2007/03/13 by L. Colina, T. Díaz-Santos, T. Diaz-Santos +5
Engineering · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #CCD and CMOS Imaging Sensors #Cosmic infrared background #Galaxy #Gamma-ray bursts and supernovae #Infrared #Luminous infrared galaxy #Stars #Supernova #astro-ph
paper · pdf · doi:10.1051/0004-6361:20067043
openalex publication_date 2007/03/13 · arxiv created 2007/03/19 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context.(Ultra)Luminous Infrared Galaxies (ULIRGs) produce massive stars in large quantities in their central starburst regions. The expected rate of supernova explosions is, on average, about one per year. Detection of these supernovae in the expected numbers has proven elusive so far.