Jong H. Chow

TL;DR: In this paper, the authors revisited the binary neutron star coalescence GW170817 and focused on longer signal durations, up until the end of the second Advanced LIGO-Virgo observing run, which was 8.5 days after the coalescence.

TL;DR: The Neutron Star Extreme Matter Observatory (NEMO) as discussed by the authors uses high-circulating laser power, quantum squeezing, and a detector topology specifically designed to achieve the high-frequency sensitivity necessary to probe nuclear matter using gravitational waves.

TL;DR: In this article, the authors reported results of a deep all-sky search for periodic gravitational waves from isolated neutron stars in data from the first Advanced LIGO observing run, where they found no significant signal candidate and set the most stringent upper limits to date on the amplitude of gravitational wave signals from the target population.

TL;DR: In this paper, the first results of an all-sky search for continuous gravitational waves from unknown spinning neutron stars in binary systems using LIGO and Virgo data were presented, using a specially developed analysis program, the TwoSpect algorithm.

TL;DR: In this article, a phase sensitive technique for remote interrogation of passive Bragg grating Fabry-Pe/spl acute/rot resonators is presented. But it is based on Pound-Drever-Hall (PDH) laser frequency locking, using radio-frequency phase modulation sidebands to derive an error signal.