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J/ApJ/554/742       Chandra Deep Survey of the HDF-N      (Hornschemeier+, 2001)
================================================================================
The Chandra Deep Survey of the Hubble Deep Field-North area.
 II. Results from the Caltech Faint Field Galaxy Redshift Survey area.
    Hornschemeier A.E., Brandt W.N., Garmire G.P., Schneider D.P., Barger A.J.,
    Broos P.S., Cowie L.L., Townsley L.K., Bautz M.W., Burrows D.N., Chartas G.,
    Feigelson E.D., Griffiths R.E., Lumb D., Nousek J.A., Ramsey L.W.,
    Sargent W.L.W.
   <Astrophys. J. 554, 742 (2001)>
   =2001ApJ...554..742H
================================================================================
ADC_Keywords: X-ray sources
Keywords: cosmology: observations - diffuse radiation - galaxies: active -
          surveys - X-rays: galaxies - X-rays: general

Abstract:
    A deep X-ray survey of the Hubble Deep Field-North (HDF-N) and its
    environs is performed using data collected by the Advanced CCD Imaging
    Spectrometer (ACIS) on board the Chandra X-Ray Observatory. Currently
    a 221.9ks exposure is available, the deepest ever presented, and here
    we give results on X-ray sources located in the 8.6'x8.7' area covered
    by the Caltech Faint Field Galaxy Redshift Survey (the "Caltech
    area"). This area has (1) deep photometric coverage in several optical
    and near-infrared bands; (2) extensive coverage at radio,
    submillimeter, and mid-infrared wavelengths; and (3) some of the
    deepest and most complete spectroscopic coverage ever obtained. It is
    also where the X-ray data have the greatest sensitivity; the minimum
    detectable fluxes in the 0.5-2keV (soft) and 2-8keV (hard) bands are
    ~1.3x10^-16^ and ~6.5x10^-16^ergs/cm^2^/s, respectively.

File Summary:
--------------------------------------------------------------------------------
 FileName   Lrecl  Records  Explanations
--------------------------------------------------------------------------------
ReadMe         80        .  This file
table4.dat    127       82  Properties of CHANDRA sources in the Caltech area
table6.dat     99       83  Multiwavelength properties of the Caltech area
                             CHANDRA sources
table8.dat     62       16  CHANDRA detections of {mu}Jy Radio Sources
table9.dat     61       11  CHANDRA detections of Faint ISOCAM Sources
table10.dat    44        4  CHANDRA detections of very red objects (VROs)
--------------------------------------------------------------------------------

See also:
 J/A+A/375/1   : IR obs. of Chandra Deep Field + HDF-South (Saracco+, 2001)
 J/AJ/119/2571 : UBVRI photometry of HDF QSOs and galaxies (Vanden Berk+, 2000)
 J/AJ/120/2206 : NTT, HDF-S and HDF-N photometric redshifts (Fontana+, 2000)
 J/ApJS/127/1  : UGRK Photometry in the Hubble Deep field region (Hogg+, 2000)
 J/ApJ/538/29  : HDF-N Caltech faint galaxy redshift survey. X. (Cohen+, 2000)
 J/AJ/121/2895 : HDF-N Caltech faint galaxy redshift survey. XIII. (Cohen 2001)
 J/ApJ/533/611 : 1.4GHz survey in HDF region (Richards+, 2000)
 J/ApJ/513/34  : HDF photometric redshifts catalog (Fernandez-Soto+, 1999)

Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
   Bytes Format Units       Label     Explanations
--------------------------------------------------------------------------------
   1-  2  I2    ---         [HBG2001] CHANDRA source number
   4- 18  A15   ---         CXOHDFN   The CXOHDFN name (1)
      20  A1    ---       l_FB        Limit flag on FB
  21- 25  F5.1  ct          FB        The full (0.5-8 keV) band CTI-corrected
                                        source counts
      27  A1    ---       f_FB        [f] Flag on FB (2)
  29- 32  F4.1  ct        e_FB        ? Error in FB counts
  34- 36  F3.1  arcsec      DisHB     ? Distance between the source detected in
                                         the FB and HB determined by WAVDETECT
      38  A1    ---       f_DisHB     [e] Flag on DisHB (2)
      40  A1    ---       l_HB        Limit flag on HB
  41- 46  F6.2  ct          HB        The hard (2-8 keV) band CTI-corrected
                                        source counts
      48  A1    ---       f_HB        [f] Flag on HB (2)
  50- 53  F4.1  ct        e_HB        ? Error in HB counts
  55- 58  F4.2  arcsec      DisSB     ? Distance between the source detected in
                                        the FB and SB determined by WAVDETECT
      60  A1    ---       f_DisSB     [e] Flag on DisSB (2)
      62  A1    ---       l_SB        Limit flag on SB
  63- 67  F5.1  ct          SB        The soft (0.5-2 keV) band CTI-corrected
                                        source counts
      69  A1    ---       f_SB        [f] Flag on SB (2)
  71- 74  F4.1  ct        e_SB        ? Error in SB counts
  76- 80  F5.1  ks          Time      Exposure time (3)
      82  A1    ---       f_Time      [gh] Flag on Time (2)
      84  A1    ---       l_BRatio    Limit flag on BRatio
  85- 88  F4.2  ---         BRatio    ? Band ratio hard/soft (4)
  90- 93  F4.2  ---       E_BRatio    ? Upper limit on BRatio (5)
  95- 98  F4.2  ---       e_BRatio    ? Lower limit on BRatio (5)
 100-103  F4.2  ---         Gamma     ? The photon index (6)
     105  A1    ---       f_Gamma     [S] Indicates a spectroscopically
                                        confirmed star (7)
     107  A1    ---       l_FFB       Limit flag on FFB
 108-112  F5.2 10-15mW/m2   FFB       Full band flux (in 10^-15^ergs/cm^2^/s)
     114  A1    ---       l_FHB       Limit flag on FHB
 115-119  F5.2 10-15mW/m2   FHB       ? Hard band flux (in 10^-15^ergs/cm^2^/s)
     121  A1    ---       l_FSB       Limit flag on FSB
 122-126  F5.2 10-15mW/m2   FSB       Soft band flux (in 10^-15^ergs/cm^2^/s)
--------------------------------------------------------------------------------
Note (1): The J2000 position given in the CXOHDFN name.
Note (2): Individual notes:
    e = Both CXOHDFN J123615.9+621515 and CXOHDFN J123621.0+621411 have
        >1.0'' positional offsets between the full-band and soft-band
        detections. These are not considered to be independent detections due
        to decreased positional certainty for the combination of low numbers
        of counts (< 10) and large off-axis angles (> 5').  For the first, the
        source is very hard even if the soft match is incorrect. For the
        second, Gamma = 1.4 is assumed regardless of the soft match due to
        the low number of counts.  Both sources have faint (R > 24.5) optical
        counterparts and no measured redshifts, so none of the conclusions
        about their identities is compromised by a false cross-band match.
        CXOHDFN J123702.8+621601 has a >1.0'' offset between full-band and
        hard-band detections, but the hard-band source has only 6 counts and
        the source spectrum is soft regardless of the hard-band match.  This
        source has a very faint optical counterpart (R {~} 25.4) and no
        redshift, so its identity would not be compromised by a false
        cross-band match.
    f = WAVDETECT photometry failed, this value is from our manual photometry
        (see section 3.3). According to WAVDETECT, the numbers of ``detected''
        counts  for CXOHDFN J123640.2+621655, CXOHDFN J123657.4+621026,
        CXOHDFN J123703.5+621447 were 3.6, 1.9 and 3.5, respectively.  For
        CXOHDFN J123704.8+621601, WAVDETECT photometry gave 27.8 counts, but
        our manual photometry found 61.4 counts.
    g = Source located on or near a gap between the CCDs for at least one
        observation.
    h = Source located at the edge of the ACIS field during observation 957
        (see Table 1).
Note (3): Source exposure times are effective exposure times taken from the
          appropriate location in the full-band exposure map (see
          section 3.2 for discussion).
Note (4): Defined as the ratio of counts between the hard and soft bands.
