A “bang” in LIGO and Virgo detectors signals most massive gravitational-wave source yet
2 Sep 2020 -- On May 21, 2019, LIGO/Virgo researchers detected a signal from the most massive black hole merger yet observed in gravitational waves. The product of the merger is the first clear detection of an “intermediate-mass” black hole, with a mass between 100 and 1,000 times that of the sun.
The detected signal, labeled GW190521, was generated by a source that is roughly 5 gigaparsecs away, making it one of the most distant gravitational-wave sources detected so far. This newest merger appears to be the most massive yet, involving two inspiraling black holes with masses about 85 and 66 times the mass of the sun. The merger created an even more massive black hole, of about 142 solar masses, and released an enormous amount of energy, equivalent to around 8 solar masses.
Still image from a numerical relativity visualization consistent with GW190521.
[Image credit: LIGO/Virgo/D. Ferguson, K. Jani, D. Shoemaker, P. Laguna.]
Webinar on latest results from the LIGO-Virgo-Kagra Collaboration
1 Sep 2020 [updated 3 Sep 2020] -- On Thursday September 3rd the LIGO-Virgo-Kagra Collaboration will hold a one-hour live-streamed Zoom webinar, discussing the latest discovery from the third observing period (O3): GW190521. The webinar is now scheduled for 1500 CEST (0900 EDT, 0600 PDT, 220 JST). (This is one hour earlier than previously advertised.)
A recording of the webinar can be found below.
LVK GW190521 Webinar. This 1hr 10 min webinar held on 3 September 2020 discusses the detection of GW190521 and associated scientific results.
LIGO detectors receive a glowing end-of-run review
12 Aug 2020 -- On April 1st 2019 the LIGO Virgo interferometer network began their third Observing Run, O3: a year-long dedicated search for gravitational waves which yielded an impressive haul of 56 candidate events. Now LIGO scientists have published a paper describing the improvements made to the Advanced LIGO detectors for O3 and reviewing the performance of the detectors throughout the Observing Run – during which the instruments were more stable and more sensitive than ever before. Read the full paper at https://arxiv.org/abs/2008.01301.
Simplified optical layout of the Advanced LIGO detectors for O3.
[Credit: LIGO Lab/Caltech/MIT]
Best constraints yet on the size of "mountains" on millisecond pulsars
29 Jul 2020 -- The LIGO and Virgo collaborations report the most stringent constraints yet on the size of deformations on millisecond pulsars in a new paper submitted to the ArXiv. Based on our analysis, the strong gravity of these rapidly spinning neutron stars constrains such deformations to be no bigger than the width of a human hair. While we have not detected gravitational-waves from millisecond pulsars, we have for the first time probed possible gravitational-wave emission mechanisms for these stars, and shown that only very small deformations would be necessary to produce observable gravitational waves.
For more details, read the full summary of our paper.
This is an artist's impression of millisecond pulsar PSR J1023+0038 (white object on the right with magnetic field lines).
It extracts matter from its companion star (red object on the left) via an accretion disk (also shown in red).
[Credit: European Space Agency (ESA).]
LIGO-Virgo finds mystery object in the 'mass gap'
23 Jun 2020 -- When the most massive stars die, they collapse under their own gravity and leave behind black holes; when stars that are a bit less massive die, they explode in supernovas and leave behind dense, dead remnants of stars called neutron stars. For decades, astronomers have been puzzled by a gap that lies between neutron stars and black holes: the heaviest known neutron star is no more than 2.5 times the mass of our sun, or 2.5 solar masses, and the lightest known black hole is about 5 solar masses. Now, scientists from LIGO and Virgo have announced the discovery of an object of 2.6 solar masses, placing it firmly in the mass gap. The object was found on August 14, 2019, as it merged with a black hole of 23 solar masses, generating gravitational waves that were detected by the LIGO and Virgo detectors.
GW190814: heaviest neutron star or lightest black hole? In August 2019, the LIGO-Virgo gravitational-wave network witnessed the merger of a black hole with 23 times the mass of our sun and a binary companion 2.6 times the mass of the sun. Scientists do not know if the companion was a neutron star or a black hole, but either way it set a record as being either the heaviest known neutron star or the lightest known black hole.
[Image credit: LIGO/Caltech/MIT/R. Hurt (IPAC).]
Webinar on latest results from the LIGO-Virgo-Kagra Collaboration
21 Jun 2020 -- On June 25th the LIGO-Virgo-Kagra Collaboration held a one-hour live-streamed Zoom webinar, discussing discoveries from the third observing period (O3). The webinar took place at 14:00 UTC (07:00 PDT, 09:00 CDT, 16:00 CEST, 23:00 JST).
A recording of the webinar can be found below.
LVK GW190814 Webinar. This 1hr 12 min webinar held on 25 June 2020 discusses the detection of GW190814 and associated scientific results.
LIGO-Virgo Detect the Merger of Two Black Holes with Unequal Masses
20 Apr 2020 -- On April 12, 2019, the twin LIGO detectors and the Virgo detector observed gravitational-waves from the merger of two black holes. While nearly all previous detections originated from binary black holes with almost equal masses, this event (labeled GW190412) displayed clear signatures of an unequal mass binary. A detailed analysis of the gravitational-wave signal indicates that the two black holes had masses of about 30 and 8 times the mass of the sun. General relativity predicts that binary systems with such mass differences will introduce higher "harmonics" into the waveform, and these were in-fact observed for the first time in this event.
For more details, see the GW190412 detection page.
