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1998A&AS..131..303Stanghellini+
J/A+AS/131/303      GHz-Peaked-Spectrum radio sources (Stanghellini+ 1998)
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A complete sample of GHz-Peaked-Spectrum radio sources and its radio properties
    Stanghellini C., O'Dea C.P., Dallacasa D., Baum S.A., Fanti R., Fanti C.
   
   =1998A&AS..131..303S      (SIMBAD/NED BibCode)
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ADC_Keywords: Radio sources
Keywords: galaxies: active - quasars: general - radio continuum: galaxies

Abstract:
    We define a complete sample of thirty-three GHz-Peaked-Spectrum (GPS)
    radio sources based on their spectral properties. We present
    measurements of the radio spectra and polarization of the complete
    sample and a list of additional GPS sources which fail one or more
    criteria to be included in the complete sample. The majority of the
    data have been obtained from quasi-simultaneous multi-frequency
    observations at the Very Large Array (VLA) during 3 observing
    sessions. Low frequency data from the Westerbork Synthesis Radio
    Telescope (WSRT) and from the literature have been combined with the
    VLA data in order to better define the spectral shape. The objects
    presented here show a rather wide range of spectral indices at high
    and low frequencies, including a few cases where the spectral index
    below the turnover is close to the theoretical value of 2.5 typical of
    self-absorbed incoherent synchrotron emission. Faint and diffuse
    extended emission is found in about 10% of the sources. In the
    majority of the GPS sources, the fractional polarization is found to
    be very low, consistent with the residual instrumental polarization of
    0.3%.

File Summary:
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  FileName      Lrecl  Records   Explanations
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ReadMe             80        .   This file
table4.dat         30      378   Flux densities for the complete sample
table5.dat         30      162   Flux densities for the additional objects
tables.tex         90      984   LaTeX version of the tables
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See also:
   VIII/42 : Texas Survey of radio sources at 365MHz (Douglas+ 1996)
   VIII/16 : Molonglo Reference Catalogue of Radio Sources (Large+ 1991)
   VIII/5  : Bright Extragalactic Radio Sources (1Jy) (Kuehr+, 1981)
   VIII/37 : The Third Bologna Survey (B3) (Ficarra+ 1985)
   VIII/18 : 6C Survey of radio sources I. (Baldwin+ 1985)
   VIII/21 : 6C Survey of radio sources II. (Hales+ 1988)
   VIII/22 : 6C Survey of Radio Sources III. (Hales+ 1990)
   VIII/23 : 6C Survey of radio sources IV. (Hales+ 1991)
   VIII/24 : 6C Survey of Radio Sources V. (Hales+ 1993)
   VIII/25 : 6C Survey of radio sources VI. (Hales+ 1993)

Byte-by-byte Description of file: table4.dat table5.dat
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   Bytes Format Units   Label     Explanations
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   1-  8  A8    ---     Name      Source Name (1)
  10- 15  F6.3  GHz     nu        Frequency
  17- 21  F5.3  Jy      Snu       Flux density
  23- 27  F5.3  Jy    e_Snu       rms uncertainty on S (2)
  29- 30  I2    ---   r_Snu       References (3)
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Note (1): Individual notes:
  0108+388: the flux density at 608 MHz and higher frequencies refers to
             the core only, while the flux density measure at 325 MHz likely
             includes the extended structure found close to the main compact
             component (Baum et al. 1990).
  0552+398: the flux density at 37 GHz is the average of the data taken in 1990
             (Terasranta et al., 1992A&AS...94..121T), and the error is the
             r.m.s of the distribution. The flux density at 90GHz is the average
             of the data taken in 1990 (Steppe et al., 1992A&AS...96..441S), and
             the error is the r.m.s of the distribution.
  2134+004: The flux density at 87 GHz is the average of the data taken between
             1985 and 1988 (Terasranta et al., 1992A&AS...94..121T), the error
             is the r.m.s of the distribution.
Note (2): The errors are taken as 3% if they were found in literature to be
            less then 3%.
Note (3): 1: VLA first session
          2: VLA second session
          3: VLA third session
          4: WSRT
          5: Northern Cross
          6: Ratan 600
          7: Douglas et al., 1996AJ....111.1945D, Cat. 
          8: Large et al., 1981MNRAS.194..693L, Cat. 
          9: Kuhr et al., 1981A&AS...45..367K, Cat. 
         10: Baum et al., 1990A&A...232...19B
         11: de Bruyn, private communication
         12: de Bruyn, 1990, in Proc. Dwingeloo Workshop, Compact Steep
              Spectrum and GHz Peaked Spectrum Radio Sources, ed. C. Fanti,
              R.Fanti, C.P. O'Dea, & R.T. Schilizzi, (Bologna: Istituto di
              Radioastronomia), p.105
         13: Steppe et al., 1988A&AS...75..317S
         14: Chandler, 1995, VLA Test Memo 192
         15: Ficarra et al., 1985A&AS...59..255F, Cat. 
         16: Esko, private communication
         17: Gower et al., 1967MmRAS..71...49G,
             Pilkington et al., 1965MmRAS..69..183P
         18: Dennison et al., 1981AJ.....86.1604D
         19: Edelson, 1987AJ.....94.1150E
         20: Terasranta et al., 1992A&AS...94..121T
         23: Fiedler et al., 1987ApJS...65..319F
         24: Steppe et al., 1992A&AS...96..441S
         25: Baldwin et al., 1985MNRAS.217..717B, Cat. 
         26: Hales et al., 1988MNRAS.234..919H, Cat. 
         27: Hales et al., 1990MNRAS.246..256H, Cat < VIII/22>
         28: Hales et al., 1991MNRAS.251...46H, Cat. 
         29: Hales et al., 1993MNRAS.262.1057H, Cat. 
         30: Hales et al., 1993MNRAS.263...25H, Cat. 
         31: Khabrakhmanov, private communication.
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Acknowledgements: Carlo Stanghellini 
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(End)                                         Patricia Bauer [CDS]   19-Mar-1998