This is supplementary material submitted with the article:
E. K. Conway, I. E. Gordon, J. Tennyson, O. L. Polyansky, S. N. Yurchenko, K. Chance, A semi-empirical potential energy surface and line list for H$_{\text{2}}$$^{\text{16}}$O extending into the near-ultraviolet, Atmos. Chem. Phys.,(2020) submitted

1) Line-List with:
Column1: Transition frequency in cm^-1.
Column2: Intensity in units of cm molecule^-1. Assume 100% abundance.
Column3: Einstein-A coefficient	in s^-1.
Column4: air-broadening in cm^-1 atm^-1. J-averaged values as described in the HITEMP2010 article by Rothman et al. (https://doi.org/10.1016/j.jqsrt.2010.05.001)
Column5: self-broadening in cm^-1 atm^-1.J-averaged values as described in the HITEMP2010 article by Rothman et al. (https://doi.org/10.1016/j.jqsrt.2010.05.001)
Column6: Lower state energy in cm^-1.
Column7: temperature dependence of air-broadening parameter. J-averaged values as described in the HITEMP2010 article by Rothman et al. (https://doi.org/10.1016/j.jqsrt.2010.05.001)
Column8,9,10,11,12,13: v1',v2',v3',v1'',v2'',v3''.
Column14,15,16,17,18,19: J',Ka',Kc',J'',Ka'',Kc''.
Column20,21: Statistical Weights of upper and lower states are given as g(2J'+1), g(2J''+1). Where g is a state dependent statistical weight which for the principal isotopologue is 1 or 3 depending on whether state is para or ortho, respectively.

2) HOT_WAT.f90 Potential Energy Surface.
Is given (R1,R2,Cosine(angle)) with (R1,R2)in units of (Bohr,Bohr) and outputs energy of this configuration in units of Hartree. 

3) VBO.txt
This file contains the calculated Vibrational Band Origins using this HOT_WAT.f90. 
Units are in cm^-1. 

4) The data used to create Figures 1 and 2, displayed in a table.