An end-to-end simulation framework for the Large Synoptic Survey Telescope

The LSST will, over a 10-year period, produce a multi-color, multi-epoch survey of more than 18000 square degrees of the southern sky. It will generate a multi-petabyte archive of images and catalogs of astrophysical sources from which a wide variety of high-precision statistical studies can be undertaken. To accomplish these goals, the LSST project has developed a suite of modeling and simulation tools for use in validating that the design and the as-delivered components of the LSST system will yield data products with the required statistical properties. In this paper we describe the development, and use of the LSST simulation framework, including the generation of simulated catalogs and images for targeted trade studies, simulations of the observing cadence of the LSST, the creation of large-scale simulations that test the procedures for data calibration, and use of end-to-end image simulations to evaluate the performance of the system as a whole.

[1]  G. Bruzual,et al.  Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.

[2]  Abhijit Saha,et al.  Simulation of autonomous observing with a ground-based telescope: the LSST experience , 2010, Astronomical Telescopes + Instrumentation.

[3]  D. Schlegel,et al.  Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .

[4]  Zeljko Ivezic,et al.  Asteroid Discovery and Characterization with the Large Synoptic Survey Telescope , 2015, Proceedings of the International Astronomical Union.

[5]  J. Lépine,et al.  Models for Interstellar Extinction in the Galaxy , 2005 .

[6]  Zeljko Ivezic,et al.  The Milky Way Tomography with SDSS , 2005 .

[7]  Karri Muinonen,et al.  OpenOrb: Open‐source asteroid orbit computation software including statistical ranging , 2009 .

[8]  David Schlegel,et al.  The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution , 2005, astro-ph/0510520.

[9]  G. Kauffmann,et al.  The formation history of elliptical galaxies , 2005, astro-ph/0509725.

[10]  J. G. Jernigan,et al.  SIMULATION OF ASTRONOMICAL IMAGES FROM OPTICAL SURVEY TELESCOPES USING A COMPREHENSIVE PHOTON MONTE CARLO APPROACH , 2015, 1504.06570.

[11]  Pierre Bergeron,et al.  PHOTOMETRIC CALIBRATION OF HYDROGEN- AND HELIUM-RICH WHITE DWARF MODELS , 1995 .

[12]  Kevin Krisciunas,et al.  A MODEL OF THE BRIGHTNESS OF MOONLIGHT , 1991 .

[13]  Z. Ivezic,et al.  THE MILKY WAY TOMOGRAPHY WITH SDSS. III. STELLAR KINEMATICS , 2009, 0909.0013.

[14]  T. B. Spahr,et al.  The Pan-STARRS Synthetic Solar System Model and its Applications , 2007 .

[15]  Durham,et al.  Testing model predictions of the cold dark matter cosmology for the sizes, colours, morphologies and luminosities of galaxies with the SDSS , 2008, 0812.4399.