activity
20022010
most citedNew Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy

1.8k citations · 4.9k across the 24 of their papers we have counts for

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astro-ph200855 cited

Spectroscopy of High-Redshift Supernovae from the ESSENCE Project: The First Four Years

R. J. Foley, T. Matheson, S. Blondin +23

We present the results of spectroscopic observations from the ESSENCE high-redshift supernova (SN) survey during its first four years of operation. This sample includes spectra of…

astro-ph2008137 cited

SN 2008S: A Cool Super-Eddington Wind in a Supernova Impostor

Nathan Smith, Mohan Ganeshalingam, Ryan Chornock +10

We present visual-wavelength photometry and spectroscopy of supernova SN2008S. Based on the low peak luminosity for a SN of M_R = -13.9 mag, photometric and spectral evolution unli…

astro-ph200882 cited

First Results from the Lick AGN Monitoring Project: The Mass of the Black Hole in Arp 151

Misty C. Bentz, Jonelle L. Walsh, Aaron J. Barth +24

We have recently completed a 64-night spectroscopic monitoring campaign at the Lick Observatory 3-m Shane telescope with the aim of measuring the masses of the black holes in 13 ne…

astro-ph200834 cited

The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125

Adria C. Updike, Joshua B. Haislip, Melissa C. Nysewander +52

We report on multi-wavelength observations, ranging from the X-ray to radio wave bands, of the IPN-localized gamma-ray burst GRB 070125. Spectroscopic observations reveal the prese…

astro-ph2008248 cited

SN 2006tf: Precursor Eruptions and the Optically Thick Regime of Extremely Luminous Type IIn Supernovae

Nathan Smith, Ryan Chornock, Weidong Li +5

SN2006tf is the third most luminous SN discovered so far, after SN2005ap and SN2006gy. SN2006tf is valuable because it provides a link between two regimes: (1) luminous type IIn su…

astro-ph200864 cited

Late-time observations of SN2006gy: Still Going Strong

Nathan Smith, Ryan J. Foley, Joshua S. Bloom +9

Owing to its extremely high luminosity and long duration, SN2006gy radiated more energy in visual light than any other known SN. Two hypotheses to explain its high luminosity -- th…