Published September 7, 2021 | Version 1.2
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Avoided crossing in gravitational wave spectra from protoneutron star

  • 1. RIken
  • 2. National Astronomical Observatory of Japan

Description

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.

Files

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md5:ae952e3f4616d99dff7ed5c553750192
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md5:cd735d56238c58ebe8dd2ddc08923f1c
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Additional details

Related works

Is supplement to
Journal article: 10.1093/mnras/staa2597 (DOI)
Preprint: arXiv:2008.00419 (arXiv)
Preprint: 2020MNRAS.498.3503S (Bibcode)