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MHz Gravitational Wave Constraints with Decameter Michelson Interferometers
Aaron S. Chou, Richard Gustafson, Craig Hogan +10
A new detector, the Fermilab Holometer, consists of separate yet identical 39-meter Michelson interferometers. Strain sensitivity achieved is better than $10^{-21} /{\sqrt{\rm{Hz}}…
Gravity Spy: Integrating Advanced LIGO Detector Characterization, Machine Learning, and Citizen Science
Michael Zevin, Scott Coughlin, Sara Bahaadini +15
(abridged for arXiv) With the first direct detection of gravitational waves, the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) has initiated a new field of as…
Null-stream pointing with pulsar timing arrays
Jeffrey S. Hazboun, Shane L. Larson
Locating sources on the sky is one of the largest challenges in gravitational wave astronomy, owing to the omni-directional nature of gravitational wave detection techniques, and t…
Distinguishing Between Formation Channels for Binary Black Holes with LISA
Katelyn Breivik, Carl L. Rodriguez, Shane L. Larson +2
The recent detections of GW150914 and GW151226 imply an abundance of stellar-mass binary-black-hole mergers in the local universe. While ground-based gravitational-wave detectors a…