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J/MNRAS/415/1597    PACO catalogue of bright sources          (Massardi+, 2011)

The Planck-ATCA Co-eval Observations project: the bright sample. Massardi M., Bonaldi A., Bonavera L., Lopez-Caniego M., De Zotti G., Ekers R.D. <Mon. Not. R. Astron. Soc., 415, 1597-1610 (2011)> =2011MNRAS.415.1597M
ADC_Keywords: Galaxies, radio ; Active gal. nuclei Keywords: galaxies: active - cosmic background radiation - radio continuum: galaxies - radio continuum: general Abstract: The Planck Australia Telescope Compact Array (Planck-ATCA) Co-eval Observations (PACO) have provided flux density measurements of well-defined samples of Australia Telescope 20GHz (AT20G) radio sources at frequencies below and overlapping with Planck frequency bands, almost simultaneously with Planck observations. We have observed with the ATCA a total of 482 sources in the frequency range between 4.5 and 40GHz in the period between 2009 July and 2010 August. Several sources were observed more than once. In this paper we present the aims of the project, the selection criteria, and the observation and data reduction procedures. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tables1.dat 386 1004 *The PACO bright catalogue
Note on tables1.dat: Catalogue of the 180 sources for which we have a flux density estimation or a lower limit
See also: VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011) J/MNRAS/416/559 : The PACO faint catalogue (Bonavera+, 2011) Byte-by-byte Description of file: tables1.dat
Bytes Format Units Label Explanations
1- 5 A5 --- --- [AT20G] 6- 19 A14 --- AT20G AT20G name (JHHMMSS+DDMMSS) 21- 30 F10.7 h RAhour Right ascension in decimal hours (J2000) 32- 42 F11.7 deg DEdeg Declination in decimal degrees (J2000) 44- 53 A10 "YYYY-MM-DD" Date Observation date 55 A1 --- fs [s-] Flag "s" to identify epochs within 10-days from Planck observations 57 A1 --- fe [e-] Flag "e" for extended sources 59 A1 --- l_S4732 Limit flag on S4732 60- 64 I5 mJy S4732 PACO flux at 4732MHz 65 A1 --- l_S5244 Limit flag on S5244 66- 70 I5 mJy S5244 PACO flux at 5244MHz 71 A1 --- l_S5756 Limit flag on S5756 72- 76 I5 mJy S5756 PACO flux at 5756MHz 77 A1 --- l_S6268 Limit flag on S6268 78- 82 I5 mJy S6268 PACO flux at 6268MHz 83 A1 --- l_S8232 Limit flag on S8232 84- 88 I5 mJy S8232 PACO flux at 8232MHz 89 A1 --- l_S8744 Limit flag on S8744 90- 94 I5 mJy S8744 PACO flux at 8744MHz 95 A1 --- l_S9256 Limit flag on S9256 96-100 I5 mJy S9256 PACO flux at 9256MHz 101 A1 --- l_S9768 Limit flag on S9768 102-106 I5 mJy S9768 PACO flux at 9768MHz 107 A1 --- l_S17232 Limit flag on S17232 108-112 I5 mJy S17232 PACO flux at 17232MHz 113 A1 --- l_S17744 Limit flag on S17744 114-118 I5 mJy S17744 PACO flux at 17744MHz 119 A1 --- l_S18256 Limit flag on S18256 120-124 I5 mJy S18256 PACO flux at 18256MHz 125 A1 --- l_S18768 Limit flag on S18768 126-130 I5 mJy S18768 PACO flux at 18768MHz 131 A1 --- l_S23232 Limit flag on S23232 132-136 I5 mJy S23232 PACO flux at 23232MHz 137 A1 --- l_S23744 Limit flag on S23744 138-142 I5 mJy S23744 PACO flux at 23744MHz 143 A1 --- l_S24256 Limit flag on S24256 144-148 I5 mJy S24256 PACO flux at 24256MHz 149 A1 --- l_S24768 Limit flag on S24768 150-154 I5 mJy S24768 PACO flux at 24768MHz 155 A1 --- l_S32232 Limit flag on S32232 156-160 I5 mJy S32232 PACO flux at 32232MHz 161 A1 --- l_S32744 Limit flag on S32744 162-166 I5 mJy S32744 PACO flux at 32744MHz 167 A1 --- l_S33256 Limit flag on S33256 168-172 I5 mJy S33256 PACO flux at 33256MHz 173 A1 --- l_S33768 Limit flag on S33768 174-178 I5 mJy S33768 PACO flux at 33768MHz 179 A1 --- l_S38232 Limit flag on S38232 180-184 I5 mJy S38232 PACO flux at 38232MHz 185 A1 --- l_S38744 Limit flag on S38744 186-190 I5 mJy S38744 PACO flux at 38744MHz 191 A1 --- l_S39256 Limit flag on S39256 192-196 I5 mJy S39256 PACO flux at 39256MHz 197 A1 --- l_S39768 Limit flag on S39768 198-202 I5 mJy S39768 PACO flux at 39768MHz 204-208 F5.1 mJy e_S4732 rms uncertainty on S4732 210-214 F5.1 mJy e_S5244 rms uncertainty on S5244 216-220 F5.1 mJy e_S5756 rms uncertainty on S5756 222-226 F5.1 mJy e_S6268 rms uncertainty on S6268 228-232 F5.1 mJy e_S8232 rms uncertainty on S8232 234-238 F5.1 mJy e_S8744 rms uncertainty on S8744 240-244 F5.1 mJy e_S9256 rms uncertainty on S9256 246-250 F5.1 mJy e_S9768 rms uncertainty on S9768 252-256 F5.1 mJy e_S17232 rms uncertainty on S17232 258-262 F5.1 mJy e_S17744 rms uncertainty on S17744 264-268 F5.1 mJy e_S18256 rms uncertainty on S18256 270-274 F5.1 mJy e_S18768 rms uncertainty on S18768 276-280 F5.1 mJy e_S23232 rms uncertainty on S23232 282-286 F5.1 mJy e_S23744 rms uncertainty on S23744 288-292 F5.1 mJy e_S24256 rms uncertainty on S24256 294-298 F5.1 mJy e_S24768 rms uncertainty on S24768 300-304 F5.1 mJy e_S32232 rms uncertainty on S32232 306-310 F5.1 mJy e_S32744 rms uncertainty on S32744 312-316 F5.1 mJy e_S33256 rms uncertainty on S33256 318-322 F5.1 mJy e_S33768 rms uncertainty on S33768 324-328 F5.1 mJy e_S38232 rms uncertainty on S38232 330-334 F5.1 mJy e_S38744 rms uncertainty on S38744 336-340 F5.1 mJy e_S39256 rms uncertainty on S39256 342-346 F5.1 mJy e_S39768 rms uncertainty on S39768 349-354 F6.3 --- a Best fit parameter a (1) 357-362 F6.3 --- b Best fit parameter b (1) 365-370 F6.3 GHz v0 Best fit parameter v0 (1) 373-378 F6.3 Jy S0 Best fit parameter S0 (1) 382-386 F5.3 --- chi2 Best fit parameter chi2
Note (1): Best fit parameters in the double power law: S(v)=S0/[(v/v0)-a+(v/v0)-b], where v is the frequency and S is the flux density in Jy.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 01-Mar-2012
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

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