- Home
- Search Results
- Page 1 of 1
Search for: All records
-
Total Resources1
- Resource Type
-
10
- Availability
-
10
- Author / Contributor
- Filter by Author / Creator
-
-
Abbott, B. P. (1)
-
Abbott, R. (1)
-
Abbott, T. D. (1)
-
Abraham, S. (1)
-
Acernese, F. (1)
-
Ackley, K. (1)
-
Adams, C. (1)
-
Adya, V. B. (1)
-
Affeldt, C. (1)
-
Agathos, M. (1)
-
Agatsuma, K. (1)
-
Aggarwal, N. (1)
-
Aguiar, O. D. (1)
-
Aiello, L. (1)
-
Ain, A. (1)
-
Ajith, P. (1)
-
Akutsu, T. (1)
-
Allen, G. (1)
-
Allocca, A. (1)
-
Aloy, M. A. (1)
-
- Filter by Editor
-
-
& Ahn, J. (0)
-
& Bateiha, S. (0)
-
& Ruiz-Arias, P.M. (0)
-
& Spitzer, S. (0)
-
& Spitzer, S.M. (0)
-
A. Beygelzimer (0)
-
A. Ghate, K. Krishnaiyer (0)
-
A. I. Sacristán, J. C. (0)
-
A. Weinberg, D. Moore-Russo (0)
-
A. Weinberger (0)
-
A.I. Sacristán, J.C. Cortés-Zavala (0)
-
ACS (0)
-
AIAA (0)
-
AIAA Propulsion and Energy 2021 (0)
-
AIAA SciTech (0)
-
ASEE Manufacturing Division (0)
-
ASME (0)
-
ASME ICEF (0)
-
ASSOCIATE EDITORS: Bahar, Ivet (Department (0)
-
Aardal, Karen (0)
-
-
Have feedback or suggestions for a way to improve these results?
!
Note: When clicking on a Digital Object Identifier (DOI) number, you will be taken to an external site maintained by the publisher.
Some full text articles may not yet be available without a charge during the embargo (administrative interval).
What is a DOI Number?
Some links on this page may take you to non-federal websites. Their policies may differ from this site.
-
Abstract We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals for the third (O3), fourth (O4) and fifth observing (O5) runs, including the planned upgrades of the Advanced LIGO and Advanced Virgo detectors. We study the capability of the network to determine the sky location of the source for gravitational-wave signals from the inspiral of binary systemsmore »