activity
20232026
most citedThe Science of the Einstein Telescope

97 citations · 235 across the 16 of their papers we have counts for

collaborators

16 papers

gr-qc2026

Shape of U: Measuring the Curvature of the Universe with Gravitational Waves

Arindam Sharma, Ish Gupta, Anuradha Gupta

Gravitational waves (GWs) from compact binary mergers are standard sirens that can measure distances across the Universe without external calibrators. When an electromagnetic count…

astro-ph.HE2026

Distinguishing Kilonovae from Binary Neutron Star and Neutron Star-Black Hole Mergers

Ish Gupta, Yugesh Bhoge, Rahul Kashyap +1

Kilonovae (KNe) are most informative when accompanied by a gravitational-wave signal, which can help identify the source as a binary neutron star (BNS) or a neutron star-black hole…

astro-ph.CO2025

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-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

astro-ph.HE2025

Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors

Sanika Khadkikar, Ish Gupta, Rahul Kashyap +3

Gravitational waves from merging binary neutron stars carry characteristic information about their astrophysical properties, including masses and tidal deformabilities, that are ne…

gr-qc2025

Optimizing Bayesian model selection for equation of state of cold neutron stars

Rahul Kashyap, Ish Gupta, Arnab Dhani +2

We introduce a computational framework, Bayesian Evidence calculation fOr Model Selection (BEOMS) to evaluate multiple Bayesian model selection methods in the context of determinin…

gr-qc2024★ 9 cited

The Critical Role of LIGO-India in the Era of Next-Generation Observatories

Shiksha Pandey, Ish Gupta, Koustav Chandra +1

We examine the role of LIGO-India in facilitating multi-messenger astronomy in the era of next generation observatories. A network with two L-shaped Cosmic Explorer (CE) detectors…

gr-qc2024

Foreground signals minimally affect inference of high-mass binary black holes in next generation gravitational-wave detectors

Ish Gupta, Koustav Chandra, B. S. Sathyaprakash

Next-generation gravitational-wave observatories are expected to detect over a thousand compact binary coalescence signals daily, with some lasting from minutes to hours. Consequen…

astro-ph.HE2024★ 1 cited

Constraining possible -ray burst emission from GW230529 using Swift-BAT and Fermi-GBM

Samuele Ronchini, Suman Bala, Joshua Wood +35

GW230529 is the first compact binary coalescence detected by the LIGO-Virgo-KAGRA collaboration with at least one component mass confidently in the lower mass-gap, corresponding to…

astro-ph.HE2024★ 2 cited

Everything everywhere all at once: A detailed study of GW230529

Koustav Chandra, Ish Gupta, Rossella Gamba +5

This study investigates the origins of GW230529, delving into its formation from massive stars within isolated binary systems. Utilizing population synthesis models, we present com…

gr-qc2024★ 56 cited

Possible Causes of False General Relativity Violations in Gravitational Wave Observations

Anuradha Gupta, K. G. Arun, Enrico Barausse +40

General relativity (GR) has proven to be a highly successful theory of gravity since its inception. The theory has thrivingly passed numerous experimental tests, predominantly in w…

astro-ph.HE2024★ 3 cited

Multi-messenger Astrophysics of Black Holes and Neutron Stars as Probed by Ground-based Gravitational Wave Detectors: From Present to Future

Alessandra Corsi, Lisa Barsotti, Emanuele Berti +12

The ground-based gravitational wave (GW) detectors LIGO and Virgo have enabled the birth of multi-messenger GW astronomy via the detection of GWs from merging stellar-mass black ho…

astro-ph.HE2024★ 6 cited

Inferring small neutron star spins with neutron star-black hole mergers

Ish Gupta

The precise measurement of neutron star (NS) spins can provide important insight into the formation and evolution of compact binaries containing NS. While traditional methods of NS…

gr-qc2024★ 33 cited

Cosmography with next-generation gravitational wave detectors

Hsin-Yu Chen, Jose María Ezquiaga, Ish Gupta

Advancements in cosmology through next-generation ground-based gravitational wave observatories will bring in a paradigm shift. We explore the pivotal role that gravitational-wave…

gr-qc2023★ 26 cited

Detectability of QCD phase transitions in binary neutron star mergers: Bayesian inference with the next generation gravitational wave detectors

Aviral Prakash, Ish Gupta, Matteo Breschi +5

We study the detectability of postmerger QCD phase transitions in neutron star binaries with next-generation gravitational-wave detectors Cosmic Explorer and Einstein Telescope. We…

gr-qc2023★ 2 cited

The Accuracy of Neutron Star Radius Measurement with the Next Generation of Terrestrial Gravitational-Wave Observatories

Rachael Huxford, Rahul Kashyap, Ssohrab Borhanian +3

In this paper, we explore the prospect for improving the measurement accuracy of masses and radii of neutron stars. We consider imminent and long-term upgrades of the Laser Interfe…