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LSST telescope integration and tests

Sebag, Jacques et al.
William Gressler; Doug Neill; Jeff Barr; Chuck Claver; John Andrew
Publication Date: 
Tuesday, July 22, 2014
Type: 
Conference Papers
SPIE
Citable: 
no
Category: 
SPIE Proceedings
Volume: 
9145
Page #: 
11
Abstract: 
The Large Synoptic Survey Telescope (LSST) Telescope integration and test plan is phased to ensure that subsystems and services are available to support the integration flow. It begins with the summit facility construction and shows how the major subsystems feed into the activities through final testing. In order to minimize the amount of hardware mated for the first time during that period, the approach is to favor all hardware mated and pre-tested at vendors’ facilities with associated hardware and software prior to delivery onsite. The integration and test plan exploits the diffraction limited on-axis image quality of the three-mirror design. In addition, fiducials will be used during optical acceptance testing at vendors’ facilities to capture the optical axis geometry of each optical element. These fiducials will be used during the integration and tests sequence to facilitate the telescope optical alignment. In this paper, we describe the major steps of the LSST telescope integration and test sequence prior to the start of commissioning with the science camera. http://adsabs.harvard.edu/abs/2014SPIE.9145E..4AS
Publication-73
Bibtex reference: 
@INPROCEEDINGS{2014SPIE.9145E..4AS, author = {{Sebag}, J. and {Gressler}, W. and {Neill}, D. and {Barr}, J. and {Claver}, C. and {Andrew}, J.}, title = "{LSST telescope integration and tests}", booktitle = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, year = 2014, series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, volume = 9145, month = jul, eid = {91454A}, pages = {91454A}, doi = {10.1117/12.2055241}, adsurl = {http://adsabs.harvard.edu/abs/2014SPIE.9145E..4AS}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} }

Financial support for Rubin Observatory comes from the National Science Foundation (NSF) through Cooperative Agreement No. 1258333, the Department of Energy (DOE) Office of Science under Contract No. DE-AC02-76SF00515, and private funding raised by the LSST Corporation. The NSF-funded Rubin Observatory Project Office for construction was established as an operating center under management of the Association of Universities for Research in Astronomy (AURA).  The DOE-funded effort to build the Rubin Observatory LSST Camera (LSSTCam) is managed by the SLAC National Accelerator Laboratory (SLAC).
The National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.
NSF and DOE will continue to support Rubin Observatory in its Operations phase. They will also provide support for scientific research with LSST data.   




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