no code implementations • 8 Feb 2021 • Ryan Magee, Deep Chatterjee, Leo P. Singer, Surabhi Sachdev, Manoj Kovalam, Geoffrey Mo, Stuart Anderson, Patrick Brady, Patrick Brockill, Kipp Cannon, Tito Dal Canton, Qi Chu, Patrick Clearwater, Alex Codoreanu, Marco Drago, Patrick Godwin, Shaon Ghosh, Giuseppe Greco, Chad Hanna, Shasvath J. Kapadia, Erik Katsavounidis, Victor Oloworaran, Alexander E. Pace, Fiona Panther, Anwarul Patwary, Roberto De Pietri, Brandon Piotrzkowski, Tanner Prestegard, Luca Rei, Anala K. Sreekumar, Marek J. Szczepańczyk, Vinaya Valsan, Aaron Viets, Madeline Wade, Linqing Wen, John Zweizig
We present results from an end-to-end mock data challenge that detects binary neutron star mergers and alerts partner facilities before merger.
High Energy Astrophysical Phenomena
1 code implementation • 9 Sep 2020 • Alexander H. Nitz, Marlin Schäfer, Tito Dal Canton
We find that for a fiducial rate of binary neutron star mergers of $1000 ~\mathrm{Gpc}^{-3} \mathrm{yr}^{-1}$, the Design, A+, and Voyager era networks can provide 18, 54, and 195s of warning for one source per year of observing, respectively, with a sky localization area $<$100 deg$^2$ at a $90\%$ credible level.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
1 code implementation • 10 Jul 2019 • Quentin Baghi, Ira Thorpe, Jacob Slutsky, John Baker, Tito Dal Canton, Natalia Korsakova, Nikos Karnesis
By listening to gravity in the low frequency band, between 0. 1 mHz and 1 Hz, the future space-based gravitational-wave observatory LISA will be able to detect tens of thousands of astrophysical sources from cosmic dawn to the present.
General Relativity and Quantum Cosmology Instrumentation and Methods for Astrophysics 83C35, 62-07 I.6; G.3
