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March
A three dimensional rendering of the baseline design for the LSST as viewed from within the dome.
Credit: 
LSST Project Office
January
A three dimensional rendering of the baseline design of the dome with a cutaway to show the telescope within.
Credit: 
J. Andrew, NOAO/LSST Project Office

Friday, December 5, 2014

As illustrated in the accompanying graphic, the different roles of the LSST Project Office (LSSTPO) and LSST Corporation (LSSTC) have been clarified to align with the responsibilities and limitations of our federal construction funding.  The Project Office has stepped out as a true construction project, responsible for Building the Future: the LSST observing facility. In contrast, the Corporation will focus its efforts on Preparing for Science, fundraising, and defining partnerships and plans for Operations. This distinction will become more clear in the coming months with the transfer of the M1M3 mirror from LSSTC to LSSTPO and emerging support from LSSTC for the science collaborations. The LSST Project Office will remain focused on the construction of the LSST facility as detailed in the baseline plan presented to the NSF and DOE federal funding agencies.

Learn more in the December issue of LSST-E-News:

 

 

Friday, November 21, 2014
Image Credit: 
LSST Project Office

The LSST primary/tertiary mirror (M1M3) shipping container was successfully delivered to the University of Arizona Steward Observatory Mirror Lab (SOML) Thursday morning. Escorted by four Tucson Police Department cars and two pilot vehicles, the 30 foot by 30 foot oversized load departed CAID Industries' facility near Tucson International Airport at 4 am. Offloading at SOML was completed by 5:30 am. Once final acceptance testing of M1M3 has been completed, the mirror will be placed in the 36 ton shipping container, which was custom-built for LSST by CAID, and stored locally in Tucson. After final integrated testing, the mirror will be shipped in the container to the Cerro Pachon summit facility in Chile. 

Saturday, November 1, 2014

Thursday, October 2, 2014

LSST Director Steve Kahn and Project Scientist Zeljko Ivezic made a tour of major astronomical institutions in Australia during the last week in October. This so-called LSST “Road Show” came at the request of the Australian astronomical community and allowed that community to interact directly with the LSST leadership in investigating possible Australian involvement in the operations phase of the program. The tour included day-long sessions at the Australian Astronomical Observatory headquarters in Sydney, at Mt. Stromlo Observatory of the Australian National University in Canberra, at Swinburne University in Melbourne, and at the International Centre for Radio Astronomy Research on the campus of the University of Western Australia in Perth.

Wednesday, May 14, 2014

The long awaited news has arrived – LSST has received its federal construction start! On Friday afternoon, August 1, the NSF authorized the LSST project for construction with $27.5M in FY14 and a budget plan that stays within a $473M overall budget cap. AURA received NSF support to manage construction of LSST; the NSF press release describes LSST construction as “taking astronomy to the next level”. This marks the official federal start of the LSST project.

The effort that brings us to this important step in making LSST a reality started in the late 1990’s when design requirements for a telescope that would detect faint solar system bodies and those needed to map dark matter via weak gravitational lensing merged into a single wide-field survey telescope initially known as the Dark Matter Telescope. A decade of further developing the science case, refining instrument requirements, and building community support resulted in the LSST, as it was now known, rising from a runner-up in the 2000 NRC Decadal Survey to the top ranking for a large-scale ground-based facility in the 2010 NRC Decadal Survey. In May 2014, the National Science Board gave the NSF conditional approval to move the project to construction status. The NSF support of AURA to manage construction of the LSST marks the official federal start of the LSST project construction.

We gratefully acknowledge the hard work by so many that contributed to this milestone:

  • the LSST Corporation for their leadership role in promoting the concept and securing initial funding, organizing the necessary support within both the astronomy and physics communities for the construction and operations of LSST
  • our private donors – led by the Charles and Lisa Simonyi Fund for Arts and Sciences and including Bill Gates, Richard Caris, the W.M. Keck Foundation, Wayne Rosing and Dorothy Largay, Eric and Wendy Schmidt, and Edgar Smith – whose early contributions kept the project viable and supported the early construction efforts
  • the staff at the National Science Foundation and Department of Energy for continued support for design and development of the LSST concept and whose perseverance and diligence navigated LSST through the federal procedures at the most challenging time in US history to initiate a major research project
  • to Sidney Wolff, John Schaefer, and Don Sweeney for their early leadership roles on the project
  • to our hundreds of science collaborators who volunteered their time to provide valuable feedback and to document a compelling science case as presented to the National Research Council as the LSST Science Book
  • and especially to the hundreds of project team members who have worked so hard and endured hundreds of reviews to define and defend the LSST concept with their expertise, experience and passion.

From a twinkle in the eye of Tony Tyson in 1996 to relentlessly scanning the sky in 2022, the LSST has broken through the technology, science, and political challenges and is on its way to revolutionizing both our cosmic knowledge and the open and collaborative methods of acquiring that knowledge. With every confidence in the project team to complete the construction task, we are excited to begin this next phase for LSST and look forward to sharing the adventure.

Article written by Steven Kahn, LSST Director

Examples of LSST Science Projects

The design and optimization of the LSST system leverages its unique capability to scan a large sky area to a faint flux limit in a short amount of time. The main product of the LSST system will be a multi-color ugrizy image of about half the sky to unprecedented depth (r ~ 27.5), with superior image quality (0.7 arsec median delivered seeing in the r band), and exquisite photometric (1% or better) and astrometric (10 mas per epoch) accuracy. The catalogs based on these imaging data will include about 10 billion galaxies and a similar number of stars.

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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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