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Title: Ab Initio Entropy Calculations of Water Predict the Interiors of 
       Uranus and Neptune to be 15-30 Percent Colder than Previous Models 
Authors: Militzer B. 
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Description of contents: This deposit includes files for the equation of state
    of liquid and superionic H2O as well as two representative
    models for the interior structure of Uranus (U123 and U125) and
    two for Neptune (N124 and N126). We also uploaded files that
    provide the gravity harmonics. The complete list of files included
    in this deposit is as follows:
    
    H2O_EOS_39_liquid_mrt.txt            Equation of state of liquid H2O
    H2O_EOS_40_superionic_mrt.txt        Equation of state of superionic H2O
    U123_layers_EOS_mrt_with_header.txt  Interior structure of Uranus of type C 
    U123_harmonics_mrt_with_header.txt   Corresponding gravity harmonics
    N124_layers_EOS_mrt_with_header.txt  Interior structure of Neptune of type C
    N124_harmonics_mrt_with_header.txt   Corresponding gravity harmonics
    U125_layers_EOS_mrt_with_header.txt  Interior structure of Uranus of type B
    U125_harmonics_mrt_with_header.txt   Corresponding gravity harmonics 
    N126_layers_EOS_mrt_with_header.txt  Interior structure of Neptune of type B
    N126_harmonics_mrt_with_header.txt   Corresponding gravity harmonics
    
System requirements: The files are formatted according to the machine
    readable format used by the AAS Journals and CDS/VizieR. Specific
    information on the structure of MRT files can be found at:

        AAS: https://journals.aas.org/mrt-overview/
        CDS: http://cds.u-strasbg.fr/doc/catstd.htx

    These files can be read in python using the astropy package:

        from astropy.table import Table
        data = Table.read("H2O_EOS_39_liquid_mrt.txt", format="ascii.cds")

    or with the most recent version of TOPCAT (> Version 4.8)

Additional comments: 

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