          These band ratios have been corrected for the differential vignetting
          in the hard and soft bands.
Note (5): Calculated following the "numerical method" described in section
          1.7.3 of Lyons (1991, Data Analysis for Physical Science Students
          (Cambridge: Cambridge Univ. Press)).
Note (6): Entries with values of 1.40 are assumed, since there are too few
          counts to determine the band ratio and then to estimate Gamma.
Note (7): A kT=0.5keV thermal bremsstrahlung X-ray spectral model was assumed.
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table6.dat
--------------------------------------------------------------------------------
   Bytes Format Units     Label     Explanations
--------------------------------------------------------------------------------
   1-  2  I2    ---       [HBG2001] CHANDRA source number
   4- 18  A15   ---       CXOHDFN   The CXOHDFN name (1)
      20  A1    ---     f_CXOHDFN   [fg] Flag on CXOHDFN (2)
      22  A1    ---     l_Rmag      2-{sigma} limit flag on Rmag
  23- 26  F4.1  mag       Rmag      The R band magnitude (3)
      28  A1    ---     f_Rmag      [i] Flag on Rmag (4)
      30  A1    ---     l_Imag      2-{sigma} limit flag on Imag
  31- 34  F4.1  mag       Imag      The I band magnitude (3)
  36- 40  F5.3  ---       z         ? Redshift
      42  A1    ---     f_z         [NS] Indicates object is a Northern (N) or
                                          Southern (S) object
  44- 49  A6    ---     r_z         Reference for z (5)
  51- 63  A13   ---       ID        Object identification (6)
  65- 71  A7    ---     r_ID        Reference for ID (5)
      73  A1    ---     l_LogFB     Limit flag on LogFB
  74- 77  F4.1  [10-7W]   LogFB     ? Log of the full band X-ray luminosity
                                       in ergs/s
      79  A1    ---     l_LogHB     Limit flag on LogHB
  80- 83  F4.1  [10-7W]   LogHB     ? Log of the hard band X-ray luminosity
                                       in ergs/s
      85  A1    ---     f_LogHB     [h] Flag on LogHB (2)
      87  A1    ---     l_LogSB     Limit flag on LogSB
  88- 91  F4.1  [10-7W]   LogSB     ? Log of the soft band X-ray luminosity
                                       in ergs/s
      93  A1    ---     f_LogSB     [h] Flag on LogHB (2)
--------------------------------------------------------------------------------
Note (1): The J2000 position given in the CXOHDFN name.
Note (2): Individual notes:
    e = Luminosity is for the rest frame of the source.
    f = For these objects, there was an optical counterpart lying within the
        aperture close to the edge. We have measured the magnitudes with the
        aperture centered on the position of this optical source (see
        section 4.2 and Figure 6). CXOHDFN J123641.8+621132 is 1.4" from the
        galaxy center but is consistent with an apparent off-center ultraviolet
        bright spot (see Hornschemeier et al., 2000ApJ...541...49H). It is
        possible that this spot may be a background AGN.
        CXOHDFN J123648.0+620941 has two optical counterparts of comparable
        brightness within the 3.0" aperture (see Figure 6). We have measured
        the magnitudes of these two sources manually. See section A.2 for more
        discussion of this source.
    g = See Figure 9 for this object's spectrum.
    h = High-redshift objects: For soft-band fluxes, the 0.5-2keV rest frame
        has been redshifted out of our observed bandpass, so these luminosities
        are extrapolations of the power law calculated from higher energy data.
        For hard-band fluxes (2 cases), this object was not detected in the
        observed 2-8keV band but since the observed 0.5-2keV band overlaps
        well with the rest-frame 2-8keV band, we use the 0.5-2keV count rate
        to calculate the hard luminosity for this source.
Note (3): Measured or calculated as described in section 4.2.
Note (4): CXOHDFN J123651.7+621221 lacks an optical counterpart in our deep
          I-band imaging, but it does have a faint V=26.7 counterpart in the
          HDF-N (see Hornschemeier et al., 2000ApJ...541...49H).
Note (5): Sources for redshifts and identifications:
    H01 = the current paper
    H00 = Hogg et al., 2000, Cat. <J/ApJS/127/1>, [HPA2000]
    C00 = Cohen et al. (2000, Cat. <J/ApJ/538/29>, [CHB2000]
    Liu = Liu et al. (1999AJ....118.1912L), [LPI99]
    B99 = Barger et al. (1999AJ....117..102B), [BCT99]
    FS  = Fernandez-Soto et al. (1999, Cat. <J/ApJ/513/34>), [FLY99]
    D   = M. Dickinson 2000, private communication
    R98 = Richards et al., 1998AJ....116.1039R, [RFK98]
Note (6): The classification system is described in section 5.3.2.  Individual
          objects are discussed in detail in section A.1 and A.2.
    SB = Starburst
    LL = Low-luminosity galaxy (see section 5.4)
