Table 1.
Properties of the sample – first 16 associated systems and then 14 intervening absorbers are presented.
| Target | Other name | zem | zabs | νobs(1) | Scont | Epoch | H I 21-cm references |
|---|---|---|---|---|---|---|---|
| (GHz) | (mJy) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J000557.17+382015.1 | B0003+38A | 0.229 | 0.2288 | 93.808 | 900 | 05–19 | Aditya & Kanekar (2018) |
| J010826.84−003724.1 | UM305 | 1.3753 | 1.3710 | 97.232 | 200 | 04–21 | Gupta et al. (2007) |
| 112.846 (a) | 07–10 | ||||||
| J014652.79−015721.2 | 4C-02.08 | 0.9590 | 0.9589 | 91.059 (a) | 20 | 05–19 | Aditya (2019) |
| J022928.93+004429.5 | J0229+0044 | 1.2161 | 1.2166 | 104.008 | 0.5 | 04–22 | Chowdhury et al. (2020) |
| J022947.23+005308.9 | J0229+0053 | – | 1.1630 | 106.582 | 2 | 04–22 | Chowdhury et al. (2020) |
| J043103.76+203734.2 | PKS0428+20 | 0.219 | 0.2202 | 94.469 | 300 | 07–10 | Vermeulen et al. (2003) |
| J104830.37+353800.8 | B2 1045+35A | 0.8464 | 0.8471 | 124.811 | 20 | 04–21 | Aditya (2019) |
| J120321.93+041419.1 | PKS1200+045 | 1.2243 | 1.2111 | 104.263 | 200 | 04–21 | Aditya & Kanekar (2018) |
| J124823.89−195918.8 | PKS1245−19 | 1.275 | 1.2750 | 101.335 | 20 | 04–21 | Aditya & Kanekar (2018) |
| J132616.51+315409.5 | 4C+32.44 | 0.3680 | 0.3680 | 84.263 | 1000 | 07–10 | Vermeulen et al. (2003) |
| J134733.36+121724.2 | 4C+12.50 | 0.1217 | 0.1217 | 102.765 | 1500 | 07–10 | Morganti et al. (2004) |
| J140700.39+282714.7 | Mrk668 | 0.0768 | 0.0775 | 106.980 | 250 | 07–10 | Gupta et al. (2006) |
| J154015.23−145341.9 | J1540−1453 | 2.104 | 2.1139 | 74.035 | 60 | 04–21 | Gupta et al. (2021) |
| J164801.53+222433.3 | J1648+2224 | 0.8227 | 0.8233 | 126.440 | 100 | 04–21 | Aditya (2019) |
| J194553.51+705548.7 | 1946+708 | 0.1008 | 0.1008 | 104.716 | 48 | 06–10 | Peck et al. (1999) |
| J205252.05+363535.3 | B2-2050+36 | 0.354 | 0.3546 | 85.096 | 214 | 06–10 | Vermeulen et al. (2003) |
| J020346.66+113445.4 | PKS0201+113 | 3.639 | 3.38714 | 131.354 | 100 | 07–10 | Kanekar et al. (2007) |
| 105.089 | 07–10 | ||||||
| J025134.54+431515.8 | Q0248+430 | 1.313 | 0.05151 | 109.624 | 150 | 07–10 | Hwang & Chiou (2004) (1) |
| J074110.70+311200.2 | 0738+313 | 0.6310 | 0.22124 | 94.389 | 800 | 06–10 | Kanekar et al. (2001),(2) |
| J080839.66+495036.5 | SBS0804+499 | 1.4344 | 1.40732 | 95.765 | 200 | 03–19,07–10 | Gupta et al. (2009), (3) |
| J083052.09+241059.8 | 0827+243 | 0.9406 | 0.52476 | 75.600 | 900 | 06–10 | Kanekar & Chengalur (2001), (2) |
| J092136.24+621552.2 | J0921+6215 | 1.4473 | 1.10360 | 109.592 | 1000 | 03–19 | Dutta et al. (2017), (4) |
| J095456.82+174331.2 | 0952+179 | 1.4749 | 0.23780 | 93.126 | 40 | 06–10 | Kanekar & Chengalur (2001) |
| J124355.79+404358.9 | B3 1241+410 | 1.5266 | 0.01714 | 113.329 | 80 | 07–10 | Gupta et al. (2018b) |
| J133335.78+164903.9 | HB1331+170 | 2.0835 | 1.77646 | 83.033 | 500 | 03–19 | Carswell et al. (2011), (2) |
| J140856.48−075226.5 | PKS1406−076 | 1.494 | 1.27464 | 101.351 | 1500 | 03–19,06–10 | Gupta et al. (2012) |
| J162439.09+234512.2 | 3C336 | 0.9272 | 0.65584 | 107.725 (a) | 100 | 06–10 | Curran et al. (2007) |
| J163956.36+112758.7 | J1639+1127 | 0.993 | 0.07909 | 106.823 | 70 | 07–10 | Srianand et al. (2013) |
| J203155.23+121940.4 | PKS2029+121 | 1.215 | 1.11614 | 84.293 (a) | 2000 | 06–10 | Gupta et al. (2012) |
| J235810.87−102008.7 | HB2355−106 | 1.6349 | 1.17304 | 106.090 | 600 | 07–10 | Gupta et al. (2007), (3) |
Notes. Columns: (1, 2) object coordinates and favored name; (3, 4) redshift of emission and absorption, the latter is based on the H I 21 cm absorption peak, except for PKS1200+045 (see text for details); (5) observed frequency, CO(1–0) or CO(2–1) except when indicated otherwise; (6) 3 mm continuum flux density in mJy based on the measurements from NED; (7) epoch of IRAM-30 m observations; (8) H I 21 cm absorption references.
References. (1) Combes et al. (2019), (2) Berg et al. (2015), (3) Quider et al. (2011), (4) Stickel & Kuhr (1993).
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