Protoplanetary disk masses from CO isotopologue line emission

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Table A.1

Species contained in the ISO chemical network (see Sect. 2.2).

H	He	C	¹³C	N	O	¹⁷O	¹⁸O	Mg	Si
S	Fe	H₂	H	CH	¹³CH	CH₂	¹³CH₂	NH	CH₃
¹³CH₃	NH₂	CH₄	¹³CH₄	OH	¹⁷OH	¹⁸OH	NH₃	H₂O	HO
HO	CO	C¹⁷O	C¹⁸O	¹³CO	¹³C¹⁷O	¹³C¹⁸O	HCN	H¹³CN	HCO
HC¹⁷O	HC¹⁸O	H¹³CO	H¹³C¹⁷O	H¹³C¹⁸O	NO	N¹⁷O	N¹⁸O	H₂CO	H₂C¹⁷O
H₂C¹⁸O	HCO	HC¹⁷O	HC¹⁸O	O₂	O¹⁷O	¹⁷O₂	O¹⁸O	¹⁷O¹⁸O	¹⁸O₂
HS	H₂S	CO₂	CO¹⁷O	C¹⁷O₂	CO¹⁸O	C¹⁷O¹⁸O	C¹⁸O₂	¹³CO₂	¹³CO¹⁷O
¹³C¹⁷O₂	¹³CO¹⁸O	¹³C¹⁷O¹⁸O	¹³C¹⁸O₂	SO	S¹⁷O	S¹⁸O	OCS	¹⁷OCS	¹⁸OCS
O¹³CS	¹⁷O¹³CS	¹⁸O¹³CS	CN	¹³CN	N₂	SiH	CS	¹³CS	HCS
H¹³CS	SO₂	SO¹⁷O	S¹⁷O₂	SO¹⁸O	S¹⁷O¹⁸O	S¹⁸O₂	SiO	Si¹⁷O	Si¹⁸O
H₂CS	HCS	H⁺	H⁻	H	H	He⁺	HCO⁺	HC¹⁷O⁺	HC¹⁸O⁺
H¹³CO⁺	H¹³C¹⁷O⁺	H¹³C¹⁸O⁺	C⁺	¹³C⁺	CH⁺	¹³CH⁺	N⁺	CH	¹³CH
NH⁺	CH	¹³CH	O⁺	¹⁷O⁺	¹⁸O⁺	NH	CH	¹³CH	OH⁺
¹⁷OH⁺	¹⁸OH⁺	NH	CH	¹³CH	H₂O⁺	HO⁺	HO⁺	H₃O⁺	HO⁺
HO⁺	Mg⁺	CN⁺	¹³CN⁺	HCN⁺	H¹³CN⁺	Si⁺	CO⁺	C¹⁷O⁺	C¹⁸O⁺
¹³CO⁺	¹³C¹⁷O⁺	¹³C¹⁸O⁺	HCNH⁺	H¹³CNH⁺	SiH⁺	NO⁺	N¹⁷O⁺	N¹⁸O⁺	SiH
S⁺	O	O¹⁷O⁺	¹⁷O	O¹⁸O⁺	¹⁷O¹⁸O⁺	¹⁸O	HS⁺	H₂S⁺	H₃S⁺
SiO⁺	Si¹⁷O⁺	Si¹⁸O⁺	CS⁺	¹³CS⁺	CO	CO¹⁷O⁺	C¹⁷O	CO¹⁸O⁺	C¹⁷O¹⁸O⁺
C¹⁸O	¹³CO	¹³CO¹⁷O⁺	¹³C¹⁷O	¹³CO¹⁸O⁺	¹³C¹⁷O¹⁸O⁺	¹³C¹⁸O	HCS⁺	H¹³CS⁺	SO⁺
S¹⁷O⁺	S¹⁸O⁺	Fe⁺	SO	SO¹⁷O⁺	S¹⁷O	SO¹⁸O⁺	S¹⁷O¹⁸O⁺	S¹⁸O	HSO
HSO¹⁷O⁺	HS¹⁷O	HSO¹⁸O⁺	HS¹⁷O¹⁸O⁺	HS¹⁸O	SiOH⁺	Si¹⁷OH⁺	Si¹⁸OH⁺	H₂CS⁺	HCS⁺
H₃CS⁺	HCS⁺	HSO⁺	HS¹⁷O⁺	HS¹⁸O⁺	OCS⁺	¹⁷OCS⁺	¹⁸OCS⁺	O¹³CS⁺	¹⁷O¹³CS⁺
¹⁸O¹³CS⁺	HOCS⁺	H¹⁷OCS⁺	H¹⁸OCS⁺	HO¹³CS⁺	H¹⁷O¹³CS⁺	H¹⁸O¹³CS⁺	S	HN	HS
e⁻	PAH⁰	PAH⁺	PAH⁻	PAH:H	JC	J¹³C	JN	JO	J¹⁷O
J¹⁸O	JCH	J¹³CH	JCH₂	J¹³CH₂	JNH	JCH₃	J¹³CH₃	JNH₂	JCH₄
J¹³CH₄	JOH	J¹⁷OH	J¹⁸OH	JNH₃	JH₂O	JHO	JHO	JCO	JC¹⁷O
JC¹⁸O	J¹³CO	J¹³C¹⁷O	J¹³C¹⁸O	JCO₂	JCO¹⁷O	JC¹⁷O₂	JCO¹⁸O	JC¹⁷O¹⁸O	JC¹⁸O₂
J¹³CO₂	J¹³CO¹⁷O	J¹³C¹⁷O₂	J¹³CO¹⁸O	J¹³C¹⁷O¹⁸O	J¹³C¹⁸O₂

Notes. H refers to vibrationally excited H₂; PAH⁰, PAH⁺ and PAH⁻ are neutral, positively and negatively charged PAHs, while PAH:H denotes hydrogenate PAHs; JX refers to species frozen-out onto dust grains.

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