Paper
24 December 2002 Deep lens survey
David M. Wittman, J. Anthony Tyson, Ian P. Dell'Antonio, Andrew Becker, Vera Margoniner, Judith G. Cohen, D. Norman, D. Loomba, G. Squires, Gillian Wilson, Christopher W. Stubbs, J. Hennawi, David N. Spergel, P. Boeshaar, A. Clocchiatti, M. Hamuy, G. Bernstein, A. Gonzalez, Puragra Guhathakurta, W. Hu, U. Seljak, Dennis Zaritsky
Author Affiliations +
Abstract
The Deep Lens Survey (DLS) is a deep BV Rz' imaging survey of seven 2°×2° degree fields, with all data to be made public. The primary scientific driver is weak gravitational lensing, but the survey is also designed to enable a wide array of other astrophysical investigations. A unique feature of this survey is the search for transient phenomena. We subtract multiple exposures of a field, detect differences, classify, and release transients on the Web within about an hour of observation. Here we summarize the scientific goals of the DLS, field and filter selection, observing techniques and current status, data reduction, data products and release, and transient detections. Finally, we discuss some lessons which might apply to future large surveys such as LSST.
© (2002) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David M. Wittman, J. Anthony Tyson, Ian P. Dell'Antonio, Andrew Becker, Vera Margoniner, Judith G. Cohen, D. Norman, D. Loomba, G. Squires, Gillian Wilson, Christopher W. Stubbs, J. Hennawi, David N. Spergel, P. Boeshaar, A. Clocchiatti, M. Hamuy, G. Bernstein, A. Gonzalez, Puragra Guhathakurta, W. Hu, U. Seljak, and Dennis Zaritsky "Deep lens survey", Proc. SPIE 4836, Survey and Other Telescope Technologies and Discoveries, (24 December 2002); https://doi.org/10.1117/12.457348
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KEYWORDS
Large Synoptic Survey Telescope

Telescopes

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