Still image from a numerical simulation of an unequal mass binary black hole merger, with parameters consistent with GW190412. [Image credit: N. Fischer, H. Pfeiffer, A. Buonanno (Max Planck Institute for Gravitational Physics), Simulating eXtreme Spacetimes project]
LIGO's Third Observing Run Suspended Early Due to COVID-19 Pandemic
26 Mar 2020 -- Due to the COVID-19 pandemic, LIGO observing mode operations will end on March 27, 2020. The decision to halt O3 was not an easy one, however the current worldwide COVID-19 pandemic demands that we make public health and safety our top priority. It is unknown at this time when observing mode operations may resume. In spite of the early suspension, the O3 run has been a tremendous success and we look forward to the science to come from the O3 events and future observing runs with the gravitational-wave detector network.For more additional details, see
- LIGO Laboratory news release on O3 suspension
- LIGO Laboratory's Response to COVID-19
- News updates on the Virgo homepage
- Updates on the LSC Observing Plans and Public Alerts webpage
LIGO-Virgo Network Catches Another Neutron Star Collision
6 Jan 2020 -- On April 25, 2019, the LIGO Livingston Observatory picked up what appeared to be gravitational ripples from a collision of two neutron stars. Now, a new study confirms that this event (GW190425) was indeed likely the result of a merger of two neutron stars. This would be only the second time this type of event has ever been observed in gravitational waves. GW190425 is the first gravitational-wave event discovered with data from a single observatory. While no electromagnetic counterpart was found, this system is notable for having a total mass that exceeds that of known galactic neutron star binaries.
For more details, see the full press release and other information at the GW190425 detection page.
Artist's rendition of a neutron star merger. [Image credit: National Science Foundation/LIGO/Sonoma State University/A. Simonnet.]
LIGO's Third Observing Run Resumes
5 Nov 2019 -- On November 1st at 15:00 UTC, the LIGO and Virgo gravitational wave detectors resumed their search for gravitational waves after taking a planned month-long break to perform maintenance and upgrades. All three sites halted operations for the entire month of October. Virtually all of the work planned for LIGO's two detectors was completed by October 31st. This included inspecting and cleaning of test masses, installation of additional baffles to reduce light scattering, replacing a turbomolecular vacuum pump, and removing an unused portion of the "H2" vacuum system. Virgo engineers focused on increasing the laser input power from 19 W to 26 W. The extent to which this work has improved the instruments’ sensitivities will be known in the weeks to come. The second half of LIGO's third observing run will conclude on April 30th, 2020.
For more details, read the full news release at the LIGO Lab webpage.
Livingston engineer, Danny Sellers, paints the mirror with a substance called "first contact". This is used to help clean the mirror, which hangs at the bottom of a quadruple pendulum suspension system to isolate it from terrestrial vibrations. [Caltech/MIT/LIGO Lab]
KAGRA to Join LIGO and Virgo in Hunt for Gravitational Waves
4 Oct 2019 -- Japan's Kamioka Gravitational-Wave Detector (KAGRA) will soon team up with the National Science Foundation's Laser Interferometer Gravitational-Wave Observatory (LIGO) and Europe's Virgo in the search for subtle shakings of space and time known as gravitational waves. Representatives for the three observatories signed a memorandum of agreement (MOA) about their collaborative efforts today, October 4. The agreement includes plans for joint observations and data sharing.
"This is a great example of international scientific cooperation," says Caltech's David Reitze, executive director of the LIGO Laboratory. "Having KAGRA join our network of gravitational-wave observatories will significantly enhance the science in the coming decade."
"At present, KAGRA is in the commissioning phase, after the completion of its detector construction this spring. We are looking forward to joining the network of gravitational-wave observations later this year," says Takaaki Kajita, principal investigator of the KAGRA project and co-winner of the 2015 Nobel Prize in Physics.
For more details, read the full news release at the LIGO Lab webpage.
An illustration of the underground KAGRA gravitational-wave detector in Japan. [Image credit: ICRR, Univ. of Tokyo.]
LIGO's Commissioning Break Commences
3 Oct 2019 -- On October 1st, LIGO’s Hanford (LHO) and Livingston (LLO) detectors will temporarily halt observations to undergo a series of instrument upgrades and fixes. This kind of “commissioning break” sometimes occurs during LIGO’s long observing runs. The current run, O3, began on April 1 2019, when Virgo, the European-based gravitational-wave detector, located at the European Gravitational Observatory (EGO) in Italy, also started observing. Virgo is also pausing this month to perform upgrades that will improve their sensitivity and their uptime. All three detectors will resume operations on November 1st.
Commissioning breaks are typically month-long breaks during observing runs (as opposed to year-or-more long breaks between observing runs) when staff can make upgrades or repairs that would take more time than is available during weekly maintenance windows. The longer break gives the observatory sites an opportunity to make sure they are working optimally for the duration of the observing run, which in this case is scheduled to end on April 30, 2020.
For more details, read the full story at the LIGO Lab webpage.
Inside a HAM chamber as Advanced LIGO was being assembled prior to its first observing run in 2015. [Credit: Caltech/MIT/LIGO Lab/Greg Grabeel]
LIGO's Third Observing Run Started with a Bang!
12 Aug 2019 -- LIGO is just four months into its third observing run (O3) and there’s already a lot to be excited about. O3 began on April 1st, 2019 with high expectations for detections thanks to a series of upgrades that were made to both instruments after LIGO’s second observing run ended on August 25th, 2017. Also joining O3 on April 1st was Virgo, the European-based gravitational-wave detector in Italy, which almost doubled its sensitivity since its last run.
By July 31st, 2019, LIGO had sent out 25 alerts regarding possible detections; three have since been retracted, leaving 22 ‘candidate’ gravitational wave events. You can learn more about each of these (and subsequent candidates) by visiting the LIGO/Virgo detection alert page GraceDB or the UK-based GW Public Alerts page.
So far, no electromagnetic counterparts related to our public alerts have been observed, but all candidates are being actively analyzed by LSC/Virgo science teams. A sensitivity improvement will be implemented in an upcoming commissioning break when LIGO will temporarily halt the observing run (from October 1 to 3, with the run resuming on November 1).
For more details, read the full story at the LIGO Lab webpage.
Selected skymap images showing the likely position of candidate gravitational wave sources. The orange blobs show the 90% probability regions for the source location. [Credit: LIGO-Virgo/Cardiff Uni./C. North]
LIGO and Virgo Detect Neutron Star Smash-Ups
2 May 2019 -- On April 25, 2019, the National Science Foundation's Laser Interferometer Gravitational-Wave Observatory (LIGO) and the European-based Virgo detector registered gravitational waves from what appears likely to be a crash between two neutron stars—the dense remnants of massive stars that previously exploded. One day later, on April 26, the LIGO-Virgo network spotted another candidate source with a potentially interesting twist: it may in fact have resulted from the collision of a neutron star and black hole, an event never before witnessed. In addition to the two new candidates involving neutron stars, the LIGO-Virgo network has, during the first month of the third observing run (O3), spotted three likely black hole mergers.
