The files PH3__SAlTY.states and PH3__SAlTY.trans form a complete PH3 line list
in the ExoMol format, full details of which can be found in "Data structures for
ExoMol: Molecular line lists for exoplanet and other atmospheres" - J. Tennyson,
C. Hill, S. N. Yurchenko, AIP Conference Proceedings 1545, 186 (2013),
http://dx.doi.org/10.1063/1.4815853.

The methods used to calculate these data are described in C. Sousa-Silva et al., 
"ExoMol line lists VII: The rotation-vibration spectrum of phosphine up to 1500 K", 
MNRS, 2014.

The file SAlTY.pf is the PH3 partition function, also in ExoMol format. See:
C. Sousa-Silva et al., 
"High temperature partition functions and thermodynamic data for ammonia and phosphine", 
JQSRT 142, 66 (2014).


Field lengths in brackets, isolated brackets represent space length

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PH3_SAlTY.states

levelID(12) | energy(12) | gns(6) | J(7) | totalSym(3) | K(3) | rotSym(3) | l(3) 
v1(3) | v2(3) | v3(3) | v4(3) | l3(3) | l4(3) | vibSym(3) | coef(4) | s1(2) 
s2(2) | s3(2) | b1(2) | b2(2) | b3(2)

e.g.

          17  4518.250655      8       0   1   0   1   0   1   0   0   2   0   0   1 1.00  1  0  0  0  0  2

Energy levels in cm-1

For all symmetries (rotational, vibrational and total) 1=A1, 2=A2 and 3=E


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PH3_SAlTY.trans

UpperEnergyID(12)(1)LowerEnergyID(12)(1)1Einstaincoeff(10)

e.g.

       67176        62215 7.4371e-07

EinsteinCoeff in 1/s

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Clara Sousa-Silva, 2014