activity
20212026
most citedLIGO Detector Characterization in the first half of the fourth Observing run

60 citations · 162 across the 14 of their papers we have counts for

collaborators

15 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…

astro-ph.IM2026

LIGO Detector Characterization in the Second and Third Parts of the Fourth Observing Run

J. Glanzer, A. F. Helmling-Cornell, A. Calafat +244

LIGO detector characterization efforts enabled the confident detection of gravitational waves from hundreds of compact binary coalescences during the fourth observing run. Reliable…

astro-ph.IM2026

Narrow spectral artifact investigation and mitigation in LIGO data from the fourth LIGO-Virgo-KAGRA observing run

E. Goetz, A. Neunzert, A. M. Knee +258

We present efforts to identify, characterize, and mitigate narrow spectral artifacts in LIGO detector data during the fourth LIGO-Virgo-KAGRA observing run. Narrow spectral artifac…

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.IM2025★ 9 cited

Improving cosmological reach of a gravitational wave observatory using Deep Loop Shaping

Jonas Buchli, Brendan Tracey, Tomislav Andric +28

Improved low-frequency sensitivity of gravitational wave observatories would unlock study of intermediate-mass black hole mergers, binary black hole eccentricity, and provide early…

physics.ins-det2024★ 1 cited

Demonstration of the minimal coupling of horizontal accelerations to rotations in a torsion balance suspended from three wires

Amit Singh Ubhi, Clive C. Speake, Emilia Chick +1

The Cavendish torsion balance is the instrument of choice for measuring weak forces, such as gravity. Although torsion balances have extremely high sensitivity for measuring forces…

astro-ph.IM2024★ 60 cited

LIGO Detector Characterization in the first half of the fourth Observing run

S. Soni, B. K. Berger, D. Davis +232

Progress in gravitational-wave astronomy depends upon having sensitive detectors with good data quality. Since the end of the LIGO-Virgo-KAGRA third Observing run in March 2020, de…

physics.ins-det2024

Sensitivity and control of a 6-axis fused-silica seismometer

Jiri Smetana, Amit Singh Ubhi, Emilia Chick +12

We present a pair of seismometers capable of measurement in all six axes of rigid motion. The vacuum-compatible devices implement compact interferometric displacement sensors to su…

physics.ins-det2023

Design and sensitivity of a 6-axis seismometer for gravitational wave observatories

Leonid Prokhorov, Sam Cooper, Amit Singh Ubhi +13

We present the design, control system, and noise analysis of a 6-axis seismometer comprising a mass suspended by a single fused silica fibre. We utilise custom-made, compact Michel…

astro-ph.IM2022★ 8 cited

Sensors and Actuators for the Advanced LIGO+ Upgrade

S J Cooper, C M Mow-Lowry, D Hoyland +6

As part of the Advanced LIGO+ (A+) project we have developed, produced, and characterised sensors and electronics to interrogate new optical suspensions. The central element is a d…

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.IM2022★ 3 cited

Cryogenic optical shadow sensors for future gravitational wave detectors

Amit Singh Ubhi, John Bryant, David Hoyland +1

Displacement sensors have a variety of applications within gravitational wave detectors. The seismic isolation chain of the LIGO core optics utilises optical shadow sensors for the…

physics.ins-det2022★ 39 cited

Compact Michelson interferometers with subpicometer sensitivity

Jiri Smetana, Rebecca Walters, Sophie Bauchinger +11

The network of interferometric gravitational-wave observatories has successfully detected tens of astrophysical signals since 2015. In this paper, we experimentally investigate com…

physics.ins-det2021★ 14 cited

A six degree-of-freedom fused silica seismometer: Design and tests of a metal prototype

Amit Singh Ubhi, Jiri Smetana, Teng Zhang +6

Ground vibrations couple to the longitudinal and angular motion of the aLIGO test masses and limit the observatory sensitivity below 30\,Hz. Novel inertial sensors have the potenti…

quant-ph2021★ 12 cited

Enhancing interferometer sensitivity without sacrificing bandwidth and stability: beyond single-mode and resolved-sideband approximation

Xiang Li, Jiri Smetana, Amit Singh Ubhi +5

Quantum noise limits the sensitivity of precision measurement devices, such as laser interferometer gravitational-wave observatories and axion detectors. In the shot-noise-limited…