Year: 2020
Type: preprint
Abstract: 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.
Source: arXiv (Cornell University)
Institutions: University of Chicago, University of California, Los Angeles
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Awards: CORE-COLLAPSE SUPERNOVAE (SNE) ARISE FROM MASSIVE STARS, WITH INITIAL MASS GREATER THAN ABOUT 8 SOLAR MASSES. THESE STARS LOSE A SIGNIFICANT AMOUNT O, From Radio to Gamma-Rays: Interpreting the Multiwavelength Emission from Young Supernovae as a Probe of their Evolution, Progenitors, and Cosmic-Ray Acceleration
OpenAlex ID: W3099055502