PRODIGE – envelope to disk with NOEMA - VI. The missing sulfur problem

Open Access

Table 1

List of studied NOEMA lines in order of increasing wavelength with atomic data retrieved from Splatalogue³ and CDMS⁴.

ν	Species	Transition	A_ij	E_u	Δν	RMS
(GHz)		Upper–lower	log(s^–1)	(K)	(kHz)	(mJy/beam)
215.5029	$H_{2}^{33} S$ ${\rm{H}}_2^{33}{\rm{S}}$	2_2,0,4–2_1,1,4	–4.374	81.6	2000	[2.0–2.9]
216.7104	H₂S	2_2,0–2_1,1	–4.312	84.0	2000	[2.0–2.9]
216.1474	OC³³S	J = 18–17	–4.420	98.6	62.5	[15–60]
218.9034	OCS	J = 18–17	–4.517	99.8	62.5	[10–50]
231.0615	OCS	J = 19–18	–4.446	111	62.5	[20–80]
237.2736	OC³⁴S	J = 20–19	–4.411	120	2000	[2.5–3.5]

Notes. For $H_{2}^{33} S$ ${\rm{H}}_2^{33}{\rm{S}}$ and OC³³S, the A_ij were calculated from the available data in CDMS. Δν is the channel width with which the transition was observed. In the last column (RMS) we give a range for the typical noise in the datacubes of each transition.

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