no code implementations • 21 Dec 2020 • K. Paterson, M. J. Lundquist, J. C. Rastinejad, W. Fong, D. J. Sand, J. E. Andrews, R. C. Amaro, O. Eskandari, S. Wyatt, P. N. Daly, H. Bradley, S. Zhou-Wright, S. Valenti, S. Yang, E. Christensen, A. R. Gibbs, F. Shelly, C. Bilinski, L. Chomiuk, A. Corsi, M. R. Drout, R. J. Foley, P. Gabor, P. Garnavich, C. J. Grier, E. Hamden, H. Krantz, E. Olszewski, V. Paschalidis, D. Reichart, A. Rest, N. Smith, J. Strader, D. Trilling, C. Veillet, R. M. Wagner, A. Zabludoff
In addition to triggered events within 24~hours, our transient search encompassed a time interval following GW events of $<120$~hrs, providing observations on $\sim$ 1/2 of the events accessible to the Mt Lemmon 1. 5 m telescope.
High Energy Astrophysical Phenomena