33 citations · 145 across the 14 of their papers we have counts for
14 papers
Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers
Joan Llobera-Querol, Eleanor Hamilton, Neha Singh +8
Determining the astrophysical origin of binary black holes and whether merger remnants are retained in their birth environments is essential for understanding hierarchical mergers…
Estimating the binary neutron star merger rate density evolution with Einstein Telescope
Neha Singh, Tomasz Bulik, Aleksandra Olejak
The Einstein Telescope (ET) is a proposed third-generation, wide-band gravitational wave (GW) detector which will have an improved detection sensitivity in low frequencies, leading…
What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
Justin Janquart, David Keitel, Rico K. L. Lo +26
On the 29th of May 2023, the LIGO-Virgo-KAGRA Collaboration observed a compact binary coalescence event consistent with a neutron star-black hole merger, though the heavier object…
ler: LVK (LIGO-Virgo-KAGRA collaboration) event (compact-binary mergers) rate calculator and simulator
Hemantakumar Phurailatpam, Anupreeta More, Harsh Narola +6
ler is a Python package for simulating compact-binary gravitational-wave populations and estimating detectable event rates for current and future LIGO-Virgo-KAGRA detector networks…
Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
Andrew L. Miller, Neha Singh, Cristiano Palomba
Next-generation gravitational-wave detectors will provide unprecedented sensitivity to inspiraling binary neutron stars and black holes, enabling detections at the peak of star for…
An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the Third Observing Run of Advanced LIGO and Advanced Virgo
Marek J. Szczepańczyk, Yanyan Zheng, Javier M. Antelis +35
We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed optically within 30 Mpc during the third observing run of A…
Reconstructing the star formation rate for compact binary populations with the Einstein telescope
Neha Singh, Tomasz Bulik, Krzysztof Belczynski +2
The Einstein Telescope (ET) is a proposed third-generation, wide-band gravitational wave (GW) detector. Given its improved detection sensitivity in comparison to the second-generat…
Exploring compact binary populations with the Einstein Telescope
Neha Singh, Tomasz Bulik, Krzysztof Belczynski +1
The Einstein Telescope (ET), a wide-band, future third generation gravitational wave detector, is expected to have detection rates of binary black hole (BBH) det…
Constraining parameters of low mass merging compact binary systems with Einstein Telescope alone
Neha Singh, Tomasz Bulik
The Einstein Telescope (ET), a future third-generation gravitational wave detector will have detection sensitivity for gravitational wave signals down to 1 Hz. This improved low-fr…
Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era
Marek Szczepanczyk, Javier Antelis, Michael Benjamin +17
We performed a detailed analysis of the detectability of a wide range of gravitational waves derived from core-collapse supernova simulations using gravitational-wave detector nois…
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…
Constraining parameters of coalescing stellar mass binary black hole systems with the Einstein Telescope alone
Neha Singh, Tomasz Bulik
The Einstein Telescope (ET) is the future third generation gravitational wave detector consisting of three independent interferometers arranged in a triangular configuration, with…
Seismic array measurements at Virgo's West End Building for the configuration of a Newtonian-noise cancellation system
M. C. Tringali, T. Bulik, J. Harms +9
Terrestrial gravity fluctuations produce so-called Newtonian noise (NN) which is expected to limit the low frequency sensitivity of existing gravitational-waves (GW) detectors LIGO…
Asymmetric accretion and thermal `mountains' in magnetized neutron star crusts
Neha Singh, Brynmor Haskell, Dipanjan Mukherjee +1
Accreting neutron stars are one of the main targets for continuous gravitational wave searches, as asymmetric accretion may lead to quadrupolar deformations, or `mountains', on the…