Table A.1.
Column description for the data release.
| Name | Units | Description |
|---|---|---|
| ID | ... | Identifier (Valentino et al. 2020a) |
| R.A. | hh:mm:ss | Right ascension |
| Dec | dd:mm:ss | Declination |
| zspec_opticalnir | ... | Optical or near-IR spectroscopic redshift (M. Salvato et al., in prep.) |
| (d)zspec_submm | ... | ALMA submillimeter spectroscopic redshift |
| Log_StellarMass | M⊙ | Logarithm of the stellar mass (Chabrier 2003 IMF, uncertainty: 0.2 dex) |
| (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 |
| 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 |
| Flag_(X) | ... | Quality and usage flag for line X (Flag=1: detection; Flag=0.5: robust upper limit) |
| Lx_210 | erg s−1 | 2−10 keV rest frame logarithmic luminosity (column #50 in Marchesi et al. 2016; negative values: upper limits) |
| Flag_Donley2012 | ... | Donley et al. (2012) AGN classification (Flag=1: AGN; Flag=0: non-AGN) |
Notes. This full table is available at the CDS. More information can be found in Valentino et al. (2020a). Whenever a difference is present, the updated estimates in this table supersede the previous version. – Lines X: CO (5 − 4), CO (2 − 1), CO (7 − 6), [C I](3P2 − 3P1), [C I](3P1 − 3P0), and CO (4 − 3). – The uncertainties have the same name of the quantity that they refer to, preceded by d (e.g., Total_LIR ± dTotal_LIR). Values −99 indicate the absence of data for a specific quantity. – The CO (5 − 4) and CO (2 − 1) fluxes, M⋆, and the angular size estimates for ID = 51280 are from Brusa et al. (2018).
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