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19972023
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations · 63.7k across the 227 of their papers we have counts for

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Showing 2008Show all

7 papers · 1 filter

astro-ph2008★ 55 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-ph2008★ 16 cited

Exploring the Outer Solar System with the ESSENCE Supernova Survey

A. C. Becker, K. Arraki, N. A. Kaib +36

We report the discovery and orbit determination of 14 trans-Neptunian objects (TNOs) from the ESSENCE Supernova Survey difference imaging dataset. Two additional objects discovered…

astro-ph2008★ 60 cited

Luminosity Indicators in the Ultraviolet Spectra of Type Ia Supernovae

Ryan J. Foley, Alexei V. Filippenko, Saurabh W. Jha

We present a complete sample of International Ultraviolet Explorer and Hubble Space Telescope ultraviolet (UV) spectra of Type Ia supernovae (SNe Ia) through 2004. We measure the e…

astro-ph2008★ 76 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-ph2008★ 148 cited

Optical Spectroscopy of Type Ia Supernovae

T. Matheson, R. P. Kirshner, P. Challis +19

We present 432 low-dispersion optical spectra of 32 Type Ia supernovae (SNe Ia) that also have well-calibrated light curves. The coverage ranges from 6 epochs to 36 epochs of spect…

astro-ph2008★ 31 cited

Two More Candidate AM Canum Venaticorum (AM CVn) Binaries from the Sloan Digital Sky Survey

S. F. Anderson, A. C. Becker, D. Haggard +18

AM CVn systems are a select group of ultracompact binaries with the shortest orbital periods of any known binary subclass; mass-transfer is likely from a low-mass (partially-)degen…