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

Home

All issues

Volume 686 (June 2024)

A&A, 686 (2024) A64

Full HTML

Open Access

Table B.1.

Summary of the physical properties derived in this work for our sample, the undetected data set, and GG22.

z bin	log M_⋆ bin	N_obj	z_median	log M_*, median	ΔMS_median	log LIR	T_dust	log M_dust	log M_gas, GDR	log M_gas, S16	f_gas, GDR	f_gas, S16
	(M_⊙)			(M_⊙)	(dex)	(L_⊙)	(K)	(M_⊙)	(M_⊙)	(M_⊙)

					Whole sample
	8≤ log M_⋆< 9	910	1.3	8.41	−0.02	10.26	29.36	7.15	10.00		< 0.98
1.0 ≤z< 1.5	9≤ log M_⋆< 10	299	1.2	9.37	0.00	10.43	29.36	7.35	9.72		< 0.69
	10≤ log M_⋆< 11	92	1.2	10.35	0.07	11.18±0.10	30.04	7.97±0.10	10.02±0.30	10.20±0.10	0.32±0.15	0.42±0.05

	8≤ log M_⋆< 9	1423	1.7	8.41	−0.08	10.21	30.84	6.97	9.97		< 0.97
1.5 ≤z< 2.0	9≤ log M_⋆< 10	353	1.8	9.31	0.13	10.66	33.16	7.28	9.80		< 0.75
	10≤ log M_⋆< 11	96	1.8	10.30	0.17	11.44±0.09	33.49	8.00±0.09	10.14±0.29	10.27±0.09	0.41±0.16	0.48±0.05

	8≤ log M_⋆< 9	881	2.3	8.50	−0.15	10.38	32.59	7.04	10.12		< 0.98
2.0 ≤z< 2.5	9≤log M_⋆< 10	274	2.3	9.31	0.04	10.74	34.70	7.17	9.80		< 0.76
	10≤ log M_⋆< 11	54	2.2	10.38	−0.03	11.61±0.07	33.59	8.16±0.07	10.34±0.27	10.43±0.07	0.47±0.15	0.53±0.04

	8≤ log M_⋆< 9	751	2.7	8.56	0.00	10.58	36.21	6.90	10.03		< 0.97
2.5 ≤z≤ 3.0	9≤ log M_⋆< 10	340	2.8	9.29	0.06	10.84	37.00	7.12	9.82		< 0.77
	10≤ log M_⋆< 11	57	2.7	10.32	−0.02	11.71±0.09	36.03	8.04±0.11	10.29±0.31	10.39±0.11	0.48±0.18	0.54±0.06

					Undetected data set

1.0 ≤z< 1.5	10≤ log M_⋆< 11	85	1.2	10.34	0.06	11.12±0.11	29.93	7.91±0.11	9.97±0.31	10.15±0.11	0.29±0.15	0.39±0.06
1.5 ≤z< 2.0	10≤ log M_⋆< 11	84	1.8	10.29	0.12	11.28±0.12	33.01	7.90±0.12	10.05±0.31	10.14±0.12	0.36±0.17	0.42±0.06
2.0 < z≤ 2.5	10≤ log M_⋆< 11	46	2.2	10.37	−0.03	11.49±0.10	33.64	8.04±0.10	10.22±0.30	10.30±0.10	0.42±0.17	0.46±0.06
2.5 ≤z≤ 3.0	10≤ log M_⋆< 11	47	2.7	10.27	0.00	11.60±0.11	36.17	7.92±0.11	10.19±0.31	10.29±0.11	0.45±0.18	0.51±0.06
					G22

1.0 ≤z< 1.5	10≤ log M_⋆< 11	4	1.2	10.63	0.10	11.77±0.09	30.33	8.56±0.09	10.55±0.29	10.79±0.09	0.46±0.16	0.59±0.05
1.5 ≤z< 2.0	10≤ log M_⋆< 11	9	1.9	10.53	0.34	12.31±0.08	36.02	8.65±0.08	10.74±0.28	10.99±0.08	0.62±0.15	0.74±0.04
2.0 < z≤ 2.5	10≤ log M_⋆< 11	6	2.2	10.65	0.09	12.40±0.12	34.77	8.84±0.12	10.94±0.32	11.02±0.12	0.66±0.17	0.70±0.06
2.5 ≤z≤ 3.0	10≤ log M_⋆< 11	10	2.8	10.49	0.11	12.26±0.18	37.43	8.51±0.18	10.71±0.37	10.89±0.18	0.62±0.20	0.72±0.09

The T_dust are those corresponding to the Schreiber et al. (2018) templates derived for the galaxies. The subindex GDR denotes that the quantity has been calculated using the gas-to-dust ratio approach. The subindex S16 means that the quantity is derived following Scoville et al. (2016). The lack of uncertainty in the gas fractions, gas and dust masses, and luminosities denotes an upper limit (3σ level). Let us recall that for the undetected data set, we also remove the G13 sources in the neighborhood of the GG22 galaxies. We have three of these neighbor objects at 1 < z < 1.5 and another 3 at 1.5 < z < 2.0 in the high-mass bin; 2 at 2.0 < z < 2.5, and none at 2.5 < z < 3.0.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.