J/ApJ/840/21  FIR data of IR-bright dust-obscured galaxies (DOGs)  (Toba+, 2017)
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Far-infrared properties of infrared-bright dust-obscured galaxies selected with
IRAS and AKARI far-infrared all-sky survey.
    Toba Y., Nagao T., Wang W.-H., Matsuhara H., Akiyama M., Goto T., Koyama Y.,
    Ohyama Y., Yamamura I.
   <Astrophys. J., 840, 21 (2017)>
   =2017ApJ...840...21T
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ADC_Keywords: Photometry, infrared ; Active gal. nuclei ; Redshifts ;
              Galaxies, IR
Keywords: catalogs ; galaxies: active ; galaxies: star formation ;
          infrared: galaxies

Abstract:
    We investigate the star-forming activity of a sample of infrared
    (IR)-bright dust-obscured galaxies (DOGs) that show an extreme red
    color in the optical and IR regime, (i-[22])_AB_>7.0. Combining an
    IR-bright DOG sample with the flux at 22{mu}m>3.8mJy discovered by
    Toba & Nagao (2016ApJ...820...46T) with the IRAS faint source catalog
    version 2 and AKARI far-IR (FIR) all-sky survey bright source catalog
    version 2, we selected 109 DOGs with FIR data. For a subsample of
    seven IR-bright DOGs with spectroscopic redshifts (0.07<z<1.0) that
    were obtained from the literature, we estimated their IR luminosity,
    star formation rate (SFR), and stellar mass based on the spectral
    energy distribution fitting. We found that (1) the WISE 22{mu}m
    luminosity at the observed frame is a good indicator of IR luminosity
    for IR-bright DOGs and (2) the contribution of the active galactic
    nucleus to IR luminosity increases with IR luminosity. By comparing
    the stellar mass and SFR relation for our DOG sample and the
    literature, we found that most of the IR-bright DOGs lie significantly
    above the main sequence of star-forming galaxies at similar redshift,
    indicating that the majority of IRAS- or AKARI-detected IR-bright DOGs
    are starburst galaxies.

File Summary:
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 FileName   Lrecl  Records  Explanations
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ReadMe         80        .  This file
table1.dat    344        8  The 8 WISE-SDSS-IRAS/AKARI specz dust-obscured
                             galaxies (DOGs) identified in this work
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See also:
 II/125  : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)
 II/298  : AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010)
 II/328  : AllWISE Data Release (Cutri+ 2013)
 VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)
 V/147   : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)
 J/ApJ/663/81   : SED of hard X-ray selected AGN in XMDS (Polletta+, 2007)
 J/ApJ/692/556  : Star forming galaxy templates (Rieke+, 2009)
 J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)
 J/ApJ/797/54   : ULIRGs in the AKARI all-sky survey (Kilerci Eser+, 2014)
 J/ApJS/219/8   : SFR for WISE + SDSS spectroscopic galaxies (Chang+, 2015)
 J/ApJ/805/90   : WISE ELIRGs and comparison with QSOs (Tsai+, 2015)
 J/ApJ/817/118  : SFR-M_*_ relation from ZFOURGE (Tomczak+, 2016)

