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19972009
most citedNew Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy

1.8k citations · 3.7k across the 8 of their papers we have counts for

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astro-ph200876 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-ph2007927 cited

Observational Constraints on the Nature of the Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey

W. M. Wood-Vasey, G. Miknaitis, C. W. Stubbs +34

We present constraints on the dark energy equation-of-state parameter, w=P/(rho c^2), using 60 Type Ia supernovae (SNe Ia) from the ESSENCE supernova survey. We derive a set of con…

astro-ph2006831 cited

Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Saurabh Jha, Adam G. Riess, Robert P. Kirshner

We present an updated version of the Multicolor Light Curve Shape method to measure distances to type Ia supernovae (SN Ia), incorporating new procedures for K-correction and extin…

astro-ph20061.8k cited

New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy

Adam G. Riess, Louis-Gregory Strolger, Stefano Casertano +18

We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to trace the history of cosmic expansion over the last 10 billion yea…

astro-ph20061 cited

A Survey for Supernovae in Massive High-Redshift Clusters

Keren Sharon, A. Gal-Yam, D. Maoz +12

We describe our ongoing program designed to measure the SN-Ia rate in a sample of massive z=0.5-0.9 galaxy clusters. The SN-Ia rate is a poorly known observable, especially at high…

astro-ph200316 cited

A search for the optical and near-infrared counterpart of the accreting millisecond X-ray pulsar XTE J1751-305

P. G. Jonker, G. Nelemans, Z. Wang +14

We have obtained optical and near-infrared images of the field of the accreting millisecond X-ray pulsar XTE J1751-305. There are no stars in the 0.7'' error circle (0.7'' is the o…