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26 results on '"H. Gabbard"'

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1. Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

2. GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence

3. On the Progenitor of Binary Neutron Star Merger GW170817

4. Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

5. Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817

6. Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B

7. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

8. Erratum: 'First Search for Gravitational Waves from Known Pulsars with Advanced LIGO' (2017, ApJ, 839, 12)

9. Development of an axial-flow centrifugal gas bubble separator for use in MSR xenon removal system

11. Development of a Venturi Type Bubble Generator for Use in the Molten-Salt Reactor Xenon Removal System

16. Control strategy to limit duty cycle impact of earthquakes on the LIGO gravitational-wave detectors.

17. Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background.

18. Matching Matched Filtering with Deep Networks for Gravitational-Wave Astronomy.

19. GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences.

20. First Search for Nontensorial Gravitational Waves from Known Pulsars.

21. Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.

22. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

23. GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence.

24. GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2.

25. Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run.

26. Directional Limits on Persistent Gravitational Waves from Advanced LIGO's First Observing Run.

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