| Name . | RA . | Dec. . | Sample . | |$z$| . | log(L6.2/L⊙) . | EW6.2 . | log(L7.7/L⊙) . | log(LIR/L⊙) . | Line . | log(|$L^{\prime }_{\rm CO}$|/L⊙) . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | [hh:mm:ss] . | [dd:mm:ss] . | . | . | . | [|$\mu$|m] . | . | . | . | . |
| NGC 3049 | 09:54:49.59 | +09:16:18.1 | SINGS | 0.006 | 7.81 ± 0.02a | – | – | 9.65 ± 0.02a | CO(3–2) | 7.68 ± 0.21b |
| IRAS 10565 + 2448 | 10:59:18.12 | +24:32:34.5 | local ULIRGs | 0.043 | 9.57 ± 0.01 | – | – | 12.04 ± 0.02c | CO(1–0) | 9.72 ± 0.03c |
| GN26 | 12:36:34.51 | +62:12:40.9 | SMGs | 1.223 | 10.48 ± 0.02 | 0.38 ± 0.04 | 11.01 ± 0.10 | 12.66 ± 0.17c | CO(2–1) | 10.92 ± 0.12c |
| GN70.211 | 12:37:10.60 | +62:22:34.5 | High-|$z$| SFGs | 1.523 | 10.39 ± 0.10 | – | 10.84 ± 0.12 | 11.94 ± 0.17c | CO(1–0) | 10.20 ± 0.12c |
| MIPS506 | 17:11:38.59 | +58:38:38.6 | High-|$z$| SBs | 2.470 | – | 0.30 ± 0.14d | 11.11 ± 0.13 | 12.93 ± 0.09e | CO(3–2) | 10.52 ± 0.09e |
| – | – | – | – | – | – | – | – | – | – |
| Name . | RA . | Dec. . | Sample . | |$z$| . | log(L6.2/L⊙) . | EW6.2 . | log(L7.7/L⊙) . | log(LIR/L⊙) . | Line . | log(|$L^{\prime }_{\rm CO}$|/L⊙) . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | [hh:mm:ss] . | [dd:mm:ss] . | . | . | . | [|$\mu$|m] . | . | . | . | . |
| NGC 3049 | 09:54:49.59 | +09:16:18.1 | SINGS | 0.006 | 7.81 ± 0.02a | – | – | 9.65 ± 0.02a | CO(3–2) | 7.68 ± 0.21b |
| IRAS 10565 + 2448 | 10:59:18.12 | +24:32:34.5 | local ULIRGs | 0.043 | 9.57 ± 0.01 | – | – | 12.04 ± 0.02c | CO(1–0) | 9.72 ± 0.03c |
| GN26 | 12:36:34.51 | +62:12:40.9 | SMGs | 1.223 | 10.48 ± 0.02 | 0.38 ± 0.04 | 11.01 ± 0.10 | 12.66 ± 0.17c | CO(2–1) | 10.92 ± 0.12c |
| GN70.211 | 12:37:10.60 | +62:22:34.5 | High-|$z$| SFGs | 1.523 | 10.39 ± 0.10 | – | 10.84 ± 0.12 | 11.94 ± 0.17c | CO(1–0) | 10.20 ± 0.12c |
| MIPS506 | 17:11:38.59 | +58:38:38.6 | High-|$z$| SBs | 2.470 | – | 0.30 ± 0.14d | 11.11 ± 0.13 | 12.93 ± 0.09e | CO(3–2) | 10.52 ± 0.09e |
| – | – | – | – | – | – | – | – | – | – |
Notes. Column (1): Source name; column (2): Right ascension in units of hours, minutes, and seconds; column (3): Declination in units of degrees, arcminutes, and arcseconds; column (4): Galaxy sample or selection; column (5): Redshift; column (6): PAH 6.2 |$\mu$|m luminosity; column (7): Equivalent width of the PAH 6.2 |$\mu$|m feature; column (8): Infrared luminosity (integrated from 8−1000 |$\mu$|m); column (9): Observed CO line; column (10): CO(1–0) luminosity.
aFrom Smith et al. (2007). IR luminosities are aperture corrected.
bFrom Wilson et al. (2012). Converted to CO(1-0) luminosities using r32/10 = 0.18 ± 0.02.
cFrom Pope et al. (2013). For the CO luminosities, we corrected higher J transitions using the conversion scheme listed in Bothwell et al. (2013): r21/10 = 0.84 ± 0.13, r32/10 = 0.52 ± 0.09, r43/10 = 0.41 ± 0.07.
dFrom Sajina et al. (2007).
eFrom Yan et al. (2010).
