activity
20232026
most citedCriteria for identifying and evaluating locations that could potentially host the Cosmic Explorer observatories

1 citations · 1 across the 5 of their papers we have counts for

collaborators

6 papers

quant-ph2026

Observing and evading quantum back-action on a kilogram-scale oscillator

Begüm Kabagöz, Eric Oelker, Dhruva Ganapathy +203

Continuous quantum displacement measurements are fundamentally limited by a trade-off between readout imprecision and measurement back-action, constrained by the Heisenberg uncerta…

physics.ins-det2026

Identifying Cost-Favorable Locations for Cosmic Explorer

Laurence Datrier, Geoffrey Lovelace, Tooba Ansar +19

Cosmic Explorer (CE) is a proposed next-generation gravitational-wave observatory that aims to extend our gravitational-wave vision to the edge of the observable universe. With a f…

astro-ph.IM2026

Scattered light noise at LIGO Livingston Observatory during O4

Debasmita Nandi, Anamaria Effler, Siddharth Soni +6

Scattered light is one of the most common sources of noise in the LIGO gravitational wave detectors. Light scattering is a highly non-linear process through which motion at low fre…

gr-qc2025

Coherent injection of magnetic noise and its impact on gravitational-wave searches

Kamiel Janssens, Jessica Lawrence, Anamaria Effler +11

Correlated noise sources, particularly magnetic noise, form a risk to future gravitational-wave searches aimed at detecting the gravitational-wave background. Potential noise conta…

physics.ins-det2024★ 1 cited

Criteria for identifying and evaluating locations that could potentially host the Cosmic Explorer observatories

Kathryne J. Daniel, Joshua R. Smith, Stefan Ballmer +19

Cosmic Explorer (CE) is a next-generation ground-based gravitational-wave observatory that is being designed in the 2020s and is envisioned to begin operations in the 2030s togethe…

astro-ph.IM2023

Modeling and Reduction of High Frequency Scatter Noise at LIGO Livingston

Siddharth Soni, Jane Glanzer, Anamaria Effler +4

The sensitivity of aLIGO detectors is adversely affected by the presence of noise caused by light scattering. Low frequency seismic disturbances can create higher frequency scatter…