Table A.1.
Structure of our 4 deg2 mock galaxy catalog.
| Column | Name | Unit | Description |
|---|---|---|---|
| 1 | id | – | source id |
| 2 | ra | degree | source position |
| 3 | dec | degree | source position |
| 4 | z | – | source redshift |
| 5 | mass | M⊙ | Stellar mass |
| 6 | SFR | M⊙ yr −1 | Star formation rate |
| 7 | passive | – | ==1 if this source is passive, otherwise active |
| 8 | LIR | L⊙ | total IR luminosity |
| 9-28 | fbands | Jy | flux density at several bandsa |
| 29 | AGN | – | ==1 if this source is assigned to an AGN |
| 30 | qir | – | qIR values for non-AGNs |
| 31 | L1.4GHz | W Hz−1 | rest-frame 1.4 GHz luminosity |
| 32 | αlow | – | spectral slope at 150 and 350 MHzb |
| 33 | αhigh | – | spectral slope at 1.4, 3, 10 and 15 GHzb |
| 34-39 | ffrequency | Jy | flux density at multiple frequenciesc |
| 40 | theta | degree | position angle |
| 41 | ellipticity | – | ellipticity of non-AGNs |
| 42 | Reff | kpc | efftive radius of non-AGNs |
Notes. The previous 28 columns were generated by EGG (see details in Schreiber et al. 2017). The later columns are information of our mock radio AGNs and non-AGNs. a: u,g,r,i,z bands of SDSS, F606W, F775W, F814W from HST, F140W, F160W,F444W from JWST, Ks band from WIRCAM, 3.6, 4.5, 5.0, 8.0 μm from IRAC, 24 μm from MIPS, 250, 350, 500 μm from Herschel. b: The spectral slope of AGNs at low and high frequencies are the same. c: We provide flux densities at 150 MHz, 350 MHz, 1.4 GHz, 3 GHz, 10 GHz and 15 GHz. Flux densities at other frequencies can be easily derived from L1.4GHz.
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