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Key Numbers

System Design

The basic characteristics of the LSST facility derives directly from its science programs. The telescope itself must have a wide field of view in order to obtain several hundred images of each area of the sky over an entire hemisphere in only 10 years. The aperture must be large in order to achieve the sensitivity required to reach faint limiting magnitudes. The wavelength coverage must be broad in order to derive photometric redshifts and to characterize the ages and metallicities of stellar populations.

 
 

List of Survey Requirements

LSST System & Survey Key Numbers

This page lists Key Numbers that describe the LSST system and survey.  More detailed information is available in the LSST Overview Paper and Science Requirements Document.  

Commissioning

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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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