Radio emission from supernovae and gamma-ray bursters

By K. Weiler, N. Panagia, M. Montes, R. Sramek. 2002

268 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/2d398d5e891932f8fe9396e1d5314ff48849516e

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In Astronomy and Astrophysics

1. E. Berger
2. B. Metzger
3. S. Smartt
4. A. Filippenko
5. Ryan Chornock
6. N. Smith
7. R. Genzel
8. Roger Davies

Citations in the corpus

• The Star-forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC 3227 (2006, background): “This implies luminosities up to 3–6× 1019WHz−1, fully consistent with the range of 1–1000× 1019WHz−1 for the peak 6 cm flux density of galactic radio supernovae given by Weiler et al. (2002).”
• DUST AND THE TYPE II-PLATEAU SUPERNOVA 2004dj (2009, methodology): “This is consistent with the date obtained by Beswick et al. (2005), who used the radio Lpeak versus rise-time relation (Weiler et al. 2002) to yield an explosion date between 2004 July 11 and July 31.”
• EVLA OBSERVATIONS CONSTRAIN THE ENVIRONMENT AND PROGENITOR SYSTEM OF Type Ia SUPERNOVA 2011fe (2012, background): “10 Mpc) core-collapse SNe (Weiler et al. 2002)— explosions that mark the death of massive stars, M & 8 M⊙ (Smartt 2009).”
• The Supernova Gamma-Ray Burst Connection (2006, unknown): “…have been reviewed previously (Wang and Wheeler, 1998; van Paradijs et al., 2000; van Paradijs, 2001; Woosley et al., 2001; Wheeler, 2001; Weiler et al., 2002; Mészáros, 2002; Bloom, 2005; Piran, 2005; Matheson, 2005; Della Valle, 2005; Höflich et al., 2005), but usually as cursory…”
• Observational Signatures of Particle Acceleration in Supernova Remnants (2012, background): “Not only the evolution of radio flux but also the evolution of the radio size is observed for very young supernova remnants (e.g. Weiler et al., 2002; Bartel, 2009; Ng et al., 2008).”
• An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients (2018, methodology): “We can further constrain the environment density using the lack of evidence for a low-frequency cutoff in the radio spectrum (Figure 7) due to free–free absorption (e.g., Weiler et al. 2002), as follows.”
• Pan-STARRS1 DISCOVERY OF TWO ULTRALUMINOUS SUPERNOVAE AT z ≈ 0.9 (2011, background): “In addition, any radio emission will be heavily absorbed due to free-free processes (Weiler et al. 2002) and synchrotron self absorption (Chevalier 1998), so any burst of radio emission will to be faint.”