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We search for gravitational-wave transients associated with gamma-ray burstsdetected by the Fermi and Swift satellites during the first part of the thirdobserving run of Advanced LIGO and Advanced Virgo (1 April 2019 15:00 UTC - 1October 2019 15:00 UTC). 105 gamma-ray bursts were analyzed using a search forgeneric gravitational-wave transients; 32 gamma-ray bursts were analyzed with asearch that specifically targets neutron star binary mergers as short gamma-rayburst progenitors. We describe a method to calculate the probability thattriggers from the binary merger targeted search are astrophysical and applythat method to the most significant gamma-ray bursts in that search. We find nosignificant evidence for gravitational-wave signals associated with thegamma-ray bursts that we followed up, nor for a population of unidentifiedsubthreshold signals. We consider several source types and signal morphologies,and report for these lower bounds on the distance to each gamma-ray burst.

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3a