A.E., Pettini M.
   <Astrophys. J., 653, 1004-1026 (2006)>
   =2006ApJ...653.1004R
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ADC_Keywords: Surveys ; Redshifts ; Galaxies, photometry ; Photometry, infrared
Keywords: cosmology: observations - galaxies: active - galaxies: evolution -
          galaxies: high-redshift - galaxies: starburst -
          galaxies: stellar content

Abstract:
    We present the results of a spectroscopic survey with LRIS-B on Keck
    of more than 280 star-forming galaxies and AGNs at redshifts
    1.4~<z~<3.0 in the GOODS-N field. Candidates are selected by their
    UnGR colors using the "BM/BX" criteria to target redshift 1.4~<z~<2.5
    galaxies and the LBG criteria to target redshift z~3 galaxies;
    combined these samples account for ~25%-30% of the R and Ks band
    counts to R=25.5 and Ks(AB)=24.4, respectively. The 212 BM/BX galaxies
    and 74 LBGs constitute the largest spectroscopic sample of galaxies at
    z>1.4 in GOODS-N. Extensive multiwavelength data allow us to
    investigate the stellar populations, stellar masses, bolometric
    luminosities (Lbol), and extinction z~2 of galaxies. Deep Chandra and
    Spitzer data indicate that the sample includes galaxies with a wide
    range in Lbol (~10^10^ to >10^12^L_{sun}_) and 4 orders of magnitude
    in dust obscuration (Lbol/LUV).

Description:
    The imaging, photometry, color selection, and spectroscopic
    observations of galaxies in the fields of our survey are described in
    several other papers published by our group (Steidel et al. 2003, Cat.
    J/ApJ/592/728, 2004ApJ...604..534S; Adelberger et al.,
    2004ApJ...607..226A; Reddy et al., 2005ApJ...633..748R). Specific
    details regarding the GOODS-N optical imaging are presented in Reddy
    et al. (2005ApJ...633..748R).

File Summary:
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 FileName   Lrecl  Records   Explanations
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ReadMe         80        .   This file
table2.dat    160      388   GOODS-N UnGR galaxies with spectroscopic redshifts
table3.dat     71      254   Stellar Population Parameters
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See also:
 J/ApJ/592/728  : Lyman break galaxies at redshift z~3 (Steidel+, 2003)
 J/AJ/127/3137  : Hawaii redshifts in the ACS-GOODS region (Cowie+, 2004)
 J/AJ/127/3121  : TKRS catalog of GOODS-North Field (Wirth+, 2004)
 J/ApJ/653/1027 : TKRS/GOODS-N Field galaxies (Weiner+, 2006)

