A data analysis technique for detecting a stochastic background of gravitational radiation

Joseph D. Romano

doi:10.1117/12.459018

26 February 2003 A data analysis technique for detecting a stochastic background of gravitational radiation

Joseph D. Romano

Proceedings Volume 4856, Gravitational-Wave Detection; (2003) https://doi.org/10.1117/12.459018
Event: Astronomical Telescopes and Instrumentation, 2002, Waikoloa, Hawai'i, United States

Abstract

We present a data analysis technique for detecting a stochastic background of gravitational radiation. Current observational constraints and upper limits on the stochastic background signal strength, and methods for dealing with cross-correlated noise are also discussed.

Citation Download Citation

Joseph D. Romano "A data analysis technique for detecting a stochastic background of gravitational radiation", Proc. SPIE 4856, Gravitational-Wave Detection, (26 February 2003); https://doi.org/10.1117/12.459018

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE

Includes PDF, HTML & Video, when available