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Jeffrey L. Carlin

Researcher at Rensselaer Polytechnic Institute

Publications -  168
Citations -  9073

Jeffrey L. Carlin is an academic researcher from Rensselaer Polytechnic Institute. The author has contributed to research in topics: Stars & Milky Way. The author has an hindex of 39, co-authored 155 publications receiving 7962 citations. Previous affiliations of Jeffrey L. Carlin include University of Virginia & Haverford College.

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LSST: From Science Drivers to Reference Design and Anticipated Data Products

Željko Ivezić, +335 more
TL;DR: The Large Synoptic Survey Telescope (LSST) as discussed by the authors is a large, wide-field ground-based system designed to obtain repeated images covering the sky visible from Cerro Pachon in northern Chile.
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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

Philip S. Cowperthwaite, +161 more
TL;DR: In this article, the Gordon and Betty Moore Foundation (GBMF5076) and the Heising-Simons Foundation (HSPF) have contributed to the creation of the DES-Brazil Consortium.
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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

Philip S. Cowperthwaite, +99 more
TL;DR: In this article, the spectral energy distribution (SED) of the binary neutron star merger GW170817 was inferred from the optical and NIR spectrograms of the first electromagnetic counterpart to a gravitational wave source from Advanced LIGO/Virgo.
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The first data release (DR1) of the LAMOST regular survey

A-Li Luo, +145 more
TL;DR: The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general survey is a spectroscopic survey that will eventually cover approximately half of the celestial sphere and collect 10 million spectra of stars, galaxies and QSOs as discussed by the authors.
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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera

Marcelle Soares-Santos, +162 more
TL;DR: The Dark Energy Camera (DECam) was used to detect the optical counterpart of the first binary neutron star merger detected through gravitational-wave emission, GW170817.