J/A+A/370/468       Variability of gamma-ray sources             (Torres+, 2001)
A variability analysis of low-latitude unidentified gamma-ray sources
    Torres D.F., Romero G.E., Combi J.A., Benaglia P., Andernach H., Punsly B.
   <Astron. Astrophys. 370, 468 (2001)>
   =2001A&A...370..468T 2001A&A...370..468T
ADC_Keywords: Gamma rays ; Radio sources
Keywords: gamma-rays: observations - gamma-rays: theory -
          ISM: supernova remnants - black holes physics
Abstract:
    We present a study of 40 low-latitude unidentified 3EG gamma-ray
    sources which were found to be not positionally coincident with any
    known class of potential gamma-ray emitters in the Galaxy (Romero et
    al., 1999A&A...348..868R 1999A&A...348..868R). We have performed a variability analysis
    which reveals that many of these 40 sources are variable. These
    sources have, in addition, a steep mean value of the gamma-ray
    spectral index, <Γ≥2.41±0.2, which, combined with the high
    level of variability, seems to rule out a pulsar origin. The
    positional coincidences with uncatalogued candidates to supernova
    remnants were also studied. Only 7 sources in the sample are spatially
    coincident with these candidates, a result that is shown to be
    consistent with the expected level of pure chance association. A
    complementary search for weak radio counterparts was also conducted
    and the results are presented as an extensive table containing all
    significant point-like radio sources within the 40 EGRET fields. We
    argue that in order to produce the high variability, steep gamma-ray
    spectra, and absence of strong radio counterparts observed in some of
    the gamma-ray sources of our sample, a new class of objects should be
    postulated, and we analyze a viable candidate.
File Summary:
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 FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe            80        .   This file
table1.dat        63       40   Unidentified 3EG sources without known possible
                                 galactic counterparts
table1.tex        74      117   LaTeX version of table1
table5.txt       110     2783   Original table5
table5a.dat       36       40   Gamma-source positions
table5b.dat      218     1883   Possible radio-counterparts for each 3EG source.
survey.dat       118      116   Survey references
table6.dat        28      101   SNRs candidates
table7.dat        75       67   Statistical variability of AGNs.
table8.dat        32       75   Variability index I for all low latitude
                                 unidentified sources
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See also:
   J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 1999)
   J/A+AS/131/11 : Radio sources related to gamma-ray emission (Reich+ 1998)
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units       Label   Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---         3EGJ    3EG source designation ("J" omitted)
      10  A1    ---       n_3EGJ    [+*] Note on 3EG source (1)
  12- 17  F6.2  deg         GLON    Galactic longitude
  19- 24  F6.2  deg         GLAT    Galactic latitude
  26- 29  F4.2  deg       e_Pos     Error in the position (2)
  31- 34  F4.2  ---         SI      Spectral index, Γ
                                      (N(E) ∝ E-Γ)
  36- 39  F4.2 ---        e_SI      rms uncertainty on SI
  41- 44  F4.1 10-8cm-2/s   Fgamma  γ-ray flux
  46- 49  F4.1 10-8cm-2/s   sigma   Standard deviation of the flux measurements
  51- 52  I2    ---         Nvp     Number of viewing periods
  54- 58  F5.1  %           mu      Fluctuation index, µ=100σ/<Fgamma>
  60- 63  F4.2  ---         I       Average statistical index of variability,
                                     I=µ/26.9
--------------------------------------------------------------------------------
Note (1): Individual notes:
      *: This source also displays short-term variability
          (Wallace et al., 2000ApJ...540..184W 2000ApJ...540..184W)
      +: Source which was suggested as possible AGN by Hartman et al.
