Citation

BibTex format

@article{Alonso:2020:10.1103/PhysRevD.101.124048,
author = {Alonso, D and Contaldi, CR and Cusin, G and Ferreira, PG and Renzini, A},
doi = {10.1103/PhysRevD.101.124048},
journal = {Physical Review D: Particles, Fields, Gravitation and Cosmology},
pages = {124048  1--124048  17},
title = {Noise angular power spectrum of gravitational wave background experiments},
url = {http://dx.doi.org/10.1103/PhysRevD.101.124048},
volume = {101},
year = {2020}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - 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 current and future ground-based experiments, as well as for planned space missions. We present our results in a language similar to that used in cosmic microwave background and intensity mapping experiments, and connect the formalism with the sensitivity curves that are common lore in GWB analyses.
AU  - Alonso,D
AU  - Contaldi,CR
AU  - Cusin,G
AU  - Ferreira,PG
AU  - Renzini,A
DO  - 10.1103/PhysRevD.101.124048
EP  - 1
PY  - 2020///
SN  - 1550-2368
SP  - 124048
TI  - Noise angular power spectrum of gravitational wave background experiments
T2  - Physical Review D: Particles, Fields, Gravitation and Cosmology
UR  - http://dx.doi.org/10.1103/PhysRevD.101.124048
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000541705000017&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.101.124048
VL  - 101
ER  -
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