papers

Publications (17)

astro-ph.CO2023

A novel approach to infer population and cosmological properties with gravitational waves standard sirens and galaxy surveys

Simone Mastrogiovanni, Danny Laghi, Rachel Gray +7

Gravitational wave (GW) sources at cosmological distances can be used to probe the expansion rate of the Universe. GWs directly provide a distance estimation of the source but no d…

astro-ph.CO2026

The impact of strong lensing on Hubble constant measurements with gravitational-wave dark sirens

Eungwang Seo, Kyungmin Kim, Zhuotao Li +3

The disagreement between early and late Universe electromagnetic measurements of the Hubble constant, , known as the Hubble tension, highlights the need for independent and co…

astro-ph.CO2023

Constraints on coasting cosmological models from gravitational-wave standard sirens

Peter Raffai, Mária Pálfi, Gergely Dálya +1

We present the first test of coasting cosmological models with gravitational-wave standard sirens observed in the first three observing runs of the LIGO-Virgo-KAGRA detector networ…

gr-qc2020

Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge

Rachel Gray, Ignacio Magaña Hernandez, Hong Qi +12

The observation of binary neutron star merger GW170817, along with its optical counterpart, provided the first constraint on the Hubble constant using gravitational wave stan…

astro-ph.IM2020

Characterization of systematic error in Advanced LIGO calibration

Ling Sun, Evan Goetz, Jeffrey S. Kissel +23

The raw outputs of the detectors within the Advanced Laser Interferometer Gravitational-Wave Observatory need to be calibrated in order to produce the estimate of the dimensionless…

physics.ins-det2021

Point absorbers in Advanced LIGO

Aidan F. Brooks, Gabriele Vajente, Hiro Yamamoto +198

Small, highly absorbing points are randomly present on the surfaces of the main interferometer optics in Advanced LIGO. The resulting nano-meter scale thermo-elastic deformations a…

gr-qc2023

Testing the nature of gravitational wave propagation using dark sirens and galaxy catalogues

Anson Chen, Rachel Gray, Tessa Baker

The dark sirens method enables us to use gravitational wave events without electromagnetic counterparts as tools for cosmology and tests of gravity. Furthermore, the dark sirens an…

gr-qc2023

Impact of modelling galaxy redshift uncertainties on the gravitational-wave dark standard siren measurement of the Hubble constant

Cezary Turski, Maciej Bilicki, Gergely Dálya +2

Gravitational wave science is a new and rapidly expanding field of observational astronomy. Multimessenger observations of the binary neutron star merger GW170817 have provided som…

astro-ph.CO2023

ICAROGW: A python package for inference of astrophysical population properties of noisy, heterogeneous and incomplete observations

Simone Mastrogiovanni, Grégoire Pierra, Stéphane Perriès +6

We present icarogw 2.0, a pure CPU/GPU python code developed to infer astrophysical and cosmological population properties of noisy, heterogeneous, and incomplete observations. ica…

astro-ph.CO2025

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum

Aman Agarwal, Ulyana Dupletsa, Konstantin Leyde +18

Gravitational Wave (GW) sources are standard sirens that provide an independent way to map the cosmic expansion history by combining with an independent redshift measurement either…

astro-ph.CO2026

Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue

Isaac McMahon, Danny Laghi, Marcelle Soares-Santos +9

Gravitational wave (GW) standard sirens enable independent measurements of the Hubble constant . In the absence of electromagnetic counterparts, the 'dark siren' method statis…

astro-ph.CO2025

Using gravitational wave dark sirens to choose between host galaxy weighting models

Zhuotao Li, Rachel Gray, Ik Siong Heng

Binary black hole (BBH) mergers,, an important source of gravitational-waves(GWs), are assumed to be hosted in galaxies. The probability of a galaxy to host a BBH is related to its…

astro-ph.CO2026

Scalable Dark Siren Cosmology with gwcosmo: GPU Acceleration, Validation and Systematics

Alexander Papadopoulos, Christian E. A. Chapman-Bird, Rachel Gray +2

As the number of confident gravitational-wave detections grows, population-level hierarchical analyses face increasing computational costs. Dark-siren cosmological inference integr…

astro-ph.CO2023

Joint cosmological and gravitational-wave population inference using dark sirens and galaxy catalogues

Rachel Gray, Freija Beirnaert, Christos Karathanasis +11

In the absence of numerous gravitational-wave detections with confirmed electromagnetic counterparts, the "dark siren" method has emerged as a leading technique of gravitational-wa…

astro-ph.CO2022

A Pixelated Approach to Galaxy Catalogue Incompleteness: Improving the Dark Siren Measurement of the Hubble Constant

Rachel Gray, Chris Messenger, John Veitch

The use of gravitational wave standard sirens for cosmological analyses is becoming well known, with particular interest in measuring the Hubble constant, , and in shedding li…

astro-ph.CO2026

Golden and Silver Dark Sirens for precise H0 measurement with HETDEX

Yixuan Dang, Ish Gupta, Robin Ciardullo +12

Gravitational waves (GWs) from compact binary coalescences are standard sirens that provide a direct measure of the source's luminosity distance, enabling an independent measuremen…

gr-qc2022

The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology

Jonathan R. Gair, Archisman Ghosh, Rachel Gray +28

We outline the ``dark siren'' galaxy catalog method for cosmological inference using gravitational wave (GW) standard sirens, clarifying some common misconceptions in the implement…