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Monday, January 4, 2016
Main Image Caption: 
Project scientists Zeljko Ivezic and Lucianne Walkowicz answer questions at the LSST booth.
 

LSST had a strong showing at the AAS227 meeting in Kissimmee, FL, 4-8 January 2016.


The LSST Booth was part of the NSF Pavilion on the Exhibit Hall Floor. 

LSST Speakers at the NSF Pavilion:

LSST Observing Strategy by Zeljko Ivezic

Evaluating the LSST Science Pipelines with Precursor Datasets2 by David Nidever

LSST DM Community Resources3 by Jonathan Sick
 

The LSST Town Hall was attended by over 120 participants and featured these speakers:

LSST participated in the Career Networking & Job Fair, sharing the message that LSST is Hiring and looking for top talent.

 


 

 

 

 

 

 

Friday, January 29, 2016

January 29, 2016 - Eleven members of the LSST Telescope and Site and Project Office have been in Madrid, Spain, this week participating in a successful Final Design Review of the Telescope Mount Assembly (TMA) with prime contractor Empresarios Agrupados (EA). The panel members evaluated EA’s design and sub-contractor efforts, reviewing design conformance and assessing risk to advancing the key components into the fabrication stage. Major assemblies such as the azimuth track assembly and the azimuth and elevation assembly showed the adequate maturity needed to allow moving forward with purchasing steel and starting fabrication. The TMA team will now begin preparation for the next milestone, which is the Manufacturing Readiness Review next August.  Elements of the TMA will begin fabrication soon to support final completion and installation in Chile in 2018.

Friday, January 29, 2016

PROJECT NEWS - Para español, vea abajo

Several members of the Telescope & Site team are in Madrid, Spain, completing a successful Final Design Review of the Telescope Mount Assembly (TMA) with prime contractor Empresarios Agrupados.  In anticipation of proceeding into full fabrication, the Asturfeito facility in the Aviles Port region of northern Spain is preparing 10-meter granite pylons to be used for testing purposes.  

Project team members from all subsystems are preparing for two reviews taking place the week of February 8th.  The NSF Status Review will assess the current status of the project and evaluate plans for the future, with emphasis on the next year of construction.  The purpose of the Internal Operations Planning review is for the LSST Operations Planning Team (LOPT) to receive a thorough evaluation of our initial operations concepts and (steady-state) FTE estimates, with a focus on LSST’s operational functions and activities.

The first science grade production sensor for the LSST focal plane has successfully completed testing at BNL, achieving a Level 2 acceptance milestone, tracked at the DOE agency level.

CORPORATION NEWS

LSSTC is excited to report that thanks to all our individual donors, the LSSTC Board, and the Institutional Member Representatives, we have succeeded in matching the $500K Charles Simonyi / Bill Gates Match Challenge. The funds are slated to support LSSTC’s Enabling Science grant program and our member institutions in support of LSST-related work. Thanks to everyone who supported this effort.

UPCOMING 2016 MEETINGS with LSST INVOLVEMENT

(those with asterisk* are LSSTC funded):

February 8-10

NSF Status Review, Tucson, AZ

February 22-24

LSST Joint Technical Meeting, Santa Cruz, CA

March 7-11

LSST Dark Energy Science Collaboration (DESC) meeting, SLAC

March 8-10

2nd Annual US-Chile Education Summit, Chile

April 5-7

Photometric Redshifts in LSST*, University of Pittsburgh

April 11-13

LSSTC Board Meeting* in Washington, DC

May 22 – 25

Cross-correlation Spectacular with LSST:  Exploring Synergies Between LSST
and External Datasets to Discover Fundamental Physics
, BNL

May 24-26

XLDB 2016 Conference and Workshop, SLAC

June  6-10

Statistical Challenges in Modern Astronomy VI*, Carnegie Mellon University

June 12-16

Meeting of the Stars, Milky Way and Local Volume Science Collaboration*
at AAS 228, San Diego, CA

June 20-24

LSST@Europe2*, Belgrade, Serbia

June 28-July

SPIE Astronomical Telescopes & Instrumentation, Edinburgh, Scotland

July 18-22

LSST DESC meeting, at Oxford, UK

August 15-19

LSST 2016 Project & Science Workshop, Tucson, AZ


Noticias del Proyecto

Varios miembros del equipo de Sitio y Telescopio se encuentran en Madrid, España, completando una revisión del diseño final del Telescope Mount Assembly (TMA) con el contratista principal Empresarios Agrupados.  En anticipación de proceder plenamente a la fabricación, la instalación Asturfeito en el Puerto de Avilés, al norte de España está preparando pilones de granito de 10 metros que se utilizaran para propósitos de prueba.  

