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L. G. Strolger

Researcher at Space Telescope Science Institute

Publications -  22
Citations -  3847

L. G. Strolger is an academic researcher from Space Telescope Science Institute. The author has contributed to research in topics: Supernova & Galaxy. The author has an hindex of 13, co-authored 22 publications receiving 3493 citations. Previous affiliations of L. G. Strolger include Western Kentucky University.

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Journal ArticleDOI

Candels: The cosmic assembly near-infrared deep extragalactic legacy survey - The hubble space telescope observations, imaging data products, and mosaics

Anton M. Koekemoer, +124 more
TL;DR: In this paper, the authors describe the Hubble Space Telescope imaging data products and data reduction procedures for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS).
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Long γ-ray bursts and core-collapse supernovae have different environments

TL;DR: In this article, the authors show that long-duration γ-ray bursts are associated with the most extremely massive stars and may be restricted to galaxies of limited chemical evolution. But they also show that the host galaxies of the long-drone bursts are significantly fainter and more irregular than the hosts of the core-collapse supernovae.
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The host galaxies of core‐collapse supernovae and gamma‐ray bursts

TL;DR: In this article, a comparative study of the galactic and small-scale environments of gamma-ray bursts (GRBs) and core-collapse supernovae (CCSNe) is presented, and the results broadly corroborate previous findings, but offer significant enhancements in spectral coverage and a factor 2-3 increase in sample size.
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"Refsdal" Meets Popper: Comparing Predictions of the Re-appearance of the Multiply Imaged Supernova Behind MACSJ1149.5+2223

TL;DR: In this article, a blind test of model predictions in extragalactic astronomy, on a timescale that is short compared to a human lifetime, was made, where seven gravitational lens models with five independent methods, based on Hubble Space Telescope (HST) Hubble Frontier Field images, along with extensive spectroscopic follow-up observations by HST, the Very Large and the Keck Telescopes.