Sulfur-bearing molecules in a sample of early star-forming cores

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Volume 692 (December 2024)

A&A, 692 (2024) A97

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Table C.1

CH₃OH integrated emission lines.

Core	W₁^a,†	Error	W₂^b,†	Error
1	14.09	0.26	11.76	0.31
2	18.73	0.47	12.18	0.43
3	13.62	0.50	12.75	0.43
4	18.28	0.14	19.34	0.14
5	4.55	0.38	0.24	0.10
6	34.62	0.92	47.05	0.91
7	57.75	1.20	52.64	0.84
8	11.66	0.44	8.98	0.35
9	35.38	0.62	21.23	0.41
10	1.77	0.06	1.09	0.03
11	40.94	0.50	28.45	0.38
12	5.67	0.13	2.14	0.03
13	21.23	0.34	12.71	0.22
14	78.71	1.82	54.57	1.48
15	34.83	0.85	12.66	0.47
16	10.11	0.15	8.66	0.24
17	30.99	0.45	32.62	0.35
18	10.34	0.12	7.97	0.09
19	34.73	0.46	13.18	0.26
20	109.57	1.02	97.94	0.89
21	15.15	0.31	11.53	0.25
22	36.73	0.78	30.23	0.87
23	95.06	1.31	46.55	1.04
24	26.66	0.86	7.46	0.21
25	7.60	0.29	2.62	0.10
26	6.22	0.32	5.50	0.12
27	7.69	0.24	1.67	0.05
28	11.46	0.42	10.35	0.45
29	225.25	3.70	215.42	3.70
30	157.87	5.33	159.87	6.58
31	42.85	1.92	32.37	1.17
32	91.56	2.01	104.36	2.72
33	11.82	0.46	12.94	0.29
34	30.50	0.12	0.51	0.05
35	0.58	0.04	-	-
36	4.02	0.32	1.15	0.05
37	43.38	1.47	24.77	0.79

^a W1: flux of the 7(1,7)–6(1, 6)++ line.

^b W₂: flux of the 12(1,11)-12(0,12)−+ line.

^† in Jy beam⁻¹ km s⁻¹.

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