Los miembros del equipo de proyecto de todos los subsistemas se preparan para dos revisiones que tendran lugar la semana del 8 de febrero. El Estado de Revisión de NSF evaluará el estado actual del proyecto y evaluara los planes para el futuro, con énfasis en el próximo año de construcción.  El propósito de la revisión interna de Operations Planning es para que el equipo de planificación de operaciones LSST (LOPT) reciba una evaluación exhaustiva de nuestros conceptos y operaciones iniciales (estado constante) estimaciones de FTE, con un enfoque sobre las funciones operacionales y actividades de LSST.

El primer sensor de producción de grado de ciencias para el plano focal de LSST ha completado exitosamente las pruebas en BNL, logrando un  hito de aceptación de nivel 2, rastreado a nivel del organismo de DOE.

Noticias de la corporación

LSSTC está entusiasmado de informar que gracias a todos nuestros donantes individuales, el LSSTC Board y los Representantes de Miembros Institucionales, hemos logrado igualar el reto de $500K Charles Simonyi / Bill Gates Match Challenge. Los fondos están programados para apoyar la del Programa de Becas de Habilitación de Ciencia de LSSTC  y nuestras instituciones miembros en apoyo de la labor relacionada con LSST. Gracias a todos los que apoyaron este esfuerzo.

PRÓXIMAS REUNIONES CON PARTICIPACIÓN LSST 2016 

(aquellos con un asterisco* son financiados por LSSTC):

Febrero 8-10

Revisión de estado de NSF, Tucson, AZ

Febrero 22-24

Reunión técnica conjunta LSST, Santa Cruz, CA

Marzo 7-11

LSST Energía Oscura Ciencia colaboración (DESC) reunión, SLAC

Marzo 8-10

Segundo anual US-Chile Education Summit, Chile

Abril 5-7

En Redshifts fotométricos LSST*, Universidad de Pittsburgh

Abril 11-13

Reunión de la Junta LSSTC* en Washington, D.C.

Mayo 22 - 25

Cross-correlation Spectacular with LSST:  Exploring Synergies Between LSST 
and External Datasets to Discover Fundamental Physics
, BNL

Mayo 24-26

XLDB 2016 Conferencia y Taller, SLAC

Junio 6-10

Statistical Challenges in Modern Astronomy VI*, de la Carnegie Mellon University

Junio 12-16

Reunión de la Stars, Milky Way and Local Volume Science Collaboration
en AAS 228, San Diego, CA.

Junio 20-24

LSST@Europe2*, Belgrado, Serbia

Junio 28-Julio

SPIE Astronomical Telescopes & Instrumentation, Edimburgo, Escocia

Julio 18-22

DESC LSST reunión, en Oxford, Reino Unido

Agosto 15-19

LSST 2016 & Science Workshop, Tucson, AZ

 

Friday, January 22, 2016

PROJECT NEWS Para español, vea abajo

S. Kahn, V. Krabbendam, and B. Willman are *not* traveling to Washington, DC, as planned for the January 22nd meeting of the AURA Management Council for LSST (AMCL) due to severe weather.  Instead the meeting will be held via videoconferencing. The AMCL provides financial oversight and advocacy for the management of LSST.

Several members of the Telescope & Site team head to Madrid, Spain next week for a Final Design Review of the Telescope Mount Assembly (TMA) with prime contractor Empresarios Agrupados. 

On Cerro Pachón, Besalco management honored its employees for completing the first year of LSST construction activities on the summit with no serious injuries or job-site accidents.

The first production sensor was received by the Camera team in December and is undergoing testing at SLAC.  Successful completion of this analysis is a Level 2 milestone, tracked at the DOE agency level.

PERSONNEL NOTES

The Project Office is happy to announce the arrival of two new employees, who are onboarding this week.  We welcome Rob Kooper (NCSA) with his expertise in workflows and middleware and Christopher Montgomery, who has joined the LSST Project Office in Tucson as our Training Coordinator.

