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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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Showing 2007Show all

22 papers · 1 filter

astro-ph2007★ 48 cited

Supernovae in Low-Redshift Galaxy Clusters: Observations by the Wise Observatory Optical Transient Search (WOOTS)

Avishay Gal-Yam, Dan Maoz, Puragra Guhathakurta +1

We describe the Wise Observatory Optical Transient Search (WOOTS), a survey for supernovae (SNe) and other variable and transient objects in the fields of redshift 0.06-0.2 Abell g…

astro-ph2007★ 92 cited

The Detection of a Light Echo from the Type Ia Supernova 2006X in M100

Xiaofeng Wang, Weidong Li, Alexei V. Filippenko +3

We report the discovery of a light echo (LE) from the Type Ia supernova (SN) 2006X in the nearby galaxy M100. The presence of the LE is supported by analysis of both the Advanced C…

astro-ph2007★ 19 cited

Optical Photometry and Spectroscopy of the Accretion-Powered Millisecond Pulsar HETE J1900.1-2455

P. Elebert, P. J. Callanan, A. V. Filippenko +4

We present phase resolved optical photometry and spectroscopy of the accreting millisecond pulsar HETE J1900.1-2455. Our R-band light curves exhibit a sinusoidal modulation, at clo…

astro-ph2007★ 246 cited

The Broad-lined Type Ic SN 2003jd

S. Valenti, S. Benetti, E. Cappellaro +27

The results of a world-wide coordinated observational campaign on the broad-lined Type Ic SN 2003jd are presented. In total, 74 photometric data points and 26 spectra were collecte…

astro-ph2007★ 70 cited

SN 2002cv: A Heavily Obscured Type Ia Supernova

N. Elias-Rosa, S. Benetti, M. Turatto +15

We present VRIJHK photometry, and optical and near-infrared spectroscopy, of the heavily extinguished Type Ia supernova (SN) 2002cv, located in NGC 3190, which is also the parent g…

astro-ph2007★ 71 cited

Constraining Cosmic Evolution of Type Ia Supernovae

Ryan J. Foley, A. V. Filippenko, C. Aguilera +27

We present the first large-scale effort of creating composite spectra of high-redshift type Ia supernovae (SNe Ia) and comparing them to low-redshift counterparts. Through the ESSE…