A rigorous detection of interstellar CH3NCO: An important missing species in astrochemical networks

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Volume 587 (March 2016)

A&A, 587 (2016) L4

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Table B.3

Model for the IRAM 30 m data based on previously analysed molecular species.

Reference	Studied species	Notes

Tercero et al. (2010) ^†	OCS, CS, H₂CS, HCS⁺, CCS, CCCS	^b^c
Tercero et al. (2011)^†	SiO, SiS	^b^c
Daly et al. (2013) ^†	CH₃CH₂CN	^a^b^c
Esplugues et al. (2013a) ^†	SO, SO₂	^b^c
Esplugues et al. (2013b) ^†	HC₃N, HC₅N	^b^c^d
López et al. (2014) ^†	CH₂CHCN	^a^b^c
Marcelino et al. (in prep.)^†	HCN, HNC, HCO⁺	^b^c^d^e
Demyk et al. (2007)	¹³C-CH₃CH₂CN	^a^c
Margulès et al. (2009)	CH₃CH₂C¹⁵N, CH₃CHDCN, CH₂DCH₂CN	^a^c
Carvajal et al. (2009)	¹³C-HCOOCH₃	^a^c
Marcelino et al. (2009)	HNCO	^c
Margulès et al. (2010)	DCOOCH₃	^a^c
Tercero et al. (2012)	¹⁸O-HCOOCH₃	^a^c
Motiyenko et al. (2012)	NH₂CHO, NH₂CHO ν₁₂ = 1	^a^c
Coudert et al. (2013)	HCOOCH₂D	^a^c
Tercero et al. (2013)	CH₃COOCH₃, CH₃CH₂OCOH	^a^c
Cernicharo et al. (2013)	NH₃D⁺	^a^c
Kolesniková et al. (2013)	c-C₆H₅OH (not detected)	^a^c
Haykal et al. (2013)	CH₂CHCH₂NC (not detected)	^a^c
Bell et al. (2014)	CH₃CN	^b^c
Kolesniková et al. (2014)	CH₃CH₂SH, CH₃SH, CH₃OH, ¹³CH₃OH, CH₃CH₂OH	^a^c
Haykal et al. (2014)	¹³C-HCOOCH₃ν_t=1	^a^c
Tercero et al. (2015)	CH₃CH₂OCH₃	^c^e
Kolesniková et al. (2015)	CH₃COOCHCH₂ (not detected)	^a^c^e
Alonso et al. (2015)	CH₂CHCOOH (not detected)	^a^c^e
López et al. (in prep.)	HCOOCH₃ν_t=0,1,2, CH₃COOH ν_t=0,1,2, CH₂OHCHO	^c^e
In progress	CH₂OCH₂, AG-OHCH₂CH₂OH	^c
In progress	¹³C-CH₃CN, CH₃CN ν₈=1	^c
In progress	CH₃OCH₃, CH₃COCH₃, HCO	^c

Notes.

^(†)

In this analysis we have include all isotopologues and vibrational excited states of the molecule.

^(a)

Papers in collaboration with spectroscopists.

^(b)

Papers dividing the analysis of the Orion surveys in different families of molecules.

^(c)

Papers based on the IRAM 30 m 1D-survey (Tercero et al. 2010) and/or 2D-survey (Marcelino et al., in prep.).

^(d)

Papers based on Herschel/HIFI data.

^(e)

Papers based on ALMA SV data.

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