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LISA Gravitational Wave Sources in A Time-Varying Galactic Stochastic Background
Matthew C. Digman, Neil J. Cornish
A unique challenge for data analysis with the Laser Interferometer Space Antenna (LISA) is that the noise backgrounds from instrumental noise and astrophysical sources will change…
Characterization of the stochastic signal originating from compact binaries populations as measured by LISA
Nikolaos Karnesis, Stanislav Babak, Mauro Pieroni +2
The Laser Interferometer Space Antenna (LISA) mission, scheduled for launch in the early 2030s, is a gravitational wave observatory in space designed to detect sources emitting in…
Getting Ready for LISA: The Data, Support and Preparation Needed to Maximize US Participation in Space-Based Gravitational Wave Science
Kelly Holley-Bockelmann, :, Jillian Bellovary +20
The NASA LISA Study Team was tasked to study how NASA might support US scientists to participate and maximize the science return from the Laser Interferometer Space Antenna (LISA)…
Prospects for Gravitational Wave Measurement of ZTFJ1539+5027
Tyson B. Littenberg, Neil J. Cornish
The short-period eclipsing binary ZTFJ1539+5027 discovered by Burdge et al. (2019) will be a strong gravitational-wave source for the Laser Interferometer Space Antenna (LISA). We…
The Laser Interferometer Space Antenna: Unveiling the Millihertz Gravitational Wave Sky
John Baker, Jillian Bellovary, Peter L. Bender +39
The first terrestrial gravitational wave interferometers have dramatically underscored the scientific value of observing the Universe through an entirely different window, and of f…
Space Based Gravitational Wave Astronomy Beyond LISA
John Baker, Simon F. Barke, Peter L. Bender +20
The Laser Interferometer Space Antenna (LISA) will open three decades of gravitational wave (GW) spectrum between 0.1 and 100 mHz, the mHz band. This band is expected to be the ric…