| Name . | RA . | Dec. . | Sample . | |$z$| . | log(L6.2/L⊙) . | EW6.2 . | log(L7.7/L⊙) . | log(LIR/L⊙) . | Line . | log(|$L^{\prime }_{\rm CO}$|/L⊙) . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | [hh:mm:ss] . | [dd:mm:ss] . | . | . | . | [|$\mu$|m] . | . | . | . | . |
| NGC 3049 | 09:54:49.59 | +09:16:18.1 | SINGS | 0.006 | 7.81 ± 0.02a | – | – | 9.65 ± 0.02a | CO(3–2) | 7.68 ± 0.21b |
| IRAS 10565 + 2448 | 10:59:18.12 | +24:32:34.5 | local ULIRGs | 0.043 | 9.57 ± 0.01 | – | – | 12.04 ± 0.02c | CO(1–0) | 9.72 ± 0.03c |
| GN26 | 12:36:34.51 | +62:12:40.9 | SMGs | 1.223 | 10.48 ± 0.02 | 0.38 ± 0.04 | 11.01 ± 0.10 | 12.66 ± 0.17c | CO(2–1) | 10.92 ± 0.12c |
| GN70.211 | 12:37:10.60 | +62:22:34.5 | High-|$z$| SFGs | 1.523 | 10.39 ± 0.10 | – | 10.84 ± 0.12 | 11.94 ± 0.17c | CO(1–0) | 10.20 ± 0.12c |
| MIPS506 | 17:11:38.59 | +58:38:38.6 | High-|$z$| SBs | 2.470 | – | 0.30 ± 0.14d | 11.11 ± 0.13 | 12.93 ± 0.09e | CO(3–2) | 10.52 ± 0.09e |
| – | – | – | – | – | – | – | – | – | – |
| Name . | RA . | Dec. . | Sample . | |$z$| . | log(L6.2/L⊙) . | EW6.2 . | log(L7.7/L⊙) . | log(LIR/L⊙) . | Line . | log(|$L^{\prime }_{\rm CO}$|/L⊙) . |
|---|---|---|---|---|---|---|---|---|---|---|
| . | [hh:mm:ss] . | [dd:mm:ss] . | . | . | . | [|$\mu$|m] . | . | . | . | . |
| NGC 3049 | 09:54:49.59 | +09:16:18.1 | SINGS | 0.006 | 7.81 ± 0.02a | – | – | 9.65 ± 0.02a | CO(3–2) | 7.68 ± 0.21b |
| IRAS 10565 + 2448 | 10:59:18.12 | +24:32:34.5 | local ULIRGs | 0.043 | 9.57 ± 0.01 | – | – | 12.04 ± 0.02c | CO(1–0) | 9.72 ± 0.03c |
| GN26 | 12:36:34.51 | +62:12:40.9 | SMGs | 1.223 | 10.48 ± 0.02 | 0.38 ± 0.04 | 11.01 ± 0.10 | 12.66 ± 0.17c | CO(2–1) | 10.92 ± 0.12c |
| GN70.211 | 12:37:10.60 | +62:22:34.5 | High-|$z$| SFGs | 1.523 | 10.39 ± 0.10 | – | 10.84 ± 0.12 | 11.94 ± 0.17c | CO(1–0) | 10.20 ± 0.12c |
| MIPS506 | 17:11:38.59 | +58:38:38.6 | High-|$z$| SBs | 2.470 | – | 0.30 ± 0.14d | 11.11 ± 0.13 | 12.93 ± 0.09e | CO(3–2) | 10.52 ± 0.09e |
| – | – | – | – | – | – | – | – | – | – |
Notes. Column (1): Source name; column (2): Right ascension in units of hours, minutes, and seconds; column (3): Declination in units of degrees, arcminutes, and arcseconds; column (4): Galaxy sample or selection; column (5): Redshift; column (6): PAH 6.2 |$\mu$|m luminosity; column (7): Equivalent width of the PAH 6.2 |$\mu$|m feature; column (8): Infrared luminosity (integrated from 8−1000 |$\mu$|m); column (9): Observed CO line; column (10): CO(1–0) luminosity.
aFrom Smith et al. (2007). IR luminosities are aperture corrected.
bFrom Wilson et al. (2012). Converted to CO(1-0) luminosities using r32/10 = 0.18 ± 0.02.
cFrom Pope et al. (2013). For the CO luminosities, we corrected higher J transitions using the conversion scheme listed in Bothwell et al. (2013): r21/10 = 0.84 ± 0.13, r32/10 = 0.52 ± 0.09, r43/10 = 0.41 ± 0.07.
dFrom Sajina et al. (2007).
eFrom Yan et al. (2010).
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