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A. Goobar

Researcher at Lawrence Berkeley National Laboratory

Publications -  93
Citations -  40185

A. Goobar is an academic researcher from Lawrence Berkeley National Laboratory. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 27, co-authored 81 publications receiving 37290 citations. Previous affiliations of A. Goobar include Stockholm University.

Papers
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Implications For The Hubble Constant from the First Seven Supernovae at z >= 0.35

TL;DR: In this article, the Supernova Cosmology Project has discovered over twenty-eight supernovae (SNe) at 0.35 = 0.2, and they find that H_0^G < 70 km/s/Mpc in a Lambda=0 universe and H_ 0^G > 78 km/m/MPC in a flat universe, correcting the distant and local SN apparent magnitudes for light curve width.
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A highly magnified supernova at z=1.703 behind the massive galaxy cluster Abell 1689

TL;DR: In this article, the discovery of one of the most distant supernovae ever found, at redshift, z = 1.703, was reported. But this supernova was found in a galaxy with a magnification of only 4.3 × p 0.0.
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An Intermediate Type Ia Supernova Between Normal And Super-Chandrasekhar

TL;DR: The early phase spectra of iPTF13asv showed absence of iron absorption, indicating that synthesized iron elements are confined to low-velocity regions of the ejecta, which implies a stratified ejecta structure along the line of sight.
Journal Article

Weak Lensing from Space I: Instrumentation and Survey Strategy

TL;DR: In this article, the authors quantify the major contributions of the Supernova/Acceleration Probe (SNAP) to the Point Spread Function (PSF) of the Wide Field Space Telescope (WFSST).
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Supernova / Acceleration Probe: A Satellite Experiment to Study the Nature of the Dark Energy

Greg Aldering, +110 more
- 12 May 2004 - 
TL;DR: The Supernova/Acceleration Probe (SNAP) as mentioned in this paper is a space-based experiment designed to study the dark energy and alternative explanations of the acceleration of the Universe's expansion by performing a series of complementary systematics-controlled astrophysical measurements.