2023MNRAS.519.3526H


Query : 2023MNRAS.519.3526H

2023MNRAS.519.3526H - Mon. Not. R. Astron. Soc., 519, 3526-3545 (2023/March-1)

QUIJOTE scientific results - IX. Radio sources in the QUIJOTE-MFI wide survey maps.

HERRANZ D., LOPEZ-CANIEGO M., LOPEZ-CARABALLO C.H., GENOVA-SANTOS R.T., PERROTT Y.C., RUBINO-MARTIN J.A., REBOLO R., ARTAL E., ASHDOWN M., BARREIRO R.B., CASAS F.J., DE LA HOZ E., FERNANDEZ-TORREIRO M., GUIDI F., HOYLAND R.J., LASENBY A.N., MARTINEZ-GONZALEZ E., PEEL M.W., PICCIRILLO L., POIDEVIN F., RUIZ-GRANADOS B., TRAMONTE D., VANSYNGEL F., VIELVA P. and WATSON R.A.

Abstract (from CDS):

We present the catalogue of Q-U-I JOint TEnerife (QUIJOTE) Wide Survey radio sources extracted from the maps of the Multi-Frequency Instrument compiled between 2012 and 2018. The catalogue contains 786 sources observed in intensity and polarization, and is divided into two separate sub-catalogues: one containing 47 bright sources previously studied by the Planck collaboration and an extended catalogue of 739 sources either selected from the Planck Second Catalogue of Compact Sources or found through a blind search carried out with a Mexican Hat 2 wavelet. A significant fraction of the sources in our catalogue (38.7 per cent) are within the |b| ≤ 20° region of the Galactic plane. We determine statistical properties for those sources that are likely to be extragalactic. We find that these statistical properties are compatible with currently available models, with a ∼1.8 Jy completeness limit at 11 GHz. We provide the polarimetric properties of (38, 33, 31, 23) sources with P detected above the $99.99{{\ \rm per\, cent}}$ significance level at (11, 13, 17, 19) GHz respectively. Median polarization fractions are in the 2.8-4.7 per cent range in the 11-19 GHz frequency interval. We do not distinguish between Galactic and extragalactic sources here. The results presented here are consistent with those reported in the literature for flat- and steep-spectrum radio sources.

Abstract Copyright: © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): cosmic background radiation - radio continuum: galaxies

Simbad objects: 22

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Number of rows : 22
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 6C 013354+473615 Bla 01 36 58.59480326 +47 51 29.1000720     19.50 19.25 15.21 ~ 537 1
2 SNR G130.7+03.1 SNR 02 05 35.73 +64 49 41.3           ~ 661 4
3 NGC 1275 Bla 03 19 48.1599902040 +41 30 42.108850836   13.10 12.48 11.09   ~ 4243 3
4 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
5 IC 443 SNR 06 17 00.0000000 +22 34 11.998901           ~ 1314 1
6 7C 064253.00+445430.00 Bla 06 46 32.02599653 +44 51 16.5901185   19.57 18.49 18.64   ~ 370 1
7 PG 0851+202 BLL 08 54 48.8749846272 +20 06 30.639583620   15.649 15.146 15.446   ~ 2513 1
8 4C 39.25 Bla 09 27 03.01394144 +39 02 20.8518067   17.17 17.00 16.486   ~ 1036 1
9 7C 112812.59+383153.00 Bla 11 30 53.28261620 +38 15 18.5469361   19.11 18.80 19.42   ~ 233 1
10 3C 273 BLL 12 29 06.6998257176 +02 03 08.597629980   13.05 14.830 14.11   ~ 6022 1
11 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
12 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4558 2
13 QSO B1413+135 BLL 14 15 58.81751033 +13 20 23.7128587   21.055 20.000 18.461   ~ 476 1
14 PCCS1 030 G002.22+65.93 ? 14 16 01.5916 +13 21 54.720           ~ 1 0
15 QSO B1502+1041 Bla 15 04 24.97978391 +10 29 39.1985309   18.97 18.56 18.94   ~ 634 1
16 4C 09.57 BLL 17 51 32.81857326 +09 39 00.7284066   17.46 16.78 15.57   ~ 1007 1
17 SNR G068.8+02.6 SNR 19 52 55 +32 54.2           ~ 361 1
18 MCG+07-41-003 Bla 19 59 28.35656837 +40 44 02.0972325   16.22 15.10     ~ 2537 2
19 NAME BL Lac BLL 22 02 43.2913536816 +42 16 39.979416792   15.66 14.72     ~ 2397 1
20 4C 31.63 BLL 22 03 14.9756830008 +31 45 38.269473228   15.85 15.58 14.33   ~ 523 1
21 3C 454.3 Bla 22 53 57.7480438728 +16 08 53.561508864   16.57 16.10 15.22   ~ 3004 2
22 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

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