2016AJ....151..120W


C.D.S. - SIMBAD4 rel 1.7 - 2021.05.16CEST20:50:52

2016AJ....151..120W - Astron. J., 151, 120-120 (2016/May-0)

Star formation in 3CR radio galaxies and quasars at z < 1.

WESTHUES C., HAAS M., BARTHEL P., WILKES B.J., WILLNER S.P., KURASZKIEWICZ J., PODIGACHOSKI P., LEIPSKI C., MEISENHEIMER K., SIEBENMORGEN R. and CHINI R.

Abstract (from CDS):

Using the Herschel Space Observatory we have observed a representative sample of 87 powerful 3CR sources at redshift z\lt 1 . The far-infrared (FIR, 70-500 µm) photometry is combined with mid-infrared (MIR) photometry from the Wide-Field Infrared Survey Explorer and cataloged data to analyze the complete spectral energy distributions (SEDs) of each object from optical to radio wavelength. To disentangle the contributions of different components, the SEDs are fitted with a set of templates to derive the luminosities of host galaxy starlight, dust torus emission powered by active galactic nuclei (AGNs), and cool dust heated by stars. The level of emission from relativistic jets is also estimated to isolate the thermal host galaxy contribution. The new data are in line with the orientation-based unification of high-excitation radio-loud AGN, in that the dust torus becomes optically thin longwards of 30 µm . The low-excitation radio galaxies and the MIR-weak sources represent an MIR- and FIR-faint AGN population that is different from the high-excitation MIR-bright objects; it remains an open question whether they are at a later evolutionary state or an intrinsically different population. The derived luminosities for host starlight and dust heated by star formation are converted to stellar masses and star-formation rates (SFR). The host-normalized SFR of the bulk of the 3CR sources is low when compared to other galaxy populations at the same epoch. Estimates of the dust mass yield a 1-100 times lower dust/stellar mass ratio than for the Milky Way, which indicates that these 3CR hosts have very low levels of interstellar matter and explains the low level of star formation. Less than 10% of the 3CR sources show levels of star formation above those of the main sequence of star-forming galaxies.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): galaxies: active - infrared: galaxies - radio continuum: galaxies

VizieR on-line data: <Available at CDS (J/AJ/151/120): table1.dat table2.dat table4.dat table5.dat table6.dat tables10-17.dat>

