J/ApJ/867/131  Blazar candidates behind the Magellanic Clouds  (Zywucka+, 2018)
Identification of blazar candidates behind Small and Large Magellanic Clouds.
    Zywucka N., Goyal A., Jamrozy M., Stawarz L., Ostrowski M., Kozlowski S.,
    Udalski A.
   <Astrophys. J., 867, 131 (2018)>
   =2018ApJ...867..131Z 2018ApJ...867..131Z
ADC_Keywords: BL Lac objects; Active gal. nuclei; QSOs; Magellanic Clouds;
              Photometry, VRI; Radio lines; Redshifts; Surveys
Keywords: BL Lacertae objects: general ; galaxies: active ; Magellanic Clouds
Abstract:
    We report the identification of blazar candidates behind the
    Magellanic Clouds. The objects were selected from the Magellanic
    Quasars Survey (MQS), which targeted the entire Large Magellanic Cloud
    (LMC) and 70% of the Small Magellanic Cloud (SMC). Among the 758 MQS
    quasars and 898 of the unidentified (featureless spectra) objects, we
    identified a sample of 44 blazar candidates, including 27
    flat-spectrum radio quasars and 17 BL Lacertae objects, respectively.
    All the blazar candidates from our sample were identified with respect
    to their radio, optical, and midinfrared properties. The newly
    selected blazar candidates possess the long-term, multicolor
    photometric data from the Optical Gravitational Lensing Experiment,
    multicolor midinfrared observations, and archival radio data for one
    frequency at least. In addition, for nine of them, the radio
    polarization data are available. With such data, these objects can be
    used to study the physics behind the blazar variability detected in
    the optical and midinfrared bands, as a tool to investigate magnetic
    field geometry of the LMC and SMC, and as an exemplary sample of
    point-like sources most likely detectable in the γ-ray range
    with the newly emerging Cherenkov Telescope Array.
Description:
    In the present study, we report the identification of blazar
    candidates behind the Large Magellanic Cloud (LMC) and Small
    Magellanic Cloud (SMC), which are selected from the catalog of the
    Magellanic Quasar Survey (MQS; Kozlowski+ 2013, J/ApJ/775/92) and a
    "featureless spectra" (FS) objects list (See Section 2).
    Both the LMC and SMC regions were observed with the Wise Infrared
    Survey Explorer (WISE) satellite (angular resolutions of 6.1" 6.4",
    6.5", and 12.0", in 3.4um, 4.6um, 12um and 22um, respectively); and
    with the Spitzer IRAC and MIPS instruments as part of the program
    Surveying the Agents of a Galaxys Evolution (SAGE; Meixner+, 2006,
    J/AJ/132/2268 and Gordon+ 2011AJ....142..102G 2011AJ....142..102G). The angular resolution
    is 1.7", 1.7", 1.9", and 2.0" in the IRAC bands, centered at 3.6, 4.5,
    5.8, and 8.0um, respectively, while it is 6.0", 18.0", and 40.0" in
    the MIPS bands centered at 24, 70, and 160um, respectively. In our
    study, we have used the simultaneous IRAC data only, in order to
    minimize uncertainties of the selection procedure.
    In order to ascertain the blazar nature of sources from the MQS and
    the FS lists, we searched for radio counterparts of the optically
    detected sources in various radio sky surveys and catalogs given in
    Table 1:
    ----------------------------------------------------------------
    Survey         Telescope        Frequency   Beam size
                                    (GHz)       (")
    ----------------------------------------------------------------
    SUMSS (1)      MOST             0.843       43 x 43csc|δ|
    AT20G (1)      ATCA             5, 8, 20    9.9, 5.5, 2.4
    PMN (3)        Parkes 64m       4.85        252
    ATPMN (4)      ATCA             4.8, 6.8    1.8, 1.2
    SMC multi (5)  ATCA and Parkes  1.42/8.64   98/15
    LMC dual (6)   ATCA             4.8, 8.6    33, 20
    SMC dual (7)   ATCA             4.8, 8.6    35, 22
    ----------------------------------------------------------------
    Note. Sky survey references as follows:
     (1) = Bock+ (1999AJ....117.1578B 1999AJ....117.1578B);
     (1) = Murphy+ (2010, J/MNRAS/402/2403);
     (3) = Griffith & Wright (1993, VIII/38);
     (4) = McConnell+ (2012, J/MNRAS/422/1527);
     (5) = Filipovic+ (2002, J/MNRAS/335/1085);
     (6) = Dickel+ (2005AJ....129..790D 2005AJ....129..790D);
     (7) = Dickel+ (2010AJ....140.1511D 2010AJ....140.1511D).
