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• W3209663619 endingPage "3440" @default.
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• W3209663619 abstract "We report on the search for electromagnetic counterparts to the nine gravitational-wave events with a $>$60% probability of containing a neutron star during the third (O3) LIGO-Virgo Collaboration (LVC) observing run with the All-Sky Automated Survey for SuperNovae (ASAS-SN). No optical counterparts associated with a gravitational wave event was found. However, thanks to its network of telescopes, the average area visible to at least one ASAS-SN site during the first 10 hours after the trigger contained $sim$30% of the integrated source location probability. Through a combination of normal operations and target-of-opportunity observations, ASAS-SN observations of the highest probability fields began within one hour of the trigger for four of the events. After 24 hours, ASAS-SN observed $>$60% of total probability for three events and $>$40% for all but one of the events. This is the largest area coverage to a depth of $g = 18.5$ mag from any survey with published coverage statistics for seven of the nine events. With its observing strategy, five sites around the world, and a large field of view, ASAS-SN will be one of the leading surveys to optically search for nearby neutron star mergers during LVC O4." @default.
• W3209663619 created "2021-11-08" @default.
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• W3209663619 date "2021-11-01" @default.
• W3209663619 modified "2023-10-16" @default.
• W3209663619 title "ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo" @default.
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• W3209663619 doi "https://doi.org/10.1093/mnras/stab3141" @default.
• W3209663619 hasPublicationYear "2021" @default.
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