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LIGO Lab | Caltech | MIT

The Laser Interferometer Gravitational-Wave Observatory (LIGO) consists of two widely separated installations within the United States — one in Hanford Washington and the other in Livingston, Louisiana — operated in unison as a single observatory. LIGO is operated by the LIGO Laboratory, a consortium of the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT). Funded by the National Science Foundation, LIGO is an international resource for both physics and astroph

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LIGO Lab | Caltech | MIT | ligo.caltech.edu Reviews
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The Laser Interferometer Gravitational-Wave Observatory (LIGO) consists of two widely separated installations within the United States — one in Hanford Washington and the other in Livingston, Louisiana — operated in unison as a single observatory. LIGO is operated by the LIGO Laboratory, a consortium of the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT). Funded by the National Science Foundation, LIGO is an international resource for both physics and astroph
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LIGO Lab | Caltech | MIT | ligo.caltech.edu Reviews

https://ligo.caltech.edu

The Laser Interferometer Gravitational-Wave Observatory (LIGO) consists of two widely separated installations within the United States — one in Hanford Washington and the other in Livingston, Louisiana — operated in unison as a single observatory. LIGO is operated by the LIGO Laboratory, a consortium of the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT). Funded by the National Science Foundation, LIGO is an international resource for both physics and astroph

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mm.ligo.caltech.edu mm.ligo.caltech.edu

LSCCompComm list archive -- Mail Index, by date

Last updated: 09 Sep 2006. Advanced LIGO Suspensions Group. TAMA-LIGO Small Working Group.

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LIGO - Laser Interferometer Gravitational Wave Observatory

Supported by the National Science Foundation. 183; for scientists. 183; for all. Dedication of Advanced LIGO. Public Release of LIGO S5 Data. Latest BICEP2/Keck Array/Planck Results on Primordial Gravitational Waves. LIGO Data Management Plan. Simulating eXtreme Spacetimes: A Caltech-Cornell Project's simulation of black holes and other extreme spacetimes. Advanced LIGO Project Funded by National Science Foundation. LIGO Celebrates Successful S5 Run . LIGO Sheds Light on Cosmic Event . Past news articles .

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LIGO IDP Selector

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LIGO Data Analysis System at www.ldas-cit.ligo.caltech.edu

Wwwldas-cit.ligo.caltech.edu. Welcome to the LDAS CIT Web Site. LDAS Problem Reporting System. The LDCG Tool Suite. LDAS System (Block Diagram). How to Build LDAS. How to Configure LDAS. How to Test LDAS. How to Install on a Single Host. LDAS Account Application Request. LDAS API Run Status. Summary of Running Jobs. API Status History Summary. LSC VO Account Request Form. LDAS CIT Log Files. LDAS (Solaris 10; sparc). Mar 23 06:05:41 PDT 2010. LDAS (CentOS 5; 32bit). Mar 23 05:48:21 PDT 2010.

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LIGO Data Analysis System at www.ldas-sw.ligo.caltech.edu

Wwwldas-sw.ligo.caltech.edu. Welcome to the LDAS Software Web Site. LDAS Problem Reporting System. The LDCG Tool Suite. How to Build LDAS. How to Configure LDAS. How to Test LDAS. How to Install on a Single Host. LDAS Account Application Request. LSC VO Account Request Form. LDAS (Solaris 10; sparc). Mar 23 06:05:41 PDT 2010. LDAS (CentOS 5; 32bit). Mar 23 05:48:21 PDT 2010. LDAS (Solaris 10; i86pc). Mar 23 05:49:37 PDT 2010. Shaded relief map courtesy Johns Hopkins University Applied Physics Laboratory.

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INTERNAL PAGES

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About | LIGO Lab | Caltech

https://www.ligo.caltech.edu/page/about

Supported by the National Science Foundation. Operated by Caltech and MIT. The design and construction of LIGO was carried out by LIGO Laboratory’s team of scientists, engineers, and staff at the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT), and collaborators from the over 80 scientific institutions world-wide that are members of the LIGO Scientific Collaboration. And the Massachusetts Institute of Technology ( MIT. What is LIGOs scientific mission?

