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advancedligo.mit.edu

Advanced LIGO

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. The Next Step in Gravitational Wave Astronomy. Read more . . . Read more . . . An Overview of the Upgrades. From the LIGO Scientific Collaboration, stimulated by the NSF's establishment of the LIGO Observatories, continue to migrate into the broader research and development community. Learn more by viewing LIGO's technology transfer case studies. Last modified Feb 13, 2015.

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Advanced LIGO | advancedligo.mit.edu Reviews
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Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. The Next Step in Gravitational Wave Astronomy. Read more . . . Read more . . . An Overview of the Upgrades. From the LIGO Scientific Collaboration, stimulated by the NSF's establishment of the LIGO Observatories, continue to migrate into the broader research and development community. Learn more by viewing LIGO's technology transfer case studies. Last modified Feb 13, 2015.
<META>
KEYWORDS
1 aligo summary
2 aligo news
3 ligo technology transfers
4 ligo lab
5 ligo hanford
6 ligo livingston
7 advanced ligo subsystems
8 auxiliary optics
9 core optics
10 data acquisition
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aligo summary,aligo news,ligo technology transfers,ligo lab,ligo hanford,ligo livingston,advanced ligo subsystems,auxiliary optics,core optics,data acquisition,data and,computing,systems,facilities,modifications,input optics,interferometer,control,laser
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Advanced LIGO | advancedligo.mit.edu Reviews

https://advancedligo.mit.edu

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. The Next Step in Gravitational Wave Astronomy. Read more . . . Read more . . . An Overview of the Upgrades. From the LIGO Scientific Collaboration, stimulated by the NSF's establishment of the LIGO Observatories, continue to migrate into the broader research and development community. Learn more by viewing LIGO's technology transfer case studies. Last modified Feb 13, 2015.

INTERNAL PAGES

advancedligo.mit.edu advancedligo.mit.edu
1

aLIGO Controls

https://www.advancedligo.mit.edu/isc.html

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. Subsystem: Interferometer Sensing and Controls. Mode cleaner control screen. Small ALS beam on laser table. Tip-tilt assembly and testing. LLO DRMI 30-second lock. Reflection and transmission from output mode cleaner. Locking the output mode cleaner. HAM 1 controls breadboard. Wavefront sensor quadrant photodiodes. First Michelson lock at LLO. Output mode cleaner test bench.

2

aLIGO PSL

https://www.advancedligo.mit.edu/psl.html

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. The pre-stabilized laser (PSL) provides frequency and intensity stabilized light for the Advanced LIGO interferometers at the specifications required for entrance to the Input Optics (IO) chain. The heart of the PSL is a three-stage laser system. The second stage delivers an output power of 35 W. Here the NPRO beam passes through four Nd:YVO4 crystals, also pumped at 808 nm.

3

Outreach

https://www.advancedligo.mit.edu/outreach.html

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. For LIGO news, summaries of recent technical papers and links to LSC Facebook and Twitter sites. LIGO Hanford Observatory (WA). LIGO Livingston Observatory (LA). An Overview of the Upgrades. Last modified Aug 5, 2016. For information about LIGO, contact info(at)ligo.caltech.edu.

4

aLIGO News

https://www.advancedligo.mit.edu/adligo_news.html

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. O1 Results Highlight the Capabilities of Advanced LIGO. LIGO has completed its analysis of the O1 data set for gravitational wave signals from binary black hole mergers,. Announced in February 2016, and the "Boxing Day" signal, GW151226. What are the features of the Advanced LIGO interferometers that facilitated these detections? Shot noise gains will continue to accrue as futur...

5

aLIGO Seismic

https://www.advancedligo.mit.edu/sei.html

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. The root mean square (RMS) differential motion of the test masses while the interferometer is locked must be held to a small value (less than 10. M per rt Hz, and a reduction in the microseism band to several tenths of a micron per rt hertz. HAM ISI riser installation. Livingston BSC 1 ISI under wraps. ISI test, high and low gain. Livingston BSC 3 cartridge in the air. LIGO is s...

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Northwestern University Center for Interdisciplinary Exploration and Research in Astrophysics - Education

http://ciera.northwestern.edu/Education.php

Join Our E-Mail List. IDEAS (Integrated Data Driven Discovery in Earth and Astrophysical Sciences) is a multi-faceted program designed for masters and PhD graduate students. All participants in the program have as a focus of their research one of three major research projects: Earthscope. IDEAS is funded by an NSF. Research Traineeship Grant (1450006), awarded to CIERA, with PI Vicky Kalogera. For more information, contact program director Michelle Paulsen. GK-12 "Reach for the Stars". Funded by the NSF.

