activity
20022008
most citedSpitzer measurements of atomic and molecular abundances in the Type IIP SN 2005af

75 citations · 174 across the 4 of their papers we have counts for

collaborators

15 papers

astro-ph200834 cited

GALEX Spectroscopy of SN 2005ay suggests a UV spectral uniformity among type II-P supernovae

A. Gal-Yam, F. Bufano, T. Barlow +24

We present the first results from our GALEX program designed to obtain ultraviolet (UV) spectroscopy of nearby core-collapse supernovae (SNe). Our first target, SN 2005ay in the ne…

astro-ph200717 cited

The Radio Evolution of SN 2001gd

Christopher J. Stockdale, Christopher L. Williams, Kurt W. Weiler +4

We present the results of observations of the radio emission from Supernova 2001gd in NGC 5033 from 2002 February 8 through 2006 September 25. The data were obtained using the Very…

astro-ph200675 cited

Spitzer measurements of atomic and molecular abundances in the Type IIP SN 2005af

Rubina Kotak, Peter Meikle, Monica Pozzo +12

We present results based on Spitzer Space Telescope mid-infrared (3.6-30 micron) observations of the nearby IIP supernova 2005af. We report the first ever detection of the SiO mole…

astro-ph200648 cited

A Spitzer Space Telescope study of SN 2002hh: an infrared echo from a Type IIP supernova

W. P. S. Meikle, S. Mattila, C. L. Gerardy +10

We present late-time (590-994 d) mid-IR photometry of the normal, but highly-reddened Type IIP supernova SN 2002hh. Bright, cool, slowly-fading emission is detected from the direct…

astro-ph2005

The Light Echo Around Supernova 2003gd in Messier 74

Schuyler D. Van Dyk, Weidong Li, Alexei V. Filippenko

We confirm the discovery of a light echo around the Type II-plateau Supernova 2003gd in Messier 74 (NGC 628), seen in images obtained with the High Resolution Channel of the Advanc…

astro-ph2005

Identification of the Red Supergiant Progenitor of Supernova 2005cs: Do the Progenitors of Type II-P Supernovae Have Low Mass?

Weidong Li, Schuyler D. Van Dyk, Alexei V. Filippenko +5

The stars that end their lives as supernovae (SNe) have been directly observed in only a handful of cases, due mainly to the extreme difficulty in identifying them in images obtain…