J/MNRAS/410/2690    CRATES sources at 30 GHz                 (Peel+, 2011)

One centimetre receiver array-prototype observations of the CRATES sources at 30 GHz. Peel M.W., Gawronski M.P., Battye R.A., Birkinshaw M., Browne I.W.A., Davis R.J., Feiler R., Kus A.J., Lancaster K., Lowe S.R., Pazderska B.M., Pazderski E., Roukema B.F., Wilkinson P.N. <Mon. Not. R. Astron. Soc., 410, 2690-2697 (2011)> =2011MNRAS.410.2690P 2011MNRAS.410.2690P
ADC_Keywords: Radio sources; Active gal. nuclei Keywords: astronomical data bases: miscellaneous - galaxies: active - galaxies: statistics - cosmology: observations Abstract: Knowledge of the population of radio sources in the range ∼2-200GHz is important for understanding their effects on measurements of the cosmic microwave background power spectrum. We report measurements of the 30-GHz flux densities of 605 radio sources from the Combined Radio All-sky Targeted Eight-GHz Survey (CRATES), which have been made with the One Centimetre Receiver Array-prototype (OCRA-p) on the Torun 32-m telescope. The flux densities of sources that were also observed by Wilkinson Microwave Anisotropy Probe (WMAP) and previous OCRA surveys are in broad agreement with those reported here, however a number of sources display intrinsic variability. We find a good correlation between the 30GHz and Fermi gamma-ray flux densities for common sources. We examine the radio spectra of all observed sources and report a number of gigahertz-peaked and inverted spectrum sources. These measurements will be useful for comparison to those from the Low Frequency Instrument of the Planck satellite, which will make some of its most sensitive observations in the region covered here. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 74 605 Flux densities for the CRATES sources from erratum (2011, MNRAS, 415, 2974) -------------------------------------------------------------------------------- See also: VIII/72 : CLASS survey of radio sources (Myers+, 2003) J/ApJS/171/61 : All-Sky Survey of Flat-Spectrum Radio Sources (Healey+, 2007) J/A+A/474/1093 : 30GHz flux densities of CJF sources (Lowe+, 2007) J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010) http://www.jodrellbank.manchester.ac.uk/research/ocra/crates : CRATES Home Page Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Name (JHHMM+DDMM) 12- 13 I2 h RAh Right ascension (J2000) 15- 16 I2 min RAm Right ascension (J2000) 18- 21 F4.1 s RAs Right ascension (J2000) 23 A1 --- DE- Declination sign (J2000) 24- 25 I2 deg DEd Declination (J2000) 27- 28 I2 arcmin DEm Declination (J2000) 30- 33 F4.1 arcsec DEs Declination (J2000) 35- 40 F6.1 mJy S1.4 1.4GHz flux density 42- 45 I4 mJy S4.8 4.8GHz flux density 47- 52 F6.1 mJy S8.4 4.8GHz flux density 54- 59 F6.1 mJy S30 30GHz flux density 61- 65 F5.1 mJy e_S30 rms uncertainty on S30 67- 74 A8 --- Notes Notes (1) -------------------------------------------------------------------------------- Note (1): Notes as follows: e = source shows extension and/or multiple components NC = source where multiple components listed in CRATES have been merged together, where 'N' is the number of components. w = WMAP sources (Gold et al. 2011ApJS..192...15G 2011ApJS..192...15G, preprint 1001.4555) c = CJF sources (Taylor et al. 1996ApJS..107...37T 1996ApJS..107...37T; Lowe et al. 2007, Cat. J/A+A/474/1093) f = Fermi point sources (Abdo et al. 2010, Cat. J/ApJS/188/405) g = Potential gigahertz-peaked spectrum (GPS) sources We note that there are two CLASS lens systems within the sample - J1609+6532 and J1938+6648 (Browne et al. 2003, Cat. VIII/72). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 12-Sep-2011
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line