2

What are Gravitational Waves? | LIGO Lab | Caltech

https://www.ligo.caltech.edu/page/what-are-gw

Supported by the National Science Foundation. Operated by Caltech and MIT. What are Gravitational Waves? Sources and Types of Gravitational Waves. LIGO - A Gravitational-Wave Interferometer. Illustration of gravitational waves produced by two orbiting black holes. (Image: Henze/NASA). What are Gravitational Waves? Two-dimensional illustration of how mass in the Universe distorts space-time (Credit: NASA). Your browser does not support this video tag. Artists impression of a binary pulsar. (Michael Kr...

3

Educational Resources | LIGO Lab | Caltech

https://www.ligo.caltech.edu/page/educational-resources

Supported by the National Science Foundation. Operated by Caltech and MIT. Try This at Home. Bring LIGO To Your Classroom. Recommended Reading, Video. Whether youre a K-12 educator, a parent, or an interested student, you should browse our education web pages. Theres something fun and educational here for everyone. All sorts of activities you can bring to your classroom that concentrate on LIGO, or concepts related to LIGO (such as, waves). Want to take a school field trip to LIGO? Try This at Home.

4

LIGO Lab | Caltech

https://www.ligo.caltech.edu/gallery

Supported by the National Science Foundation. Operated by Caltech and MIT. Spiral Dance of Black Holes. June 15, 2016. An illustration showing the merger of two black holes and the gravitational waves that ripple outward as the black holes spiral toward each ot. Black Holes with Known Masses. June 15, 2016. An image showing black holes with known masses. LIGO's First Observing Run. June 15, 2016. Mapping LIGO’s New Detection on the. June 15, 2016. Mapping LIGO’s Detections During Fi. June 15, 2016. Febru...

5

Learn More | LIGO Lab | Caltech

https://www.ligo.caltech.edu/page/learn-more

Supported by the National Science Foundation. Operated by Caltech and MIT. LIGO - A Gravitational-Wave Interferometer. Merging neutron stars. (Image: Price and Rosswog). LIGO is a research facility designed to listen for gravitational waves from the depths of space with the aid of a laser interferometer. Visit the links below to learn more about gravitational waves and LIGO’s remarkable engineering, which makes the search for gravitational waves possible. Learn more about what were looking for.

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SUPA TEOPS Activities

http://teops.lowtemp.org/activities.html

Various activities are currently taking place and have now been completed across TEOPS, generally involving links with external bodies both within academia and with industry. This work involves research towards improved structures for the SLHC Silicon tracker, based on studying different support materials (carbon fibre, SiC, CSiC and ceramics). Thermal studies will examine the heat flow from the modules to the cooling fluid with the aim of optimizing the sensor temperature. The work involves:. Operation ...

lsc-group.phys.uwm.edu lsc-group.phys.uwm.edu

UWM LSC: Members

http://www.lsc-group.phys.uwm.edu/people

UWM LIGO Scientific Collaboration Research Group. June 15, 2016. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence. February 18, 2016. The Right Place At The Right Spacetime. February 11, 2016. Observation of Gravitational Waves from a Binary Black Hole Merger. LIGO Lab Weekly Report. Grid, Cloud Techs. IdM and CMP Architect and Programmer. Center for Gravitation and Cosmology.

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UWM LSC: Outreach

http://www.lsc-group.phys.uwm.edu/outreach

UWM LIGO Scientific Collaboration Research Group. June 15, 2016. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence. February 18, 2016. The Right Place At The Right Spacetime. February 11, 2016. Observation of Gravitational Waves from a Binary Black Hole Merger. LIGO Lab Weekly Report. Sounding Out the Big Bang. Gravitational Waves: New Observatories for New Astronomy. LIGO and the Detection of Gravitational Waves. Physics Today; October, 1999). Virtual labora...

lsc-group.phys.uwm.edu lsc-group.phys.uwm.edu

UWM LSC: Recent Articles

http://www.lsc-group.phys.uwm.edu/publications

UWM LIGO Scientific Collaboration Research Group. June 15, 2016. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence. February 18, 2016. The Right Place At The Right Spacetime. February 11, 2016. Observation of Gravitational Waves from a Binary Black Hole Merger. LIGO Lab Weekly Report. 1 Aasi, J., Abadie, J., Abbott, B.P., Abbott, R., Abbott, T.D., Abernathy, M., Accadia, T., Acernese, F. and others. PhysRev.D 88 (2013) 062001. PhysRev.D 87 (2013) 042001.

