Table 2
Luminosity (2) of the [OIII]λ5007 line (Zakamska et al. 2003) is given in logarithmic units of L⊙.
| Object | log[OIII] |
|
M(H2) | FWHM CO | V CO − [OIII] | F 60 μm | F 100 μm | L FIR | L IR | ||||
| ×109 | ×109M⊙ | km s-1 | km s-1 | mJy | mJy | ×1012L⊙ | ×1012L⊙ | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (10) | (11) | ||||
|
|
|||||||||||||
| SDSS J0903+02 | 8.42 | <12.0 | <9.6 | – | – | 390 | 540 | 2.5 | 3.8 | ||||
| SDSS J1337-01 | 8.72 | <5.3 | <4.3 | – | – | 140 | N/A | 1.4 |
2.1 |
||||
| SDSS J1520-01 | 8.29 | <6.8 | <5.4 | – | – | N/A | 490 | 1.2 |
1.8 |
||||
| SDSS J1543-00 | 8.40 | 11.7 ± 1.8 | 9.4 ± 1.4 | 575 ± 102 | 128 ± 47 | 130 | N/A | 1.1 |
1.65 |
||||
Notes. (3) is in units of ×109 K km s-1 pc2, where the upper limits correspond to 3σ. A conversion factor α = 0.8 M⊙ (K km s-1 pc2)-1 has been assumed to calculate the molecular gas mass (4), with M(H
. VCO − [OIII] is the velocity redshift of the CO(1–0) line relative to zSDSS. Columns (8) and (9) give the total infrared (~8–1000 μm) and far-infrared (~40–500 μm) IRAS fluxes in mJy, while the luminosities are shown in (10) and (11) in units of ×1012L⊙.
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