Measuring the gas reservoirs in 108 < M⋆ < 1011 M⊙ galaxies at 1 ≤ z ≤ 3

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Volume 686 (June 2024)

A&A, 686 (2024) A64

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Table 1.

Summary of the properties of our data set and the comparison samples shown in Fig. 2 and described in Sect. 3.

	z	log M_⋆	i − H	b − i	ΔMS
		(M_⊙)	(mag)	(mag)	(dex)
Mass-complete samples

This work	1.9 $_{1.5}^{2.4}$ $_{1.5}^{2.4}$	8.6 $_{8.3}^{9.1}$ $_{8.3}^{9.1}$	0.81 $_{0.29}^{1.31}$ $_{0.29}^{1.31}$	0.12 $_{- 0.04}^{0.35}$ $_{-0.04}^{0.35}$	$- 0 . 03_{- 0.25}^{0.17}$ $-0.03_{-0.25}^{0.17}$
COSMOS2020^* (W22)	1.8 $_{1.3}^{2.2}$ $_{1.3}^{2.2}$	9.0 $_{8.6}^{9.6}$ $_{8.6}^{9.6}$	0.85 $_{0.51}^{1.21}$ $_{0.51}^{1.21}$	0.59 $_{0.37}^{0.89}$ $_{0.37}^{0.89}$	$- 0 . 06_{- 0.39}^{0.28}$ $-0.06_{-0.39}^{0.28}$

Individual (sub-)mm detections + stacks

T20	1.4 $_{1.1}^{2.0}$ $_{1.1}^{2.0}$	10.6 $_{10.4}^{10.8}$ $_{10.4}^{10.8}$	1.87 $_{1.45}^{2.36}$ $_{1.45}^{2.36}$	0.95 $_{0.76}^{1.40}$ $_{0.76}^{1.40}$	$0 . 33_{0.02}^{0.67}$ $0.33_{0.02}^{0.67}$

Individual (sub-)mm detections

Super-deblended (K21)	1.6 $_{1.1}^{2.0}$ $_{1.1}^{2.0}$	10.4 $_{10.1}^{10.7}$ $_{10.1}^{10.7}$	1.85 $_{1.35}^{2.34}$ $_{1.35}^{2.34}$	1.24 $_{0.88}^{1.71}$ $_{0.88}^{1.71}$	$0 . 34_{0.14}^{0.55}$ $0.34_{0.14}^{0.55}$
A³COSMOS (L19)	2.1 $_{1.8}^{2.6}$ $_{1.8}^{2.6}$	10.7 $_{10.5}^{10.9}$ $_{10.5}^{10.9}$	1.89 $_{1.46}^{2.27}$ $_{1.46}^{2.27}$	1.24 $_{0.86}^{1.61}$ $_{0.86}^{1.61}$	$0 . 58_{0.36}^{0.76}$ $0.58_{0.36}^{0.76}$
GG22	2.2 $_{1.9}^{2.7}$ $_{1.9}^{2.7}$	10.5 $_{10.3}^{10.7}$ $_{10.3}^{10.7}$	1.98 $_{1.30}^{2.54}$ $_{1.30}^{2.54}$	0.82 $_{0.41}^{1.36}$ $_{0.41}^{1.36}$	$0 . 46_{0.22}^{0.83}$ $0.46_{0.22}^{0.83}$

Notes. The comparison samples are limited to the redshifts and stellar masses studied in this work. The values here shown correspond to the median and first and third quartiles. The names between brackets refer to the scaling relations that are based on each data set (see Sect. 5.2). W22 refers to the Wang et al. (2022) relation, K21 to the relation from Kokorev et al. (2021), and L19 to that of Liu et al. (2019a). The T20 data set was used in that same work to obtain their scaling relation.

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