Simbad objects: 97

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Number of rows : 97

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 3C 6.1 BLL 00 16 31.60 +79 16 51.7   22       ~ 115 1
2 3C 20 Sy2 00 43 09.6 +52 03 35   19.0       ~ 202 0
3 3C 22.0 Sy1 00 50 57.0 +51 12 04   22.0       ~ 143 0
4 NGC 383 rG 01 07 24.95870 +32 24 45.2140   13.6 12.14     ~ 733 3
5 2C 94 Sy2 01 08 52.8701245540 +13 20 14.257796477   15.19       ~ 448 2
6 3C 33.1 Sy1 01 09 44.3 +73 11 57   19.5       ~ 138 1
7 3C 34.0 rG 01 10 18.60 +31 47 20.0   21       ~ 162 2
8 3C 35 QSO 01 12 02.216 +49 28 35.24     15.6     ~ 138 0
9 3C 41.0 rG 01 26 44.30 +33 13 11.0   21       ~ 158 1
10 2E 437 Sy1 01 36 24.4206016519 +20 57 27.523115842   18.15 18.10     ~ 347 2
11 3C 48 QSO 01 37 41.2995845985 +33 09 35.079126038   16.62 16.20     ~ 2585 2
12 3C 49 rG 01 41 09.10 +13 53 28.0   22.327 20.920 20.876   ~ 175 1
13 3C 55.0 rG 01 57 10.7 +28 51 40   20.8       ~ 145 1
14 3C 79.0 Sy2 03 10 00.096140 +17 05 58.61497   19.54 18.75     ~ 245 3
15 2C 349 Sy2 03 58 54.4385123848 +10 26 02.820631972   16.68 15.41     ~ 325 2
16 ICRF J041340.3+111214 Sy1 04 13 40.3410078 +11 12 14.785960   18.96 18.01     ~ 301 2
17 3C 111 Sy1 04 18 21.2773655604 +38 01 35.801523843   19.75 18.05     ~ 874 1
18 Mrk 1506 Sy1 04 33 11.0958197353 +05 21 15.617543663   15.72 15.05 10.08   ~ 1879 2
19 NAME Per B AGN 04 37 04.37510272 +29 40 13.8184969   21.7       ~ 480 2
20 ICRF J052109.8+163822 Sy1 05 21 09.88592749 +16 38 22.0517668   19.37 18.84 18.480   ~ 771 1
21 ICRF J054236.1+495107 Sy1 05 42 36.13789843 +49 51 07.2337251   18.45 17.80 17.210   ~ 1314 1
22 2C 524 Sy2 06 09 32.701768 +48 04 17.04207   21.198 18.00 18.767   ~ 172 1
23 3C 171.0 Sy2 06 55 14.7 +54 08 59   19.94 19.08     ~ 242 0
24 3C 172 rG 07 02 08.31 +25 13 53.5   20.5       ~ 115 0
25 3C 173.1 rG 07 09 18.124 +74 49 31.80   19.982 18.9 17.540   ~ 127 1
26 2E 1790 Sy1 07 13 02.4221654766 +11 46 16.271366187   17.06 16.60     ~ 255 1
27 3C 175.1 rG 07 14 04.60 +14 36 22.0   21.5       ~ 98 2
28 3C 184 rG 07 39 24.40 +70 23 10.0   21.5       ~ 132 1
29 2XMM J080535.0+240951 Sy2 08 05 35.0057673498 +24 09 50.334614040   15.46       ~ 317 1
30 3C 196 Sy1 08 13 36.056090 +48 13 02.63597   18.36 17.79     ~ 491 2
31 3C 200 rG 08 27 25.4 +29 18 45   20       ~ 166 1
32 ICRF J084047.5+131223 Sy1 08 40 47.58841798 +13 12 23.5641152   18.58 18.15 17.622   ~ 394 1
33 3C 217 Rad 09 08 51.0 +37 48 18   22       ~ 122 1
34 ICRF J090933.4+425346 Sy2 09 09 33.4971425 +42 53 46.481984   19.98 19.42 18.220   ~ 469 0
35 3C 219 Sy1 09 21 08.6263828902 +45 38 57.345842278   19.56 18.69     ~ 390 2
36 3C 220.1 BLL 09 32 39.4 +79 06 30   20.5       ~ 130 1
37 3C 220.3 G 09 39 23.40 +83 15 26.2   20.5   20.140   ~ 87 1
38 3C 226.0 Sy1 09 44 16.5 +09 46 16   19.5       ~ 123 2
39 3C 228 rG 09 50 10.7 +14 19 58   21       ~ 157 2
40 7C 095855.89+290131.00 Sy1 10 01 49.5226070599 +28 47 08.913353395   18.21 17.27     ~ 404 1
41 3C 236.0 BLL 10 06 01.7502377 +34 54 10.401469   15.97       ~ 423 2
42 3C 247 QSO 10 58 58.70 +43 01 23.0   21.5       ~ 153 1
43 2E 2389 Sy1 11 04 13.8613944317 +76 58 58.192391742   15.70 15.72 15.40   ~ 515 1
44 3C 254 QSO 11 14 38.7251514286 +40 37 20.333882148   17.62 17.42     ~ 305 2
45 2E 2503 Sy1 11 39 57.0253396181 +65 47 49.482487703   16.50 16.32     ~ 493 1
46 3C 263.1 QSO 11 43 25.083 +22 06 56.08   20       ~ 137 1
47 3C 265.0 Sy1 11 45 29.0 +31 33 50   20.0       ~ 237 0
48 3C 268.1 rG 12 00 19.2 +73 00 46   22       ~ 142 1
49 3C 268.3 Sy1 12 06 24.70656 +64 13 36.8760   21.847 20.790 19.910   ~ 182 1
