P. Groot
Radboud University Nijmegen
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Publication
Featured researches published by P. Groot.
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
Nature | 1998
Titus J. Galama; Paul M. Vreeswijk; J. van Paradijs; C. Kouveliotou; T. Augusteijn; H. Böhnhardt; James Brewer; V. Doublier; J.-F. Gonzalez; Bruno Leibundgut; C. Lidman; Olivier R. Hainaut; Ferdinando Patat; J. Heise; J. in't Zand; Kevin C. Hurley; P. Groot; R. Strom; Paolo A. Mazzali; Koichi Iwamoto; K. Nomoto; Hideyuki Umeda; Takashi Nakamura; T. R. Young; T. Suzuki; T. Shigeyama; T. M. Koshut; Marc Kippen; C. R. Robinson; P. de Wildt
8.0\times10^4
Nature | 1997
Kailash C. Sahu; Mario Livio; Larry Petro; D. Machetto; J. van Paradijs; C. Kouveliotou; G. J. Fishman; Charles A. Meegan; P. Groot; Titus J. Galama
years. We infer the component masses of the binary to be between 0.86 and 2.26
The Astrophysical Journal | 2009
Patrick A. Woudt; D. Steeghs; M. Karovska; Brian Warner; P. Groot; G. Nelemans; Gijs H. A. Roelofs; T. R. Marsh; Takahiro Nagayama; Derck P. Smits; T. J. O'Brien
M_\odot
Monthly Notices of the Royal Astronomical Society | 2007
Gijs H. A. Roelofs; Gijs Nelemans; P. Groot
, 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
Monthly Notices of the Royal Astronomical Society | 2014
G. Barentsen; H. J. Farnhill; Janet E. Drew; E. Gonzalez-Solares; R. Greimel; M. J. Irwin; Brent Miszalski; C. Ruhland; P. Groot; A. Mampaso; S. E. Sale; A.A. Henden; A. Aungwerojwit; M. J. Barlow; P.R. Carter; Romano L. M. Corradi; Jeremy J. Drake; J. Eislöffel; J. Fabregat; B. T. Gänsicke; N. P. Gentile Fusillo; A. Hales; Simon T. Hodgkin; Leo Huckvale; J. Irwin; Robert R. King; Christian Knigge; T. Kupfer; E. Lagadec; Daniel J. Lennon
M_\odot
Monthly Notices of the Royal Astronomical Society | 2009
S. E. Sale; Janet E. Drew; Yvonne C. Unruh; M. J. Irwin; Christian Knigge; Steven Phillipps; Albert A. Zijlstra; B. T. Gänsicke; R. Greimel; P. Groot; A. Mampaso; Rhys Morris; R. Napiwotzki; D. Steeghs; N. A. Walton
, with the total mass of the system
Astronomy and Astrophysics | 2013
Else Starkenburg; V. Hill; Eline Tolstoy; P. Francois; M. J. Irwin; Leon Boschman; Kim A. Venn; T. J. L. de Boer; B. Lemasle; Pascale Jablonka; G. Battaglia; P. Groot; L. Kaper
2.74^{+0.04}_{-0.01}\,M_\odot
Astrophysical Journal Supplement Series | 2011
P. G. Jonker; C. G. Bassa; G. Nelemans; D. Steeghs; M. A. P. Torres; Thomas J. Maccarone; Robert I. Hynes; James L. Clem; A. Dieball; V. Mikles; C. T. Britt; L. Gossen; A. Collazzi; Rudy Wijnands; J. in't Zand; Mariano Mendez; N. Rea; E. Kuulkers; E. M. Ratti; L.M. van Haaften; Craig O. Heinke; Feryal Ozel; P. Groot; F. Verbunt
. The source was localized within a sky region of 28 deg
Monthly Notices of the Royal Astronomical Society | 2012
S. Scaringi; Elmar Körding; P. Uttley; Christian Knigge; P. Groot; Martin Still
^2