    ----------------------------------------------------------------
File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl  Records  Explanations
--------------------------------------------------------------------------------
ReadMe          80        .  This file
table2.dat     106       48  The radio fluxes of flat-spectrum radio quasar
                              (FSRQ) type blazar candidates
table3.dat      78       44  Newly identified FSRQ and BL Lac type blazar
                              candidates
--------------------------------------------------------------------------------
See also:
 VIII/38   : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)
 IX/10     : ROSAT All-Sky Bright Source Catalogue (Voges+ 1999)
 VIII/81   : Sydney University Molonglo Sky Survey (SUMSS V2.1) (Mauch+ 2008)
 VII/274   : The Roma BZCAT - 5th edition (Massaro+, 2015)
 J/AJ/115/1253    : Deep X-Ray Radio Blazar Survey (DXRBS). I. (Perlman+ 1998)
 J/A+AS/139/277   : LMC X-ray sources ROSAT PSPC catalogue (Haberl+, 1999)
 J/A+AS/142/41    : SMC X-ray sources ROSAT PSPC catalogue (Haberl+, 2000)
 J/MNRAS/323/757  : Deep X-Ray Radio Blazar Survey (DXRBS). II. (Landt+, 2001)
 J/MNRAS/329/877  : The CLASS blazar survey. II. (Caccianiga+, 2002)
 J/MNRAS/335/1085 : ATCA SMC Radio Continuum Source. I. (Filipovic+, 2002)
 J/AJ/123/855     : Magellanic Clouds Photometric Survey: SMC (Zaritsky+, 2002)
 J/AJ/128/1606    : Magellanic Clouds Photometric Survey: LMC (Zaritsky+, 2004)
 J/AJ/132/2268    : SAGE calibration stars (Meixner+, 2006)
 J/ApJ/655/212    : S3MC IRAC and MIPS photometry (Bolatto+, 2007)
 J/AJ/134/799     : Multiwaveband polarimetry of 15 AGN (Jorstad+, 2007)
 J/ApJ/698/895    : Variations in QSOs optical flux (Kelly+, 2009)
 J/ApJ/701/508    : 5000 AGNs behind the Magellanic clouds (Kozlowski+, 2009)
 J/ApJ/715/429    : First Fermi-LAT AGN catalog (1LAC) (Abdo+, 2010)
 J/ApJ/718/587    : The Fermi-AT20G catalog (Mahony+, 2010)
 J/MNRAS/402/2403 : Australia Telescope 20GHz Survey Catalog, (Murphy+, 2010)
 J/AJ/139/390     : Opt selected BL Lac objects from SDSS-DR7 (Plotkin+, 2010)
 J/ApJS/194/22    : Magellanic QSOs Survey: QSOs behind SMC (Kozlowski+, 2011)
 J/ApJ/748/68     : WISE IR colors of gamma-ray blazars (D'Abrusco+, 2012)
 J/ApJ/746/27     : Magellanic QSOs Survey.II.AGNs behind LMC (Kozlowski+, 2012)
 J/ApJ/759/25     : Rotation measures at 1.4GHz toward the LMC (Mao+, 2012)
 J/MNRAS/422/1527 : Australia Telescope PMN follow-up survey (McConnell+, 2012)
 J/ApJS/199/31    : Fermi LAT second source catalog (2FGL) (Nolan+, 2012)
 J/ApJ/775/92     : MQS III: AGNs behind LMC and SMC (Kozlowski+, 2013)
 J/ApJ/767/14     : MASIV survey III. Optical identifications (Pursimo+, 2013)
 J/A+A/549/A29    : Quasars behind the Magellanic system (Cioni+, 2013)
 J/ApJS/215/14    : WISE candidate γ-ray blazar radio (D'Abrusco+, 2014)
 J/other/Nat/515.376  : Relativistic jet powers in blazars (Ghisellini+, 2014)
 J/other/AstBu/69.266 : RATAN-600 flux densities 37 blazars (Mufakharov+,2014)
 J/MNRAS/450/2658 : RATAN-600 flux densities of 123 blazars (Mufakharov+, 2015)
Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
   Bytes Format Units   Label   Explanations
--------------------------------------------------------------------------------
   1-  1 I1     ---     Set     [1/2] Subset (G1)
   3- 12 A10    ---     Name    Shortened object name (JHHMM+DDMM)
                                 as in Table 3 (G2)
  14- 14 A1     ---   f_Name    [a] Flag on Name: a=Dubious Source
  16- 20 F5.1   mJy     F0.84   [6/177]? SUMSS/MOST 0.843GHz flux density
  22- 24 F3.1   mJy   e_F0.84   [0.8/8]? Uncertainty in F0.84
  26- 30 F5.1   mJy     F1.42   [45/112]? ATCA/Parkes SMC 1.42GHz
                                flux density
  32- 34 F3.1   mJy   e_F1.42   [2/6]? Uncertainty in F1.42
  36- 39 F4.1   mJy     F2.37   [4/77.4]? ATCA/Parkes SMC 2.37GHz
                                flux density
