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20022008
most citedImproved Cosmological Constraints from New, Old and Combined Supernova Datasets

1.6k citations · 2.1k across the 8 of their papers we have counts for

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astro-ph20081.6k cited

Improved Cosmological Constraints from New, Old and Combined Supernova Datasets

M. Kowalski, D. Rubin, G. Aldering +67

We present a new compilation of Type Ia supernovae (SNe Ia), a new dataset of low-redshift nearby-Hubble-flow SNe and new analysis procedures to work with these heterogeneous compi…

astro-ph2007182 cited

SN 2003du: 480 days in the Life of a Normal Type Ia Supernova

V. Stanishev, A. Goobar, S. Benetti +29

An extensive set of optical and NIR photometry and low-resolution spectra the Type Ia supernova (SN Ia) 2003du was obtained using a number of facilities. The observations started 1…

astro-ph200710 cited

Spectroscopic observations of eight supernovae at intermediate redshift

C. Balland, M. Mouchet, R. Amanullah +16

We present spectra of six Type Ia and two Type II supernovae obtained in June 2002 at the William Herschel Telescope during a search for Type Ia supernovae (SNIa) at intermediate r…

astro-ph200764 cited

Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study

G. Garavini, G. Folatelli, S. Nobili +44

We develop a method to measure the strength of the absorption features in Type Ia supernova (SN Ia) spectra and use it to make a quantitative comparison between the spectra of Type…

astro-ph200773 cited

ESC observations of SN 2005cf: II. Optical Spectroscopy and the high velocity features

G. Garavini, S. Nobili, S. Taubenberger +11

The ESC-RTN optical spectroscopy data-set for SN 2005cf is presented and analyzed. The observations range from -11.6 and +77.3 days with respect to B-band maximum light. The evolut…

astro-ph2007109 cited

ESC observations of SN 2005cf. I. Photometric Evolution of a Normal Type Ia Supernova

A. Pastorello, S. Taubenberger, N. Elias-Rosa +20

We present early-time optical and near-infrared photometry of supernova (SN) 2005cf. The observations, spanning a period from about 12 days before to 3 months after maximum, have b…