Fetching the paper…
Reading the bibliography…
Roughly every 2-10 minutes, a pair of stellar mass black holes merge somewhere in the Universe.
G Malmquist, “On some relations in stellar statistics,” Meddelanden fran Lunds Astronomiska Observatorium Series I 100
1922
Earlier work this paper cites.
H. Jeffreys, Theory of Probability , 3rd ed. (Oxford, Oxford, England, 1961)
1961
Earlier work this paper cites.
R W Hellings and G S Downs, ““upper limits on the isotropic gravitational radiation background from pulsar timing analysis,” Astrophys. J. Lett. 265
1983
Earlier work this paper cites.
N Christensen, “Measuring the stochastic gravitational-radiation background with laser-interferometric antennas,” Phys. Rev. D 46
1992
Earlier work this paper cites.
D. R. Lorimer, L. Nicastro, A. G. Lyne, M. Bailes, R. N. Manchester, S. Johnston, J. F. Bell, N. D’Amico, and P. A. Harrison, “Four new millisecond pulsars in the galactic disk,” Astrophys. J. 439
1995
Earlier work this paper cites.
C Cutler, “Angular resolution of the LISA gravitational wave detector,” Phys. Rev. D 57
1998
Earlier work this paper cites.
B Allen and J D Romano, “Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities,” Phys. Rev. D 59
1999
Earlier work this paper cites.
Thibault Damour and Alexander Vilenkin, “Gravitational wave bursts from cosmic strings,” Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
Michele Maggiore, “Gravitational wave experiments and early universe cosmology,” Phys. Rep. 331
2000
Earlier work this paper cites.
E. S. Phinney, “A Practical Theorem on Gravitational Wave Backgrounds,” ArXiv Astrophysics e-prints (2001), astro-ph/0108028
2001
Earlier work this paper cites.
S Drasco and E E Flanagan, “Detection methods for non-gaussian gravitational wave stochastic backgrounds,” Phys. Rev. D 67
2003
Earlier work this paper cites.
C Cutler and J Harms, “Big Bang Observer and the neutron-star-binary subtraction problem,” Phys. Rev. D 73
2006
Earlier work this paper cites.
Douglas Reynolds, “Gaussian mixture models,” in Encyclopedia of Biometrics , edited by Stan Z. Li and Anil Jain (Springer US, Boston, MA, 2009) pp. 659–663
2009
Earlier work this paper cites.
M Favata, “The gravitational-wave memory effect,” Class. Quant. Grav. 27
2010
Earlier work this paper cites.
P A Rosado, “Gravitational wave background from binary systems,” Phys. Rev. D 84
2011
Earlier work this paper cites.
X-J Zhu, E Howell, T Regimbau, D Blaire, and Z-H Zhu, “Stochastic gravitational wave background from coalescing binary black holes,” Astrophys. J. 739
2011
Earlier work this paper cites.
Matthew R. Adams, Neil J. Cornish, and Tyson B. Littenberg, “Astrophysical model selection in gravitational wave astronomy,” Phys. Rev. D 86
2012
Earlier work this paper cites.
E Thrane, “Measuring the non-gaussian stochastic gravitational-wave background: A method for realistic interferometer data,” Phys. Rev. D 87
2013
Cited alongside, same era.
K Cannon, C Hanna, and D Keppel, “Method to estimate the significance of coincident gravitational-wave observations from compact binary coalescence,” Phys. Rev. D 88
2013
Cited alongside, same era.
A Gelman, J B Carlin, H S Stern, D B Dunson, A Vehtari, and D B Rubin, Bayesian Data Analysis, Third Edition , Chapman & Hall/CRC Texts in Statistical Science (Taylor & Francis, 2013)
2013
Cited alongside, same era.
A Sesana, “Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band,” MNRASL 433
2013
Cited alongside, same era.
E Thrane and J D Romano, “Sensitivity curves for searches for gravitational-wave backgrounds,” Phys. Rev. D 88
J Powell, D Trifiro, E Cuoco, I-S Heng, and M Cavaglia, Class. Quant. Grav. 32
2015
Later among the works it cites.
Thomas Callister, Letizia Sammut, Shi Qiu, Ilya Mandel, and Eric Thrane, “Limits of astrophysics with gravitational-wave backgrounds,” Phys. Rev. X 6
2016
Later among the works it cites.
