Table 1.
Relations used to include CO lines in SPRITZ for different J and galaxy populations.
| J | Spirals, SF-AGN, | SB-AGN, AGN1, |
|---|---|---|
| SB, Irr | AGN2 | |
| 1 | a | b |
| 2, 3 | c, g | b, g |
| 4 | c, d, e, g | b, d, e, g |
| 5 | c, d, e, f, g | b, d, e, f, g |
| 6, 7, 8 | c, d, e, g | b, d, e, g |
| 9, 10, 11, 12 | b, d, e, g | b, d, e, g |
| 13 | b, e, g | b, e, g |
| ≥14 | h | h |
References. (a) Sargent et al. (2014); (b) Greve et al. (2014); (c) Boogaard et al. (2020); (d) Liu et al. (2015); (e) Rosenberg et al. (2015); (f) Liu et al. (2021); (g) Esposito et al. (2022). For J ≥ 14 we considered the observed CO SLED by (h) Mashian et al. (2015) as reference.
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