Gravitational wave data
-----------------------

This folder contains the gravitational wave (GW) strain data from

    The gravitational wave signal from core-collapse supernovae
    Viktoriya Morozova, David Radice, Adam Burrows, and David Vartanyan
    Submitted to ApJ, arXiv:1801.01914

The naming convention for all models is explained in Tab. 1 of that paper,
reproduced here below.

    Progenitor    EOS    Inner angular      Gravity    Many-body    Explosion   Label
    mass [Msun]          velocity [rad/s]   solver    corrections               

    10            LS220        0           monopole       yes         no     M10_LS220     
    10            LS220        0           monopole       no          no     M10_LS220_no_manybody
    10            SFHo         0           monopole       yes         yes    M10_SFHo
    10            DD2          0           monopole       yes         no     M10_DD2     
    13            SFHo         0           monopole       yes         no     M13_SFHo
    13            SFHo         0.2         multipole      yes         yes    M13_SFHo_rotating
    19            SFHo         0           monopole       yes         yes    M19_SFHo

For each model, we give the GW strain signal due to the matter terms alone,
neutrino memory is not included in these files at the moment, though it was calculated
for all models. The data are in ASCII format and the two columns are

    1:time      time since bounce in sec
    2:hplus     plus polarization of the GW strain times distance in cm

The data are sampled at ~20 kHz, but, due to timestep fluctuations in the
simulation, the sampling is not perfectly uniform in time. Therefore resampling
might be necessary.