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Home All issues Volume 536 (December 2011) A&A, 536 (2011) A14 Full HTML
Planck early results
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Table 3

VLA observations on a set of bright ERCSC sources.

ERCSC name VLA RA VLA Dec S4.86   GHz S8.46   GHz S22.46   GHz S43.34   GHz VLA obs. date Planck obs. datea
[J2000] [J2000] [Jy] [Jy] [Jy] [Jy] [yymmdd] [yymmdd]
G052.38-36.49 21:34:10.3 –01:53:17 ... ... 1.698 1.218 091103 091102, 091103, 091108–091110, 100509–100511, 100517
G056.70+80.65b 13:31:08.3 30:30:33 7.485 5.202 2.516 1.444 091022, 100103 091230, 091231
G075.68-29.62 22:03:26.9 17:25:48 0.987 1.055 1.035 1.073 091211 091121, 091128–091202, 100524–100527, 100602, 100603
G077.45-38.54 22:32:36.4 11:43:51 5.594 5.827 4.407 3.606 091211 091127, 091203–091207, 100531–100603
100506–100510, 100519, 100520
G085.72+26.08 18:24:07.1 56:51:01 1.403 1.876 1.771 1.258 090724 090827–090829, 100417–100422, 100503,100504
G085.86+83.31 13:10:28.7 32:20:44 1.427 2.133 2.856 1.977 100103 091221–091225, 100102, 100103
G085.95-18.77c 22:03:15.0 31:45:38 2.165 2.495 2.576 2.841 091211 091202, 091203, 091211–091215, 100531–100603
G086.12-38.18c 22:53:57.8 16:08:54 9.463 8.176 11.834 21.570 091211 091206, 091207, 091213–091216
G090.11–25.64 22:36:22.5 28:28:57 1.285 1.273 1.412 1.547 091211 091210, 091211, 091218–091221
G090.14+09.66 20:23:55.8 54:27:36 0.952 1.132 0.804 0.502 090724 091222, 091223, 100517, 100518
G092.62–10.44 22:02:43.3 42:16:39 3.994 3.996 3.440 3.085 091211 091213, 091214, 091222–091226, 100606, 100607
G096.08+13.77 20:22:06.7 61:36:59 3.110 3.800 1.946 0.836 090724 091220–091222, 100103–100108, 100526–100531, 100602
G097.46+25.04 18:49:16.1 67:05:42 1.284 2.431 3.553 2.956 090724 091012–091014, 091017–091022, 091112-091114, 091225–091227,
100112–100119, 100512–100514, 100516–100521
G098.28+58.29 14:19:46.6 54:23:14 1.178 1.249 1.231 1.176 100103 091206, 091207, 091209–091212, 091226, 091227
G098.51+25.79 18:42:33.6 68:09:25 0.765 0.892 0.676 0.461 090724 091013–091015, 091110–091112, 091231,
100101, 100116–100119, 100121, 100122, 100514–100516, 100518–100521, 100523, 100524
G110.05+29.07 18:00:45.7 78:28:04 2.098 2.850 2.598 1.936 090724 091011–091016, 091026, 091027, 100202, 100203, 100214–100219
G126.44–64.29c 00:57:34.9 –01:23:28 0.338 0.097 0.060 0.070 091103 100107, 100108
G128.95+11.97 02:17:30.8 73:49:33 4.168 4.090 2.623 1.709 090827 090911–090914, 090920, 090921, 100211, 100212, 100217–100220
G133.94–28.63b 01:37:41.3 33:09:35 5.426 3.140 1.098 0.501 090827, 091211 100130, 100131
G143.55+34.41 08:41:24.4 70:53:42 1.762 1.485 2.267 2.900 091022 091012–091014, 091019, 100316, 100317, 100324–100327
G145.58+64.96 11:53:24.5 49:31:09 1.167 0.949 0.885 0.798 100103 091116–091119, 091125, 091126, 100511, 100512, 100522–100526
G174.47+69.79 11:30:53.3 38:15:19 1.334 1.356 1.019 0.680 100103 091121, 100527
G195.26–33.13 04:23:15.8 –01:20:33 ... ... 7.500 7.289 091103 090828–090830, 090903, 100221, 100225–100227
G199.42+78.39 11:59:31.8 29:14:44 1.609 1.530 1.416 1.141 100103 091204–091207, 091214, 100531, 100601
G200.06+31.89 08:30:52.1 24:11:00 1.269 1.246 1.050 0.825 091022 091021–091023, 091027, 100409, 100410, 100414–100416
G208.18+18.75 07:50:52.0 12:31:05 3.685 4.486 4.400 3.939 091022 091014–091016, 091020, 100404, 100408–100410
G211.33+19.05 07:57:06.6 09:56:35 1.143 1.530 1.863 1.846 091022 091015–091018, 091022, 100406, 100410–100412
G216.97+11.36 07:39:18.0 01:37:04 1.143 1.260 1.514 1.553 091022 091012–091014, 100408–100410
G221.26+22.36 08:25:50.3 03:09:24 0.777 0.737 0.668 0.648 091022 091024, 091025, 100419, 100420
G251.59+52.70 10:58:29.6 01:33:59 3.193 4.186 5.317 5.078 100103 091207–091210, 091216, 100524, 100530–100602
G255.00+81.65 12:24:54.5 21:22:47 1.233 1.267 1.412 1.184 100103 091218–091221
G283.75+74.54c 12:30:49.4 12:23:28 62.000 39.000 12.000 ... 100103 091226–091229, 100104, 100628, 100629

Notes. 

(a)

Planck observation dates record the days that the source is observed by any of the 30, 44 and 70 GHz channels.

(b)

Standard VLA flux calibrator, observed twice. Reported flux densities are the average of the two observations.

(c)

Resolved source in the VLA.

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