P. Canizares
Radboud University Nijmegen
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by P. Canizares.
Physical Review Letters | 2017
B. Abbott; S. Bloemen; P. Canizares; S. Ghosh; P. Groot; T. Hinderer; G. Nelemans; D. Nichols; S. Nissanke; P. Schmidt; A.R. Williamson
On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per
Physical Review Letters | 2018
B. Abbott; S. Bloemen; P. Canizares; S. Ghosh; P. Groot; T. Hinderer; G. Nelemans; David A. Nichols; S. Nissanke; P. Schmidt; A. R. Williamson
8.0\times10^4
Physical Review D | 2018
B. Abbott; S. Bloemen; P. Canizares; S. Ghosh; P. Groot; G. Nelemans; David A. Nichols; S. Nissanke; P. Schmidt
years. We infer the component masses of the binary to be between 0.86 and 2.26
Physical Review D | 2018
B. Abbott; R. Abbott; T. D. Abbott; F. Acernese; K. Ackley; S. Bloemen; P. Canizares; S. Ghosh; P. Groot; T. Hinderer; G. Nelemans; S. Nissanke; P. Schmidt; A. R. Williamson; M. E. Zucker; J. Zweizig
M_\odot
International Journal of Modern Physics A | 2017
F. Acernese; S. Bloemen; P. Canizares; S. Ghosh; P. Groot; G. Nelemans; D. Nichols; S. Nissanke; P. Schmidt
, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17 to 1.60
