Mansi M. Kasliwal, the Principal Investigator of the Global Relay of Observatories Watching Transients Happen (GROWTH) collaboration, shares her enthusiasm about the future of multi-messenger astrophysics.
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Kasliwal, M. M. Seeing gravitational waves. Science 340, 555–556 (2013).
Abbott, B. P. et al. GW170817: observation of gravitational waves from a binary neutron star inspiral. Phys. Rev. Lett. 119, 161101 (2017).
Abbott, B. P. et al. Multi-messenger observations of a binary neutron star merger. Astrophys. J. Lett. 848, L12 (2017).
Kasliwal, M. M. et al. Spitzer mid-infrared detections of neutron star merger GW170817 suggests synthesis of the heaviest elements. Mon. Not. R. Astron. Soc. Lett. slz007 (2019).
Kasliwal, M. M. et al. Illuminating gravitational waves: a concordant picture of photons from a neutron star merger. Science 358, 1559–1565 (2017).
Evans, P. A. et al. Swift and NuSTAR observations of GW170817: detection of a blue kilonova. Science 358, 1565–1570 (2017).
Hallinan, G. et al. A radio counterpart to a neutron star merger. Science 358, 1579–1583 (2017).
Andreoni, I. et al. GROWTH on s190814bv: deep synoptic limits on the optical/near-infrared counterpart to a neutronstar–black hole merger. Astrophys. J. 890, 131 (2020).
De, K. et al. Palomar Gattini-IR: survey overview, data processing system, on-sky performance and first results. Publ. Astron. Soc. Pac. 132, 025001 (2020).
Kasliwal, M. M. et al. Kilonova luminosity function constraints based on Zwicky Transient Facility searches for 13 neutron star mergers. Preprint at arXiv:2006.11306 (2020).
GROWTH is a National Science Foundation Partnership in International Research and Education programme that comprises 16 institutions around the world: California Institute of Technology (USA), University of Maryland College Park (USA), University of Wisconsin Milwaukee (USA), Texas Tech University (USA), San Diego State University (USA), University of Washington Seattle (USA), Los Alamos National Laboratory (USA), Tokyo Institute of Technology (Japan), National Central University (Taiwan), Indian Institute of Astrophysics (India), Indian Institute of Technology Bombay (India), Weizmann Institute of Science (Israel), The Oskar Klein Centre at Stockholm University (Sweden), Humboldt University (Germany), Liverpool John Moores University (UK) and University of Sydney (Australia).
The authors declare no competing interests.
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The GROWTH Collaboration: http://growth.caltech.edu/
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Kasliwal, M.M. The future is now. Nat Rev Phys 2, 452–454 (2020). https://doi.org/10.1038/s42254-020-0227-z