activity
19952004
most citedSpectropolarimetry of Core-Collapse Supernovae

5 citations · 11 across the 10 of their papers we have counts for

collaborators
Showing astro-phShow all

32 papers · 1 filter

astro-ph200876 cited

Time Dilation in Type Ia Supernova Spectra at High Redshift

S. Blondin, T. M. Davis, K. Krisciunas +29

We present multiepoch spectra of 13 high-redshift Type Ia supernovae (SNe Ia) drawn from the literature, the ESSENCE and SNLS projects, and our own separate dedicated program on th…

astro-ph200863 cited

First-Year Spectroscopy for the SDSS-II Supernova Survey

Chen Zheng, Roger W. Romani, Masao Sako +77

This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital Sky Survey-II Supernova Survey. This program searches for and measures multi-band…

astro-ph200742 cited

The host galaxy of GRB031203: a new spectroscopic study

R. Margutti, G. Chincarini, S. Covino +11

The host galaxy of the long-duration gamma-ray burst (GRB) 031203 (HG031203) offers a precious opportunity to study in detail the environment of a nearby GRB. The aim is to better…

astro-ph200774 cited

The Dual-Axis Circumstellar Environment of the Type IIn Supernova 1997eg

Jennifer L. Hoffman, Douglas C. Leonard, Ryan Chornock +3

We present multi-epoch spectral and spectropolarimetric observations of the Type IIn supernova (SN) 1997eg that indicate the presence of a flattened disk-like concentration of circ…

astro-ph2007141 cited

ESC and KAIT Observations of the Transitional Type Ia SN 2004eo

A. Pastorello, P. A. Mazzali, G. Pignata +31

We present optical and infrared observations of the unusual Type Ia supernova (SN) 2004eo. The light curves and spectra closely resemble those of the prototypical SN 1992A, and the…

astro-ph2007927 cited

Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey

W. M. Wood-Vasey, G. Miknaitis, C. W. Stubbs +34

We present constraints on the dark energy equation-of-state parameter, w=P/(rho c^2), using 60 Type Ia supernovae (SNe Ia) from the ESSENCE supernova survey. We derive a set of con…