The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z = 5.66

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Table 1.

Global physical quantities of HZ10.

Property	Value
(1) z	5.659
(2) D_L [Mpc]	54988
(3) Angular Scale Conversion [kpc/′′]	6.023
(4) log[SFR_IR/(M_⊙ yr⁻¹)]	2.48 $_{- 0.25}^{+ 0.15}$ $^{+0.15}_{-0.25}$
(5) log[SFR_UV/(M_⊙ yr⁻¹)]	1.56 $_{- 0.06}^{+ 0.06}$ $^{+0.06}_{-0.06}$
(6) log[M_⋆/M_⊙]	10.39 $_{- 0.17}^{+ 0.17}$ $^{ +0.17}_{-0.17}$

Notes. Row (1): Lyα redshift. Rows (2) and (3): Luminosity distance and the angular scale conversion factor, respectively. Row (4): IR star-formation rate (SFR_IR). Row (5): rest-UV SFR derived from rest-UV luminosity. Row (6): stellar mass derived from SED fitting to the photometry available in the COSMOS or GOODS-S fields using LE_PHARE. Rows (1), (5) and (6) are taken from Capak et al. (2015). Row (4) are drawn from Faisst et al. (2020).

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