Byte-by-byte Description of file: table1.dat
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   Bytes Format Units       Label  Explanations
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       1 I1     ---         Seq    Running sequence number
   3-  9 I7     ---         FIS    ? Object ID in AKARI FIS BSC version 2
  11- 27 A17    ---         Name   Souce name
  29- 30 I2     h           RAh    SDSS-DR12 Hour of Right Ascension (J2000)
  32- 33 I2     min         RAm    Minute of Right Ascension (J2000)
  35- 38 F4.1   s           RAs    Second of Right Ascension (J2000)
      40 A1     ---         DE-    SDSS-DR12 Sign of the Declination (J2000)
  41- 42 I2     deg         DEd    SDSS-DR12 Degree of Declination (J2000)
  44- 45 I2     arcmin      DEm    Arcminute of Declination (J2000)
  47- 50 F4.1   arcsec      DEs    Arcsecond of Declination (J2000)
  52- 55 F4.2   ---         z      [0.1/1] NED redshift
  57- 61 F5.2   mag         umag   [19.4/22.7] SDSS u band AB magnitude
  63- 66 F4.2   mag       e_umag   [0.05/0.4] Uncertainty in umag
  68- 72 F5.2   mag         gmag   [18.6/23] SDSS g band AB magnitude
  74- 77 F4.2   mag       e_gmag   [0.01/0.2] Uncertainty in gmag
  79- 83 F5.2   mag         rmag   [18/21.6] SDSS r band AB magnitude
  85- 88 F4.2   mag       e_rmag   [0.01/0.2] Uncertainty in rmag
  90- 94 F5.2   mag         imag   [17.7/20.5] SDSS i band AB magnitude
  96- 99 F4.2   mag       e_imag   [0.01/0.06] Uncertainty in imag
 101-105 F5.2   mag         zmag   [17.6/20.1] SDSS z band AB magnitude
 107-110 F4.2   mag       e_zmag   [0.03/0.2] Uncertainty in zmag
 112-116 F5.2   mag         Jmag   [17.4/18.8]? 2MASS J band AB magnitude
 118-121 F4.2   mag       e_Jmag   [0.1/0.2]? Uncertainty in Jmag
 123-127 F5.2   mag         Hmag   [16.4/17.6]? 2MASS H band AB magnitude
 129-132 F4.2   mag       e_Hmag   [0.07/0.3]? Uncertainty in Hmag
 134-138 F5.2   mag         Ksmag  [15.3/16.7]? 2MASS Ks band AB magnitude
 140-143 F4.2   mag       e_Ksmag  [0.04/0.2]? Uncertainty in Ksmag
 145-148 F4.2   mJy         F3.4   [0.1/8.7] WISE 3.4um (W1) band flux density
 150-153 F4.2   mJy       e_F3.4   [0.01/0.2] Uncertainty in F3.4
 155-159 F5.2   mJy         F4.6   [0.1/16.7] WISE 4.6um (W2) band flux density
 161-164 F4.2   mJy       e_F4.6   [0.01/0.4] Uncertainty in F4.6
 166-170 F5.2   mJy         F12    [7/76] IRAS 12 micron band flux density
 172-175 F4.2   mJy       e_F12    [0.2/1.1] Uncertainty in F12
 177-182 F6.2   mJy         F22    [26/237] WISE 22um (W4) band flux density
 184-187 F4.2   mJy       e_F22    [1/5] Uncertainty in F22
 189-194 F6.2   mJy         F25    [71/312]? IRAS 25 micron band flux density
 196-200 F5.2   mJy       e_F25    [17/94]? Uncertainty in F25
     202 I1     ---       q_F25    [1/2]? Quality flag on F25 (1)
 204-209 F6.2   mJy         F60    [189/397]? IRAS 60 micron band flux density
 211-215 F5.2   mJy       e_F60    [32/68]? Uncertainty in F60
     217 I1     ---       q_F60    [3]? Quality flag on F60 (3=high) (1)
 219-224 F6.2   mJy         F65    [61/599]? AKARI 65 micron band flux density
 226-231 F6.2   mJy       e_F65    [191/256]? Uncertainty in F65
     233 I1     ---       q_F65    [1]? Quality flag on F65 (1)
 235-240 F6.2   mJy         F90    [396/685]? AKARI 90 micron band flux density
 242-246 F5.2   mJy       e_F90    [46/65]? Uncertainty in F90
     248 I1     ---       q_F90    [3]? Quality flag on F90 (3=high) (1)
 250-255 F6.2   mJy         F100   [500/819]? IRAS 100 micron band flux density
 257-262 F6.2   mJy       e_F100   [115/172]? Uncertainty in F100
     264 I1     ---       q_F100   [1]? Quality flag on F100 (1)
 266-272 F7.2   mJy         F140   [40/1333]? AKARI/FIS 140um band flux density
 274-279 F6.2   mJy       e_F140   [189/259]? Uncertainty in F140
     281 I1     ---       q_F140   [1]? Quality flag on F140 (1)
 283-288 F6.2   mJy         F160   [53/434]? AKARI/FIS 160um band flux density
 290-295 F6.2   mJy       e_F160   [325/339]? Uncertainty in F160
     297 I1     ---       q_F160   [1]? Quality flag on F160 (1)
 299-303 F5.2   [Lsun]      logLIR [11/14]? log IR luminosity
 305-308 F4.2   [Lsun]    e_logLIR [0.01/0.2]? Lower uncertainty in logLIR
 310-313 F4.2   [Lsun]    E_logLIR [0.04/0.2]? Upper uncertainty in logLIR
 315-319 F5.2   [Msun]      logM*  [9/13]? log stellar mass
 321-324 F4.2   [Msun]    e_logM*  [0/0.2]? Lower uncertainty in logM*
 326-329 F4.2   [Msun]    E_logM*  [0.01/0.3]? Upper uncertainty in logM*
 331-334 F4.2   [Msun/yr]   logSFR [1.9/3.2]? log Star Formation Rate
 336-339 F4.2   [Msun/yr] e_logSFR [0.04/0.6]? Lower uncertainty in logSFR
 341-344 F4.2   [Msun/yr] E_logSFR [0.06/0.3]? Upper uncertainty in logSFR
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Note (1): Quality flag as follows:
    1 = The source is not confirmed for 65, 90, 140, and 160 micron flux
        while an upper limit for 25, 60, and 100 micron flux;
    3 = High quality.
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History:
    From electronic version of the journal

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(End)                  Prepared by [AAS], Emmanuelle Perret [CDS]    07-Dec-2017