50 3C 273 BLL 12 29 06.6996828061 +02 03 08.598846466   13.05 14.830 14.11   ~ 5436 1
51 3C 274.1 rG 12 35 31.00 +21 20 51.3   20       ~ 136 1
52 3C 275.1 QSO 12 43 57.6490661384 +16 22 53.396063536   19.23 19.00     ~ 289 1
53 3C 277.2 Sy1 12 53 33.3 +15 42 31   21.5       ~ 146 0
54 2C 1066 SyG 12 56 57.9 +47 20 20   22.0       ~ 269 0
55 2MASX J13211781+4235153 Sy2 13 21 17.813 +42 35 15.38   16.86 16.23     ~ 258 0
56 3C 286 Sy1 13 31 08.2885060664 +30 30 32.960825107   17.51 17.25     ~ 3866 2
57 3C 289 QSO 13 45 26.7 +49 46 31   23       ~ 153 1
58 4C 64.19 rG 13 50 42.04 +64 29 30.0   20.7 20.7 21.1   ~ 76 1
59 3C 300 AGN 14 22 59.9 +19 35 37   19.66 18.73     ~ 186 2
60 IC 1065 Sy2 14 49 21.5921149894 +63 16 13.816373757   17.30 16.39     ~ 344 1
61 ICRF J145907.5+714019 Sy1 14 59 07.5831170610 +71 40 19.867413302   17.24 16.78 17.2   ~ 460 1
62 VV 204 AGN 15 04 57.120 +26 00 58.46   15.24       ~ 277 0
63 4C 26.47 AGN 15 13 40.0227468596 +26 07 23.710955469   16.30       ~ 220 1
64 3C 319.0 rG 15 24 05.60 +54 28 18.4   18.5       ~ 144 1
65 3C 321 Sy2 15 31 43.473 +24 04 18.93   16.0   15.40   ~ 311 1
66 3C 326 Rad 15 52 26.60 +20 06 00.0   17.87 17.08     ~ 212 3
67 NAME 3C 330G2 Sy2 16 09 35.0 +65 56 39   20.33       ~ 260 1
68 2E 3648 Sy1 16 20 21.8184966430 +17 36 23.952696503   16.53 16.41 20.5   ~ 392 2
69 4C 23.43 Sy1 16 24 39.0836869355 +23 45 12.221830474   17.91 17.47     ~ 320 1
70 3C 341 rG 16 28 03.50 +27 41 36.1   19       ~ 135 1
71 3C 337 QSO 16 28 53.9 +44 19 03   20.0       ~ 139 1
72 3C 340 rG 16 29 37.9 +23 20 14   22       ~ 121 1
73 3C 343 Sy2 16 34 33.8067419 +62 45 35.895020   21.06 20.61     ~ 207 1
74 3C 343.1 Sy2 16 38 28.2249692 +62 34 44.313080   20.7 20.7     ~ 157 2
75 3C 345 QSO 16 42 58.8100340220 +39 48 36.999540578   16.81 16.59 16.84   ~ 1581 2
76 3C 349 rG 16 59 32.00 +47 02 16.0   19 19.0     ~ 149 1
77 2A 1705+609 Sy1 17 04 41.3742389551 +60 44 30.522600868   15.65 15.40 15.30   ~ 728 1
78 3C 352 rG 17 10 44.1001 +46 01 29.834   22.8       ~ 139 1
79 ICRF J182931.7+484446 Sy1 18 29 31.7812801678 +48 44 46.158815781   17.05 16.81 16.860   ~ 642 1
80 2MASX J18334627+4727027 Sy1 18 33 46.2946109378 +47 27 02.568353862   18.64 17.24     ~ 195 1
81 ICRF J183503.3+324146 Sy1 18 35 03.3896681512 +32 41 46.856048508   16.50 15.39 10.50   ~ 594 1
82 3C 386.0 rG 18 38 26.237 +17 11 49.75   15.85 14.6     ~ 187 2
83 ICRF J184208.9+794617 Sy1 18 42 08.9910523393 +79 46 17.129210139   16.06 15.38     ~ 1234 0
84 3C 388.0 SyG 18 44 02.417 +45 33 29.81   16.91 15.56     ~ 310 1
85 2C 1590 BLL 18 45 37.60 +09 53 44.0           ~ 72 1
86 3C 401 SyG 19 40 25.2 +60 41 34   19.1       ~ 195 1
87 NAME Cyg A Sy2 19 59 28.35645829 +40 44 02.0966496   16.22 15.10     ~ 2168 2
88 3C 424 BLL 20 48 12.1 +07 01 17   18 18.40     ~ 136 1
89 3C 427.1 rG 21 04 07.3 +76 33 08   23.3 21.1     ~ 146 1
90 2MASX J21234458+2504272 Sy2 21 23 44.582 +25 04 27.23   17.660 16.350     ~ 304 0
91 3C 436 AGN 21 44 11.720 +28 10 18.86   18.5       ~ 176 1
92 2MASX J21555232+3800285 SyG 21 55 52.324 +38 00 28.51   19.20       ~ 216 1
93 3C 441 rG 22 06 04.90 +29 29 20.0   21.0       ~ 186 3
94 3C 452 Sy2 22 45 48.787 +39 41 15.36   17.60 16.56     ~ 345 1
95 3C 454.3 Bla 22 53 57.74798 +16 08 53.5611   16.57 16.10 15.22   ~ 2571 2
96 3C 455.0 Sy2 22 55 03.9 +13 13 35   19.535 19.590 19.190   ~ 188 2
97 2C 1883 Sy2 23 16 35.1925435787 +04 05 18.292942690   17.54 16.68 17.220   ~ 280 1

    Equat.    Gal    SGal    Ecl

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2021.05.16-20:50:52

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