Science Opportunities with LSST

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The LSST design is driven by four science themes: dark energy and matter, Galactic structure, transient objects, and the Solar System inventory. These and many other science opportunities are described in the LSST Science Book: http://www.lsst.org/lsst/scibook
The LSST will carry out a ten-year very deep imaging survey of 18,000 sq.deg. of the sky in six broad optical bands, with a deep stack reaching r 27.5 (5 sigma, point source). The LSST design, with an 8.4m (6.7m effective) primary mirror and a 9.6 square degree field of view, will allow about 10,000 square degrees of sky to be imaged to an effective depth of r=24.5 every three nights. Each patch of the sky will be visited over 800 times with pairs of 15 sec exposures, opening a new window on the universe: faint time-domain. The resulting petabytes of data will be made available to the US and Chilean communities for scientific investigations ranging from the properties of near-Earth asteroids, to characterizations of dark energy from strong and weak lensing, galaxy clustering, and distant supernovae.
More information is available at http://www.lsst.org
Eleven LSST Science Collaborations are actively laying the groundwork for first light: working on image analysis algorithms and database design, exploring cadence choices, developing commissioning plans, and outlining scientific opportunities. These Collaborations have over 200 members to date, with membership open to the US and Chilean communities via an application process administered by NOAO. Full end-to-end LSST image simulations are a useful resource for exploring science capability.
LSST Science Collaborations:
Supernovae
Weak Lensing
Stellar Populations
Active Galactic Nuclei
Solar System
Galaxies
Transients/variable stars
Large-scale structure and baryon oscillations
Milky Way and Local Volume Structure
Strong Lensing
Informatics and Statistics

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