Rory Smith, Scott E Field, Kent Blackburn, Carl-Johan Haster, Michael Pürrer, Vivien Raymond, and Patricia Schmidt, “Fast and accurate inference on gravitational waves from precessing compact binaries,” Phys. Rev. D 94
2016
Later among the works it cites.
Xilong Fan, Yanbei Chen, and Christopher Messenger, “Method to detect gravitational waves from an ensemble of known pulsars,” Phys. Rev. D 94
2016
Later among the works it cites.
X-J Zhu, L Wen, J Xiong, Y Xu, Y Wang, S. D. Mohanty, G. Hobbs, and R. N. Manchester, “Detection and localization of continuous gravitational waves with pulsar timing arrays: the role of pulsar terms,” MNRAS 461
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
2013
Cited alongside, same era.
L Martinelli and T Regimbau, “Semiparametric approach to the detection of non-gaussian gravitational wave stochastic backgrounds,” Phys. Rev. D 89
2014
Cited alongside, same era.
Mark Hannam, Patricia Schmidt, Alejandro Bohé, Le \ \backslash ” \ \backslash ila Haegel, Sascha Husa, Frank Ohme, Geraint Pratten, and Michael Pürrer, “Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms,” Phys. Rev. Lett. 113
2014
Cited alongside, same era.
S Vitale, Ryan Lynch, John Veitch, Vivien Raymond, and Riccardo Sturani, “Measuring the spin of black holes in binary systems using gravitational waves,” Phys. Rev. Lett. 112
2014
Cited alongside, same era.
D Talukder, E Thrane, S Bose, and T Regimbau, “Measuring neutron-star ellipticity with measurements of the stochastic gravitational-wave background,” Phys. Rev. D 89
2014
Cited alongside, same era.
Luc Blanchet, “Gravitational radiation from post-newtonian sources and inspiralling compact binaries,” Living Reviews in Relativity 17
2014
Cited alongside, same era.
L Martinelli and T Regimbau, “Efficiency of the cross-correlation statistic for gravitational wave stochastic background signals with non-gaussian noise and heterogeneous detector sensitivities,” Phys. Rev. D 92
2015
Cited alongside, same era.
J Veitch et al. , “Parameter estimation for compact binaries with ground-based gravitational-wave observations using the lalinference software library,” Phys. Rev. D 91
2015
Cited alongside, same era.
2016
Later among the works it cites.
J D Romano and N J Cornish, “Detection methods for stochastic gravitational-wave backgrounds: a unified treatment,” Living. Rev. Relativ. 20
2017
Closest in time.
2017
Closest in time.
M. Isi, R. Smith, S. Vitale, et al. , (2017 in preparation)
2017
Closest in time.
C Talbot and E Thrane, “Determining the population properties of spinning black holes,” Phys. Rev. D 96
2017
Closest in time.
Ilya Mandel, Will M Farr, Andrea Colonna, Simon Stevenson, Peter Tiňo, and John Veitch, “Model-independent inference on compact-binary observations,” MNRAS 465
2017
Closest in time.
Maya Fishbach, Daniel Holz, and Ben Farr, “Are LIGO’s Black Holes Made From Smaller Black Holes?” Astrophys. J. Lett. 840
2017
Closest in time.
S Stevenson, C Berry, and I Mandel, “Hierarchical analysis of gravitational-wave measurements of binary black hole spin–orbit misalignments,” MNRAS 471
2017
Closest in time.
C. Callister, M. Isi, R Smith, and E. Thrane, (2017 in preparation)
2017
Closest in time.
2017
Closest in time.
K Crocker, T Prestegard, V Mandic an T Regimbau, K Olive, and E Vangioni, Phys. Rev. D 95
2017
Closest in time.
Craig Cahillane, Joe Betzwieser, Duncan A. Brown, Evan Goetz, Evan D. Hall, Kiwamu Izumi, Shivaraj Kandhasamy, Sudarshan Karki, Jeff S. Kissel, Greg Mendell, Richard L. Savage, Darkhan Tuyenbayev, Alex Urban, Aaron Viets, Madeline Wade, and Alan J. Weinstein, “Calibration uncertainty for advanced ligo’s first and second observing runs,” Phys. Rev. D 96
2017
Closest in time.