VizieR Online Data Catalog: Electromagnetic follow-up with LIGO/Virgo (Singer+, 2014)
Abstract
Aasi et al. (2013, arXiv:1304.0670) outline five observing scenarios representing the evolving configuration and capability of the Advanced GW detector array, from the first observing run in 2015, to achieving final design sensitivity in 2019, to adding a fourth detector at design sensitivity by 2022. In this study, we focus on the first two epochs. The first, in 2015, is envisioned as a three-month science run. LIGO Hanford (H) and LIGO Livingston (L) Observatories are operating with an averaged (1.4, 1.4) Mȯ BNS range between 40 and 80 Mpc. The second, in 2016-2017, is a six-month run with H and L operating between 80 and 120 Mpc and the addition of Advanced Virgo (V) with a range between 20 and 60 Mpc.
(4 data files).- Publication:
-
VizieR Online Data Catalog
- Pub Date:
- May 2017
- DOI:
- 10.26093/cds/vizier.17950105
- Bibcode:
- 2017yCat..17950105S
- Keywords:
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- Stars: double and multiple;
- Polarization;
- Stars: distances;
- Stars: masses;
- Surveys;
- Interferometry