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April
Credit: 
LSST Project Office
April
Credit: 
LSST Project Office
April
Credit: 
LSST Project Office

Tuesday, April 21, 2015

Tucson, AZ - Dr. Beth Willman has accepted the position of Deputy Director of the Large Synoptic Survey Telescope (LSST). She will perform this role as an Associate Astronomer at the Steward Observatory of the University of Arizona.  Her appointment will become effective September 1, 2015. 

LSST is the top-ranked large-scale ground-based project for the next decade as recommended by the National Research Council’s Astronomy and Astrophysics decadal survey (Astro2010). By digitally imaging the sky for a decade, the LSST will address the most pressing questions in astronomy and physics, drive advances in big-data science and computing, and create opportunities for transformative STEM education.  LSST received its federal construction start in 2014 as a joint project of the National Science Foundation and the Department of Energy, resulting in the onset of operations in late 2022.

Dr. Willman received her B.A. in astrophysics at Columbia University and a Ph.D. in astronomy at the University of Washington.  She has been a James Arthur Fellow at the Center for Cosmology and Particle Physics at New York University, and a Clay Fellow at the Harvard-Smithsonian Center for Astrophysics.  Since 2008 she has been a professor of Astronomy at Haverford College in Pennsylvania. 

Dr. Willman has been active with LSST for seven years, as chair of the Stars, Milky Way and Local Volume Science Collaboration, as lead author of the Milky Way chapter of the LSST Science Book, as a member of the Publication Board, and as a member of the Science Advisory Committee.   Her research has focused on using the Milky Way and its neighborhood to further our understanding of dark matter and galaxy formation. 

“LSST excites me because of the transformative impact it will have on our understanding of cosmic structures from the Solar System to massive superclusters, and because of the democratizing impact it will have on astronomy and astronomy education,” said Dr. Willman.  “I’m thrilled for this opportunity to have a guiding hand in the LSST construction Project to help realize this vision.”

LSST Director Dr. Steven Kahn said "We are extremely fortunate to have Beth Willman assume the LSST Deputy Directorship at this exciting time.  Her leadership abilities and respect within the scientific community make her the ideal person to help guide the Project, and to represent it to its relevant stakeholders.  I am certain she will excel in connecting with both the LSST Project Team and the external scientific community, so as, to ensure that the design and operation of the LSST is optimized scientifically."

More information about the LSST including current images, graphics, and animation can be found at http://www.lsst.org  See also http://www.lsst.org/News/enews/willman-0910.html. 

Financial support for LSST comes from the National Science Foundation(NSF), the Department of Energy(DOE), and private funding raised by the LSST Corporation. The NSF-funded LSST Project Office is managed by the Association of Universities for Research in Astronomy(AURA). The DOE-funded effort is managed by the SLAC National Accelerator Laboratory

Tuesday, March 3, 2015

Symmetry Magazine

Tuesday, April 21, 2015
Main Image Caption: 
The LSST First Stone is unveiled by (L-R) US Ambassador to Chile Michael A. Hammer, Chilean President Michelle Bachelet, NSF Director France Cordova, and LSST Director Steven Kahn.
Image Credit: 
Gentileza Presidencia

On April 14, 2015, LSST marked a major milestone, with the traditional First Stone (Primera Piedra) ceremony on Cerro Pachón, Chile.

Dr. Beth Willman has accepted the position of Deputy Director of the Large Synoptic Survey Telescope (LSST).    She will perform this role as an Associate Astronomer at the Steward Observatory of the University of Arizona. Her appointment will become effective September 1, 2015. See the announcement

Charles Simonyi and Bill Gates have given a spectacular boost to the private fund raising efforts of LSST Corporation with their $1M Challenge Match, a fresh start to the important mission of Enabling Science.

Completion of the LSST M1M3 substrate was celebrated in January at the UA Steward Observatory Mirror Lab. The polished mirror has since been relocated to a shipping container for a short journey to a storage facility where it will await a mirror cell and final transport to Chile in a couple years.