Employees are invited to attend an LSST Orientation & Onboarding Session on Tuesday, January 26th at 1:30PM in Room 27 in Tucson. This orientation is not intended solely for new employees; it is important that we all share a common understanding of LSST policies, standards, culture, practices, and tools as we continue toward our mutual goal of building the LSST.  Those interested in participating remotely should contact Daniel Calabrese.

UPCOMING MEETINGS with LSST INVOLVEMENT

(those with asterisk* are LSSTC funded):

February 8-10

NSF Status Review, Tucson, AZ

February 22-24

LSST Joint Technical Meeting, Santa Cruz, CA

March 7-11

LSST Dark Energy Science Collaboration (DESC) meeting, SLAC

March 8-10

2nd Annual US-Chile Education Summit, Chile

April 11-13

LSSTC Board Meeting* in Washington, DC

May 22 – 25

Cross-correlation Spectacular with LSST:  Exploring Synergies Between LSST
and External Datasets to Discover Fundamental Physics
, BNL

May 24-26

XLDB 2016 Conference and Workshop, SLAC

June  6-10

Statistical Challenges in Modern Astronomy VI*, Carnegie Mellon University

June 12-16

Meeting of the Stars, Milky Way and Local Volume Science Collaboration* at AAS 228, San Diego, CA

June 20-24

LSST@Europe2*, Belgrade, Serbia

June 28-July

SPIE Astronomical Telescopes & Instrumentation, Edinburgh, Scotland

July 18-22

LSST DESC meeting, at Oxford, UK

August 15-19

LSST 2016 Project & Science Workshop, Tucson, AZ


Noticias del Proyecto

S. Kahn, V. Krabbendam y B. Willman *no* viajaran a Washington, DC, como estaba previsto el 22 de Enero para la Reunión del Consejo de Administración de AURA para LSST (AMCL) debido a condiciones climáticas severas.  Por el contrario, la reunión se celebrará a través de videoconferencia.  La AMCL proporciona supervisión financiera y la promoción de la gestión de LSST.

Varios miembros del equipo de telescopio y del sitio van a Madrid, España la próxima semana para una revisión del diseño final del Telescopio Mount Assembly (TMA) con el contratista principal Empresarios Agrupados.

En Cerro Pachón, la gerencia de Besalco rindió homenaje a sus empleados por completar el primer año de  actividades de la construcción de LSST sin graves lesiones o accidentes en el sitio de trabajo.

El primer sensor de producción fue recibido por el equipo de cámara en diciembre y se está probando en SLAC.  La exitosa culminación de este análisis es un hito L2, rastreado al nivel de agencia de DOE.

Notas del personal

La Oficina del Proyecto incorpora esta semana a dos empleados, la. Le damos la bienvenida a Rob Kooper (NCSA) con su experiencia en flujos de trabajo y middleware y Christopher Montgomery, quien se ha unido a la oficina del proyecto LSST en Tucson como nuestro coordinador de capacitación.

Los empleados están invitados a asistir a una sesión de orientación& Integración de LSST el martes, 26 de enero a las 1:30h en la sala 27, en Tucson. Esta orientación no está destinada únicamente para los nuevos empleados; es importante que todos compartamos un entendimiento común de las políticas, normas, cultura, prácticas y herramientas de LSST para continuar hacia nuestro objetivo común de construir LSST. Los interesados en participar deben contactar de forma remota a Daniel Calabrese.

PROXIMAS REUNIONES CON PARTICIPACION DE LSST

(aquellos con asterisco * son financiado por LSSTC):

Febrero 8-10

Revisión de estado de NSF, Tucson, AZ

Febrero 22-24

Reunión técnica conjunta LSST, Santa Cruz, CA

Marzo 7-11

LSST Energía Oscura Ciencia colaboración (DESC) reunión, SLAC

Marzo 8-10

Segundo anual US-Chile Education Summit, Chile

Abril 11-13

Reunión de la Junta LSSTC* en Washington, D.C.

Mayo 22 - 25

Cross-correlation Spectacular with LSST:  Exploring Synergies Between LSST 
and External Datasets to Discover Fundamental Physics
, BNL

Mayo 24-26

XLDB 2016 Conferencia y Taller, SLAC

Junio 6-10

Statistical Challenges in Modern Astronomy VI*, de la Carnegie Mellon University

Junio 12-16

Reunión de la Stars, Milky Way and Local Volume Science Collaboration* en AAS 228, San Diego, CA.

