Emission-line-selected galaxies at z = 0.6–2 in GOODS South: Stellar masses, SFRs, and large-scale structure

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Volume 580 (August 2015)

A&A, 580 (2015) A42

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Table 3

Physical parameters resulting from SED fitting with fixed redshift.

ID	log(mass)	log(SFR)	Redshift

ELG#	log M_⊙	log(M_⊙/yr)	fixed

3	9.01	0.06	0.619
4	8.63	0.45	1.144
5^c	9.12	1.41	1.86
6	9.04	1.13	1.86
9	8.15	–0.90	0.62
10	9.27	0.21	0.62
11	7.86	–0.91	0.62
12^c	10.21	2.38	1.843
14^c	8.67	0.76	1.85
15^c	9.12	1.58	1.85
16^c	9.87	1.52	1.85
20^c	8.92	1.20	1.85
21^c	8.89	1.07	1.85
22^c	9.40	1.84	1.85
23	8.74	0.74	1.85
25^c	8.86	1.33	1.85
26	8.85	0.36	1.15
28	8.28	–0.37	1.15
34	8.48	–0.63	1.15
35	9.41	1.27	1.85
36	8.31	–0.38	1.15
37	8.49	0.77	1.85
41	8.89	1.02	1.85
43	8.43	–0.29	1.15
45	8.50	–0.55	0.62
51	8.77	0.09	1.15
52	8.43	–0.62	1.15
53	9.61	1.47	1.85
54	9.06	1.53	1.85
55	9.29	1.49	1.15
58	8.68	–0.11	1.15
62	7.97	–1.09	0.62
65	8.61	–0.06	1.15
66¹	8.48	0.48	1.85
68	9.10	0.61	1.85
70	8.99	0.32	1.15
75¹	8.50	0.88	1.85
76	9.55	1.56	1.85
78	9.77	1.10	0.624

		Ambiguous cases

66²	7.91	0.38	1.15
75²	8.02	0.49	1.15
30³	6.72	–1.15	0.62
30³	7.31	–0.82	1.15
30³	7.83	–0.39	1.85

Notes.

^(c)

Cluster member galaxy.

⁽¹⁾

Primary fixed redshift solution used for ELG66 and 75.

⁽²⁾

Secondary fixed redshift solution used for ELG66 and 75.

⁽³⁾

No preferred redshift for ELG30, although z = 0.62 Hα is disfavoured.

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