LSST Science Book, Version 2.0
LSST Science Collaborations: Paul A. Abell, Julius Allison, Scott F., Anderson, John R. Andrew, J. Roger P. Angel, Lee Armus, David Arnett, S. J., Asztalos, Tim S. Axelrod, Stephen Bailey, D. R. Ballantyne, Justin R., Bankert, Wayne A. Barkhouse, Jeffrey D. Barr

TL;DR
The LSST Science Book outlines a decade-long, wide-field optical survey with the LSST telescope, aiming to revolutionize multiple areas of astronomy and cosmology through extensive imaging and data collection.
Contribution
It provides a comprehensive overview of LSST's hardware, software, observing plans, and scientific goals, highlighting its potential to transform various astrophysical research fields.
Findings
High-resolution imaging of the Solar System and galaxies
Detection of transient and variable objects at high redshift
Constraints on cosmological models and dark energy
Abstract
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. The Large Synoptic Survey Telescope (LSST) will have an effective aperture of 6.7 meters and an imaging camera with field of view of 9.6 deg^2, and will be devoted to a ten-year imaging survey over 20,000 deg^2 south of +15 deg. Each pointing will be imaged 2000 times with fifteen second exposures in six broad bands from 0.35 to 1.1 microns, to a total point-source depth of r~27.5. The LSST Science Book describes the basic parameters of the LSST hardware, software, and observing plans. The book discusses educational and outreach opportunities, then goes on to describe a broad range of science that LSST will revolutionize: mapping the inner and outer Solar System, stellar populations in the Milky Way and…
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Taxonomy
TopicsAstronomy and Astrophysical Research
