\texttt{GWBird}: a toolkit for the characterization of the Stochastic Gravitational Wave Background for Ground, Space, and Pulsar Timing Array detectors
Ilaria Caporali, Angelo Ricciardone

TL;DR
GWBird is a comprehensive, user-friendly toolkit that enables detailed characterization of the stochastic gravitational wave background across various detector types and polarization modes, aiding in signal detection and origin analysis.
Contribution
It introduces a unified framework and open-source tool supporting diverse polarization modes and detector types for SGWB analysis, including anisotropic and parity-violating signals.
Findings
Supports all polarization modes (tensor, scalar, vector)
Enables analysis for ground, space, and pulsar timing detectors
Includes functions for circular polarization and anisotropy characterization
Abstract
The detection of the Stochastic Gravitational Wave Background (SGWB) is one of the most challenging tasks for both current and next-generation detectors. Successfully distinguishing the SGWB from instrumental noise and environmental effects requires accurate and flexible analysis tools capable of detecting the signal and determining its origin. In this paper, we introduce a unified framework and a user-friendly tool for SGWB characterization: \texttt{GWBird} (Gravitational Wave Background Inventory of Response functions for Detectors). This code enables the computation of overlap reduction functions (ORFs), power-law integrated sensitivity curves (PLS), angular response functions, and angular PLS (APLS). It supports the full range of gravitational wave polarization modes (tensor, scalar, and vector), allowing for the characterization of both isotropic and anisotropic SGWB components for…
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