"The universe is keeping us on our toes," says Patrick Brady, spokesperson for the LIGO Scientific Collaboration and a professor of physics at the University of Wisconsin-Milwaukee. "We're especially curious about the April 26 candidate. Unfortunately, the signal is rather weak. It's like listening to somebody whisper a word in a busy café; it can be difficult to make out the word or even to be sure that the person whispered at all. It will take some time to reach a conclusion about this candidate."
More information is contained in the the full press release.
LSC Elects Patrick Brady as New Spokesperson
31 Mar 2019 -- Patrick Brady, Professor of Physics and current Director of the Leonard E Parker Center for Gravitation, Cosmology and Astrophysics at the University of Wisconsin Milwaukee, has been elected spokesperson of the LIGO Scientific Collaboration. He succeeds outgoing spokesperson David Shoemaker. More information about Patrick can be found here.
Patrick Brady [Image credit: UWM]
LIGO and Virgo Resume Search for Ripples in Space and Time
26 Mar 2019 -- LIGO is set to resume its hunt for gravitational waves—ripples in space and time—on April 1, after receiving a series of upgrades to its lasers, mirrors, and other components. LIGO now has a combined increase in sensitivity of about 40 percent over its last run, which means that it can survey an even larger volume of space for gravitational-wave events like black hole collisions.
Joining the search will be Virgo, the European-based gravitational-wave detector, located at the European Gravitational Observatory (EGO) in Italy, which has almost doubled its sensitivity since its last run and is also starting up April 1.
For more information, read the full press release.
(Left Image): Detector engineers Hugh Radkins (foreground) and Betsy Weaver (background) are pictured here inside the vacuum system of the detector at LIGO Hanford Observatory, beginning the hardware upgrades necessary for Advanced LIGO's third observing run. [Image credit: LIGO/Caltech/MIT/Jeff Kissel].
(Right Image): LIGO team members install in-vacuum equipment that is part of the squeezed-light upgrade. [Image credit: LIGO/Caltech/MIT/Matt Heintze]
O2 Data Set Now Available
27 Feb 2019 -- LIGO and Virgo are pleased to announce that the strain data from the O2 observing run have been released. These data are now available through the Gravitational Wave Open Science Center (gw-openscience.org).
The O2 observing run began on November 30, 2016 and ended on August 25, 2017. The release includes over 150 days of data from each of the two LIGO observatories, as well as 20 days of data from Virgo, making this the largest data set of “advanced” gravitational wave detectors to date. Observations in O2 include seven binary black hole mergers, as well as the first binary neutron star merger observed in gravitational waves, all recently published with the GWTC-1 catalog. The LIGO Scientific Collaboration and Virgo Collaboration have published a number of papers based on these data; please see the LIGO Scientific Collaboration web pages for a list of these papers, and several more will be appearing soon. Along with the strain data, the release contains detailed documentation and links to open source software tools.
O2 is the second observing run of Advanced LIGO, and the first observing run of Advanced Virgo, which joined O2 on August 1st, 2017. Data from Advanced LIGO’s first observing run (O1) are already available online, and have been used in a number of scientific publications, text books, artistic projects, and classroom activities. As with previous data releases, the O2 data set should be useful for both scientific investigations and educational activities.
Image adopted from arXiv:1811.12907 by the LIGO Scientific Collaboration and the Virgo Collaboration.
LIGO Receives New Funding to Upgrade Detectors
15 Feb 2019 -- Research grants from the NSF, along with UK and Australian funding agencies, will fund a future upgrade to the twin LIGO detectors. The $35 million upgrade---called "Advanced LIGO Plus"---will use squeezed light and new mirror coating technologies to increase the sensitivity to gravitational-waves. Advanced LIGO Plus is expected to commence operations in 2024, increasing the volume of space the observatory can survey by as much as seven times. This will lead to a higher rate of detections, improvements to tests of general relativity, and a better understanding of neutron star physics. Funding for the upgrade includes $20.4 million from the NSF, $14.1 million from UK Research and Innovation, and additional funds from the Australian Research Council.
Image credit: Matt Heintze/Caltech/MIT/LIGO Lab
LIGO and Virgo release catalog of gravitational-wave events from first and second observing runs
3 Dec 2018 -- The LIGO Scientific Collaboration and the Virgo Collaboration have released the results of their search for stellar-mass coalescing compact binaries during the first and second observing runs using an advanced gravitational-wave detector network. This includes the confident detection of ten binary black hole mergers and one binary neutron star merger. Four of the ten black hole mergers are being reported for the first time and include the most distant and massive gravitational-wave source ever observed (GW170729).
Image credit: Teresita Ramirez / Geoffrey Lovelace / SXS Collaboration / LIGO-Virgo Collaboration
Winners of 2018 Excellence in Detector Characterization and Calibration Award Are Announced
21 Nov 2018 -- The LIGO Laboratory has announced the winners of the first Award for Excellence in Detector Characterization and Calibration: Derek Davis (Syracuse University) and T.J. Massinger (Caltech). The $1000 prize will be shared by Davis and Massinger; they are invited to present colloquia at one of the LIGO Lab sites and will be recognized at the March 2019 LIGO-Virgo Collaboration Meeting. Additional details on their award can be found on the LIGO Laboratory news website.
LIGO and Virgo Collaborations Working to Make Data and Analysis Techniques Available to All
1 Nov 2018 -- Claims in a paper by Creswell et al. of puzzling correlations in LIGO data have broadened interest in understanding the publicly available LIGO data around the times of the detected gravitational-wave events. The features presented in Creswell et al. arose from misunderstandings of public data products and the ways that the LIGO data need to be treated. The LIGO Scientific Collaboration and Virgo Collaboration (LVC) have full confidence in our published results. We are preparing a paper that will provide more details about LIGO detector noise properties and the data analysis techniques used by the LVC to detect gravitational-wave signals and infer their source properties. The entire gravitational-wave signal data stream from the first observing run is already publicly available at the Gravitational-Wave Open Science Center, along with additional information on analyzing LIGO data. This resource, along with presentations from a recent Open Data Workshop, will be of interest to all who wish to understand our results in more depth.