Junio 20-24

LSST@Europe2*, Belgrado, Serbia

Junio 28 - Julio

SPIE Astronomical Telescopes & Instrumentation, Edimburgo, Escocia

Julio 18-22

Reunión DESC LSST, en Oxford, Reino Unido

Agosto 15-19

LSST 2016 & Science Workshop, Tucson, AZ

 

Friday, January 15, 2016

PROJECT NEWS - Para español, vea abajo

With our first Weekly News Digest of 2016 we link to our holiday card, and point out that only the tree was added with PhotoShop - everything else is real!  Additional construction images are being added weekly to the LSST Image Gallery; others appear on Facebook, accessible directly or from the LSST News Page.  

LSST had a strong presence at AAS227, with a well-attended Town Hall, a table at the Career Fair, active participation in the LSST-supported Hack Day, and an exhibit in the NSF pavilion showing our updated video.  Project Scientist Zeljko Ivezic’s talk on the LSST Observing Cadence has been archived in Zenodo and made available through the online Image Gallery and Publications links on lsst.org.   

Operations planning is proceeding rapidly, with a review of operations functions to take place Feb 11-12, 2016 in Tucson.  The review panel is: Bob Blum (NOAO), Adam Bolton (NOAO), Brenna Flaugher (Fermilab), Nancy Levenson (Gemini), Ashish Mahabal (Caltech), and Connie Rockosi (UCSC/Lick).  Review materials will be shared with LSST Project members and presented for discussion at the February Joint Technical Meeting.

Operations discussions are also underway with AURA's other ground-based optical facilities, NOAO and Gemini, to identify possible models for operational coordination and resource sharing.  These discussions will include focus on NSF cost efficiencies that could be achieved by a closer coordination between LSST and NOAO during operations.

PERSONNEL NOTES

Welcome to LSST Telescope & Site, Tomi Vucina, Coating System Engineer.  Tomi transferred from Gemini South where he worked twelve years with the Coating and Optics group. He is now working for LSST and will be living in Tucson the next few years to manage the LSST Coating Plant contract effort and support other Telescope related activities.

UPCOMING MEETINGS with LSST INVOLVEMENT

(those with asterisk* are LSSTC funded):

February 8-10, 2016

NSF Status Review, Tucson, AZ

February 22-24, 2016

LSST Joint Technical Meeting, Santa Cruz, CA

March 7-11, 2016

LSST Dark Energy Science Collaboration (DESC) meeting, SLAC

March 8-10, 2016

2nd Annual US-Chile Education Summit, Chile

April 11-13, 2016

LSSTC Board Meeting* in Washington, DC

May 22 – 25, 2016

Cross-correlation Spectacular with LSST: Exploring Synergies Between LSST 
and External Datasets to Discover Fundamental Physics
, BNL*

May 24-26, 2016

XLDB 2016 Conference and Workshop, SLAC

June  6-10, 2016

Statistical Challenges in Modern Astronomy VI*, Carnegie Mellon University

June 20-24, 2016

LSST@Europe2*, Belgrade, Serbia

June 28-July 1, 2016

SPIE Astronomical Telescopes & Instrumentation, Edinburgh, Scotland

July 18-22, 2016

LSST DESC meeting, at Oxford, UK

August 15-19, 2016

LSST 2016 Project & Science Workshop, Tucson, AZ


Noticias del Proyecto

Con nuestro primer resumen semanal de noticias de 2016 se enlace nuestra holiday card, y señalar que solamente el árbol fue añadido con PhotoShop - todo lo demás es real! Imágenes adicionales de la construcción están siendo añadidas semanalmente al LSST Image Gallery; otros aparecen en Facebook, accesible directamente o a través del LSST News Page.

LSST tuvo una fuerte presencia en AAS227, con una nutrida participación en el Ayuntamiento, una mesa en la Feria de Empleo,  participación activa en el Hack Day apoyado por LSST, y una exposición en el pabellón de NSF mostrando nuestro video actualizado updated video. La charla del Científico del Proyecto Zeljko Ivezic sobre el LSST Observing Cadence ha sido archivada en Zenodo y disponible a través de la online Image Gallery y Publications enlaces en lsst.org.

La planificación de operaciones avanza rápidamente, con una revisión de las funciones de operaciones que tendrá lugar el 11-12 de febrero, 2016 en Tucson. El panel de revisión está compuesto por: Bob Blum (NOAO), Adam Bolton (NOAO), Brenna Flaugher (Fermilab), Nancy Levenson (Gémini), Ashish Mahabal (Caltech), y Connie Rockosi (UCSC/lamer). El material de la revisión será compartido con miembros del proyecto LSST y presentado para su discusión en la Reunión técnica conjunta de febrero.