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Research Projects |

http://www.ideas.ciera.northwestern.edu/projects

Management for Scientists and Engineers. Information for IDEAS Students. Information for Future Partners. All graduate Fellows in the program will be involved with one of three major NSF projects; each of these projects are at the forefront of scientific promise as well as technical challenge for data analytics: the Large Synoptic Survey Telescope ( LSST. The Advanced Laser Interferometer Gravitational-wave Observatory ( aLIGO. Winter Quarter Machine Learning Meet-Up. Feb 21, 2017. Nov 11, 2016.

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News from the Frontiers of Cosmology: A companion to the book The Edge of Physics — The Edge of Physics Blog

http://edgeofphysics.com/blog

The Edge of Physics Blog. News from the Frontiers of Cosmology: A companion to the book The Edge of Physics. Want to go underground to build a sensitive observatory capable of detecting gravitational waves that are thought be generated when black holes merge. The “Einstein Observatory” will 100 times more sensitive than existing detectors, and will likely be able to detect gravitational waves generated just after the Big Bang. Already, the next generation of detectors, such as Advanced LIGO. If such an i...

scienceblog.dk scienceblog.dk

Forskning | ScienceBlog

http://www.scienceblog.dk/kategori/forskning

Indlæg om naturvidenskabelig forskning. Åh, der er ikke noget så godt som en god Lomborg artikel. At starte dagen på, her ovenpå ferien. Det er godt at få gang i blodomløbet, og få grinet lidt over at denne mand stadig har taletid i den danske presse, og stadig kan få hvad jeg regner som nogenlunde intelligente mennesker til at hoppe med på den. Det kan i hvert fald få mig til at slukke for fjæsbogen i et par timer, hvilket jo nok er meget godt for min produktivitet. Jeg har før skrevet indlæg. Det er ri...

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Chapter 6 | SixDay Science

https://sixdayscience.com/curriculum/textbooks/chapter-6

Faith in Science Science in Faith. This chapter was copied with permission from Nick Strobel’s. Go to his site at www.astronomynotes.com. For the updated and corrected version. I discuss Einstein’s Special Relativity and General Relativity theories. The concepts of spacetime and gravity as a warping of spacetime are introduced along with observational proofs of his theories. This revolutionary leap in our understanding of gravity and the nature of space and time was made by. By any two observers regardle...

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vallis.org::blog

http://www.vallis.org/posts/20141017.html

Fly, little data, and be free! LIGO observatory near Hanford, WA. In August 2014 the gravitational-wave community celebrated an important milestone when the LIGO Open Science Center. LOSC), which I've been privileged to help build, released two years of LIGO data. As stated eloquently in the Panton principles. Nevertheless, the data from LIGO. Arguably one of the most high-profile endeavors. An experiment, rather than an observatory. Operating LIGO as an observatory. That serves data to an external commu...

stuver.blogspot.com stuver.blogspot.com

Living LIGO: First Software Engineering Run for Advanced LIGO

http://stuver.blogspot.com/2012/01/first-software-engineering-run-for.html

Thursday, January 19, 2012. First Software Engineering Run for Advanced LIGO. Most of the visible work on Advanced LIGO. Has been revolving around the installation of new instruments that are needed to increase the sensitivity of LIGO about 10 fold. While this is exciting, it can feel a little like being on the outside looking in for data analysts like myself. But there is still much to prepare for! But what is a channel? This is a close look at the computers in the racks (as we call the large rectangula...

gravityswings.wordpress.com gravityswings.wordpress.com

Avery | Gravity's Wings

https://gravityswings.wordpress.com/author/gravityswings

Shouting into the void since 2012. On persevering in the face of failure. Asymp; 3 Comments. This is kinda a big deal, everyone. I got paid to write at From Quarks to Quasars, a popular science news site. My first post went up yesterday. Scientists at Rothamstead Research, an agricultural research group in the UK, have published the results of their years-long study on genetic modification of wheat plants, despite setbacks from anti-GMO protesters. To those naysayers who want us to quit now, you don&#821...

ligo.org ligo.org

LIGO Scientific Collaboration - The science of LSC research

http://www.ligo.org/science/Publication-S6ligoDetchar/index.php

Cleaning Up LIGO Data. Nearly a century ago, Einstein predicted gravitational waves. Ripples in space and time that travel at the speed of light, as part of his general theory of relativity. The energy carried by these waves was shown by Hulse and Taylor to be responsible for the inspiral of binary neutron stars, such as PSR B1913 16. Gravitational waves from violent astrophysical systems, such as colliding black holes. The Laser Interferometer Gravitational Wave Observatory ( LIGO. Such as supernovae re...

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Advanced LIGO

Are the organizational units of the overall project. Follow the links below to view the mission and progress of each subsystem. The Next Step in Gravitational Wave Astronomy. Read more . . . Read more . . . An Overview of the Upgrades. From the LIGO Scientific Collaboration, stimulated by the NSF's establishment of the LIGO Observatories, continue to migrate into the broader research and development community. Learn more by viewing LIGO's technology transfer case studies. Last modified Feb 13, 2015.

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