Molecular gas budget of strongly magnified low-mass star-forming galaxies at cosmic noon

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Table 1.

Summary of the properties of the galaxies included in this study.

Arc	Abbreviation	Coordinates	z_spec	12 + Log[O/H]	μ	Discovery
SGASJ003341.5+024217	J0033	00:33:41.55	2.3900⁽¹⁾	8.61±0.02⁽²⁾	24 $_{- 5}^{+ 9}$ $^{+9}_{-5}$	(1)
		+02:42:16.58⁽¹⁾
SGASJ010842.2+062444	J0108	01:08:42.21	1.9099⁽¹⁾	8.39±0.03⁽²⁾	5 $_{- 2}^{+ 4}$ $^{+4}_{-2}$	(3)
		+06:24:44.41⁽¹⁾
SGASJ090003.3+223408	J0900A/J0900B	09:00:03.33	2.0323⁽¹⁾	8.27±0.02⁽²⁾	6 $_{- 2}^{+ 4}$ $^{+4}_{-2}$ /8 $_{- 3}^{+ 5}$ $^{+5}_{-3}$	(7)
		+22:34:07.57⁽¹⁾
SGAS J105039.6+001730 C.1	J1050	10:50:39.398	3.6258⁽¹⁰⁾	8.30±0.09⁽¹⁰⁾	72 $_{- 10}^{+ 9}$ $^{+9}_{-10}$	(10)
		+00:17:28.78⁽⁶⁾
SGAS J105039.6+001730 A.1	J1050A	10:50:40.358	2.4034⁽¹⁰⁾	8.51±0.02	19±1	(10)
		+00:16:48.54⁽⁶⁾
SGASJ122651.3+215220	J1226A/J1226B	12:26:51.32	2.9252⁽¹⁾	8.22±0.03⁽²⁾	84 $_{- 10}^{+ 13}$ $^{+13}_{-10}$ /31 $_{- 4}^{+ 6}$ $^{+6}_{-4}$	(8)
		+21:52:20.00⁽¹⁾
BG J1429+1202 B	J1429	14:29:54.857⁽¹⁾	2.8241⁽¹⁾	8.45±0.03⁽²⁾	6 $_{- 1}^{+ 2}$ $^{+2}_{-1}$	(12)
		+12:02:38.68
SGAS J152745.1+065219	J1527	15:27:45.17	2.7627⁽¹⁾	8.38±0.04⁽²⁾	12 $_{- 1}^{+ 2}$ $^{+2}_{-1}$	(11)
		+06:52:19.17⁽¹¹⁾
SGASJ211118.9−011431	J2111	21:11:18.95	2.8590⁽¹⁾	8.51±0.02	27 $_{- 10}^{+ 10}$ $^{+10}_{-10}$	(9)
		−01:14:31.44⁽¹⁾
PSZ1G311.6518.4	Sunburst	15:49:59.83	2.3709⁽⁵⁾	8.43±0.03⁽²⁾	171⁽¹³⁾	(4)
		−78:11:13.2⁽⁴⁾

Notes. The first column indicates the complete name of the arc, while the second column shows the abbreviation used in this work. Column 3 indicates the coordinates of each arc, and Column 4 the spectroscopic redshifts. The fifth column presents the metallicity of the galaxies, and column 6 shows the magnification of each of the studied arcs. Column 7 indicates the discovery paper of the galaxy. ⁽¹⁾Rigby et al. (2018), ⁽²⁾Chisholm et al. (2019), ⁽³⁾Rigby et al. (2014), ⁽⁴⁾Dahle et al. (2016), ⁽⁵⁾Rivera-Thorsen et al. (2017), ⁽⁶⁾Sharon et al. (2020), ⁽⁷⁾Diehl et al. (2009), ⁽⁸⁾Koester et al. (2010), ⁽⁹⁾Oguri et al. (2009), ⁽¹⁰⁾Bayliss et al. (2014), ⁽¹¹⁾Koester et al. (2010), ⁽¹²⁾Marques-Chaves et al. (2017), ⁽¹³⁾Solimano et al. (2021).

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