Control of the Cerro Pachón summit has been transferred to the Summit Facility Contractor as the pace of construction accelerates. The final sculpting of the site and the forthcoming facility construction are viewable in real time from two webcams linked from the gallery.

The baseline for fabrication of the LSST Camera has achieved a significant milestone, with “Critical Decision 2” approval from the DOE. Other camera developments include the successful demonstration of the final sensors and electronics in a test camera at Brookhaven National Lab and a successful subscale refrigeration system test at SLAC.

The distributed LSST project plans to come together again this year for its annual Project and Community Workshop the week of August 17th in Bremerton, WA. This is an open meeting; details will be posted as they become known at the meeting web page. Project-focused meetings early in the week will be followed by a Cadence workshop at the end of the week.

Read more in the April 2015 issue of LSST E-News

From the Project Office, April 2015

Spring is the season of new beginnings, and it’s no exception around the LSST Project. Charles Simonyi and Bill Gates have given a spectacular boost to the private fund raising efforts of LSST Corporation with their $1M Challenge Match, a fresh start to the important mission of Enabling Science. Completion of the LSST M1M3 substrate was celebrated in January at the UA Steward Observatory Mirror Lab. The polished mirror has since been relocated to a shipping container for a short journey to a storage facility where it will await a mirror cell and final transport to Chile in a couple years. Control of the Cerro Pachón summit has been transferred to the Summit Facility Contractor as the pace of construction accelerates. The final sculpting of the site and the forthcoming facility construction are viewable in real time from two webcams linked from the gallery. The baseline for fabrication of the LSST Camera has achieved a significant milestone, with “Critical Decision 2” approval from the DOE. Other camera developments include the successful demonstration of the final sensors and electronics in a test camera at Brookhaven National Lab and a successful subscale refrigeration system test at SLAC.

The distributed LSST project plans to come together again this year for its annual Project and Community Workshop the week of August 17th in Bremerton, WA. This is an open meeting; details will be posted as they become known at the meeting web page. Project-focused meetings early in the week will be followed by a Cadence workshop at the end of the week. These two aspects of the meeting will run sequentially this year, not in parallel, in an attempt to avoid scheduling conflicts as much as possible. The Project Staff continues to increase and the LSST 2015 workshop will be another great opportunity to bring the team and science community together.

On April 14, 2015, LSST marked a major milestone, with the traditional First Stone (Primera Piedra) ceremony on Cerro Pachón, Chile. Laying of the first stone is a Chilean tradition marking the construction start for a new astronomical observatory. Chilean President Michelle Bachelet, U.S. Ambassador to Chile Michael A. Hammer, NSF Director France Córdova, and Charles Simonyi were among the dignitaries present to mark this start of summit construction. All these activities remind us that the construction start is real and the ten years of design and development that brought us to this point are about to bear fruit. Spring has indeed brought a new beginning to the LSST.

M1M3 Milestone Achieved

In February, LSST achieved a significant milestone with the primary/tertiary mirror (M1M3) – completion of the mirror surfaces’ polishing effort and successfully placing the $20 million mirror substrate in its storage container, where the LSST team will conduct additional integrated testing before final shipment to Chile in the coming years.

On February 13, the LSST Project accepted the M1M3 mirror surfaces without conditions, given their outstanding characteristics and overall expected performance. Acceptance, which marked completion of the polishing effort, followed rigorous testing and analysis jointly performed by Steward Observatory Mirror Lab (SOML) and LSST Project staff.

New Hires

The LSST Hiring Campaign continues in full force as the project staffs up to meet the demands of the construction effort. Current positions, along with those filled and coming soon, are posted online at http://www.lsst.org/hiring. The individuals below have joined the project recently as examples of Top Talent Working in a Team Environment that Inspires Excellence - welcome!

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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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