  41- 43 F3.1   mJy   e_F2.37   [0.2/4]? Uncertainty in F2.37
  45- 50 F6.2   mJy     F4.8    [2.8/288]? ATCA/Parkes 4.8GHz flux density
  52- 55 F4.1   mJy   e_F4.8    [0.7/15]? Uncertainty in F4.8
  57- 57 A1     ---   f_F4.8    [e] Flag on F4.8 (1)
  59- 62 F4.1   mJy     F4.85   [26/95]? PMN Parkes 64m 4.85GHz
                                flux density
  64- 66 F3.1   mJy   e_F4.85   [6/8]? Uncertainty in F4.85
  68- 71 F4.1   mJy     F5.0    [17/72]? AT20G/ATCA 5.0GHz flux density
  73- 75 F3.1   mJy   e_F5.0    [2/7]? Uncertainty in F5.0
  77- 80 F4.1   mJy     F8.0    [56/72]? AT20G/ATCA 8.0GHz flux density
  82- 84 F3.1   mJy   e_F8.0    [3/4]? Uncertainty in F8.0
  86- 90 F5.2   mJy     F8.6    [6/61]? ATCA/Parkes 8.6GHz flux density
  92- 95 F4.1   mJy   e_F8.6    [1/10]? Uncertainty in F8.6
  97- 97 A1     ---   f_F8.6    [e] Flag on F8.6 (1)
  99-102 F4.1   mJy     F20.0   [46/74]? AT20G/ATCA 20.0GHz flux density
 104-106 F3.1   mJy   e_F20.0   [3/4]? Uncertainty in F20.0
--------------------------------------------------------------------------------
Note (1): The 4.8 and 8.6GHz flux-densities flagged with "e" are measured
    by authors based on the 4.8 and 8.6GHz ATCA radio surveys of the MCs
    i.e., Dickel et al. (2005AJ....129..790D 2005AJ....129..790D) for LMC and Dickel et al.
    (2010AJ....140.1511D 2010AJ....140.1511D) for SMC. Unflagged 4.8 and 8.6GHz measurements
    are drawn from multiple surveys. See the "Description" section above.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
   Bytes Format Units    Label   Explanations
--------------------------------------------------------------------------------
   1-  1 I1     ---      Set     [1/2] Subset (G1)
   3- 12 A10    ---      Name    Shortened object name (JHHMM+DDMM) (G2)
  14- 14 A1     ---    f_Name    [a] Flag on name, a=Dubious Source
  16- 17 I2     h        RAh     [0/6] Hour of right ascension (J2000) (1)
  18- 20 I3     min      RAm     Minute of right ascension (J2000) (1)
  21- 26 F6.2   s        RAs     Second of right ascension (J2000) (1)
  28 -28 A1     ---      DE-     [-] Sign of the declination (J2000) (1)
  29- 30 I2     deg      DEd     [66/73] Degree of declination (J2000)  (1)
  31- 33 I3     arcmin   DEm     Arcminute of declination (J2000) (1)
  34- 39 F6.2   arcsec   DEs     Arcsecond of declination (J2000) (1)
  41- 44 I4     ---      R       [12/7020]? Radio-loudness R parameter (2)
  46- 50 F5.3   ---      z       [0.2/3.4]? Redshift (1)
  52- 56 F5.2   ---      ar      [-0.6/1.4]? Radio spectral index αr
  58- 61 F4.2   ---    e_ar      [0/0.4]? Uncertainty in ar
  63- 67 F5.2   ---      aIR     [-0.5/3.1]? Mid-IR spectral index αIR
  69- 72 F4.2   ---    e_aIR     [0/0.5]? Uncertainty in aIR
  74- 78 F5.2   mag      Imag    [16.5/21.3] I band magnitude (1)
--------------------------------------------------------------------------------
Note (1): The coordinates, z, and I band magnitude for the FSRQ type blazars
    were taken from the MQS catalogue (Kozlowski+ J/ApJ/775/92).
    The coordinates and I band magnitudes for the BL Lac type blazars were
    taken from the featureless spectra list ("FS" list -- priv. comm.)
Note (2): R=F5GHz/FB≥10; see Kellermann+ (1989AJ.....98.1195K 1989AJ.....98.1195K);
    Stocke+ (1992ApJ...396..487S 1992ApJ...396..487S); Ho (2002ApJ...564..120H 2002ApJ...564..120H).
--------------------------------------------------------------------------------
Global notes:
Note (G1): Subset flag as follows:
    1 = FSRQ blazar type candidates (27 occurrences);
    2 = BL Lac type blazar candidates (17 occurrences).
Note (G2): Sources from the Magellanic Quasars Survey (MQS;
 Kozlowski+, 2012, J/ApJ/746/27) are named  in Simbad.
--------------------------------------------------------------------------------
History:
    From electronic version of the journal
(End)                           Prepared by [AAS], Coralie FIX [CDS] 16-Oct-2019