LIGO Scientists Awarded New Horizons in Physics Prize
18 Oct 2018 -- Three LSC scientists were awarded the 2019 New Horizons in Physics prize. Rana Adhikari (Caltech), Lisa Barsotti (MIT), and Matthew Evans (MIT) were recognized “for research on present and future ground-based detectors of gravitational waves.” The New Horizons prize is awarded by the Breakthrough Prize Foundation. The LSC congratulates their colleagues on this major recognition. For more information see the Breakthrough Prize press release and the LIGO Lab news item.
"Ripples of Gravity, Flashes of Light" One Year On
16 Oct 2018 -- Exactly one year ago the LIGO Scientific Collaboration and Virgo Collaboration announced the detection of the binary neutron star merger GW170817 - the first ever cosmic event viewed in both gravitational waves and light. This remarkable discovery was made by the LIGO and Virgo detectors on 17 August 2017, and the aftermath of the merger was subsequently observed by thousands of astronomers around the world – marking an exciting new dawn for “multi-messenger” astronomy.
You can re-live the excitement of our GW170817 press conference or read more about the binary merger on our GW170817 detection page. And our latest results on the physical properties of neutron stars, from our observations of GW170817, have just been published in Physical Review Letters.
Meanwhile, preparations continue for the start of LIGO’s Third Observing Run, planned for early in 2019, with the promise of many more gravitational wave detections to come. Read more about our exciting “O3” plans.
Image credit: NSF/LIGO/Sonoma State University/A. Simonnet
LSC Congratulates our IceCube colleagues on multi-messenger breakthrough
12 Jul 2018 -- The LIGO Scientific Collaboration (LSC) congratulates members of the IceCube Collaboration on discovering the first ever evidence that links high-energy cosmic neutrinos to the nuclei of active galaxies powered by supermassive black holes. This remarkable discovery, confirmed by electromagnetic telescopes around the world, illuminates a century-old puzzle about the origins of high-energy cosmic rays and marks a major breakthrough for the emerging new field of multi-messenger astrophysics.
The LSC looks forward to the global network of gravitational-wave detectors beginning their next observing run, and the exciting prospect of detecting electromagnetic radiation, gravitational waves, and neutrinos from the most powerful astrophysical events in the cosmos.
For additional information see the associated NSF press release.
Image credit: IceCube Collaboration
Update on the start of LIGO's 3rd observing run
24 Apr 2018 -- LIGO's second observing run (O2) ended on August 25, 2017, and preparations for the third observing run (O3) began shortly thereafter. The detector installation and commissioning program between O2 and O3 has generally been proceeding well at all the LIGO and Virgo detector sites. Along with this progress we have also incurred delays in the start of full interferometer commissioning. As as result, the start of O3 is currently projected to begin in early 2019. Updates will be provided once the installation phase is complete and the commissioning phase has begun. An update on the engineering run prior to O3 will be provided by late summer 2018.
LIGO and Virgo announce black hole merger detected in June 2017
15 Nov 2017 -- The LIGO and Virgo Collaborations detected another binary black hole merger on June 8, 2017. The gravitational waves were detected by the twin LIGO detectors. With components 12 and 7 solar masses, this is the lightest binary black hole merger observed so far.
LIGO and Virgo make first detection of gravitational waves produced by colliding neutron stars
16 Oct 2017 -- For the first time, scientists have directly detected gravitational waves — ripples in space-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. The discovery was made on August 17, 2017 using the U.S.-based Laser Interferometer Gravitational-Wave Observatory (LIGO); the Europe-based Virgo detector; and some 70 ground- and space- based observatories.
Image credit: Karan Jani/Georgia Tech
Media Release: Scientists to discuss new developments in gravitational-wave astronomy
11 Oct 2017 -- Scientists representing LIGO, Virgo, and some 70 observatories will reveal new details and discoveries made in the ongoing search for gravitational waves. This will take place on Monday, October 16th, at 10:00am EDT at the National Press Club in Washington, D.C. A live-stream of the press conference can be viewed at this link. An alternate link will also carry the live-stream, followed by a 30-minute YouTube question & answer session with gravitational-wave scientists.
For additional information see the full media advisory here [pdf].
The LSC congratulates Rainer Weiss, Barry Barish, and Kip Thorne on winning the 2017 Nobel Prize in Physics
3 Oct 2017 -- The LIGO Scientific Collaboration is absolutely delighted to congratulate Rainer Weiss, Barry Barish, and Kip Thorne on winning the 2017 Nobel Prize in Physics. Weiss and Thorne are two of the founders of the LIGO project. Barish was the Principal Investigator of LIGO from 1994 to 2005, during the period of its construction and initial operation.
Image credit: LIGO/Caltech/MIT
LIGO and Virgo make the first joint detection of merging black holes
27 Sep 2017 -- The Virgo Collaboration and the LIGO Scientific Collaboration have jointly observed the merger of two black holes. This is the fourth confirmed detection of a binary black hole merger, and the first detection made using a network of three interferometers.
The detected waves—observed on August 14th, 2017 at 10:30:43 UTC (6:30AM EDT) —were produced by a pair of black holes with 31 and 25 solar masses. They merged to produce a spinning black hole of 53 solar masses. Combining the signal from Virgo with the signal observed in the two LIGO observatories improved the sky localization of the source by over a factor of 10.
Image credit: LIGO/Virgo/Caltech/MIT/Leo Singer (Milky Way image: Axel Mellinger)
A very exciting LIGO-Virgo Observing run is drawing to a close August 25
25 August 2017 -- The Virgo and LIGO Scientific Collaborations have been observing since November 30, 2016 in the second Advanced Detector Observing Run ‘O2’ , searching for gravitational-wave signals, first with the two LIGO detectors, then with both LIGO and Virgo instruments operating together since August 1, 2017. Some promising gravitational-wave candidates have been identified in data from both LIGO and Virgo during our preliminary analysis, and we have shared what we currently know with astronomical observing partners. We are working hard to assure that the candidates are valid gravitational-wave events, and it will require time to establish the level of confidence needed to bring any results to the scientific community and the greater public. We will let you know as soon we have information ready to share.
