A stochastic background of gravitational waves could be created by the superposition of a
large number of independent sources. The physical processes occurring at the earliest …

Gravitational-wave detection has been pursued relentlessly for over 40 years. With the
imminent operation of a new generation of laser interferometers, it is expected that …

TianQin is a proposal for a space-borne detector of gravitational waves in the millihertz
frequencies. The experiment relies on a constellation of three drag-free spacecraft orbiting …

We propose a space-based interferometer surveying the gravitational wave (GW) sky in the
milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in …

We present a data analysis methodology for a model-independent reconstruction of the
spectral shape of a stochastic gravitational wave background with LISA. We improve a …

Following the selection of The Gravitational Universe by ESA, and the successful flight of
LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's …

These lecture notes are based on a course given by Mark Hindmarsh at the 24th Saalburg
Summer School 2018 and written up by Marvin L\" uben, Johannes Lumma and Martin …

The Laser Interferometer Space Antenna (LISA) is a planned space-based observatory to
measure gravitational waves in the millihertz frequency band. This frequency band is …

Beyond individually resolvable gravitational wave events such as binary black hole and
binary neutron star mergers, the superposition of many more weak signals coming from a …

Realistic models of the Galactic double white dwarf (DWD) population are crucial for testing
and quantitatively defining the science objectives of the Laser Interferometer Space Antenna …