1998/01/02 by Piero Madau, Madau, Piero
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Radio Astronomy Observations and Technology #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9801005
LaTeX, 9 pages, 3 figures, to appear in ``The Young Universe: Galaxy Formation and Evolution at Intermediate and High Redshift'', 1998, S. D'Odorico, A. Fontana & E. Giallongo (editors), PASP
arxiv created 1998/01/02 · openalex publication_date 1998/01/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Ongoing searches for supernovae (SNe) at cosmological distances have recently started to provide a link between SN Ia statistics and galaxy evolution. In this talk I will use recent estimates of the global history of star formation to compute the theoretical Type Ia and Type II SN rates as a function of cosmic time. I will compare the predicted values with the rates observed in the range 0