Byte-by-byte Description of file: table2.dat
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   Bytes Format Units   Label     Explanations
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   1- 10  A10   ---     Name      Name (G1)
  12- 13  I2    h       RAh       Right ascension (J2000.0)
  15- 16  I2    min     RAm       Right ascension (J2000.0)
  18- 22  F5.2  s       RAs       Right ascension (J2000.0)
      24  A1    ---     DE-       Declination sign (J2000.0)
  25- 26  I2    deg     DEd       Declination (J2000.0)
  28- 29  I2    arcmin  DEm       Declination (J2000.0)
  31- 34  F4.1  arcsec  DEs       Declination (J2000.0)
      36  A1    ---   u_zem       [:] Uncertainty flag on zem
  37- 41  F5.3  ---     zem       ? Emission redshift (2)
      43  A1    ---   u_zabs      [:] Uncertainty flag on zabs
  44- 48  F5.3  ---     zabs      ? Absorption redshift (3)
  50- 53  A4    ---     Mcl       Morphological class (4)
  55- 59  F5.2  mag     Rmag      ? R magnitude in AB unit (G2)
  61- 65  F5.2  mag     G-R       ? G-R colour index (G2)
      66  A1    ---   l_Un-G      Limit flag, upper limits given for galaxies
                                   undetected in Un
  67- 71  F5.2  mag     Un-G      ? Un-G colour index (G2)
      73  A1    ---   l_Jmag      Limit flag on Jmag
  74- 78  F5.2  mag     Jmag      ? J magnitude (5)
      80  A1    ---   l_Ksmag     Limit flag on Ksmag
  81- 85  F5.2  mag     Ksmag     ? Ks magnitude (5)
  87- 91  F5.2  mag     m3.6      ? magnitude at 3.6um
  93- 96  F4.2  mag   e_m3.6      ? rms uncertainty on m3.6
  98-102  F5.2  mag     m4.5      ? magnitude at 4.5um
 104-107  F4.2  mag   e_m4.5      ? rms uncertainty on m4.5
 109-113  F5.2  mag     m5.8      ? magnitude at 5.8um
 115-118  F4.2  mag   e_m5.8      ? rms uncertainty on m5.8
 120-124  F5.2  mag     m8.0      ? magnitude at 8.0um
 126-129  F4.2  mag   e_m8.0      ? rms uncertainty on m8.0
 131-135  F5.1  uJy     F24       ? flux at 24um
 137-140  F4.1  uJy   e_F24       ? rms uncertainty on F24
 142-160  A19   ---     Notes     Notes (6)
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Note (2): Emission-line redshift. An entry with a colon indicates that the
     redshift is uncertain. A blank entry indicates that an emission-line
     redshift could not be measured.
Note (3): Absorption-line redshift. An entry with a colon indicates that
     the redshift is uncertain. A blank entry indicates that an
     absorption-line redshift could not be measured.
Note (4): Source type, either galaxy (GAL), AGN, QSO, or STAR. The
     distinction between QSO and AGN classification is based on the line
     widths, as described in Steidel et al. (2002ApJ...576..653S), where an
     object is classified as a QSO if it has any emission line with FWHM
     >2000km/s. AGNs identified using other means (X-ray or mid-IR
     emission) are discussed in Sect. 6.2.
Note (5): A blank entry indicates that the object did not lie in the region
     with near-IR imaging.
Note (6): Galaxies in common with the LBG survey in the HDF-N are indicated
     by their names (S03-XXX) as given in Steidel et al. (2003, Cat.
     J/ApJ/592/728). Galaxies with X-ray counterparts within are indicated
     by their names (B03-XXX) in the spectroscopic follow-up to the Chandra
     2 Ms survey by Barger et al. (2003, Cat. <J/AJ/126/632>). Galaxies
     satisfying the distant red galaxy (DRG) criteria of Franx et al.
     (2003ApJ...587L..79F) are indicated by DRG.
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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- 10  A10   ---           Name      Name (G1) (1)
  12- 16  F5.3  ---           z         Redshift
  18- 21  F4.2  mag           E(B-V)i   Reddening E(B-V) calculated with
                                         constant formation
  23- 26  I4    Myr           Age.i     Age calculated with constant formation
  28- 31  I4    solMass/yr    SFR.i     Stellar Formation Rate calculated with
                                         constant formation
  33- 38  F6.3  10+10solMass  Mass.i    Stellar mass calculated with constant
                                         formation
  40- 43  I4    Myr           tau       Best-fit star formation history
                                         decay timescale (2)
  45- 49  F5.2  mag           E(B-V)tau Reddening E(B-V) calculated with tau
  51- 54  I4    Myr           Age.tau   Age calculated with tau
  56- 59  I4    solMass/yr    SFR.tau   Stellar Formation Rate calculated
                                         with tau
  61- 66  F6.3  10+10solMass  Mass.tau  Stellar mass calculated with tau
  68- 71  A4    ---           Note      [IRAC Ks] Notes (3)
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Note (1): We did not fit the stellar populations of galaxies that had no
     data longward of R band, had uncertain redshifts, or are identified as
     AGN/QSO from their optical spectra. We also do not present SED
     parameters for those galaxies with optical and IRAC photometry
     inconsistent with a simple stellar population (these sources had 
     large {chi}^2^>10) or those sources with 8 or 24um excesses.
Note (2): In some cases, a model with constant star formation (infinity)
     provided the best fit.
Note (3): Objects with large Ks band residuals are indicated (i.e., those
     sources whose Ks band measurement lies more than 3{sigma} away from
     the best-fit stellar population). MD31 is the only directly detected
     X-ray source that shows no optical signatures of an AGN, has a
     relatively faint 24um flux, and has photometry that is consistent with
     a stellar population. The IRAC photometry for BX1267 may suffer from a
     deblending problem, and these (IRAC) data were not used in the SED fit.
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Global notes:
Note (G1): Nomenclature note:
     Names S03-XXX are identified as SAS-LBG HDF-XXX in Simbad.
     All other objects are identified as [RSE2006] Name in Simbad
Note (G2): Filters are:
    Un = identitical to SDSS u' filter 
     R = bandpass centered at 683nm, FWHM = 125nm
     G = similar to SDSS g' (same effective wavelength but slightly narrower)
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History:
    From electronic version of the journal
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(End)                                      Patricia Vannier [CDS]    31-Jul-2008
