Bolometric and UV Light Curves of Core-Collapse Supernovae
Autor: | T. A. Pritchard, Lucille H. Frey, Peter J. Brown, Amanda J. Bayless, P. W. A. Roming |
---|---|
Rok vydání: | 2013 |
Předmět: |
Physics
High Energy Astrophysical Phenomena (astro-ph.HE) Astrophysics::High Energy Astrophysical Phenomena Bolometer FOS: Physical sciences Astronomy and Astrophysics Astrophysics Visible radiation Astrophysics::Cosmology and Extragalactic Astrophysics Light curve law.invention Core (optical fiber) Telescope Supernova Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science law Astrophysics::Solar and Stellar Astrophysics Astrophysics - High Energy Astrophysical Phenomena Ultraviolet radiation Astrophysics::Galaxy Astrophysics Solar and Stellar Astrophysics (astro-ph.SR) |
DOI: | 10.48550/arxiv.1303.1190 |
Popis: | The Swift UV-Optical Telescope (UVOT) has been observing Core-Collapse Supernovae (CCSNe) of all subtypes in the UV and optical since 2005. We present here 50 CCSNe observed with the Swift UVOT, analyzing their UV properties and behavior. Where we have multiple UV detections in all three UV filters (\lambda c = 1928 - 2600 \AA), we generate early time bolometric light curves, analyze the properties of these light curves, the UV contribution to them, and derive empirical corrections for the UV-flux contribution to optical-IR based bolometric light curves. |
Databáze: | OpenAIRE |
Externí odkaz: |