Multi-messenger observations of a binary neutron star merger
BP Abbott - 2017 - iopscience.iop.org
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programmes
The discovery of the first electromagnetic counterpart to a gravitational wave signal has
generated follow-up observations by over 50 facilities world-wide, ushering in the new era of …
generated follow-up observations by over 50 facilities world-wide, ushering in the new era of …
[PDF][PDF] Multi-messenger observations of a binary neutron star merger
W Hartley - The Astrophysical Journal Letters, 2017 - research-collection.ethz.ch
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
Searching for stochastic gravitational waves using data from the two colocated LIGO Hanford detectors
J Aasi, J Abadie, BP Abbott, R Abbott, T Abbott… - Physical Review D, 2015 - APS
Searches for a stochastic gravitational-wave background (SGWB) using terrestrial detectors
typically involve cross-correlating data from pairs of detectors. The sensitivity of such cross …
typically involve cross-correlating data from pairs of detectors. The sensitivity of such cross …
Multi-messenger Observations of a Binary Neutron Star Merger** Any correspondence should be addressed to lvc. publications@ ligo. org.
BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2017 - escholarship.org
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
[HTML][HTML] Solar wind associated with near equatorial coronal hole
Present study probes temporal changes in the area and radiative flux of near equatorial
coronal hole associated with solar wind parameters such as wind speed, density, magnetic …
coronal hole associated with solar wind parameters such as wind speed, density, magnetic …
Multi-messenger observations of a binary neutron star merger
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
[HTML][HTML] Multi-messenger observations of a binary neutron star merger
M Jamrozy, M Ostrowski, Ł Stawarz… - 2017 - ruj.uj.edu.pl
Multi-messenger observations of a binary neutron star merger Skocz do treści EU EU
Repository logo Repository logo Authority index News Communities & Collections Help …
Repository logo Repository logo Authority index News Communities & Collections Help …
Multi-messenger Observations of a Binary Neutron Star Merger
AP Beardmore, PA Evans, JP Osborne, C Pagani… - 2017 - figshare.le.ac.uk
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
Multi-messenger observations of a binary neutron star merger
On 2017 August 17 a binary neutron star coalescence candidate (later designated
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …
GW170817) with merger time 12: 41: 04 UTC was observed through gravitational waves by …