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19932025
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations · 118k across the 790 of their papers we have counts for

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21 papers · 1 filter

astro-ph2004★ 101 cited

On the Progenitor of the Type II Supernova 2004et in NGC 6946

Weidong Li, Schuyler D. Van Dyk, Alexei V. Filippenko +1

Supernova (SN) 2004et is the eighth historical SN in the nearby spiral galaxy NGC 6946. Here we report on early photometric and spectroscopic monitoring of this object. SN 2004et i…

astro-ph2004★ 368 cited

The Centers of Early-Type Galaxies with HST. V. New WFPC2 Photometry

Tod R. Lauer, S. M. Faber, Karl Gebhardt +14

We analyze HST+WFPC2 images of 77 early-type galaxies. Brightness profiles are classed into "core" or "power-law" forms. Cores are typically rounder than power-law galaxies. Nearly…

astro-ph2004★ 2 cited

Supernovae and Their Massive Star Progenitors

Alexei V. Filippenko

I briefly describe the Lick Observatory Supernova Search with the 0.76-m Katzman Automatic Imaging Telescope. I then present an overview of optical observations of Type II, IIb, Ib…

astro-ph2004★ 68 cited

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

T. Matheson, S. Blondin, R. J. Foley +28

We present the results of spectroscopic observations of targets discovered during the first two years of the ESSENCE project. The goal of ESSENCE is to use a sample of ~200 Type Ia…

astro-ph2004★ 277 cited

The binary progenitor of Tycho Brahe's 1572 supernova

Pilar Ruiz-Lapuente, Fernando Comeron, Javier Mendez +8

The brightness of type Ia supernovae, and their homogeneity as a class, makes them powerful tools in cosmology, yet little is known about the progenitor systems of these explosions…

astro-ph2004★ 43 cited

Type Ia Supernovae and Cosmology

Alexei V. Filippenko

I discuss the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshift SNe Ia (z < 0.1) demonstrate that the Hubble expansion is linear with H_0 =…