Supernovae and gamma-Ray Bursters

By T. Galama. 2003

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Ultraviolet Detection of the Tidal Disruption of a Star by a Supermassive Black Hole (2006, background): “Supernovae (SNe) have light curves that extend over months, similar to the flare observed here, but their emission peaks at optical wavelengths, and is intrinsically faint shortward of ∼ 3000 Å (Panagia 2003; Brown et al. 2005).”
The C4 Clustering Algorithm: Clusters of Galaxies in the Sloan Digital Sky Survey (2005, background): “…and groups of galaxies are used extensively throughout extragalactic astronomy and cosmology, from constraining the cosmological parameters (e.g., Oukbir & Blanchard 1992; Henry & Arnaud 1991; Viana & Liddle 1996; Bahcall, Fan & Cen 1997; Reichart et al. 1999; Miller et al. 2001a,b), to…”
Nebular emission-line profiles of Type Ib/c supernovae - Probing the ejecta asphericity (2009, methodology): “Another 4 spectra of the Asiago archive were shown by Turatto (2003) and Valenti et al. (2008) before.”