Upgraded Virgo joins LIGO during the 2nd observing run (O2)
1 August 2017 -- On August 1, 2017 the Virgo detector began taking science-quality data in concert with LIGO. While LIGO and Virgo have operated together in the past, this marks the first time they are jointly taking data after significant upgrades to both detectors. This 2nd observing run (O2) began at the end of November 2016 and will continue until August 25, 2017.
Virgo, located near Pisa, Italy, began taking engineering-mode data alongside the two LIGO detectors in mid-June. Since that time the Virgo team has been working to hunt down sources of instrument noise and improve the stable operation of the interferometer. Besides providing further confirmation of any detected events, the addition of Virgo is expected to improve their sky localization by an average factor of 2 or better. At the end of O2 both detectors will return to improving their sensitivities in preparation for the next joint observation run (O3, currently scheduled to begin in Fall 2018).
For more information see the Virgo press release.
LIGO and Virgo Collaborations preparing a brief guide to LIGO detector noise and extraction of gravitational-wave signals
Recent claims in a preprint by Creswell et al. of puzzling correlations in LIGO data have broadened interest in understanding the publicly available LIGO data around the times of the detected gravitational-wave events. We see that the features presented in Creswell et al. arose from misunderstandings of public data products. The LIGO Scientific Collaboration and Virgo Collaboration (LVC) have full confidence in our published results, and we are preparing a paper in which we will provide more details about LIGO detector noise properties and the data analysis techniques used by the LVC to detect gravitational-wave signals and infer their waveforms.
July 2017 update on LIGO's second observing run
7 July 2017 -- The second Advanced LIGO run began on November 30, 2016 and is scheduled to end on August 25, 2017. The run was suspended on May 8 for some in-vacuum commissioning activities at both sites; it resumed on May 26 at LIGO Livingston Observatory and on June 8 at LIGO Hanford Observatory. As of June 23, approximately 81 days of Hanford-Livingston coincident science data have been collected. The average reach of the LIGO network for binary merger events has been around 70 Mpc for 1.4+1.4 Msun, 300 Mpc for 10+10 Msun and 700 Mpc for 30+30 Msun mergers, with relative variations in time of the order of 10%.
As of June 23, 8 triggers, identified by online analysis using a loose false-alarm-rate threshold of one per month, have been identified and shared with astronomers who have signed memoranda of understanding with LIGO and Virgo for electromagnetic followup. One of these triggers has been confirmed by offline analysis, given the name GW170104, and published on June 1. A thorough investigation of the data and offline analysis are in progress; results will be shared when available.
Advanced Virgo has joined the network for few days in June in engineering mode, performing full tests in preparation for the triple-observing run planned for later this summer.
First triple lock of LIGO and Virgo interferometers
17 June 2017 -- For the first time, all three second generation interferometers---LIGO Hanford, LIGO Livingston, and Virgo---are simultaneously in a locked state. (When an interferometer is "locked" it means that an optical resonance is set up in the arm cavities and is producing a stable interference pattern at the photodetector.) Virgo is joining in an engineering mode, in preparation for the full triple-observing mode planned for later this summer. Congratulations, Virgo!
Image Credit: Virgo Collaboration
LIGO Detects Gravitational Waves for Third Time
1 Jun 2017 -- The LIGO Scientific Collaboration and the Virgo collaboration confirmed a third gravitational wave event in data from the Advanced LIGO detectors in Livingston, Louisiana, and Hanford, Washington, USA.
The detected waves—observed on January 4th, 2017 at 10:11:58.6 UTC (5:12AM EST) —were produced by a binary black hole system. Stellar-mass black holes with 31.2 and 19.4 solar masses merged to produce a spinning black hole of 48.7 solar masses. The detected signal is completely consistent with the predictions of general relativity.
Image credit: LIGO/Caltech/MIT/Sonoma State (Aurore Simonnet)
LSC elects David Shoemaker as new spokesperson
29 March 2017 -- David Shoemaker, MIT senior research scientist, was elected spokesperson of the LIGO Scientific Collaboration. Shoemaker was the leader of the Advanced LIGO project. He succeeds outgoing spokesperson Gabriela González. More information can be found on the MIT press release.
Image Credit: Bryce Vickmark
LSC mourns the passing of LIGO co-founder Ronald Drever
9 March 2017 -- Ronald William Prest Drever, co-founder of LIGO and emeritus professor of physics at Caltech, passed away on 7 March 2017 at the age of 85. A full obituary can be found on the Caltech website, the Scotsman, and Science Magazine.
Image Credit: Caltech Archives
LIGO Leadership recognized by National Academy of Sciences and American Astronomical Society prizes; LIGO Team recognized by Royal Astronomical Society
27 January 2017 -- Present and past leaders of the LIGO Laboratory and the LIGO Scientific Collaboration were recognized with major prizes by the National Academy of Sciences and the American Astronomical Society. The entire LIGO Team was recognized by the UK Royal Astronomical Society.
On January 25th the High Energy Astrophysics Division (HEAD) of the American Astronomical Society (AAS) awarded the Bruno Rossi Prize to Gabriela González and the LIGO Scientific Collaboration (LSC). The Rossi Prize is awarded annually to recognize "a significant contribution to High Energy Astrophysics, with particular emphasis on recent, original work." González is a professor of physics and astronomy at Louisiana State University (LSU) and has been the LSC spokesperson since 2011. More information about the award can be found on the AAS website.
On January 26th the National Academy of Scienes (NAS) awarded the Henry Draper Medal to Barry Barish and Stan Whitcomb, and the NAS Award for Scientific Discovery to Gabriela González, David H. Reitze, and Peter R. Saulson.
The Henry Draper Medal is awarded every four years and honors "a recent, original investigation in astronomical physics, of importance and benefit to science to merit such recognition." Barry Barish is the Linde Professor of Physics, Emeritus at the California Institute of Technology. Barish was the Principal Investigator of LIGO from 1994 to 2005, during the period of its construction and initial operation. Stan Whitcomb is the LIGO Laboratory Chief Scientist at the California Institute of Technology. Whitcomb has been working on gravitational-wave detection since 1980; he led the team that designed and commissioned the initial LIGO detectors and helped train the team that built Advanced LIGO. More information about the award can be found on the website for the 2017 NAS Henry Draper Medal.
