Cherry Ng

TL;DR: The High Time Resolution Universe (HTRU) survey as discussed by the authors is an international collaboration with expertise shared among the MPIfR in Germany, ATNF/CASS and Swinburne University of Technology in Australia, University of Manchester in the UK and INAF in Italy.

TL;DR: The first gamma-ray pulsars were discovered by volunteer distributed computing via Einstein@Home and methods originally developed in gravitational-wave astronomy as mentioned in this paper, and the pulsars PSRs J0554+3107, J1422-6138, J1522-5735, and J1932+1916 were found using a novel search approach, combining volunteer distributed computation via Einstein-@Home.

TL;DR: In this paper, the solar electron density with the NANOGrav 11-year pulsar timing array (PTA) dataset was studied using Bayesian analyses, and the solar wind model was incorporated into a global fit starting from pulse times-of-arrival.

TL;DR: In this paper , the authors performed multiepoch 4-8 GHz observations of the inner ≈15 pc of our galaxy using the Robert C. Byrd Green Bank Telescope in 2019 August-September.

TL;DR: Three further aspects of HTRU discoveries and highlights include the ‘Diamond-planet pulsar’ binary J1719-1438 and a second similar system recently discovered, and an innovative segmented search technique which aims to increase the chances of discovering highly accelerated relativistic binary systems, potentially including pulsar-black-hole binaries.