| . | J1208|$-$|0200 . | J2228|$+$|0152 . | J2239|$+$|0207 . |
|---|---|---|---|
| |$z_{\rm [C\, \small {II}]}$| | 6.1165 ± 0.0002 | 6.0805 ± 0.0004 | 6.2497 ± 0.0004 |
| FWHM |$_{\rm [C\, \small {II}]}$| (km s|$^{-1}$|) | 184 ± 28 | 266 ± 48 | 607 ± 44 |
| |$S_{\rm [C\, \small {II}]}$| (Jy km s|$^{-1}$|) | 0.280 ± 0.056 | 0.253 ± 0.059 | 0.955 ± 0.085 |
| |$L_{\rm {[C\, \small {II}]}}$| (10|$^8 \, L_\odot$|) | 2.71 ± 0.54 | 2.43 ± 0.57 | 9.53 ± 0.85 |
| |$f_{\rm 1.2mm}$| (μJy) | 85 ± 20 | |$\lt $|47 | 1110 ± 26 |
| EW |$_{\rm {[C\, \small {II}]}}$| (μm) | 1.73 ± 0.52 | |$\gt $|2.82 | 0.45 ± 0.04 |
| SFR |$_{\rm [C\, \small {II}]}$| (|$M_\odot$| yr|$^{-1}$|) | 18 ± 4 | 16 ± 5 | 63 ± 8 |
| Assumption: |$T_{\rm d}$| = 47 K, |$\beta$| = 1.6, |$\kappa _{\rm 250}$| = 0.4 cm|$^2$| g|$^{-1}$| | |||
| |$L_{\rm FIR}$| (10|$^{11} \, L_\odot$|) | 1.62 ± 0.37 | |$\lt $|0.94 | 21.74 ± 0.51 |
| |$L_{\rm TIR}$| (10|$^{11} \, L_\odot$|) | 2.29 ± 0.52 | |$\lt $|1.34 | 30.65 ± 0.72 |
| SFR |$_{\rm TIR}$| (|$M_\odot$| yr|$^{-1}$|) | 34 ± 8 | |$\lt $|20 | 453 ± 10 |
| |$M_{\rm dust}$| (|$10^7\, M_{\odot }$|) | 1.2 ± 0.3 | |$\lt $|0.7 | 15 ± 1 |
| |$L_{\rm [C\, \small {II}]}/L_{\rm FIR}$| (|$10^{-3}$|) | 1.67 ± 0.51 | |$\gt $|2.58 | 0.44 ± 0.04 |
| . | J1208|$-$|0200 . | J2228|$+$|0152 . | J2239|$+$|0207 . |
|---|---|---|---|
| |$z_{\rm [C\, \small {II}]}$| | 6.1165 ± 0.0002 | 6.0805 ± 0.0004 | 6.2497 ± 0.0004 |
| FWHM |$_{\rm [C\, \small {II}]}$| (km s|$^{-1}$|) | 184 ± 28 | 266 ± 48 | 607 ± 44 |
| |$S_{\rm [C\, \small {II}]}$| (Jy km s|$^{-1}$|) | 0.280 ± 0.056 | 0.253 ± 0.059 | 0.955 ± 0.085 |
| |$L_{\rm {[C\, \small {II}]}}$| (10|$^8 \, L_\odot$|) | 2.71 ± 0.54 | 2.43 ± 0.57 | 9.53 ± 0.85 |
| |$f_{\rm 1.2mm}$| (μJy) | 85 ± 20 | |$\lt $|47 | 1110 ± 26 |
| EW |$_{\rm {[C\, \small {II}]}}$| (μm) | 1.73 ± 0.52 | |$\gt $|2.82 | 0.45 ± 0.04 |
| SFR |$_{\rm [C\, \small {II}]}$| (|$M_\odot$| yr|$^{-1}$|) | 18 ± 4 | 16 ± 5 | 63 ± 8 |
| Assumption: |$T_{\rm d}$| = 47 K, |$\beta$| = 1.6, |$\kappa _{\rm 250}$| = 0.4 cm|$^2$| g|$^{-1}$| | |||
| |$L_{\rm FIR}$| (10|$^{11} \, L_\odot$|) | 1.62 ± 0.37 | |$\lt $|0.94 | 21.74 ± 0.51 |
| |$L_{\rm TIR}$| (10|$^{11} \, L_\odot$|) | 2.29 ± 0.52 | |$\lt $|1.34 | 30.65 ± 0.72 |
| SFR |$_{\rm TIR}$| (|$M_\odot$| yr|$^{-1}$|) | 34 ± 8 | |$\lt $|20 | 453 ± 10 |
| |$M_{\rm dust}$| (|$10^7\, M_{\odot }$|) | 1.2 ± 0.3 | |$\lt $|0.7 | 15 ± 1 |
| |$L_{\rm [C\, \small {II}]}/L_{\rm FIR}$| (|$10^{-3}$|) | 1.67 ± 0.51 | |$\gt $|2.58 | 0.44 ± 0.04 |
|$^*$|These were measured with a common |${1{^{\prime \prime}_{.}}0}$| aperture. The FIR luminosities were estimated with a graybody spectrum model. The upper limits are the 3 |$\sigma$| values. |$\mathit {SFR}_{\rm [C\, \small {II}]}/M_{\odot }\:$|yr|$^{-1}$| = 1.0 |$\times$| 10|$^{-7}$| (|$L_{\rm [C\, \small {II}]}/L_\odot )^{0.98}$| (De Looze et al. 2011). |$\mathit {SFR}_{\rm TIR}/M_{\odot }\:{\rm yr^{-1}} = 1.49 \times 10^{-10} L_{\rm TIR}/L_\odot$| (Murphy et al. 2011).
