Table 1.
Observational conditions.
| Object | RA | Dec | zqso | νobs(EMIR-band), transition | Θbeam | Tsys | texp |
|---|---|---|---|---|---|---|---|
| J2000 | J2000 | [GHz] | [″] | [K] | [h] | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| PSJ0147+4630 | 01:47:10.15 | 46:30:42.5 | 2.377 | 102.40(E0), J = 3-2 | 24.1 | 75 | 11.0 |
| SDSS J0924+0219 | 09:24:55.79 | 02:19:24.9 | 1.523 | 91.37(E0), J = 2-1 | 26.8 | 107 | 8.4 |
| SDSS J1330+1810 | 13:30:18.65 | 18:10:32.9 | 1.393 | 96.34(E0), J = 2-1 | 25.5 | 91 | 18.8 |
| H1413+117 | 14:15:46.24 | 11:29:43.4 | 2.56 | 97.13(E0), J = 3-2 | 25.3 | 82 | 5.5 |
| J2145+6345 | 21:45:05.11 | 63:45:41.2 | 1.56 | 90.05(E0), J = 2-1 | 27.3 | 101 | 8.0 |
| PMNJ0134-0931 | 01:34:35.66 | -09:31:02.9 | 2.22 | 107.39(E0), J = 3-2 | 22.9 | 85 | 7.4 |
| COSMOS5921+0638 | 09:59:21.77 | 02:06:38.3 | 3.14 | 83.53(E0), J = 3-2 | 29.4 | 119 | 8.7 |
| SDSS J1004+4112 | 10:04:34.31 | 41:12:42.5 | 1.74 | 84.14(E0), J = 2-1 | 29.2 | 87 | 8.0 |
| J1042+1641 | 10:42:22.11 | 16:41:15.3 | 2.517† | 98.80(E0), J = 3-2 | 24.8 | 88 | 5.3 |
| HE1113-0641 | 11:16:23.53 | -06:57:38.9 | 1.235 | 103.15(E0), J = 2-1 | 23.8 | 134 | 7.4 |
| SDSS J1138+0314 | 11:38:03.73 | 03:14:57.8 | 2.44 | 100.43(E0), J = 3-2 | 24.4 | 105 | 11.5 |
| HST14113+5211 | 14:11:19.61 | 52:11:29.7 | 2.811 | 90.74(E0), J = 3-2 | 27.1 | 93 | 10.6 |
| B1422+231 | 14:24:38.09 | 22:56:00.6 | 3.62 | 74.85(E0), J = 3-2 | 32.8 | 92 | 11.5 |
| SDSS J1433+6007 | 14:33:22.80 | 60:07:15.6 | 2.74 | 92.46(E0), J = 3-2 | 26.6 | 102 | 6.0 |
| J1817+2729 | 18:17:30.85 | 27:29:40.1 | 3.07 | 84.96(E0), J = 3-2 | 28.9 | 95 | 7.6 |
| B1933+503 | 19:34:30.90 | 50:25:23.2 | 2.64 | 95.05(E0), J = 3-2 | 25.8 | 119 | 3.2 |
| SDSS J2222+2745 | 22:22:09.50 | 27:45:33.8 | 2.82 | 90.52(E0), J = 3-2 | 27.1 | 102 | 2.3 |
Notes. (1) Object name. (2) Right Ascension. (3) Declination. (4) Redshift. (5) Observing CO transition. (6) Beam size. (7) System temperature. (8) Total on-source exposure time. †: the redshift of J1042+1642 was reported as 2.25 by Stacey et al. (2022), while other observations, including X-ray, optical, and near-infrared spectra, all reported a redshift of about 2.52 (Matsuoka et al. 2018; Walton et al. 2022; Glikman et al. 2023). Therefore, we adopted 2.517 as the correct redshift measured from optical spectra of this object (Glikman et al. 2023).
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