activity
20062024
most citedLIGO: The Laser Interferometer Gravitational-Wave Observatory

1.2k citations · 2.7k across the 27 of their papers we have counts for

collaborators

28 papers

astro-ph.IM2024

Tilt-to-length coupling in LISA Pathfinder: long-term stability

M Armano, H Audley, J Baird +75

The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular timespans. In this work, we investigate the long-term st…

astro-ph.IM2024★ 12 cited

Precision measurements of the magnetic parameters of LISA Pathfinder test masses

M Armano, H Audley, J Baird +76

A precise characterization of the magnetic properties of LISA Pathfinder free falling test-masses is of special interest for future gravitational wave observatory in space. Magneti…

astro-ph.IM2024★ 13 cited

Magnetic-induced force noise in LISA Pathfinder free-falling test masses

M Armano, H Audley, J Baird +76

LISA Pathfinder was a mission designed to test key technologies required for gravitational wave detection in space. Magnetically driven forces play a key role in the instrument sen…

astro-ph.IM2024★ 37 cited

In-depth analysis of LISA Pathfinder performance results: Time evolution, noise projection, physical models, and implications for LISA

M. Armano, H. Audley, J. Baird +77

We present an in-depth analysis of the LISA Pathfinder differential acceleration performance over the entire course of its science operations, spanning approximately 500 days. We f…

astro-ph.IM2023

NanoNewton electrostatic force actuators for femtoNewton-sensitive measurements: system performance test in the LISA Pathfinder mission

M Armano, H Audley, J Baird +87

Electrostatic force actuation is a key component of the system of geodesic reference test masses (TM) for the LISA orbiting gravitational wave observatory and in particular for per…

astro-ph.IM2023★ 21 cited

Tilt-to-length coupling in LISA Pathfinder: a data analysis

M Armano, H Audley, J Baird +76

We present a study of the tilt-to-length coupling noise during the LISA Pathfinder mission and how it depended on the system's alignment. Tilt-to-length coupling noise is the unwan…

astro-ph.IM2022★ 27 cited

Charging of free-falling test masses in orbit due to cosmic rays: results from LISA Pathfinder

LISA Pathfinder Collaboration, M. Armano, H. Audley +72

A comprehensive summary of the measurements made to characterize test mass charging due to the space environment during the LISA Pathfinder mission is presented. Measurements of th…

astro-ph.IM2022★ 35 cited

Transient acceleration events in LISA Pathfinder data: properties and possible physical origin

LISA Pathfinder Collaboration

We present an in depth analysis of the transient events, or glitches, detected at a rate of about one per day in the differential acceleration data of LISA Pathfinder. We show that…

astro-ph.IM2022★ 3 cited

Cold Atoms in Space: Community Workshop Summary and Proposed Road-Map

Ivan Alonso, Cristiano Alpigiani, Brett Altschul +246

We summarize the discussions at a virtual Community Workshop on Cold Atoms in Space concerning the status of cold atom technologies, the prospective scientific and societal opportu…

astro-ph.IM2020★ 36 cited

Spacecraft and interplanetary contributions to the magnetic environment on-board LISA Pathfinder

M. Armano, H. Audley, J. Baird +79

LISA Pathfinder (LPF) has been a space-based mission designed to test new technologies that will be required for a gravitational wave observatory in space. Magnetically driven forc…

physics.space-ph2019★ 25 cited

LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode

M. Armano, H. Audley, J. Baird +75

We report on the results of the LISA Pathfinder (LPF) free-fall mode experiment, in which the control force needed to compensate the quasistatic differential force acting on two te…

astro-ph.IM2019★ 62 cited

Temperature stability in the sub-milliHertz band with LISA Pathfinder

M. Armano, H. Audley, J. Baird +79

LISA Pathfinder (LPF) was a technology pioneering mission designed to test key technologies required for gravitational wave detection in space. In the low frequency regime (milli-H…

physics.space-ph2019★ 23 cited

Forbush decreases and 2-day GCR flux non-recurrent variations studied with LISA Pathfinder

C. Grimani, M. Armano, H. Audley +82

Non-recurrent short term variations of the galactic cosmic-ray (GCR) flux above 70 MeV n were observed between 2016 February 18 and 2017 July 3 aboard the European Space Age…

astro-ph.IM2019★ 3 cited

LISA Pathfinder

Michele Armano, Heather Audley, Jonathon Baird +75

Since the 2017 Nobel Prize in Physics was awarded for the observation of gravitational waves, it is fair to say that the epoch of gravitational wave astronomy (GWs) has begun. Howe…

astro-ph.IM2018★ 89 cited

Experimental results from the ST7 mission on LISA Pathfinder

G Anderson, J Anderson, M Anderson +145

The Space Technology 7 Disturbance Reduction System (ST7-DRS) is a NASA technology demonstration payload that operated from January 2016 through July of 2017 on the European Space…

physics.ins-det2018★ 65 cited

Precision Charge Control for Isolated Free-Falling Test Masses: LISA Pathfinder Results

M. Armano, H. Audley, J. Baird +82

The LISA Pathfinder charge management device was responsible for neutralising the cosmic ray induced electric charge that inevitably accumulated on the free-falling test masses at…

astro-ph.IM2018★ 42 cited

Calibrating the system dynamics of LISA Pathfinder

M. Armano, H. Audley, J. Baird +75

LISA Pathfinder (LPF) was a European Space Agency mission with the aim to test key technologies for future space-borne gravitational-wave observatories like LISA. The main scientif…

physics.space-ph2018★ 40 cited

Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a Forbush decrease with LISA Pathfinder

M. Armano, H. Audley, J. Baird +82

Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated by the solar activity, the solar polarity and structures of solar and interplanetary origin…

astro-ph.HE2012★ 48 cited

A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007

The ANTARES Collaboration, the LIGO Scientific Collaboration, the Virgo Collaboration +959

We present the results of the first search for gravitational wave bursts associated with high energy neutrinos. Together, these messengers could reveal new, hidden sources that are…

astro-ph.HE2012★ 127 cited

Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3

The LIGO Scientific Collaboration, Virgo Collaboration, J. Abadie +807

We present the results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments in 2009-2010, dur…

astro-ph.HE2012★ 78 cited

Implications For The Origin Of GRB 051103 From LIGO Observations

The LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +568

We present the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically det…

astro-ph.CO2011★ 110 cited

Directional limits on persistent gravitational waves using LIGO S5 science data

J. Abadie, B. P. Abbott, R. Abbott +712

The gravitational-wave (GW) sky may include nearby pointlike sources as well as astrophysical and cosmological stochastic backgrounds. Since the relative strength and angular distr…

astro-ph.HE2011★ 167 cited

Beating the spin-down limit on gravitational wave emission from the Vela pulsar

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +747

We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been…

gr-qc2010★ 3 cited

A search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar

The LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +499

The physical mechanisms responsible for pulsar timing glitches are thought to excite quasi-normal mode oscillations in their parent neutron star that couple to gravitational wave e…