The prospects for the observation of electromagnetic emissions by gravitational wave sources first detected using a network of interferometers are discussed. Various emission mechanisms and detection techniques for compact binary inspirals are studied to show that the pointing ability of gravitational wave observatories and the efficacy of electromagnetic detectors can be combined to predict that counterpart detections are improbable for the Initial interferometers, possible with Advanced LIGO detectors, and likely with an Advanced detector in Europe. Results from a new position estimation algorithm for unmodeled sources are also presented, and are discussed in the context of the observation of counterparts to burst sources of gravitational...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
The most likely sources of gravitational radiation that may be seen by the large-scale laser-interfe...
The prospects for the observation of electromagnetic emissions by gravitational wave sources first d...
Simultaneous observations of an electromagnetic counterpart from gravitational wave (GW) sources is ...
The detection of the electromagnetic counterparts of gravitational wave sources enables to gain a we...
The kilometer-scale ground based gravitational wave (GW) detectors, LIGO and Virgo, are being upgrad...
Many gravitational wave sources will produce electromagnetic signals as they emit gravitational wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
The most likely sources of gravitational radiation that may be seen by the large-scale laser-interfe...
The prospects for the observation of electromagnetic emissions by gravitational wave sources first d...
Simultaneous observations of an electromagnetic counterpart from gravitational wave (GW) sources is ...
The detection of the electromagnetic counterparts of gravitational wave sources enables to gain a we...
The kilometer-scale ground based gravitational wave (GW) detectors, LIGO and Virgo, are being upgrad...
Many gravitational wave sources will produce electromagnetic signals as they emit gravitational wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave...
The most likely sources of gravitational radiation that may be seen by the large-scale laser-interfe...