Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- D. Stern3 profiles493 · h 97
- F. Harrison2 profiles182 · h 58
- P. Eisenhardt3 profiles168 · h 59
- S. Boggs124 · h 60
- F. Christensen123 · h 58
- C. Hailey120 · h 59
- W. Craig2 profiles120 · h 49
- S. Stanford2 profiles117 · h 75
- S. Turyshev116 · h 38
- D. Walton2 profiles108 · h 53
- K. Stapelfeldt104 · h 70
- D. Mawet98 · h 53
- California Institute of TechnologyUS4.7k papers
- Centre National de la Recherche ScientifiqueFR2k papers
- Center for Astrophysics Harvard & SmithsonianUS1.3k papers
- Goddard Space Flight CenterUS1.2k papers
- University of California, BerkeleyUS1.2k papers
- University of ArizonaUS1k papers
- Infrared Processing and Analysis CenterUS1k papers
- University College LondonGB984 papers
- Princeton UniversityUS924 papers
- University of CambridgeGB871 papers
- Institut d'Astrophysique de ParisFR858 papers
- Space Telescope Science InstituteUS808 papers
12 papers · 2 filters
Accelerating relativistic reference frames in Minkowski space-time
Slava G. Turyshev, Olivier L. Minazzoli, Viktor T. Toth
We study accelerating relativistic reference frames in Minkowski space-time under the harmonic gauge. It is well-known that the harmonic gauge imposes constraints on the components…
Reduced Basis representations of multi-mode black hole ringdown gravitational waves
Sarah Caudill, Scott E. Field, Chad R. Galley +2
We construct compact and high accuracy Reduced Basis (RB) representations of single and multiple quasinormal modes (QNMs). The RB method determines a hierarchical and relatively sm…
The gravitational-wave memory from eccentric binaries
Marc Favata
The nonlinear gravitational-wave memory causes a time-varying but nonoscillatory correction to the gravitational-wave polarizations. It arises from gravitational waves that are sou…
Beyond Fisher: exact sampling distributions of the maximum-likelihood estimator in gravitational-wave parameter estimation
Michele Vallisneri
Gravitational-wave astronomers often wish to characterize the expected parameter-estimation accuracy of future observations. The Fisher matrix provides a lower bound on the spread…
Support for temporally varying behavior of the Pioneer anomaly from the extended Pioneer 10 and 11 Doppler data sets
Slava G. Turyshev, Viktor T. Toth, Jordan Ellis +1
The Pioneer anomaly is a small sunward anomalous acceleration found in the trajectory analysis of the Pioneer 10 and 11 spacecraft. As part of the investigation of the effect, anal…
A nonlinear scalar model of extreme mass ratio inspirals in effective field theory II. Scalar perturbations and a master source
Chad R. Galley
The motion of a small compact object (SCO) in a background spacetime is investigated further in a class of model nonlinear scalar field theories having a perturbative structure ana…
OSS (Outer Solar System): A fundamental and planetary physics mission to Neptune, Triton and the Kuiper Belt
Bruno Christophe, Linda J. Spilker, John D. Anderson +46
The present OSS mission continues a long and bright tradition by associating the communities of fundamental physics and planetary sciences in a single mission with ambitious goals…
An improved, "phase-relaxed" F-statistic for gravitational-wave data analysis
Curt Cutler
Rapidly rotating, slightly non-axisymmetric neutron stars emit nearly periodic gravitational waves (GWs), quite possibly at levels detectable by ground-based GW interferometers. We…
Pulsar Timing Sensitivities to Gravitational Waves from Relativistic Metric Theories of Gravity
Marcio Eduardo da Silva Alves, Massimo Tinto
Pulsar timing experiments aimed at the detection of gravitational radiation have been performed for decades now. With the forthcoming construction of large arrays capable of tracki…
Nano-Hertz Gravitational Waves Searches with Interferometric Pulsar Timing Experiments
Massimo Tinto
We estimate the sensitivity to nano-Hertz gravitational waves of pulsar timing experiments in which two highly-stable millisecond pulsars are tracked simultaneously with two neighb…
Pulsar Timing Sensitivity to Very-Low-Frequency Gravitational Waves
Fredrick A. Jenet, J. W. Armstrong, Massimo Tinto
At nanohertz frequencies gravitational waves (GWs) cause variations in time-of-arrival of pulsar signals potentially measurable via precision timing observations. Here we compute v…
Reduced basis catalogs for gravitational wave templates
Scott E. Field, Chad R. Galley, Frank Herrmann +3
We introduce a reduced basis approach as a new paradigm for modeling, representing and searching for gravitational waves. We construct waveform catalogs for non-spinning compact bi…