The NAS Award for Scientific Discovery is presented every two years for "an accomplishment or discovery in basic research, achieved within the previous five years, that is expected to have a significant impact on one or more of the following fields: astronomy, biochemistry, biophysics, chemistry, materials science, or physics." The 2017 award recognizes the first three elected spokespersons of the LIGO Scientific Collaboration: Saulson, Reitze, and González. (Rai Weiss was the first spokesperson of the LSC). Peter Saulson is the Martin A. Pomerantz ’37 Professor of Physics at Syracuse University. David Reitze is the Executive Director of LIGO Laboratory at Caltech and a Professor of Physics at the University of Florida. The award recognizes the role of the current and past spokespersons in leading the LIGO team to the first direct detections of gravitational waves in 2015. More information can be found on the webpage for the 2017 NAS Award for Scientific Discovery.
On January 13, 2017 the UK Royal Astronomical Society (RAS) awarded their 2017 Group Achievement Award in Astronomy to the LIGO Team, in recognition of the first direct detection of gravitational waves. More information can be found at the RAS news release.
LIGO to be honored at Special Breakthrough Prize Ceremony on December 4th; watch LIVE
3 December 2016 -- On Sunday, December 4th, at 10ET/9c, tune into the National Geographic channel to watch LIGO and other remarkable scientists and mathematicians receive this year’s Breakthrough Prizes. The star-studded ceremony will be hosted by Morgan Freeman, and will include a performance by Alicia Keys.
In May of this year, LIGO was named the recipient of a Special Breakthrough Prize in Fundamental Physics. This “Special” prize (separate from the 'regular' Breakthrough Prize) can be awarded at any time by the selection committee, which includes an impressive array of internationally renowned scientists. Previous winners of the Special Prize include seven leaders of the Large Hadron Collider teams that discovered the Higgs Boson. This time, the $3 million dollar prize acknowledges LIGO’s historic detection of gravitational waves and the subsequent empirical confirmation of the most difficult-to-detect predication of general relativity. The prize will be shared between LIGO founders Ronald W. P. Drever, Kip S. Thorne and Rainer Weiss, and 1012 contributors to the discovery. The Breakthrough Prize in Fundamental Physics was founded in 2012 by Yuri Milner to recognize those individuals who have made profound contributions to human knowledge.
Kip Thorne and Rai Weiss will be on hand to accept the award on behalf of the LIGO Scientific Collaboration. If you can’t tune in live this Sunday, Fox Network and NatGeo stations will re-air a one-hour version of the ceremony on Sunday, Dec. 18, at 7:00-8:00 PM ET/PTth. For more details on the Breakthrough Prize and on how to watch this event live, check out these websites:
The Ceremony: https://breakthroughprize.org/News/33
LIGO Named as Special Prize Winner: https://breakthroughprize.org/News/32
Breakthrough Prize website: https://breakthroughprize.org
LIGO Resumes Search for Gravitational Waves
30 November 2016 -- After a series of upgrades, the twin detectors of LIGO, the Laser Interferometer Gravitational-wave Observatory, have turned back on and resumed their search for ripples in the fabric of space and time known as gravitational waves. LIGO transitioned from engineering test runs to science observations at 8 a.m. Pacific Standard Time on November 30.
On February 11, 2016, the LIGO Scientific Collaboration (LSC) and the Virgo Collaboration announced that LIGO had made the first-ever direct observation of gravitational waves. The waves were generated by a tremendously powerful collision of two black holes 1.3 billion light-years away and were recorded by both of LIGO's detectors—one in Hanford, Washington, and the other in Livingston, Louisiana. A second gravitational-wave detection by LIGO was announced on June 15, 2016, also from merging black holes.
The initial detections were made during LIGO's first run after undergoing major technical upgrades in a program called Advanced LIGO. That run lasted from September 2015 to January 2016. Since then, engineers and scientists have been evaluating LIGO's performance and making improvements to its lasers, electronics, and optics—resulting in an overall increase in LIGO's sensitivity.
"For our first run, we made two confirmed detections of black-hole mergers in four months," says Caltech's Dave Reitze, executive director of the LIGO Laboratory, which operates the LIGO observatories. "With our improved sensitivity, and a longer observing period, we will likely observe even more black-hole mergers in the coming run and further enhance our knowledge of black-hole dynamics. We are only just now, thanks to LIGO, learning about how often events like these occur."
The Livingston detector now has about a 25 percent greater sensitivity—or range for detecting gravitational waves from binary black holes—than during the first observing run. That means it can see black-hole mergers at further distances than before, and therefore should see more mergers than before. The sensitivity for the Hanford detector is similar to that of the first observing run.
"The Livingston detector has improved sensitivity for lower gravitational-wave frequencies, below about 100 hertz, primarily as the result of reducing the level of scattered light, which can be a pernicious source of noise in the interferometers," says Peter Fritschel, the associate director for LIGO at MIT and LIGO's chief detector scientist. "This is important for detecting massive systems like the merger of two black holes. We are confident that we'll see more black-hole mergers."
"LIGO Hanford scientists and engineers have successfully increased the power into the interferometer, and improved the stability of the detector," says Caltech's Mike Landry, the head of LIGO Hanford Observatory. "Significant progress has been made for the future utilization of still higher power, which will ultimately lead to improved sensitivity in future runs. Furthermore, with the addition of specialized sensors called balance-beam tilt meters in the corner and end stations, the detector is now more stable against wind and low-frequency seismic motion, thereby increasing the amount of time the detector can be in observing mode."
The LIGO team will continue to improve the observatories' sensitivities over the coming years, with increases planned for each successive observing run. As more black-hole mergers are detected by LIGO, scientists will start to get their first real understanding of black-hole pairs in the universe—including their population numbers, masses, and spin rates. LIGO may also detect the merger of neutron stars—the dense cores of exploded stars. Knowledge of both black-hole and neutron-star mergers will improve our understanding of stellar evolution and death.
