First detection of NHD and ND2 in the interstellar medium - Amidogen deuteration in IRAS 16293–2422

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Table C.5

HFS components used to reproduce the transition of ND₂.

Frequency	LGINT	Up. state			Lo. state

(MHz)	(nm² MHz)			F′	F₁	I_{D, tot}	F
786 826.0110	−3.4286	1.5	2	0.5	0.5	2	1.5

786 828.1584	−3.2317	1.5	2	1.5	0.5	2	1.5

786 832.1370	−3.2842	1.5	2	2.5	0.5	2	1.5

786 832.2338	−3.0963	2.5	2	3.5	1.5	2	3.5

786 834.3398	−2.9932	2.5	2	2.5	1.5	2	2.5

786 834.9400	−3.0538	2.5	2	1.5	1.5	2	1.5

786 835.0841	−3.2113	2.5	2	0.5	1.5	2	0.5

786 836.6556	−3.1210	1.5	2	2.5	0.5	2	2.5

786 836.7849	−3.0547	1.5	0	1.5	0.5	0	0.5

786 836.9956	−3.2843	2.5	2	1.5	1.5	2	0.5

786 836.9995	−2.6241	2.5	0	2.5	1.5	0	1.5

786 838.1735	−2.9018	2.5	2	2.5	1.5	2	1.5

786 838.3241	−2.3974	2.5	2	4.5	1.5	2	3.5

786 838.9615	−2.6275	2.5	2	3.5	1.5	2	2.5

786 842.7431	−2.7050	1.5	2	3.5	0.5	2	2.5

786 864.1688	−3.4603	0.5	2	1.5	0.5	2	1.5

786 868.6874	−3.0107	0.5	2	1.5	0.5	2	2.5

786 872.8893	−3.1436	0.5	0	0.5	0.5	0	0.5

786 873.4617	−2.8638	0.5	2	2.5	0.5	2	1.5

786 877.9803	−3.0524	0.5	2	2.5	0.5	2	2.5

786 887.3254	−3.4508	1.5	2	2.5	1.5	2	3.5

786 890.0744	−3.3125	1.5	2	1.5	1.5	2	2.5

786 891.7607	−3.4671	1.5	2	0.5	1.5	2	1.5

786 893.4129	−2.9898	1.5	2	3.5	1.5	2	3.5

786 893.6763	−3.1369	1.5	0	1.5	1.5	0	1.5

786 894.0531	−3.4158	1.5	2	2.5	1.5	2	2.5

786 897.8867	−3.4000	1.5	2	2.5	1.5	2	1.5

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