          (1999, Cat. J/ApJS/123/79)
Note (2): Error in the position, assumed to be represented by the 95%
       confidence contours given by the 3EG catalog
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Byte-by-byte Description of file: table5a.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  4  A4    ---     ---       [3EGJ]
   5- 13  A9    ---     3EGJ      Gamma-ray 3EG source designation ("J" omitted)
  17- 18  I2    h       RAh       Right ascension (J2000.0)
  20- 21  I2    min     RAm       Right ascension (J2000.0)
  23- 26  F4.1  s       RAs       Right ascension (J2000.0)
      28  A1    ---     DE-       Declination sign (J2000.0)
  29- 30  I2    deg     DEd       Declination (J2000.0)
  32- 33  I2    arcmin  DEm       Declination (J2000.0)
  35- 36  I2    arcsec  DEs       Declination (J2000.0)
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Byte-by-byte Description of file: table5b.dat
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   Bytes Format Units     Label     Explanations
--------------------------------------------------------------------------------
   1-  4  A4    ---       ---       [3EGJ]
   5- 13  A9    ---       3EGJ      Gamma-ray 3EG source name ("J" omitted)
  15- 17  A3    ---       Seq       Sequential number (or letter) for group of
                                     radio source around gamma-ray source
  19- 23  A5    ---       Survey    Radio survey used (ref. in surveys.dat file)
  25- 41  A17   ---       RSource   Radio source name
  42- 43  I2    h         RAh       ? Right ascension (J2000)
  45- 46  I2    min       RAm       ? Right ascension (J2000)
  48- 52  F5.2  s         RAs       ? Right ascension (J2000)
  55- 60  F6.3  s       e_RAs       ? rms uncertainty on right ascension
      61  A1    ---     n_RAs       [?n] Note (1)
      63  A1    ---       DE-       Declination sign (J2000)
  64- 65  I2    deg       DEd       ? Declination (J2000)
  67- 68  I2    arcmin    DEm       ? Declination (J2000)
  70- 74  F5.2  arcsec    DEs       [0,60]? Declination (J2000)
  76- 83  F8.2  arcsec  e_DEs       ? rms uncertainty on declination
      84  A1    ---     n_DEs       [?n] Note (1)
  88- 94  F7.1  MHz       Freq      ? Observed frequency
      95  A1    ---     u_Freq      [?n] Note (1)
      96  A1    ---     l_Flux      Limit flag on Flux
  97-106  F10.6 Jy        Flux      ? Flux at the observed frequency
     107  A1    ---     n_Flux      [pn] Note (1)
 110-116  F7.5  Jy      e_Flux      ? rms uncertainty on Flux
     117  A1    ---   neFlux      [?np] Note (1)
 119-148  A30   ----      Com       Comments (2)
--------------------------------------------------------------------------------
Note (1): Notes:
       ?: unknown
       n: not analysed
       p: peak flux
Note (2): Abbreviations:
       B: blend of several sources
      EX: extended source
      IS: inverted spectrum
      FS: flat spectrum
     GLC: gravitational lens. candidate
       P: indicates an unresolved source (size limit for NVSS typically
           <20", but more for other surveys).
     Otherwise the DEconvolved size and position angles are given.
      PN: planetary nebula
      SI: spectral index
      SP: possibly spurious source
      SS: steep spectrum
       V: variable
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Byte-by-byte Description of file: survey.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  5  A5    ---     Survey    Survey designation
   6-  7  I2    ---   n_Survey    ? Part of the survey
   9- 27  A19   ---     BibCode   BibCode
  29- 53  A25   ---     Aut       Author's names
  55-118  A64   ---     Com       Comments
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Byte-by-byte Description of file: table6.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  5  F5.1  deg     GLON      Galactic longitude
   7- 11  F5.1  deg     GLAT      Galactic latitude
  13- 18  F6.1  arcmin  Theta     Diameter of the extended source
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Byte-by-byte Description of file: table7.dat
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   Bytes Format Units        Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---          3EGJ      3EG source designation ("J" omitted)
  12- 19  A8    ---          AGN       AGN Name
  23- 27  F5.1  deg          GLON      Galactic longitude
  31- 35  F5.1  deg          GLAT      Galactic latitude
  39- 42  F4.2  ---          SI        ? Spectral index, Γ
                                          (N(E) ∝ E-Γ)
  46- 50  F5.2 10-8cm-2/s    Fgamma    γ-ray flux
  53- 57  F5.1 10-8cm-2/s  e_Fgamma    rms uncertainty on Fgamma
  61- 62  I2    ---          Nvp       Number of viewing periods
  65- 69  F5.1  %            mu        Fluctuation index,
                                        µ=100σ/<Fgamma>
  72- 75  F4.1  ---          I         Average statistical index of variability,
                                        I=mu/26.9
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Byte-by-byte Description of file: table8.dat
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   Bytes Format Units   Label     Explanations
--------------------------------------------------------------------------------
   1-  9  A9    ---     3EGJ      3EG source designation ("J" omitted)
  11- 13  F3.1  ---     I         Average statistical index of variability,
                                          I=mu/26.9
--------------------------------------------------------------------------------
Acknowledgements: Diego Torres 
References:
     Romero et al., Paper I,   1999A&A...348..868R 1999A&A...348..868R
(End)                                          Patricia Bauer [CDS]  16-Feb-2001