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Friday, September 25, 2015

UPDATE: EARTHQUAKE IN CHILE

Damage to LSST was minimal from last week’s earthquake, including no injuries to LSST personnel, as described in our 9/18/15 Facebook posting: https://www.facebook.com/myLSST.  LSST Site Manager Eduardo Serrano has since informed us that the concrete plant has been leveled and the road to the summit is now open; the 70-ton crane is on site.  Besalco's surveyors are doing a General Survey of all reference points used for construction post-earthquake, work that will take a few more days to complete.

PROJECT OFFICE NEWS

  • Beth Willman visited LSST Corporation Member Institution Texas A&M this week to talk about LSST and near-field cosmology.
  • The Project Office has taken steps to ensure that LSST can operate normally for a period of time in the event of an October 1 government shutdown and possible continuing resolution. 
  • Managers participated in a two-day training session to determine if LSST is required to obtain export control licenses or exemptions for our data, parts, and components; a compliance plan suitable for LSST’s situation is being developed.
  • Steve Kahn, Zeljko Ivezic, and Mario Juric made a visit to NASA Headquarters in Washington to discuss LSST’s capabilities for near earth object (NEO) detection and orbit characterization; see today’s blog posting for more information.
  • Results of the Intra-Project Communications Survey, Workplace Culture notecards, and LSST2015 Exit Survey have been shared with LSST team members and posted on the meeting website.

PROJECT SUBSYSTEM NEWS

Camera: The recent wavefront sensor review went well as did the Ball Aerospace Final Design Review for the L1-L2 Lens Assembly.
Data Management: A series of “Boot Camps” are starting up for new DM hires; dates are October 5 - 7 and the venues are Princeton, University of Washington, and LSST Tucson.  All sessions will be recorded for broader distribution at a later time.
Telescope & Site: Several members of the T&S team will be in Madrid, Spain next week for a Preliminary Design Review with the Telescope Mount Assembly vendor GHESA Ingeniería y Tecnología.
Systems Engineering: Four requests were approved at this week’s Change Control Board meeting including placement of the Operations Simulation Requirements under formal change control.
Education & Public Outreach: The EPO Manager position has been rescoped to emphasize the technical nature of the position and is now posted on lsst.org/hiring.org


LSST CORPORATION NEWS

The LSST Corporation will have its annual face-to-face meetings of the Executive Board and the Board of Directors in Tucson at the Westward Look on October 8-9, 2015. 

The LSST Corporation is supporting an Enabling Science workshop entitled Astro Hack Week 2015 to be held at New York University September 28-October 2.  This week-long event is focused on astrostatistics and data-intensive astronomy. 

SCIENCE COLLABORATION NEWS

The chairs of the LSST Science Collaborations met during the LSST2015 meeting in Bremerton in mid-August, to discuss the activities of each science collaboration, roadmap plans, and scientific challenges ahead.  We are working to give each science collaboration a web presence; many of them already have websites in place. 

The LSST Corporation is supporting a variety of meetings and workshops of the science collaborations, under its Enabling Science initiative.

SCIENCE ADVISORY COMMITTEE NEWS

The LSST Science Advisory Committee meets monthly, and posts the minutes of its meetings to its website.  Its members cover the full gamut of LSST science themes, from the solar system to dark energy, and has the responsibility to communicate the interests and concerns of the science community to the LSST Project Office.   

Recent topics of discussion include mechanisms for making decisions on the LSST cadence, best practices in communication between the LSST Project and the scientific community, and understanding the detailed nature of Level 1 and Level 2 data releases.

SAVE THE DATE:

November 8-13, 2015: 47th DPS Meeting
January 4-8, 2016: AAS 227, Kissammee, FL                
February 22 – 24, 2016: LSST Joint Technical Meeting, Santa Cruz, CA
Week of August 15, 2016: LSST2016, Tucson, AZ


 

September

Observing the sky: LSST simulation

This is an animation of a potential LSST observing strategy, from simulated survey 'enigma_1189'. more
September
This exploded view of the LSST’s digital camera highlights its various components, including lenses, shutter and filters.
Credit: 
SLAC National Accelerator Laboratory
September

Flight Cerro Tololo - Cerro Pachon - LSST

LSST looks great from the air. Nice flyby video from David Walker. more

Monday, September 21, 2015

Metrics Analysis Framework (MAF)

The Metrics Analysis Framework (MAF) is an open-source python framework developed to provide a user-friendly, customizable, easily-extensible set of tools for analyzing data sets. Its initial goal is to provide a tool to evaluate Operations Simulator (OpSim) simulated surveys to help understand the effects of telescope scheduling on survey performance, however, MAF can be applied to a much wider range of datasets.

Monday, August 31, 2015

(SLAC National Accelerator Laboratory)

The Large Synoptic Survey Telescope's 'Eye' Will be Built at SLAC

Menlo Park, Calif. — The Department of Energy has approved the start of construction for a 3.2-gigapixel digital camera – the world’s largest – at the heart of the Large Synoptic Survey Telescope (LSST).  Assembled at the DOE's SLAC National Accelerator Laboratory, the camera will be the eye of LSST, revealing unprecedented details of the universe and helping unravel some of its greatest mysteries.

See the SLAC Press Release.

 

Friday, August 28, 2015
Rebar on the Summit, August 27, 2015
Main Image Caption: 
Construction for the LSST Summit Facilities Buildling on Cerro Pachon now reaches above the surface, August 27, 2015

As the Chilean winter snow melts, the LSST facility on Cerro Pachón begins to emerge above the ground level - rebar posts extend from the concrete footings of the support columns of the observatory building. The summit construction is progressing to be ready for the initial integration with the dome in January 2017 and be fully completed by January 2018. The facility will provide 3,000 square meters of maintenance and support space in a footprint that extends from 17 meters below the summit platform to 38 meters above the summit to the top of the dome. Over 5,000 cubic meters of concrete have been poured to establish the foundation of the facility that will provide space for the telescope, mirror coating plant, camera clean room, control room and required operational space.

August
More than 220 project team members and scientists attended the LSST2015 Workshop in Bremerton, WA
Credit: 
R. Sparks / LSST Project Office

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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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