"LIGO's scientific and operational staff have been working hard for the past year and are enthusiastic to restart round-the-clock observations. We are as curious as the rest of the world about what nature will send our way this year," says LIGO Livingston Observatory head Joe Giaime of Caltech and Louisiana State University.
Caltech and MIT conceived of, built, and operate the LIGO Observatories, with funding provided by the National Science Foundation (NSF). The Advanced LIGO detector was constructed by Caltech and MIT with funding from NSF and contributions from LSC institutions worldwide, including the Max Planck Society in Germany, the Science and Technology Facilities Council (STFC) in the U.K., and the Australian Research Council, among many others.
LIGO research is carried out by the international LIGO Scientific Collaboration (which includes the GEO Collaboration and the Australian Consortium for Interferometric Gravitational Astronomy) and the Virgo Collaboration in Europe.
GravitySpy, A Crowdsourcing Tool for Finding Glitches in LIGO Data, Is Launched
12 October 2016 -- Gravity Spy, a crowdsourcing tool for finding and analyzing glitches in LIGO data, has been publicly launched today. Glitches, or noise, in the LIGO data are a byproduct of very high sensitivity of LIGO instruments. The presence of these non-gravitational-wave disturbances in the data can obscure or mimic true gravitational-wave signals. The origin of some glitches is well-understood, while others remain a mystery. The rates at which the glitches occur vary depending on what's going on with the detectors and their environments. At their highest rates, glitches happen at 3x/sec. At such rates and with more than 2 dozen types of glitches observed so far, it takes an enourmous amount of data processing to sort out and classify them. To facilitate this process, the Gravity Spy tool is crowdsourcing the glitch identification to citizen scientists. With each new classification, LIGO will move closer and closer to discovering new gravitational-wave signals by identifying possible noise patterns in its data and filtering them out. Read more, and sign up, at the Gravity Spy website.
The Gravity Spy tool is a result of collaborative efforts of several LSC groups. The Gravity Spy team consists of LIGO researchers at the Center for Interdisciplinary Exploration and Research in Astronomy (CIERA) at Northwestern University, LIGO researchers at Caltech, machine learning researchers at Northwestern University, crowd-sourced science researchers at Syracuse University, and Zooniverse web developers.
LIGO Celebrates First Anniversary of Historic Gravitational Wave Detection
14 September 2016 -- Today LIGO celebrates the 1st anniversary of its gravitational-wave detection. Read this article about how this historic discovery was made, and about its significance for the future of gravitational-wave astronomy, at the LIGO Lab website.
Image: A. Simonnet
Advanced LIGO Engineering Team Wins OSA's 2016 Paul F. Forman Award
7 September 2016 -- The Advanced LIGO Engineering Team has been awarded the Paul F. Forman Team Engineering Excellence Award from the Optical Society. This award recognizes technical achievements such as product engineering, process, software and patent development, as well as contributions to society such as engineering education, publication and management, and furthering public appreciation of optical engineering. In addition to members of the LIGO Laboratory at all 4 locations, the team includes individuals from Albert Einstein Institute and Laser Zentrum Hannover, Glasgow University, Rutherford Appleton Laboratory, Standford University, and University of Florida. (See the full list of Advanced LIGO awardees.) The award will be presented at the Frontiers in Optics, the 100th OSA meeting that will take place in October 2016, followed by an article in Optics & Photonics News on the winners. LIGO Chief Engineer Dennis Coyne and LIGO Senior Optical Engineer GariLynn Billingsley will collect the award on behalf of the Advanced LIGO team. Congratulations to all the team members!
LSC Congratulates the LISA Pathfinder Team on the Satellite Mission Success
6 September 2016 -- The LIGO Scientific Collaboration would like to congratulate the LISA Pathfinder team on the fantastic success of their space satellite mission. This technology test mission has demonstrated acceleration noise at mHz frequencies which is better than required for the full LISA mission, and interferometric readout noise which far better than required. The Pathfinder triumph shows that LISA technology is sound, and paves the way towards multi-wavelength gravitational wave astronomy, as advocated in the recent US National Academy of Science "Review of Progress Toward the Decadal Survey Vision in New Worlds, New Horizons in Astronomy and Astrophysics". LISA, together with LIGO, its partners, and future ground-based detectors, will make it possible to "listen" to the universe over a frequency band that is more than 30 octaves wide. We can hardly wait to discover this unknown world!
Image: Artist's impression of the LISA Pathfinder. Credit: ESA
Gravitational Waves Detected from Second Pair of Colliding Black Holes
15 June 2016 -- The LIGO Scientific Collaboration and the Virgo collaboration identify a second gravitational wave event in the data from Advanced LIGO detectors.
On December 26, 2015 at 03:38:53 UTC, scientists observed gravitational waves — ripples in the fabric of spacetime — for the second time. The gravitational waves were detected by both of the twin Laser Interferometer Gravitational - Wave Observatory (LIGO) detectors, located in Livingston, Louisiana, and Hanford, Washington, USA.
LIGO Founders Are the Winners of the 2016 Kavli Prize in Astrophysics
2 June 2016 -- Three founders of LIGO are the recipients of the prestigious Kavli Prize in Astrophysics. The Kavli Foundation announced that Ronald W.P. Drever (Caltech), Kip S. Thorne (Caltech) and Rainer Weiss (MIT) are the 2016 awardees of the $1 million prize. The prize, which is awarded every 2 years, recognizes "scientists for their seminal advances in three research areas," including Astrophysics, Kavli Prize website states. The three founders of LIGO are being honored for "their ingenuity, inspiration, intellectual leadership and tenacity [which] were the driving force behind [the] epic discovery" of gravitationa waves, the prize citation reads.
Update 6 Sep 2016: The Kavli Prize was presented to (below, l-r) Ian Drever (representing his brother Ronald); Rainer Weiss; and Kip S. Thorne by Crown Prince of Norway Haakon at a ceremony in Oslo, Norway:
Credit: The Kavli Prize.
LIGO Founders Receive The Shaw Prize in Astronomy
31 May 2016 -- The three researchers who founded LIGO have been awarded the 2016 Shaw Prize in Astronomy, The Shaw Foundation announced. Ronald W.P. Drever (Caltech), Kip S. Thorne (Caltech) and Rainer Weiss (MIT) are the recipients of the $1.2 million prize, awarded annually. According to the prize citattion, the award recognizes their collective work on "conceiving and designing the Laser Interferometer Gravitational-Wave Observatory (LIGO), whose recent direct detection of gravitational waves opens a new window in astronomy, with the first remarkable discovery being the merger of a pair of stellar mass black holes."
