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2011MNRAS.415.1597Massardi+
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.
=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
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Note on tables1.dat: Catalogue of the 180 sources for which we have a flux
density estimation or a lower limit
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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
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Bytes Format Units Label Explanations
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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 chi^2^
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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.
--------------------------------------------------------------------------------
================================================================================
(End) Patricia Vannier [CDS] 01-Mar-2012
J/MNRAS/416/559 PACO faint sources catalog (Bonavera+, 2011)
================================================================================
The Planck-ATCA coeval observations project: the faint sample.
Bonavera L., Massardi M., Bonaldi A., Gonzalez-Nuevo J., De Zotti G.,
Ekers R.D.
=2011MNRAS.416..559B
================================================================================
ADC_Keywords: Galaxies, radio ; Active gal. nuclei
Keywords: galaxies: active - radio continuum: galaxies -
radio continuum: general
Abstract:
The Planck-ATCA Coeval Observations (PACO) project collected data
between 4.5 and 40GHz for 482 sources selected within the Australia
Telescope 20GHz (AT20G) catalogue and observed with the Australia
Telescope Compact Array. Observations were done almost simultaneously
with the Planck satellite, in the period between 2009 July and 2010
August. In this paper, we present and discuss the data for the
complete sample of 159 sources with S_AT20G_>200mJy in the South
Ecliptic Pole region.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
catalog.dat 386 674 The PACO faint catalogue
--------------------------------------------------------------------------------
See also:
J/MNRAS/415/1597 : Bright sources PACO catalogue (Massardi+, 2011)
Byte-by-byte Description of file: catalog.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 --- f1 [s-] Flag "s" to identify epochs within
10-days from Planck observations
57 A1 --- f2 [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 --- v0 ? Best fit parameter {nu}_0_ (1)
373-378 F6.3 mJy S0 ? Best fit parameter S_0_ (1)
382-386 F5.3 --- chi2 ? Best fit parameter {chi}^2^
--------------------------------------------------------------------------------
Note (1): Best fit parameters in the double power law:
S({nu})=S_0_/[({nu}/{nu}_0_)^-a^ + ({nu}/{nu}_0_)^-n^], where
{nu} is the frequency and S is the flux density in Jy.
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History:
From electronic version of the journal
================================================================================
(End) Patricia Vannier [CDS] 03-Mar-2012