← Back to rubinobservatory.org


LSST mirror system status: from design to fabrication and integration

Lead Author: 
Araujo-Huack, Constanza
Other Authors/Credits: 
Sebag, J.; Liang, M.; Neill, D.; Muller, G.; Thomas, S.J.; Vucina, T.; Gressler, W. J.
Publication Date: 
Wednesday, July 27, 2016
Conference Papers
Constanza Araujo-Hauck ; Jacques Sebag ; Ming Liang ; Douglas Neill ; Gary Muller, et al. " LSST mirror system status: from design to fabrication and integration ", Proc. SPIE 9906, Ground-based and Airborne Telescopes VI, 99060L (July 27, 2016); doi:10.1117/12.2232923; http://dx.doi.org/10.1117/...
Journal or Publication name: 
SPIE Proceedings
In the construction phase since 2014, the Large Synoptic Survey Telescope (LSST) is an 8.4 meter diameter wide-field (3.5 degrees) survey telescope located on the summit of Cerro Pachón in Chile. The reflective telescope uses an 8.4 m f/1.06 concave primary, an annular 3.4 m meniscus convex...

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.   

Contact   |   We are Hiring

Admin Login

Back to Top