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Pan-STARRS: A Large Synoptic Survey Telescope Array

N. KaiserHerve AusselBarry E. BurkeH. BoesgaardK. C. ChambersMark ChunJ. N. HeasleyK. W. HodappBobby R. HuntRobert JedickeD. JewittRolf P. KudritzkiGerard A. LuppinoMichael MaberryE. A. MagnierD. G. MonetPeter M. OnakaA. J. PicklesP. H. RhoadsTheodore SimonAlexander S. SzalayIstván SzapudiD. J. TholenJ. TonryM. WatersonJohn W. Wick

Abstract

The IFA and collaborators are embarking on a project to develop a 4-telescope synoptic survey instrument. While somewhat smaller than the 6.5m class telescope envisaged by the decadal review in their proposal for a LSST, this facility will nonetheless be able to accomplish many of the LSST science goals. In this paper we will describe the motivation for a 'distributed aperture' approach for the LSST, the current concept for Pan-STARRS -- a pilot project for the LSST proper -- and its performance goals and science reach. We will also discuss how the facility may be expanded.

Adaptive optics and wavefront sensingStellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchLarge Synoptic Survey TelescopeTelescopeComputer scienceAperture (computer memory)Class (philosophy)Systems engineeringRemote sensingPhysicsAstronomyGeology
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