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LIGO Data Grid: LIGO Data Grid

https://www.lsc-group.phys.uwm.edu/lscdatagrid

LSC LIGO Scientific Collaboration. What is LSC DataGrid? LDG Clusters Usage [Ganglia]. Available Data per site. Grid Service Details [Monitoring]. How to get started. Install Data Grid Client. Request Software changes to SCCB. Admin Manual [(*) = optional]. Include site into Grid Monitoring. LAMS / VOMS Admin [LSC internal]. Syracuse X4500 wiki [passwd required]. Edit these web pages. Request Tracking System [RT]. LDG trouble ticket system. LIGO VO in Open Science Grid [OSG]. Welcome to the LSC DataGrid.

lsc-group.phys.uwm.edu lsc-group.phys.uwm.edu

UWM LSC: Visitors

http://www.lsc-group.phys.uwm.edu/visitors.html

UWM LIGO Scientific Collaboration Research Group. June 15, 2016. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence. February 18, 2016. The Right Place At The Right Spacetime. February 11, 2016. Observation of Gravitational Waves from a Binary Black Hole Merger. LIGO Lab Weekly Report. Scenic Lake Route From All Directions:. Is often scarce when classes are in session. Some curb parking in the neighborhood surrounding UWM is available, with restrictions. UWM u...

lsc-group.phys.uwm.edu lsc-group.phys.uwm.edu

Nemo: Index

http://www.lsc-group.phys.uwm.edu/beowulf/nemo/index.html

Nemo: The 780 Node (1560 CPU core) Beowulf cluster. Search the Nemo Web Pages. UWM LSC Group Computing Wiki. Becoming a LSC DataGrid User. Running Codes With Condor. NFS Data Node Recovery. Bid Q And A. Cluster Room Noise New. Welcome to the Nemo cluster at UWM! Nemo is a large beowulf-class. Parallel computer, built and operated by the LSC group at the University of Wisconsin - Milwaukee (UWM). Nemo is used by members of the LIGO Scientific Collaboration (LSC). A few facts about Nemo. The total cost is ...

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Portugal@Home - Einstein@Home

http://www.portugalathome.org/einstein.php

URL do Projecto: http:/ einstein.phys.uwm.edu. Aderir à Portugal@Home - Einstein@Home. Há algum tempo atrás, Albert Einstein. Sugeriu que nos encontramos à deriva num universo cheio de ondas. Buracos negros em colisão, estrelas em colapso e objectos celestiais compactos giratórios como pulsares criam ondulações no tecido espaço e tempo que distorcem o mundo à nossa volta. O que é o Einstein@Home? O que são o GEO 600 e o LIGO? O que é uma onda gravitacional? O que mostra a parte gráfica? Os cientistas acr...

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Einstein's Messengers

http://einsteinsmessengers.org/resources.htm

Connections to Science Standards. Student Study Guide and Teachers' Guide. Resources and Contacts for Teachers. Teachers, students and the public can help LIGO search for gravitational waves! Download the Einstein@Home screen saver; when the screen saver runs, your computer will be analyzing data from a gravitational wave interferometer. http:/ einstein.phys.uwm.edu. Check the LIGO Lab main page for links to recent LIGO news plus LIGO Caltech and LIGO MIT links. Http:/ www.ligo.org/. Operate a virtual LI...

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LIGO Hanford Observatory

Up and Coming at LIGO Hanford . . . Teacher workshops at LIGO during the week. Teachers between grades K and 8 are invited to attend one or more of LIGO's August workshops: Astronomy Basics. Wave Behavior in the NextGen (WA) Standards. Send an email to outreach@ligo-wa.caltech.edu to register! LIGO Hanford presents a series of special events to celebrate light. July 31, 2015 10:30 AM - 4:30 PM. A meeting for university undergraduates. August 14, 2015 8:00 PM - 1:00 AM. Night Sky at LIGO. 149; For problem...

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LIGO Lab | Caltech | MIT

Supported by the National Science Foundation. Operated by Caltech and MIT. LIGO and Virgo make first detection of gravitational waves produced by colliding neutron stars. Press release • October 16, 2017. For the first time, scientists have directly detected gravitational waves — ripples in space and time — in addition to light from the spectacular collision of two neutron stars. This marks the first time that a cosmic event has been viewed in both gravitational waves and light. How does it affect us?

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