Table D.1.
Column description for the data release.
Name | Units | Description |
---|---|---|
ID | ... | Identifier |
RA | hh:mm:ss | Right ascension |
Dec | dd:mm:ss | Declination |
zspec_opticalnir | ... | Optical or near-IR spectroscopic redshift (Salvato et al., in prep.) |
(d)zspec_submm | ... | ALMA submillimeter spectroscopic redshift |
Log_StellarMass | M⊙ | Logarithm of the stellar mass (Chabrier 2003 IMF) |
(d)Total_LIR | L⊙ | Total 8−1000 μm LIR (Draine & Li 2007; Mullaney et al. 2011) |
(d)SF_LIR | L⊙ | LIR, SFR from the star-forming component (LIR, SFR = LIR − LIR, AGN) |
(d)AGN_LIR | L⊙ | LIR, AGN from the AGN component (LIR, AGN = LIR × fAGN) |
(d)fAGN | ... | Fraction of LIR due to the AGN emission |
(d)Mdust | M⊙ | Dust mass (Draine & Li 2007) |
(d)U | ... | Mean intensity of the interstellar radiation field (Draine & Li 2007) |
DistanceMS | ... | Distance from the main sequence as parameterized in Sargent et al. (2014) |
(d)Size | arcsec | Source angular size from ALMA |
OneSigma_Size | arcsec | 1σ upper limit on the source angular size from ALMA |
Probability_Unresolved | Probability of being unresolved (Puglisi et al. 2019) | |
Flux_Line(X) | Jy km s−1 | Velocity integrated flux of line X |
SNR_(X) | ... | Signal to noise ratio of the flux of line X |
OneSigma_(X) | Jy km s−1 | 1σ upper limit on the flux of line X |
Width_(X) | km s−1 | Velocity width of line X |
(d)ApertureCorr_(X) | ... | Applied aperture correction for line X |
Prob_Line(X) | ... | Probability of spurious detection of line X |
Flag_(X) | ... | Quality and usage flag for line X |
FreqContinuumBand(B)_(X) | GHz | Frequency in Band B under line X for the estimate of the continuum emission |
(d)ContinuumBand(B)_(X) | mJy | Continuum emission in Band B under line X |
Notes. This full table is available at the CDS. Lines X: CO (5 − 4), CO (2 − 1), CO (7 − 6), [C I](3P2 − 3P1), [C I](3P1 − 3P0), and CO (4 − 3). Bands B: Band 6, Band 3, and Band 7. The uncertainties have the same name of the quantity that they refer to, preceded by d (e.g., Total_LIR ± dTotal_LIR).
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