CDMS

Diazenylium

N-15-N-15-H+

v=0

Tag: 31516

Version: 1*

Date of Entry: Aug. 2, 2017

Contributor: H. S. P. Müller

A	0 MHz
B	44132.188 MHz
C	0 MHz

µ_a	3.4 D
µ_b	0 D
µ_c	0 D

detected in ISM/CSM	no
Egy	0.0 1/cm
HTML-Title	N-15-N-15-H+
Isotope Corr.	-4.872
Lines Listed	22
log STR0	-6.0
log STR1	-4.0
Max. Frequency	2000 GHz
Max. J	22

	All
Q(2.725 /K)	1.6817
Q(5.0 /K)	2.7249
Q(9.375 /K)	4.7755
Q(18.75 /K)	9.1939
Q(37.5 /K)	18.0435
Q(75.0 /K)	35.7502
Q(150.0 /K)	71.1733
Q(225.0 /K)	106.6059
Q(300.0 /K)	142.0478

Description

The rest frequencies were taken from
(1) L. Dore, L. Bizzocchi, E. S. Wirström, C. Degli Esposti, F. Tamassia, and S. B. Charnley, 2017, Astron. Astrophys. 604, Art. No. A26.
The predictions are sufficiently accurate for all radio astronomical observations.
The dipole moment was assumed to agree with that of the main species, see e029506.cat.

ID	Name	Type
8902	c031516.cat	mrg
8903	c031516.egy	egy
8904	15N2H+.lin	lin
8905	c031516i.cat	cat

Filename	Type	Comment	Createdate
c031516i.cat	cat	Predicted transition frequencies without experimental values	Sept. 26, 2017, 6:40 p.m.
e031516.cat	doc	wundervolle CDMS-Dokumentation	Sept. 26, 2017, 6:33 p.m.
c031516.egy	egy	State energy listing	Sept. 26, 2017, 6:42 p.m.
15N2H+.fit	fit	Spfit's log file	Sept. 26, 2017, 6:37 p.m.
15N2H+.int	int	Input file for spcat (dipole)	Sept. 26, 2017, 6:38 p.m.
15N2H+.lin	lin	Experimental transition frequencies	Sept. 26, 2017, 6:38 p.m.
c031516.lit	lit	References	Sept. 26, 2017, 6:39 p.m.
c031516.cat	mrg	Predicted transition frequencies with experimental values merged	Sept. 26, 2017, 6:39 p.m.
c031516.out	out	Partition functions	Sept. 26, 2017, 6:40 p.m.
15N2H+.par	par	Input file for spfit (parameters)	Sept. 26, 2017, 6:38 p.m.
15N2H+.var	var	Input file for spcat (parameters, variance)	Sept. 26, 2017, 6:39 p.m.

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