239 citations · 985 across the 21 of their papers we have counts for
21 papers
Measuring neutron-star distances and properties with gravitational-wave parallax
Magdalena Sieniawska, David Ian Jones, Andrew Lawrence Miller
Gravitational-wave astronomy allows us to study objects and events invisible to electromagnetic waves. So far, only signals triggered by coalescing binaries have been detected. How…
Probing Ensemble Properties of Vortex-avalanche Pulsar Glitches with a Stochastic Gravitational-Wave Background Search
Federico De Lillo, Jishnu Suresh, Antoine Depasse +3
A stochastic gravitational-wave background (SGWB) is expected to be produced by the superposition of individually undetectable, unresolved gravitational-wave (GW) signals from cosm…
Virgo Detector Characterization and Data Quality: tools
F. Acernese, M. Agathos, A. Ain +491
Detector characterization and data quality studies -- collectively referred to as {\em DetChar} activities in this article -- are paramount to the scientific exploitation of the jo…
Virgo Detector Characterization and Data Quality: results from the O3 run
F. Acernese, M. Agathos, A. Ain +491
The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave (GW) signals in the past few years, alongside the two Adv…
Assessing the impact of non-Gaussian noise on convolutional neural networks that search for continuous gravitational waves
Takahiro S. Yamamoto, Andrew L. Miller, Magdalena Sieniawska +1
We present a convolutional neural network that is capable of searching for continuous gravitational waves, quasi-monochromatic, persistent signals arising from asymmetrically rotat…
Virgo Detector Characterization and Data Quality during the O3 run
F. Acernese, M. Agathos, A. Ain +491
The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave signals in the past few years, alongside the two LIGO ins…
The Virgo O3 run and the impact of the environment
F. Acernese, M. Agathos, A. Ain +486
Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient…
Gravitational-wave searches in the era of Advanced LIGO and Virgo
Sarah Caudill, Shivaraj Kandhasamy, Claudia Lazzaro +3
The field of gravitational-wave astronomy has been opened up by gravitational-wave observations made with interferometric detectors. This review surveys the current state-of-the-ar…
Gravitational waves from spinning neutron stars as not-quite-standard sirens
M. Sieniawska, D. I. Jones
As is well known, gravitational wave detections of coalescing binaries are standard sirens, allowing a measurement of source distance by gravitational wave means alone. In this pap…
Detectability of continuous gravitational waves from isolated neutron stars in the Milky Way: the population synthesis approach
Marek Cieślar, Tomasz Bulik, Małgorzata Curyło +3
Aims. We estimate the number of pulsars, detectable as continuous gravitational wave sources with the current and future gravitational-wave detectors, assuming a simple phenomenolo…
All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems
The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1369
Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter…
Probing elastic quark phases in hybrid stars with radius measurements
Jonas P. Pereira, Michał Bejger, Lucas Tonetto +4
The internal composition of neutron stars is currently largely unknown. Due to the possibility of phase transitions in quantum chromodynamics, stars could be hybrid and have quark…
Continuous gravitational waves from neutron stars: current status and prospects
Magdalena Sieniawska, Michał Bejger
Gravitational waves astronomy allows us to study objects and events invisible in electromagnetic waves. It is crucial to validate the theories and models of the most mysterious and…
All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1186
We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gra…
Follow-up procedure for gravitational wave searches from isolated neutron stars using the time-domain -statistic method
Magdalena Sieniawska, Michał Bejger, Andrzej Królak
Among promising sources of gravitational waves are long-lived nearly periodic signals produced by rotating, asymmetric neutron stars. Depending on the astrophysical scenario, the s…
All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1130
We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis,…
Followup procedure in time-domain F-statistic searches for continuous gravitational waves
Magdalena Sieniawska, Michał Bejger, Paweł Ciecieląg +1
Potentially interesting gravitational-wave candidates (outliers) from the blind all-sky searches have to be confirmed or rejected by studying their origin and precisely estimating…
Tidal deformability and other global parameters of compact stars with strong phase transitions
Magdalena Sieniawska, Władysław Turczański, Michał Bejger +1
Using parametric equations of state (relativistic polytropes and a simple quark bag model) to model dense-matter phase transitions, we study global, measurable astrophysical parame…
A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
M. Fishbach, R. Gray, I. Magaña Hernandez +316
We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817.…
Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2
Virgo Collaboration, F. Acernese, T. Adams +281
In August 2017, Advanced Virgo joined Advanced LIGO for the end of the O2 run, leading to the first gravitational waves detections with the three-detector network. This paper descr…
Estimating the EOS from the measurement of NS radii with 5% accuracy
M. Sieniawska, M. Bejger, B. Haskell
Observations of heavy () neutron stars in addition to the recent measurement of tidal deformability from the binary neutron-star merger GW170817, place interest…