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20022008
most citedSpectral Identification of an Ancient Supernova using Light Echoes in the LMC

120 citations · 194 across the 4 of their papers we have counts for

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astro-ph2008120 cited

Spectral Identification of an Ancient Supernova using Light Echoes in the LMC

A. Rest, T. Matheson, S. Blondin +26

We report the successful identification of the type of the supernova responsible for the supernova remnant SNR 0509-675 in the Large Magellanic Cloud (LMC) using Gemini spectra of…

astro-ph200647 cited

Lightcurves of Type Ia Supernovae from Near the Time of Explosion

Arti Garg, Christopher W. Stubbs, Peter Challis +18

We present a set of 11 type Ia supernova (SN Ia) lightcurves with dense, pre-maximum sampling. These supernovae (SNe), in galaxies behind the Large Magellanic Cloud (LMC), were dis…

astro-ph200611 cited

The FSVS Cluster Catalogue: Galaxy Clusters and Groups in the Faint Sky Variability Survey

Ilona K. Soechting, Mark E. Huber, Roger G. Clowes +1

We describe a large sample of 598 galaxy clusters and rich groups discovered in the data of the Faint Sky Variability Survey. The clusters have been identified using a fully automa…

astro-ph200616 cited

Color and Variability Characteristics of Point Sources in the Faint Sky Variability Survey

M. E. Huber, M. E. Everett, S. B. Howell

We present an analysis of the color and variability characteristics for point sources in the Faint Sky Variability Survey (FSVS). The FSVS cataloged ~23 square degrees in BVI filte…

astro-ph2005

Echoes from Ancient Supernovae in the Large Magellanic Cloud

A. Rest, N. B. Suntzeff, K. Olsen +13

In principle, the light from historical supernovae could still be visible as scattered-light echoes even centuries later. However, while echoes have been discovered around some nea…

astro-ph2003

Searching for Variability in the Globular Cluster Messier 4

Robert D. Ferdman, Harvey B. Richer, James Brewer +11

Time-series data taken with the Hubble Space Telescope of a field six core radii (~5') from the center of the globular cluster Messier 4, and covering a period of about 10 weeks in…