Avoided crossing in gravitational wave spectra from protoneutron star
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The data of the gravitational wavefroms of core-collapse supernovae, which are used in Sotani and Takiwaki (2020), Monthly Notices of the Royal Astronomical Society, Volume 498, Issue 3, pp.3503-3512. Data Format: The data are in ASCII format and the two columns are1:time time since bounce in sec 2:hplus plus polarization of the GW amplitude. We assume the source distance of 10 kpc. The data are sampled at ~10 kHz, but, the sampling is not uniform in time. Therefore resampling might be necessary.
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Zenodo创建时间：
2021-09-07
