402 citations · 2k across the 41 of their papers we have counts for
44 papers
Align Before You Combine: Reference Space Calibration for Supervision Without Ground Truth
Jackson Eshbaugh, Jorge Silveyra
We introduce a calibration-first framework that produces supervision scores without access to ground-truth labels or a shared annotation space. Our framework aligns subset-specific…
Gravitational-wave dark sirens as astrophysical probes: inferring galaxy-merger relations and identifying individual hosts
Alessandro Agapito, Michele Mancarella
Gravitational-wave (GW) ``dark siren'' techniques, namely the statistical association of GW events with a galaxy catalog, have so far been used as a cosmological tool. Yet this ass…
Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope
Ulyana Dupletsa, Francesco Iacovelli, Mikhail Korobko +23
We investigate the relationship between instrumental requirements and the scientific performance of the Einstein Telescope (ET), a third-generation (3G) gravitational-wave (GW) obs…
Gravitational-wave constraints on are robust to putative redshift evolution in the binary black hole mass spectrum at current sensitivity
Alessandro Agapito, Viola De Renzis, Michele Mancarella
Spectral-siren cosmology constrains the Hubble constant using gravitational-wave observations of compact-binary coalescences. The method combines luminosity distances inferre…
Cosmology and modified GW propagation from the BNS mass function at third-generation detector networks
Dounia Nanadoumgar-Lacroze, Niccolò Muttoni, Michele Maggiore +1
We perform forecasts for the Hubble parameter H_0 and for the parameter Xi_0 that describes modified gravitational-wave propagation, using information from the binary neutron star…
Pushing spectral siren cosmology into the third-generation era: a blinded mock data challenge
Matteo Tagliazucchi, Michele Moresco, Alessandro Agapito +6
Gravitational wave (GW) spectral sirens offer a promising method for measuring cosmological parameters using GW data only - without relying on external redshift information such as…
Probing Cosmic Expansion and Early Universe with Einstein Telescope
Angelo Ricciardone, Mairi Sakellariadou, Archisman Ghosh +52
Over the next two decades, gravitational-wave (GW) observations are expected to evolve from a discovery-driven endeavour into a precision tool for astrophysics, cosmology, and fund…
Impact of facility timing and coordination for next-generation gravitational-wave detectors
Ssohrab Borhanian, Arianna Renzini, Philippa S. Cole +3
While the Einstein Telescope and Cosmic Explorer proposals for next-generation, ground-based detectors promise vastly improved sensitivities to gravitational-wave signals, only joi…
Fusing Bluetooth With Pedestrian Dead Reckoning: A Floor Plan-Assisted Positioning Approach
Wenxuan Pan, Yang Yang, Mingzhe Chen +3
Floor plans can provide valuable prior information that helps enhance the accuracy of indoor positioning systems. However, existing research typically faces challenges in efficient…
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…
Multi-messenger observations in the Einstein Telescope era: binary neutron star and black hole - neutron star mergers
Alberto Colombo, Om Sharan Salafia, Giancarlo Ghirlanda +6
The Einstein Telescope (ET), a proposed next-generation gravitational wave (GW) observatory, will expand the reach of GW astronomy of stellar-mass compact object binaries to unprec…
Sampling the full hierarchical population posterior distribution in gravitational-wave astronomy
Michele Mancarella, Davide Gerosa
We present a full sampling of the hierarchical population posterior distribution of merging black holes using current gravitational-wave data. We directly tackle the most relevant…
Confusion noise from astrophysical backgrounds at third-generation gravitational-wave detector networks
Enis Belgacem, Francesco Iacovelli, Michele Maggiore +2
At third-generation (3G) gravitational-wave detector networks, compact binaries coalescences produce a ``confusion noise'' due to unresolved sources and to the error in the reconst…
Comparison of global networks of third-generation gravitational-wave detectors
Michele Maggiore, Francesco Iacovelli, Enis Belgacem +2
We study the performances of a world-wide network made by a European third-generation gravitational-wave (GW) detector, together with a 40km Cosmic Explorer detector in the US, con…
The spectral density of astrophysical stochastic backgrounds
Enis Belgacem, Francesco Iacovelli, Michele Maggiore +2
We provide a detailed derivation of the spectral density of the stochastic background generated by the superposition of coalescing compact binaries. We show how the expression ofte…
Forecasting the population properties of merging black holes
Viola De Renzis, Francesco Iacovelli, Davide Gerosa +2
Third-generation gravitational-wave detectors will observe up to millions of merging binary black holes. With such a vast dataset, stacking events into population analyses will arg…
Combining underground and on-surface third-generation gravitational-wave interferometers
Francesco Iacovelli, Enis Belgacem, Michele Maggiore +2
Recently, detailed studies have been made to compare the performance of the European next generation GW observatory Einstein Telescope (ET) in a single-site triangular configuratio…
Accurate Standard Siren Cosmology with Joint Gravitational-Wave and -Ray Burst Observations
Michele Mancarella, Francesco Iacovelli, Stefano Foffa +2
Joint gravitational-wave (GW) and -ray burst (GRB) observations are among the best prospects for standard siren cosmology. However, the strong selection effect for the coinciden…
The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
Parameswaran Ajith, Pau Amaro Seoane, Manuel Arca Sedda +83
The Lunar Gravitational-wave Antenna (LGWA) is a proposed array of next-generation inertial sensors to monitor the response of the Moon to gravitational waves (GWs). Given the size…
Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
Nicola Borghi, Michele Mancarella, Michele Moresco +4
With the growing number of gravitational-wave detections and the advent of large galaxy redshift surveys, a new era in cosmology is unfolding. This study explores the synergies bet…
Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy
Sveva Castello, Michele Mancarella, Nastassia Grimm +3
Upcoming galaxy surveys provide the necessary sensitivity to measure gravitational redshift, a general relativistic effect that generates a dipole in galaxy clustering data when co…
Multi-messenger prospects for black hole - neutron star mergers in the O4 and O5 runs
Alberto Colombo, Raphaël Duqué, Om Sharan Salafia +13
The existence of merging black hole-neutron star (BHNS) binaries has been ascertained through the observation of their gravitational wave (GW) signals. However, to date, no definit…
Nuclear physics constraints from binary neutron star mergers in the Einstein Telescope era
Francesco Iacovelli, Michele Mancarella, Chiranjib Mondal +5
The next generation of ground-based gravitational-wave detectors, Einstein Telescope (ET) and Cosmic Explorer (CE), present a unique opportunity to put constraints on dense matter,…
Searching for Primordial Black Holes with the Einstein Telescope: impact of design and systematics
G. Franciolini, F. Iacovelli, M. Mancarella +3
Primordial Black Holes (PBHs) have recently attracted much attention as they may explain some of the LIGO/Virgo/KAGRA observations and significantly contribute to the dark matter i…