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Introduction to the LIGO Caltech PDMWorks Vault and a summary of the drawing & data templates, macros, bill of materials and customized toolbox created for SolidWorks.
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Gather all necessary personal information and documents.
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Definition for the Tagalog word ligo: [noun] bath • taking a bath / shower.
The design and construction of LIGO was carried out by a team of scientists, engineers, and staff at the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT), and collaborators from over 80 scientific institutions around the world that are members of the LIGO Scientific
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool.
The International Thermonuclear Experimental Reactor (ITER) and the Large Hadron Collider (LHC), for example, cost over ten billion dollars each. LIGO only cost 1.2 billion dollars, spread over almost 30 years. So what do we get for those 1.2 billion dollars?
Located outside of Pisa, Italy, Virgo is a gravitational wave interferometer with arms 3km long (LIGO's are 4km long). Virgo is hosted by the European Gravitational Observatory (EGO), a collaboration of the Italian and French governments.
This animation illustrates how the twin observatories of LIGO work. One observatory is in Hanford, Washington, the other in Livingston, Louisiana. Each houses a large-scale interferometer, a device that uses the interference of two beams of laser light to make the most precise distance measurements in the world.
The acronym, LIGO, stands for "Laser Interferometer Gravitational-wave Observatory". Wholly supported by the U.S. National Science Foundation, LIGO is the world's largest gravitational wave observatory and a marvel of precision engineering.
Here again, two detectors are required for LIGO to operate as a single nation-wide observatory. Another important reason for placing the detectors so far apart is to aid in localizing the source of the GW on the sky.

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Advanced LIGO is a large-scale project designed to detect gravitational waves, which are ripples in spacetime caused by massive astronomical events, such as merging black holes or neutron stars. It enhances the sensitivity of the original LIGO detectors.
Researchers and scientists involved in gravitational wave detection experiments, as well as institutions conducting related studies, may be required to file reports and data associated with Advanced LIGO.
Filling out information related to Advanced LIGO typically involves providing specific data on gravitational wave events detected, methodologies used, and results obtained. Detailed guidelines are usually provided by the governing body overseeing research compliance.
The purpose of Advanced LIGO is to enhance the capabilities of gravitational wave astronomy, allowing scientists to observe and analyze cosmic phenomena, thereby advancing our understanding of the universe and fundamental physics.
Reporting on Advanced LIGO must include details about the detected gravitational wave events, the observational data collected, analysis methods, and findings. Compliance with scientific reporting standards is essential.
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