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19942019
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 11.1k across the 70 of their papers we have counts for

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Showing astro-ph.IMShow all

6 papers · 1 filter

astro-ph.IM2018★ 93 cited

First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Photometric Pipeline and Light Curve Data Release

D. Brout, M. Sako, D. Scolnic +89

We present griz light curves of 251 Type Ia Supernovae (SNe Ia) from the first 3 years of the Dark Energy Survey Supernova Program's (DES-SN) spectroscopically classified sample. T…

astro-ph.IM2018★ 38 cited

Star-galaxy classification in the Dark Energy Survey Y1 dataset

I. Sevilla-Noarbe, B. Hoyle, M. J. Marchã +75

We perform a comparison of different approaches to star-galaxy classification using the broad-band photometric data from Year 1 of the Dark Energy Survey. This is done by performin…

astro-ph.IM2017★ 5 cited

DES Science Portal: Creating Science-Ready Catalogs

Angelo Fausti Neto, Luiz da Costa, Aurelio Carnero Rosell +55

We present a novel approach for creating science-ready catalogs through a software infrastructure developed for the Dark Energy Survey (DES). We integrate the data products release…

astro-ph.IM2017★ 107 cited

Forward Global Photometric Calibration of the Dark Energy Survey

D. Burke, E. S. Rykoff, S. Allam +56

Many scientific goals for the Dark Energy Survey (DES) require calibration of optical/NIR broadband photometry that is stable in time and uniform over the celestial sky…

astro-ph.IM2017★ 66 cited

Astrometric calibration and performance of the Dark Energy Camera

G. M. Bernstein, R. Armstrong, A. A. Plazas +53

We characterize the ability of the Dark Energy Camera (DECam) to perform relative astrometry across its 500~Mpix, 3 deg^2 science field of view, and across 4 years of operation. Th…

astro-ph.IM2009★ 924 cited

LSST Science Book, Version 2.0

LSST Science Collaboration, Paul A. Abell, Julius Allison +245

A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade.…