Table 1.
Basic CARS sample characteristics from the literature.
| Target | Other name (a) | α (J2000) | δ (J2000) | z(b) | MBJ | f1.4 GHz(c) | f0.1 − 2.4 keV(d) | ICO(1 − 0)(e) | IH I(f) |
|---|---|---|---|---|---|---|---|---|---|
| [h:m:s] | [°:′:″] | [mag] | [mJy] | [10−12 erg s−1 cm−2] | [K km s−1] | [Jy km s−1] | |||
| HE0021–1810 | 00:23:39.4 | −17:53:54 | 0.0537 | −20.44 | 40.0 ± 1.3 | 1.2 ± 0.2 | < 0.1 | ... | |
| HE0021–1819 | 00:23:55.4 | −18:02:51 | 0.0533 | −20.18 | < 2.5 | 1.0 ± 0.1 | 0.4 ± 0.0 | < 2.0 | |
| HE0040−1105 | RBS101 | 00:42:36.9 | −10:49:22 | 0.0419 | −19.38 | < 2.5 | 7.4 ± 0.8 | 1.0 ± 0.1 | < 1.6 |
| HE0045−2145 | MCG-04-03-014 | 00:47:41.2 | −21:29:28 | 0.0214 | −20.09 | 8.0 ± 0.5 | ... | 8.2 ± 0.2 | 3.3 ± 0.1 |
| HE0108−4743 | RBS162 | 01:11:09.7 | −47:27:37 | 0.0239 | −19.92 | < 2.5 | 6.2 ± 0.6 | 2.2 ± 0.1 | ... |
| HE0114−0015 | RBS175 | 01:17:03.6 | 00:00:27 | 0.0458 | −20.29 | 1.3 ± 0.1 | 3.7 ± 0.4 | 0.9 ± 0.1 | < 1.8 |
| HE0119−0118 | Mrk1503 | 01:21:59.8 | −01:02:24 | 0.0548 | −21.35 | 4.2 ± 0.5 | 7.8 ± 1.1 | 2.4 ± 0.1 | < 1.4 |
| HE0150−0344 | 01:53:01.5 | −03:29:23 | 0.0480 | −20.02 | 3.2 ± 0.5 | ... | 0.9 ± 0.1 | 2.7 ± 0.3 | |
| HE0203−0031 | Mrk1018 | 02:06:16.0 | −00:17:29 | 0.0425 | −21.59 | 4.2 ± 0.4 | 3.6 ± 0.3 | < 0.2 | ... |
| HE0212−0059 | Mrk590 | 02:14:33.6 | −00:46:00 | 0.0264 | −21.17 | 16.2 ± 0.6 | 25.5 ± 0.8 | 3.5 ± 0.1 | 2.0 ± 0.2 |
| HE0224−2834 | AM0224-283 | 02:26:25.9 | −28:21:01 | 0.0602 | −20.84 | 2.6 ± 0.5 | 0.8 ± 0.3 | 0.7 ± 0.1 | 2.6 ± 0.3 |
| HE0227−0913 | Mrk1044 | 02:30:05.5 | −08:59:53 | 0.0165 | −19.86 | 2.4 ± 0.5 | 83.4 ± 3.4 | 1.9 ± 0.2 | 2.6 ± 0.2 |
| HE0232−0900 | NGC985 | 02:34:37.8 | −08:47:15 | 0.0427 | −22.04 | 15.3 ± 1.0 | 38.7 ± 2.1 | 6.9 ± 0.3 | 3.3 ± 0.4 |
| HE0253−1641 | 02:56:02.6 | −16:29:15 | 0.0319 | −20.09 | 14.2 ± 1.0 | 2.6 ± 0.6 | 2.9 ± 0.1 | < 2.6 | |
| HE0345+0056 | 03:47:40.2 | 01:05:14 | 0.0310 | −21.26 | 32.0 ± 1.0 | 1.9 ± 0.8 | < 0.1 | ... | |
| HE0351+0240 | RBS489 | 03:54:09.5 | 02:49:31 | 0.0354 | −19.09 | 3.7 ± 0.5 | 4.1 ± 0.4 | < 0.2 | ... |
| HE0412−0803 | 04:14:52.7 | −07:55:40 | 0.0380 | −20.69 | 8.9 ± 0.5 | 2.7 ± 0.2 | < 0.1 | ... | |
| HE0429−0247 | RBS550 | 04:31:37.1 | −02:41:24 | 0.0423 | −19.49 | < 2.5 | 29.0 ± 3.1 | < 0.3 | ... |
| HE0433−1028 | Mrk618 | 04:36:22.2 | −10:22:34 | 0.0355 | −20.76 | 17.0 ± 0.7 | 61.9 ± 4.2 | 9.4 ± 0.3 | < 2.2 |
| HE0853−0126 | 08:56:17.8 | −01:38:08 | 0.0596 | −20.85 | 2.5 ± 0.5 | 18.4 ± 2.9 | 1.3 ± 0.1 | < 1.0 | |
| HE0853+0102 | 08:55:54.2 | 00:51:11 | 0.0527 | −20.32 | 0.9 ± 0.2 | ... | < 0.2 | ... | |
| HE0934+0119 | Mrk707 | 09:37:01.0 | 01:05:43 | 0.0507 | −20.70 | < 2.5 | 14.5 ± 1.1 | < 0.1 | ... |
