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Supernova X-Ray Database (SNaX) Updated to Ensure Long-term Stability

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arxiv 2011.04427 v1 pith:6LZXXFMV submitted 2020-11-03 astro-ph.HE

classification astro-ph.HE
keywords databasex-raydatalong-termsnaxstabilitysupernovaupdated
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The Supernova X-Ray Database (SNaX) was established a few years ago to make X-ray data on supernovae (SNe) publicly available via an elegant searchable web interface. The database has recently been updated to PhP7, had security updates done, and moved to a new server, ensuring its long-term stability. We urge astronomers to continue to download the data as needed for their work. Those with X-ray data on SNe are requested to upload it to the database via the easily fillable spreadsheet, making it accessible to everyone.

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Cited by 1 Pith paper

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  1. On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars

    astro-ph.HE 2025-05 conditional novelty 3.0 of 10

    A compilation of 115 supernova X-ray light curves and selected spectra concludes that Type Ib/c and low-mass-loss Type IIP supernovae emit non-thermally, while Type IIn supernovae emit thermally, with inferred progeni...

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