Unlocking the sulphur chemistry in intermediate-mass protostars of Cygnus X - Connecting the cold and warm chemistry

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Table 1

Observational details of the SMA and IRAM observations.

Parameters	SMA Maunakea		IRAM-30 m
	Cyg X-N12	Cyg X-N30	Cyg X-N12
Phase center α ^(a)	20^h36^m57^s.6	20^h38^m36^s.6	20^h36^m57^s.6
δ ^(a)	420	42°370	420
Date of observations	21/06–10/11/2017	20/06–19/10/2017	14–18/08/2019
Spatial resolution	1′′5	1′′5	27′′0 ± 6
Line sensitivity ^(b)	0.15 Jy km s⁻¹ beam⁻¹	0.15 Jy km s⁻¹ beam⁻¹	3 mK for 3 mm band

Notes. ^(a)Coordinates are in the J2000 format. ^(b)The line sensitivity is in ~0.48 km s⁻¹ channels for SMA data and in 0.8 km s⁻¹ channels for IRAM data.

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