March 5, 2019 - The object in this photo, called the calibration screen reflector, was manufactured in the National Optical Astronomy Observatory (NOAO) instrument shop, which is located in the same building as the LSST Project Office in Tucson, Arizona. Our talented instrumentation team has been working on this piece of equipment for many months, and it shows! The reflector will be an important component of the calibration system inside the dome of LSST; this system is designed to determine how real-world factors like dust, and evolution to the sensitivity of the equipment over time, affect the images taken by the LSST Camera.
February 8, 2019 - The challenge to viewing and imaging celestial objects from the Earth’s surface is that the Earth’s atmosphere distorts light from space. When you look up at the stars and see them twinkle, you’re experiencing this phenomenon; light from stars is (generally) constant, but the light that reaches your eyes has been pushed around by turbulence in the Earth’s atmosphere. That turbulence is caused by the interaction of varying temperature and density layers between the Earth’s surface and space. Twinkling stars might be pretty to look at, but they’re pretty annoying for scientists who want a crisp, clear view of the objects they’re studying.
January 28, 2019 - The LSST Primary/Tertiary Mirror (M1M3) is currently in the Richard F Caris Mirror Lab at the University of Arizona for optical testing. In January, the M1M3 on its support system was positioned at the bottom of the lab’s interferometry tower in anticipation of two test campaigns. The first, which has just concluded, took place from January 14-25. The second campaign is scheduled for February 11-22.
The tests use specialized optical equipment to evaluate the figures of the M1 and M3 mirror surfaces. Separate instruments, called interferometers, are used to perform measurements on each of the two mirrors that make up the monolith. The interferometer used to test M1 is at the very top of the tower, and the one used to test M3 is lower down, on a movable bridge. The mirror surfaces are tested separately, first M1, then M3, then M3 again, then M1. When M1 is being tested, the lower interferometer is moved out of the optical path.
During the test process, the interferometer in use emits two beams of light. One travels to the mirror and bounces back, and the other goes to a reference within the interferometer. The interaction between the two beams of light is recorded in an image called an interferogram (the black and white image in the photo to the left). The lines in the image are called interference fringes, and each one represents approximately 300 nanometers. A tight grouping of lines indicates a steep change in the height of the surface, much like tight lines on a topographic map indicate steep terrain. A “perfect” mirror interferogram would be a solid color, because its measurements would be recorded as a single fringe. But according to LSST Telescope and Site Mechanical Engineer Tucker Booth, achieving perfection on individual mirrors isn’t the goal. Instead, it’s the optimization of the entire M1M3 monolith that will ensure the best possible images during LSST Operations.
Allowing adequate time for optical testing, analysis, and optimization in Tucson reduces the work that will have to be done to prepare for operations once the telescope is assembled in Chile. Additionally, the unique testing environment available at the Richard F Caris Mirror Lab isn’t available in the summit facility building, so LSST is fortunate to have access to this world-class facility for the M1M3 optical test campaigns. M1M3 is currently scheduled to ship from the U.S. to Chile in May.
January 14, 2019 - The 233rd Meeting of the American Astronomical Society (AAS) wrapped up on January 10; this year’s winter meeting took place in Seattle, WA, with more than 3000 people registered. LSST staffed an exhibitor booth during the meeting within the National Science Foundation’s (NSF) Pavilion, giving project updates and answering questions from conference attendees. Numerous posters and talks were presented by LSST Project and Science Collaboration members.
It’s hard to believe another calendar year is drawing to a close! 2018 was jam-packed with activity for LSST, so it’s no wonder the year seemed to pass in a flash. Here’s a look back at some of the major accomplishments and milestones the LSST Project celebrated this year:
The LSST Secondary Mirror (M2) also arrived in Chile on December 7th, and will reach Cerro Pachon before the end of the year. What’s in store for 2019? Delivery of more critical pieces of equipment to the summit, including the Telescope Mount Assembly and M1M3 Mirror and Cell Assembly; coating of the Secondary Mirror (M2) on the summit; progress towards determining the LSST observing cadence; and much more. Visit lsst.org and follow LSST on social media for the latest updates!
