activity
20072026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 36.7k across the 113 of their papers we have counts for

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Showing astro-ph.IMShow all

11 papers · 1 filter

astro-ph.IM2026

LIGO A: Detector Design and Science Prospects Beyond A+

L. Sun, K. Kuns, B. J. J. Slagmolen +1153

We present the LIGO A detector concept, an upgrade for the LIGO observatories based on room-temperature interferometers beyond the fifth observing run (O5). Building on th…

astro-ph.IM2026

Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz

Amit Singh Ubhi, Lari Koponen, Jiri Smetana +11

Extending the sensitivity of terrestrial gravitational-wave detectors below 20 Hz is a long-standing challenge, limited by ground motion and inertial sensing noise. In this letter,…

astro-ph.IM2023★ 39 cited

Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee

Matthew Evans, Alessandra Corsi, Chaitanya Afle +73

Gravitational-wave astronomy has revolutionized humanity's view of the universe, a revolution driven by observations that no other field can make. This white paper describes an obs…

astro-ph.IM2022★ 16 cited

Active platform stabilisation with a 6D seismometer

Amit Singh Ubhi, Leonid Prokhorov, Sam Cooper +9

We demonstrate the control scheme of an active platform with a six degree of freedom (6D) seismometer. The inertial sensor simultaneously measures translational and tilt degrees of…

astro-ph.IM2020★ 201 cited

A Cryogenic Silicon Interferometer for Gravitational-wave Detection

Rana X Adhikari, Odylio Aguiar, Koji Arai +108

The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravitational wave astronomy, revealing a previously hidden side of the cosmos. To ma…

astro-ph.IM2018★ 109 cited

Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO

J. C. Driggers, S. Vitale, A. P. Lundgren +228

The Advanced LIGO detectors have recently completed their second observation run successfully. The run lasted for approximately 10 months and lead to multiple new discoveries. The…