First Demonstration of Early Warning Gravitational-wave Alerts
Creators
- Magee, Ryan1
- Anderson, Stuart1
- Chatterjee, Deep2
- Singer, Leo P.3
- Sachdev, Surabhi4
- Godwin, Patrick4
- Hanna, Chad4
- Kovalam, Manoj5
- Chu, Qi5
- Clearwater, Patrick5
- Codoreanu, Alex5
- Mo, Geoffrey6
- Brady, Patrick7
- Brockill, Patrick7
- Cannon, Kipp8
- Dal Canton, Tito9
- Drago, Marco10
- Ghosh, Shaon11
- Greco, Giuseppe12
- Kapadia, Shasvath J.13
- and others
- 1. LIGO, California Institute of Technology, Pasadena, CA 91125 (United States)
- 2. Center for Astrophysical Surveys, National Center for Supercomputing Applications, Urbana, IL 61801 (United States)
- 3. Astroparticle Physics Laboratory, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771 (United States)
- 4. Department of Physics, The Pennsylvania State University, University Park, PA 16802 (United States)
- 5. Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav) (Australia)
- 6. LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)
- 7. Leonard E. Parker Center for Gravitation, Cosmology, and Astrophysics, University of Wisconsin-Milwaukee, Milwaukee, WI 53201 (United States)
- 8. Research Center for the Early Universe, The University of Tokyo, 113-0033 (Japan)
- 9. Université Paris-Saclay, CNRS/IN2P3, IJCLab, F-91405 Orsay (France)
- 10. Università di Roma "La Sapienza," I-00185 Roma (Italy)
- 11. Department of Physics and Astronomy, Montclair State University, Montclair, NJ 07043 (United States)
- 12. Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino (Italy)
- 13. International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560089 (India)
Description
Gravitational-wave observations became commonplace in Advanced LIGO-Virgo's recently concluded third observing run. 56 nonretracted candidates were identified and publicly announced in near real time. Gravitational waves from binary neutron star mergers, however, remain of special interest since they can be precursors to high-energy astrophysical phenomena like γ-ray bursts and kilonovae. While late-time electromagnetic emissions provide important information about the astrophysical processes within, the prompt emission along with gravitational waves uniquely reveals the extreme matter and gravity during—and in the seconds following—merger. Rapid communication of source location and properties from the gravitational-wave data is crucial to facilitate multimessenger follow-up of such sources. This is especially enabled if the partner facilities are forewarned via an early warning (pre-merger) alert. Here we describe the commissioning and performance of such a low-latency infrastructure within LIGO-Virgo. We present results from an end-to-end mock data challenge that detects binary neutron star mergers and alerts partner facilities before merger. We set expectations for these alerts in future observing runs.
Availability note (English)
Available from http://dx.doi.org/10.3847/2041-8213/abed54Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal Letters
- Journal Volume
- 910
- Journal Issue
- 2
- Journal Page Range
- [7 p.]
- ISSN
- 2041-8205
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 53071913
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; GRAVITATIONAL WAVES; NEUTRON STARS
- Descriptors DEC
- PHYSICS; STARS