It is with great regret that we inform you of the sudden passing of Jim Parsons, one of our NCSA colleagues. Our thoughts are with his family and our team at NCSA. There will be a DM community post (https://community.lsst.org/c/dm) with arrangements when we know them, and an opportunity to express sentiments to be forwarded to the family.
November 20, 2018 - The LSST Network Engineering Team (NET) had a strong presence at the Supercomputing 2018 Conference (SC18) in Dallas, TX, last week, including a successful demonstration of the data transfer capabilities of the fiber optic networks that will be used during LSST operations. Digital data were transferred from the Base Site in La Serena, Chile, to the LSST Data Facility at the National Center for Supercomputing Applications (NCSA) in Champaign, IL. During the data transfer demonstration, a peak rate of 100 Gigabits/second (Gb/s) was achieved for short periods, and a sustained rate of 80 Gb/s was achieved over a three hour period, exceeding the test target.
November 12, 2018 - It looked a lot like a space ship before it was wrapped for shipping, but it’s actually a very earth-bound piece of cargo: the Coating Chamber for the mirrors of the Large Synoptic Survey Telescope (LSST). The Coating Chamber arrived on the summit of Cerro Pachón in Chile on November 11, 2018, and is now positioned on the service floor of the LSST summit facility building. The Coating Chamber and its associated equipment will share this level with the camera maintenance rooms, the vertical platform lift, and the shipping and receiving area. The Coating Chamber will be used to coat LSST’s mirrors when they arrive on Cerro Pachón, and to re-coat the mirrors periodically during Operations.
One of the activities included in Factory Acceptance Testing of the Telescope Mount Assembly (TMA) is installation and removal of the camera surrogate, a steel structure that approximates the mass of the LSST camera assembly, using the camera lifting fixture. The camera lifting fixture, like the TMA, was fabricated at the Asturfeito factory in Spain. Using a camera surrogate for these tests ensures that any issues arising during the installation or removal process can be addressed long before the real—and far more delicate—camera is integrated with the TMA in Chile. This video contains footage of the installation and removal of the surrogate camera using the camera lifting fixture.
October 30, 2018 - On the morning of October 25th, at the Richard F. Caris Mirror Lab on the University of Arizona campus, the LSST Primary/Tertiary Mirror (M1M3) was successfully lifted out of its transport container and onto the M1M3 Cell. The mirror lift was performed with a special lifting fixture, outfitted with 54 vacuum pads, that was designed specifically to safely lift and lower the 37,000 lb (16,780 kg) glass monolith. The M1M3 Mirror was lifted onto the Cell, interfacing successfully with the 355 static supports (wire rope isolators), that hold it above the upper surface of the mirror cell.
In order to minimize the risk of damage to the glass, the M1M3 Mirror will only be lifted in this manner this four times during the entirety of LSST construction and operations. This lift was the second; the first lift occurred in February of 2015, when the Mirror’s fabrication was complete and it was lifted into its protective transport container. The third lift will occur when it’s time to put the Mirror back into its protective box for transport to Chile, and the fourth will integrate M1M3 and the Cell for the last time in the LSST summit facility. Once M1M3 is integrated with the Cell at the observatory site, it will not be removed from the Cell again—not even for coating. The M1M3 Mirror can be coated while installed on the Cell, thanks to an internal cylindrical vacuum barrier. When rolled into place under the Coating Chamber lid using the transport cart, the Cell takes the place of the bottom half of the Coating Chamber, allowing a vacuum to be drawn and the M1M3 Mirror to be coated.
Over the next few weeks, work in the Mirror Lab will focus on the integration of the Mirror and Cell, which includes installing hardpoints, actuators, and electronics. These activities will be followed by functional testing of the assembled system. The Mirror is scheduled to move under the Mirror Lab’s interferometery tower for optical testing in January, 2019.
Financial support for LSST 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 LSST 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 LSST camera 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.