activity
20022014
most citedImproved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

1.9k citations · 4.4k across the 15 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008★ 124 cited

Discovery of an Unusual Optical Transient with the Hubble Space Telescope

K. Barbary, K. S. Dawson, K. Tokita +27

We present observations of SCP 06F6, an unusual optical transient discovered during the Hubble Space Telescope Cluster Supernova Survey. The transient brightened over a period of ~…

astro-ph2008★ 21 cited

Light curve studies of nearby Type Ia Supernovae with a Multi-band Stretch method

N. Takanashi, M. Doi, N. Yasuda

We create new U, B, V, R and I-band light curve templates of type Ia Supernovae (SNe Ia) and re-analyze 122 nearby (redshift < 0.11) SNe Ia using a new ``Multi-band Stretch method,…

astro-ph2008★ 12 cited

Implications for Galaxy Evolution from the Cosmic Evolution of Supernova Rate Density

T. Oda, T. Totani, N. Yasuda +4

We report a comprehensive statistical analysis of the observational data of the cosmic evolution of supernova (SN) rate density, to derive constraints on cosmic star formation hist…

astro-ph2007★ 71 cited

A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys

N. Kuznetsova, K. Barbary, B. Connolly +27

We present a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST…

astro-ph2007★ 15 cited

Rest-Frame R-band Lightcurve of a z~1.3 Supernova Obtained with Keck Laser Adaptive Optics

J. Melbourne, K. S. Dawson, D. C. Koo +24

We present Keck diffraction limited H-band photometry of a z~1.3 Type Ia supernova (SN) candidate, first identified in a Hubble Space Telescope (HST) search for SNe in massive high…

astro-ph2007★ 64 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…