LIGO Members Awarded The 2016 Gruber Prize in Cosmology
4 May 2016 -- The three principal founders of LIGO, along with the entire LIGO discovery team, have been awarded The 2016 Gruber Prize in Cosmolgy, the Gruber Foundation announced.
Ronald W.P. Drever (Caltech), Kip S. Thorne (Caltech), and Rainer Weiss (MIT) will each receive a gold medal and will share a $500,000 award. The Prize citation reads: "The Gruber Foundation proudly presents the 2016 Cosmology Prize to Rainer Weiss, Kip Thorne, Ronald Drever, and the entire LIGO team for pursuing a vision to observe the universe in gravitational waves, leading to a first detection that emanated from the collision of two black holes. This remarkable event provided the first glimpse into the strong‐gravity regime of Einstein's theory of general relativity that governs the dynamics of black holes, giving direct evidence for their existence, and demonstrating that their nature is consistent with the predictions of general relativity."
LIGO Awarded Special Breakthrough Prize in Fundamental Physics
2 May 2016 -- Members of the LIGO and Virgo collaborations have been awarded a Special Breakthrough Prize in Fundamental Physics, the Prize Selection Committee announced.
The award recognizes "the scientists and engineers contributing to the momentuous detection of gravitational waves", which was announced by LIGO on Feb 11, 2016, stated the announcement by the Selection Committee.
The Special Breakthrough Prize can be awarded at any time in recognition of an exceptional scientific achievement. The $3 million prize will be shared as follows: the three LIGO founders -- Ronald W.P. Drever (Caltech); Kip S. Thorne (Caltech); and Rainer Weiss (MIT) -- will share $1 million; and the 1012 contributing scientists, engineers, and staff will share $2 million.
NSF Signs a LIGO-India MOU
31 March 2016 -- The US and India have signed a Memorandum of Understanding for establishing an advanced gravitational-wave detector in India. France A. Córdova, Director of the National Science Foundation, and representatives of India's Department of Atomic Energy and Department of Science and Technology, signed the MoU in the presence of India's Prime Minister Narendra Modi. (Image: NSF/Fleming Crim.)
From the NSF website: "Today, National Science Foundation (NSF) Director France A. Córdova signed a Memorandum of Understanding (MOU) to lead the way for establishing an advanced gravitational-wave detector in India. The MOU was also signed by representatives from India's Department of Atomic Energy and India's Department of Science and Technology."
Read the NSF Press Release.
LIGO Team Testifies Before US Congress on the Discovery
24 February 2016 -- As a follow-up to the announcement of LIGO's first observation of gravitational waves, the House Committee on Science, Space, and Technology has asked LIGO Scientific Collaboration members to testify on the discovery, its meaning for science and society, and what the future may hold. LSC members to testify at the Full House Committee Hearing were the LIGO Lab Executive Director David Reitze, the LSC Spokesperson Gabriela Gonzalez, and the LIGO MIT Director David Shoemaker. Details at house.gov.
Watch the hearing below:
17 February 2016 -- The LIGO-India project has been formally approved by the Union Cabinet. The formal approval will clear the path for funding of the LIGO-India project, as well as for other activities that are critical for the start of building a gravitational-wave detector in India.
Read an article in The Hindu.
White House Congratulates the LIGO Team
12 February 2016 -- On February 11, President Obama tweeted his congratulations to the LIGO team:
On Feb 12, 2016, John P. Holdren, Assistant to the President for Science and Technology and Director of the White House Office of Science and Technology Policy, posted a statement on the White House blog with congratulations to the LIGO team.
Read the full statement on https://www.whitehouse.gov/blog.
Gravitational Waves Detected 100 Years after Einstein's General Relativity
11 February 2016 -- For the first time, scientists have observed ripples in the fabric of spacetime called gravitational waves, arriving at the earth from a cataclysmic event in the distant universe. This confirms a major prediction of Albert Einstein's 1915 general theory of relativity and opens an unprecedented new window onto the cosmos.
Gravitational waves carry information about their dramatic origins and about the nature of gravity that cannot otherwise be obtained. Physicists have concluded that the detected gravitational waves were produced during the final fraction of a second of the merger of two black holes to produce a single, more massive spinning black hole. This collision of two black holes had been predicted but never observed.
The gravitational waves were detected on September 14, 2015 at 5:51 a.m. Eastern Daylight Time (9:51 a.m. UTC) by both of the twin Laser Interferometer Gravitational-wave Observatory (LIGO) detectors, located in Livingston, Louisiana, and Hanford, Washington, USA. The LIGO Observatories are funded by the National Science Foundation (NSF), and were conceived, built, and are operated by Caltech and MIT. The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration (which includes the GEO600 Collaboration and the Australian Consortium for Interferometric Gravitational Astronomy) and the Virgo Collaboration using data from the two LIGO detectors.
LSC Statement on Harassment
16 January 2016 -- There have been recent reports of harassment involving LIGO Scientific Collaboration members, specifically involving a Caltech faculty member and a student. That faculty member is no longer a member of the LSC. As a collaboration, we will not tolerate harassment and strive to provide a supportive environment for all members of our collaboration. We practice the principles enshrined in the LSC Diversity Statement, with guidelines in https://dcc.ligo.org/LIGO-M1400285/public:
"As members of the LIGO Scientific Collaboration, we recognize the importance of diversity to enrich our research and scholarship. We pledge to provide a welcoming, inclusive environment to talented individuals regardless of characteristics such as, but not limited to, physical ability, race, ethnicity, gender, sexual orientation, economic status, or personal religious practices, and to support the professional growth of all collaboration members.
We also pledge to work to increase the numbers of women and under-represented minorities that actively participate in the LSC, to pursue recruitment, mentoring, retention and promotion of women and under-represented minority scientists and engineers and to maximize their contribution to excellence in our research. As a collaboration, we will strive to create a professional climate that encourages inclusion and that respects and values diversity."