Noise angular power spectrum of gravitational wave background experiments

We construct a model for the angular power spectrum of the instrumental noise in interferometer networks mapping gravitational wave backgrounds (GWBs) as a function of detector noise properties, network configuration, and scan strategy. We use the model to calculate the noise power spectrum for curr...

תיאור מלא

מידע ביבליוגרפי
Main Authors: Alonso, D, Contaldi, CR, Cusin, G, Ferreira, PG, Renzini, AI
פורמט: Journal article
שפה:English
יצא לאור: American Physical Society 2020