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Parkes observations for project P1338 semester 2025APRS_61
Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a... -
Parkes observations for project P1183 semester 2025APRS_23
After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we... -
Parkes observations for project P1054 semester 2025APRS_19
With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourtytwo sources have been discovered in targeted... -
Parkes observations for project P1032 semester 2025APRS_04
With this proposal, we aim to continue P1032, the rapid measurements of relativistic parameters of southern binary pulsar systems using data from the Parkes Ultra Wideband Low... -
Parkes observations for project P1183 semester 2025APRS_24
After nearly two years of monitoring, comprising 126.7 hours over 57 observations with the Parkes telescope and 49.4 hours across 101 observations with the FAST telescopes, we... -
Long-term project observations for project P1041 semester 2025APRS_06
Omega Cen is the largest globular cluster in the Milky Way. I contains at least 18 known MPSs, and there are solid hints for the presence of an even larger pulsar population. We... -
Parkes observations for project P1327 semester 2025APRS_13
The radio radiation neutron star includes objects with spin periods ranging from milliseconds to tens of seconds. In the past years, however, the discovery of ultra-long period... -
Parkes observations for project P1338 semester 2025APRS_62
Fast radio bursts (FRBs) are millisecond-duration radio bursts of extragalactic origin. Since the discovery of the first FRB in the archival Parkes/Murriyang multibeam data, a... -
Long-term project observations for project P885 semester 2025APRS_13
We propose a modest program to continue monitoring 4 of the 6 known radio magnetars in order to achieve three primary science goals. The first is to characterise magnetar... -
Parkes observations for project P1327 semester 2025APRS_14
The radio radiation neutron star includes objects with spin periods ranging from milliseconds to tens of seconds. In the past years, however, the discovery of ultra-long period... -
Parkes observations for project P1032 semester 2025APRS_05
With this proposal, we aim to continue P1032, the rapid measurements of relativistic parameters of southern binary pulsar systems using data from the Parkes Ultra Wideband Low... -
Parkes observations for project P1345 semester 2025APRS_21
This proposal aims to constrain burst rates and spin down properties of a sample of new Rotating Radio Transients (RRATs) discovered with the ASKAP CRAFT Coherent upgrade... -
Long-term project observations for project P1361 semester 2025APRS_08
PSR J1227-6208 is a recycled pulsar in a bianry with a massive white dwarf companion. A recent timing measurement from combined MeerKAT and Parkes observations shows the... -
Parkes observations for project P1363 semester 2025APRS_15
We propose to monitor the bursts from the hyperactive repeating fast radio burst FRB 20240619D over six months using the Murriyang UWL receiver. The primary aim is to study the... -
Long-term project observations for project P1101 semester 2025APRS_09
We propose a long-term project to monitor a very active repeater, FRB 20190520B, with Murriyang's UWL system. Our previous observations show that FRB 20190520B is not only among... -
Parkes observations for project P512 semester 2008APRS_01
We propose to complete a pulsar survey along the Galactic Plane using the new Methanol Multibeam receiver in order to uncover pulsars previously selected against in lower... -
Parkes observations for project P1327 semester 2025APRS_15
The radio radiation neutron star includes objects with spin periods ranging from milliseconds to tens of seconds. In the past years, however, the discovery of ultra-long period... -
Error-mitigated quantum computing SEMO Python dynamic module
Qubit noise is one of the major barriers limiting broad adoption of quantum computing in solving complex real-word problems, such as optimisation. The qubit noise and the local... -
HCAS 3.3 (1988-2024) base model estimate of habitat condition (90m grid),...
Citation: Valavi R, Levick SR, Lehmann EA, Liu N, Giljohann KM, Williams KJ, Collings S, Johnson S, Botha EJ, Munroe SEM, Van Niel TG, Newnham G, Paget M, Malley C, Carlile P,... -
Otway CCS methane data from the 2011 controlled release experiment
Hourly averaged and minutely averaged atmospheric methane concentrations from measurements made at CO2CRC's Otway Carbon Capture and Storage (CCS) site in Victoria (Australia)...