activity
20082026
most citedFrequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era

1.1k citations · 7.4k across the 52 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

gr-qc2024★ 6 cited

Revisiting the relationship of black-hole kicks and multipole asymmetries

Jannik Mielke, Shrobana Ghosh, Angela Borchers +1

Precession in black-hole binaries is caused by a misalignment between the total spin and the orbital angular momentum. The gravitational-wave emission of such systems is anisotropi…

gr-qc2024★ 1 cited

Compact binary coalescences: gravitational-wave astronomy with ground-based detectors

K. Chatziioannou, T. Dent, M. Fishbach +4

The era of gravitational wave astronomy began in 2015 with the observation of the signal from the merger of two black holes by the LIGO detectors; by 2021, almost 100 more such tra…

gr-qc2024★ 6 cited

Observability of spin precession in the presence of a black-hole remnant kick

Angela Borchers, Frank Ohme, Jannik Mielke +1

Remnants of binary black-hole mergers can gain significant recoil or kick velocities when the binaries are asymmetric. The kick is the consequence of anisotropic emission of gravit…

gr-qc2024★ 1 cited

Modern tools for computing neutron star properties

Wolfgang Kastaun, Frank Ohme

Astronomical observations place increasingly tighter and more diverse constraints on the properties of neutron stars (NS). Examples include observations of radio or gamma-ray pulsa…

astro-ph.IM2024★ 7 cited

Convolutional Neural Networks for signal detection in real LIGO data

Ondřej Zelenka, Bernd Brügmann, Frank Ohme

Searching the data of gravitational-wave detectors for signals from compact binary mergers is a computationally demanding task. Recently, machine learning algorithms have been prop…