L. P. Singer, H.-Y. Chen, D. E. Holz, W. M. Farr, L. R. Price, V. Raymond, S. B. Cenko, N. Gehrels, J. Cannizzo, M. M. Kasliwal, S. Nissanke, M. Coughlin, B. Farr, Alex L. Urban, S. Vitale, J. Veitch, P. Graff, C. P. L. Berry, S. Mohapatra, and I. MandelRead at arXiv.org
This web page provides additional online material related to the paper
Going the Distance: Mapping Host Galaxies of LIGO Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up and the accompanying Supplement paper.
The paper explores three-dimensional reconstruction positions of gravitational-wave transients that are detectable by LIGO and Virgo. It builds upon an earlier pair of papers on sky localization with gravitational-wave detectors, but adds directionally resolved LIGO distance estimates in order to facilitate deep searches of potential host galaxies for electromagnetic counterparts of LIGO sources.
The table below shows thumbnail images of 500 simulated Advanced LIGO volume reconstructions. Each image is a volume rendering of the probability distribution for a given event, projected in the plane of the distribution's two most significant principal axes.
O2 buttons in the toolbar to switch between Advanced LIGO observing runs. Touch any of the
Sort by buttons to reorder the thumbnails by detector network, enclosed volume, enclosed area, network signal-to-noise ratio, or signal-to-noise ratio in LIGO Hanford (H) or LIGO Livingston (L).
|SNR (H/L/V)||/ /|