| HE0949−0122 | Mrk1239 | 09:52:19.2 | −01:36:43 | 0.0197 | −20.12 | 62.2 ± 1.9 | 1.5 ± 0.4 | 1.2 ± 0.1 | 5.9 ± 0.5 |
| HE1011−0403 | PG1011-040 | 10:14:20.6 | −04:18:40 | 0.0587 | −22.26 | < 2.5 | 0.1 ± 0.0 | 1.4 ± 0.1 | < 0.6 |
| HE1017−0305 | Mrk1253 | 10:19:32.9 | −03:20:14 | 0.0491 | −20.80 | < 2.5 | 5.4 ± 0.6 | 1.2 ± 0.1 | < 1.2 |
| HE1029−1831 | 10:31:57.4 | −18:46:34 | 0.0405 | −20.99 | 10.3 ± 0.6 | 5.6 ± 0.9 | 4.2 ± 0.2 | 1.1 ± 0.1 | |
| HE1107−0813 | 11:09:48.5 | −08:30:15 | 0.0585 | −21.44 | 7.3 ± 1.2 | ... | 0.8 ± 0.1 | < 1.0 | |
| HE1108−2813 | ESO438-9 | 11:10:48.0 | −28:30:04 | 0.0240 | −20.88 | 15.2 ± 0.6 | 2.9 ± 0.3 | 8.3 ± 0.3 | < 0.5 |
| HE1126−0407 | PG1126-041 | 11:29:16.6 | −04:24:08 | 0.0605 | −22.69 | 1.2 ± 0.1 | ... | 1.5 ± 0.1 | < 1.8 |
| HE1237−0504 | NGC4593 | 12:39:39.4 | −05:20:39 | 0.0083 | −19.16 | 4.4 ± 0.5 | 40.5 ± 2.0 | 7.5 ± 0.6 | 7.5 ± 0.4 |
| HE1248−1356 | IC3834 | 12:51:32.4 | −14:13:17 | 0.0145 | −16.99 | 2.9 ± 0.6 | ... | 3.0 ± 0.2 | 0.8 ± 0.0 |
| HE1310−1051 | PG1310-109 | 13:13:05.8 | −11:07:42 | 0.0343 | −20.29 | < 2.5 | 4.1 ± 0.4 | < 0.2 | ... |
| HE1330−1013 | MCG-02-35-001 | 13:32:39.1 | −10:28:53 | 0.0225 | −19.30 | < 2.5 | 119.0 ± 10.7 | 1.8 ± 0.2 | 1.8 ± 0.3 |
| HE1338−1423 | RBS1303 | 13:41:13.0 | −14:38:41 | 0.0413 | −21.32 | 5.3 ± 0.6 | 33.2 ± 3.1 | < 0.1 | ... |
| HE1353−1917 | ES O578-9 | 13:56:36.7 | −19:31:45 | 0.0348 | −19.36 | 12.6 ± 0.6 | 2.9 ± 0.7 | 3.2 ± 0.2 | < 2.4 |
| HE1417−0909 | 14:20:06.2 | −09:23:14 | 0.0437 | −20.06 | < 2.5 | 2.2 ± 0.3 | < 0.1 | ... | |
| HE2128−0221 | 21:30:49.9 | −02:08:15 | 0.0527 | −19.76 | < 2.5 | 7.2 ± 1.7 | < 0.1 | ... | |
| HE2211−3903 | ESO344-16 | 22:14:42.0 | −38:48:23 | 0.0397 | −20.62 | 3.5 ± 0.6 | 16.9 ± 1.4 | 1.9 ± 0.1 | ... |
| HE2222−0026 | 22:24:35.3 | −00:11:04 | 0.0581 | −19.97 | < 2.5 | ... | 0.2 ± 0.0 | < 1.2 | |
| HE2233+0124 | 22:35:42.0 | 01:39:33 | 0.0567 | −20.67 | < 2.5 | 1.6 ± 0.5 | 0.9 ± 0.1 | < 2.9 | |
| HE2302−0857 | Mrk926 | 23:04:43.4 | −08:41:09 | 0.0470 | −20.91 | 32.6 ± 1.1 | 30.9 ± 1.3 | 2.3 ± 0.2 | 1.9 ± 0.2 |
Notes.
Accurate systemic redshift of the host galaxies based on the stellar continuum in our observed IFU data.
Flux density at 1.4GHz as measured by the NRAO VLA sky survey (NVSS) and the VLA FIRST survey if undetected in NVSS. For non-detection we assume the completeness limit of NVSS at 2.5 mJy as the upper limit for the source.
CO(1-0) line fluxes and upper limits for non-detection as reported in Bertram et al. (2007).
H I line fluxes and upper limits for non-detection as reported in König et al. (2009).
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