Discusiones sobre operaciones están siendo llevadas a cabo con otras instalaciones ópticas basadas en tierra de AURA, NOAO y Gemini, para identificar posibles modelos para la coordinación operativa y el intercambio de recursos. Estas discusiones incluirán el foco en eficiencias de costes de NSF que podrían lograrse mediante una coordinación más estrecha entre el LSST y NOAO durante las operaciones.

Notas personal

Bienvenido al Telescopio & Site LSST! Tomi Vucina, Ingeniero de sistemas de revestimiento. Tomi se ha transferido desde Gémini Sur donde trabajó 12 años con el grupo de Óptica y recubrimiento. Él está trabajando ahora para LSST y estará viviendo en Tucson los próximos años para gestionar el esfuerzo del contrato de la planta de revestimiento de LSST y el apoyo de otras actividades relacionadas con el telescopio.

Las próximas reuniones con participación LSST (aquellos con un asterisco* son financiados por LSSTC):

Febrero 8-10, 2016

Revisión de estado de NSF, Tucson, AZ

Febrero 22-24, 2016

Reunión técnica conjunta LSST, Santa Cruz, CA

Marzo 11, 2016

LSST Energía Oscura Ciencia colaboración (DESC) reunión, SLAC

Marzo 8-10, 2016

Segundo anual US-Chile Education Summit, Chile

Abril 11-13, 2016

Reunión de la Junta LSSTC* en Washington, D.C.

Abril o Mayo, 2016

Taller Universidad de Pittsburgh: Photometics Redshifts in LSST

Mayo 24-26, 2016

XLDB 2016 Conferencia y Taller, SLAC

Junio, 2016

Reunion de Trabajo Stars, Milky Way and Local Volume Science Collaboration en AAS 228 San Diego, CA

Junio 6-10, 2016

Statistical Challenges in Modern Astronomy VI*, de la Carnegie Mellon University

Junio 20-24, 2016

LSST@Europe2*, Belgrado, Serbia

Junio 28-Julio 1 2016

SPIE Astronomical Telescopes & Instrumentation, Edimburgo, Escocia

Julio 18-22, 2016

DESC LSST reunión, en Oxford, Reino Unido

Agosto 15-19, 2016

LSST 2016 & Science Workshop, Tucson, AZ

 

Tuesday, January 12, 2016
Main Image Caption: 
Altitude of inspection drone = ~100 meters
Image Credit: 
LSST

A DJI Phantom 3 Pro Drone is being used on Cerro Pachón to monitor LSST construction progress from a birds-eye view. Multiple images will be used to generate a 3D model of the Summit Facility, suitable for inspection via virtual reality. In these initial images taken by Systems Engineer Jacques Sebag on January 8, 2016, preparation of the telescope pier is clearly visible.

From an altitude of 100 meters, infrastructure for the entire Summit Facility is clearly seen, including the construction of the second floor of the support building (on the right) where the telescope control room, computer room and offices will be located. From an altitude of 30 meters, closer to the actual height of the top of the dome, you can see the telescope pier emerging from the bedrock. The “hole in the donut” is the excavation for the pier foundation, and the recessed ring around it is the base for the foundation of the lower enclosure that will support the dome. The 16-meter diameter by 15-meter-high concrete pier will provide an extremely stiff base structure, to dampen vibration from rapid motion of the telescope in operation and resist damage when the earth moves rapidly in response to seismic events. The summit facility and dome are on schedule to be substantially completed in late 2017.

Altitude of inspection drone = ~30 meters

Altitude of inspection drone = ~30 meters

The height of the top of the dome above ground level is ~38 meters.

The height of the top of the dome above ground level is ~38 meters.

Detailed, cut-away view of the LSST Summit Facility shows how the pieces fit together.

Detailed, cut-away view of the LSST Summit Facility shows how the pieces fit together.

 

Monday, December 28, 2015

Holiday Greetings from LSST - On behalf of the Project Office, we wish you a joyous holiday season and Happy New Year! 

Saludos de fin de año del LSST - En nombre de la oficina del proyecto, les deseamos unas felices fiestas y un próspero año nuevo

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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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