Table 1.
Extremely luminous Hot DOG sample: Basic properties.
| Name | RA | Dec | zUV | zALMA | Δv | Ang. scale | LIR | Lbol |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | [km s−1] | [kpc/″] | [1013 L⊙] | [1013 L⊙] | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| W0116–0505 | 01h16m01.41s | –05d05m04.1s | 3.173 (a) | 3.1904 (c) | 1250 | 7.71 | 8.2 | 11.7 |
| W0134–2922 | 01h34m35.69s | –29d22m45.4s | 3.0579 (b) | 3.0574 | –44 | 7.82 | 6.2 | 11.3 |
| W0220+0137 | 02h20m52.12s | +01d37m11.6s | 3.122 (a) | 3.1356 | 989 | 7.76 | 9.6 | 12.9 |
| W0236+0528 | 02h36m31.59s | +05d28m03.1s | 2.958 (b) | 2.9559 ( † ) | … | 7.88 | … | … |
| W0410–0913 | 04h10m10.60s | –09d13m05.2s | 3.592 (a) | 3.6301 (d) | 2487 | 7.38 | 11.3 | 16.8 |
| W0831+0140 | 08h31m53.25s | +01d40m10.8s | 3.9128 (b) | 3.9136 | 98 | 7.17 | 12.0 | 18.0 |
| W2246–0526 | 22h46m07.55s | –05d26m35.0s | 4.6021 (b) | 4.6009 | 423 | 6.68 | 22.1 | 34.9 |
Notes. (1) Galaxy name; (2) Right ascension; (3) Declination; (4) Redshift derived from rest-frame UV emission lines: (a)Wu et al. (2012), (b)Eisenhardt et al. (in prep.); (5) Redshift derived from [C II], except (c)CO(4→3) and (d)CO(6→5); (6) Velocity shift between zALMA (either zCO or z[CII]) and zUV, with Δv = c(zIR − zUV)/(1 + zUV); (7) Angular scale; (8) Infrared luminosity (8−1000 μm); (9) Bolometric luminosity. ( † )The line in W0236+0528 is a tentative detection (see Sect. 4.1).
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