    HL = High-luminosity galaxy
    NL = narrow-line AGN
    BL = broad-line AGN
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table8.dat
--------------------------------------------------------------------------------
   Bytes Format Units     Label      Explanations
--------------------------------------------------------------------------------
   1- 19  A19   ---       VLA        VLA object designation
      20  A1    ---     n_VLA        [cde] Note on VLA (1)
  22- 24  F3.1  arcsec    Offset     Offset between the radio and Chandra
                                      source positions
  26- 30  F5.1  uJy       S1.4GHz    Flux at 1.4GHz
      32  A1    ---     l_Sp+Index   Limit flag on Sp+Index
  33- 37  F5.2  ---       Sp+Index   ? Radio spectral index (2)
  39- 41  F3.1  arcsec    theta      ? Radio spatial extent (2)
  43- 47  F5.3  ---       z          ? Redshift
      49  A1    ---     l_BRatio     Limit flag on BRatio
  50- 53  F4.2  ---       BRatio     ? Band ratio hard/soft X-ray
  55- 57  A3    ---       Class      R00 classification (3)
  59- 62  F4.1  [10-7W]   logL0.5-8  ? log of the full 0.5-8keV luminosity
--------------------------------------------------------------------------------
Note (1): Individual notes:
           c: See footnote e in Table 4 and footnote f in Table 6 about this
               object (CXOHDFN J123615.9+621515).
           d: This source was detected in neither the full nor the hard band
           e: This source was not detected independently in either the soft
               or hard bands
Note (2): Radio spectral index and spatial extent determined by Richards,
           2000, Cat. <J/ApJ/533/611>
Note (3): Richards (2000ApJ...533..611R) classification:
          AGN for AGN
          S for starburst-type
          U for unknown
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table9.dat
--------------------------------------------------------------------------------
   Bytes Format Units     Label      Explanations
--------------------------------------------------------------------------------
   1- 16  A16   ---       ISOCAM     ISOCAM Object designation
      17  A1    ---     n_ISOCAM     [b] Note in ISOCAM (1)
  19- 21  F3.1  arcsec    Offset      Offset between the infrared and Chandra
                                        source positions
  23- 27  F5.3  ---       z          ? Redshift
      28  A1    ---     n_z          [c] Note on z (1)
      30  A1    ---     l_F7um       Limit flag on F7um
  31- 33  I3    uJy       F7um       ? Flux at 7{mu}m
  35- 36  I2    uJy     E_F7um       ? Error on F7um (upper limit)
  38- 39  I2    uJy     e_F7um       ? Error on F7um (lower limit)
      41  A1    ---     l_F15um      Limit flag on F15um
  42- 44  I3    uJy       F15um      Flux at 15{mu}m
  46- 47  I2    uJy     E_F15um      ? Error on F15um (upper limit)
  49- 50  I2    uJy     e_F15um      ? Error on F15um (lower limit)
      52  A1    --      l_BRatio     Limit flag on BRatio
  53- 56  F4.2  ---       BRatio     ? Band ratio hard/soft X-ray
  58- 61  F4.1  [10-7W]   logL0.5-8  ? log of the full 0.5-8keV lumonosity
--------------------------------------------------------------------------------
Note (1): Individual notes:
           b: This source was only detected in the soft band. This luminosity is
               in the soft band
           c: This redshift is photometric (M. Dickinson 2000, priv. com.)
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table10.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1- 16  A16   ---     [HPA2000] Hogg et al., (2000, Cat. <J/ApJS/127/1>)
                                   source designation
  18- 21  F4.2  mag     R-Ks      {R}-K_s_ colour index (1)
  23- 27  F5.2  mag     Ks        Ks magnitude
      29  A1    ---   l_BRatio    Limit flag on BRatio
  30- 33  F4.2  ---     BRatio    Band ratio hard/soft X-ray
  35- 39  F5.3  ---     z         ? Redshift (2)
  41- 44  F4.1  [10-7W] logL2-8   ? Log of the full 2-8keV luminosity
--------------------------------------------------------------------------------
Note (1): {R}=0.46F606W+0.54F814W-0.02mag, see Hogg et al., Cat. <J/ApJS/127/1>.
Note (2): Redshifts from Cohen et al. (2000, Cat. <J/ApJ/538/29>; these were
           determined on the basis of a single emission line assumed to be
           [OII] {lambda}3727.
--------------------------------------------------------------------------------

History:
    From electronic version of the journal

References:
   Hornschemeier et al., Paper I, 2000ApJ...541...49H, CXOHDFN JHHMMSS.s+DDMMSS
================================================================================
(End)                    Greg Schwarz [AAS], Patricia Bauer  [CDS]   28-Sep-2001

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