152 citations · 314 across the 18 of their papers we have counts for
6 papers · 1 filter
A new model for the continuum spectra of AM CVn binaries and multi-messenger inference with normalizing flows
Nathan Steinle, Samar Safi-Harb, Austin MacMaster +5
Future electromagnetic telescopes, such as , , and an -like mission, along with milli-Hz gravitational-wave (GW) detectors such…
Constraints on neutrino natal kicks from black-hole binary VFTS 243
Alejandro Vigna-Gómez, Reinhold Willcox, Irene Tamborra +8
The recently reported observation of VFTS 243 is the first example of a massive black-hole binary system with negligible binary interaction following black-hole formation. The blac…
Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
Floor S. Broekgaarden, Edo Berger, Simon Stevenson +9
Making the most of the rapidly increasing population of gravitational-wave detections of black hole (BH) and neutron star (NS) mergers requires comparing observations with populati…
Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
Tom Wagg, Floor S. Broekgaarden, Selma E. de Mink +3
Future searches for gravitational waves from space will be sensitive to double compact objects (DCOs) in our Milky Way. We present new simulations of the populations of double blac…
LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors
Tom Wagg, Katelyn Breivik, Selma E. de Mink
We present LEGWORK (LISA Evolution and Gravitational Wave Orbit Kit), an open-source Python package for making predictions about stellar-origin gravitational wave sources and their…
The redshift evolution of the binary black hole merger rate: a weighty matter
L. A. C. van Son, S. E. de Mink, T. Callister +7
Gravitational wave detectors are starting to reveal the redshift evolution of the binary black hole (BBH) merger rate, . We make predictions for $R_{\mathrm{BB…