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. Author manuscript; available in PMC: 2020 Nov 4.
Published in final edited form as: Astron Astrophys. 2020 Jul 23;639:A135. doi: 10.1051/0004-6361/202038149

Table 2. Ground-state spectroscopic parameters of syn-glycolamide (A-Reduction, Ir-Representation).

Parameters This study Stark experiment(a)
A(b) (MHz) 10454.26296 (48)(f) 10454.260 (6)
B (MHz) 4041.15605 (24) 4041.163 (4)
C (MHz) 2972.07260 (20) 2972.083 (5)
J (kHz) 0.77546 (14) 0.80 (2)
K (kHz) 2.35393 (55) 2.36 (6)
JK (kHz) 6.47368 (90) 6.3 (2)
δJ (kHz) 0.204628 (23) 0.202 (5)
δK (kHz) 2.0742 (21) 1.8 (2)
ΦJ (mHz) -0.492 (36) -
ΦJK (Hz) -0.02302 (28) -
ΦK (Hz) 0.04078 (77) -
φJK (Hz) -0.01456 (71) -
φK (Hz) -0.1638 (21) -
χaa (c) (MHz) 2.051 (4) 2.3 (2)
χbb (MHz) 1.930 (6) 2.2 (1)
χcc (MHz) -3.982 (6) -3.5 (1)
(d)
N 1480 121
σ(e) (kHz) 50 34

Notes.

(a)

The parameters for the previous Stark experiment were published in Maris (2004).

(b)

A, B, and C represent the rotational constants.

(c)

χaa, χbb, χcc are the diagonal elements of the 14N nuclear quadrupole coupling tensor.

(d)

N is the number of measured transitions.

(e)

σ is the root mean square (rms) deviation of the fit.

(f)

Standard error in parentheses in units of the last digit.