| . | J1208|$-$|0200 . | J2228|$+$|0152 . | J2239|$+$|0207 . |
|---|---|---|---|
| |$z_{\rm [C\, \small {II}]}$| | 6.1165 ± 0.0002 | 6.0805 ± 0.0004 | 6.2497 ± 0.0004 |
| FWHM |$_{\rm [C\, \small {II}]}$| (km s|$^{-1}$|) | 184 ± 28 | 266 ± 48 | 607 ± 44 |
| |$S_{\rm [C\, \small {II}]}$| (Jy km s|$^{-1}$|) | 0.280 ± 0.056 | 0.253 ± 0.059 | 0.955 ± 0.085 |
| |$L_{\rm {[C\, \small {II}]}}$| (10|$^8 \, L_\odot$|) | 2.71 ± 0.54 | 2.43 ± 0.57 | 9.53 ± 0.85 |
| |$f_{\rm 1.2mm}$| (μJy) | 85 ± 20 | |$\lt $|47 | 1110 ± 26 |
| EW |$_{\rm {[C\, \small {II}]}}$| (μm) | 1.73 ± 0.52 | |$\gt $|2.82 | 0.45 ± 0.04 |
| SFR |$_{\rm [C\, \small {II}]}$| (|$M_\odot$| yr|$^{-1}$|) | 18 ± 4 | 16 ± 5 | 63 ± 8 |
| Assumption: |$T_{\rm d}$| = 47 K, |$\beta$| = 1.6, |$\kappa _{\rm 250}$| = 0.4 cm|$^2$| g|$^{-1}$| | |||
| |$L_{\rm FIR}$| (10|$^{11} \, L_\odot$|) | 1.62 ± 0.37 | |$\lt $|0.94 | 21.74 ± 0.51 |
| |$L_{\rm TIR}$| (10|$^{11} \, L_\odot$|) | 2.29 ± 0.52 | |$\lt $|1.34 | 30.65 ± 0.72 |
| SFR |$_{\rm TIR}$| (|$M_\odot$| yr|$^{-1}$|) | 34 ± 8 | |$\lt $|20 | 453 ± 10 |
| |$M_{\rm dust}$| (|$10^7\, M_{\odot }$|) | 1.2 ± 0.3 | |$\lt $|0.7 | 15 ± 1 |
| |$L_{\rm [C\, \small {II}]}/L_{\rm FIR}$| (|$10^{-3}$|) | 1.67 ± 0.51 | |$\gt $|2.58 | 0.44 ± 0.04 |
| . | J1208|$-$|0200 . | J2228|$+$|0152 . | J2239|$+$|0207 . |
|---|---|---|---|
| |$z_{\rm [C\, \small {II}]}$| | 6.1165 ± 0.0002 | 6.0805 ± 0.0004 | 6.2497 ± 0.0004 |
| FWHM |$_{\rm [C\, \small {II}]}$| (km s|$^{-1}$|) | 184 ± 28 | 266 ± 48 | 607 ± 44 |
| |$S_{\rm [C\, \small {II}]}$| (Jy km s|$^{-1}$|) | 0.280 ± 0.056 | 0.253 ± 0.059 | 0.955 ± 0.085 |
| |$L_{\rm {[C\, \small {II}]}}$| (10|$^8 \, L_\odot$|) | 2.71 ± 0.54 | 2.43 ± 0.57 | 9.53 ± 0.85 |
| |$f_{\rm 1.2mm}$| (μJy) | 85 ± 20 | |$\lt $|47 | 1110 ± 26 |
| EW |$_{\rm {[C\, \small {II}]}}$| (μm) | 1.73 ± 0.52 | |$\gt $|2.82 | 0.45 ± 0.04 |
| SFR |$_{\rm [C\, \small {II}]}$| (|$M_\odot$| yr|$^{-1}$|) | 18 ± 4 | 16 ± 5 | 63 ± 8 |
| Assumption: |$T_{\rm d}$| = 47 K, |$\beta$| = 1.6, |$\kappa _{\rm 250}$| = 0.4 cm|$^2$| g|$^{-1}$| | |||
| |$L_{\rm FIR}$| (10|$^{11} \, L_\odot$|) | 1.62 ± 0.37 | |$\lt $|0.94 | 21.74 ± 0.51 |
| |$L_{\rm TIR}$| (10|$^{11} \, L_\odot$|) | 2.29 ± 0.52 | |$\lt $|1.34 | 30.65 ± 0.72 |
| SFR |$_{\rm TIR}$| (|$M_\odot$| yr|$^{-1}$|) | 34 ± 8 | |$\lt $|20 | 453 ± 10 |
| |$M_{\rm dust}$| (|$10^7\, M_{\odot }$|) | 1.2 ± 0.3 | |$\lt $|0.7 | 15 ± 1 |
| |$L_{\rm [C\, \small {II}]}/L_{\rm FIR}$| (|$10^{-3}$|) | 1.67 ± 0.51 | |$\gt $|2.58 | 0.44 ± 0.04 |
|$^*$|These were measured with a common |${1{^{\prime \prime}_{.}}0}$| aperture. The FIR luminosities were estimated with a graybody spectrum model. The upper limits are the 3 |$\sigma$| values. |$\mathit {SFR}_{\rm [C\, \small {II}]}/M_{\odot }\:$|yr|$^{-1}$| = 1.0 |$\times$| 10|$^{-7}$| (|$L_{\rm [C\, \small {II}]}/L_\odot )^{0.98}$| (De Looze et al. 2011). |$\mathit {SFR}_{\rm TIR}/M_{\odot }\:{\rm yr^{-1}} = 1.49 \times 10^{-10} L_{\rm TIR}/L_\odot$| (Murphy et al. 2011).
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