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Long-term project observations for project P1101 semester 2025APRS_08
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 P1183 semester 2025APRS_16
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... -
IMOS Biological Ocean Observer - sysdata.rda
This is the sysdata.rda file that is used to populate the IMOS Biological Ocean Observer (BOO) Shiny App. The IMOS biological and supporting data is accessed directly from the... -
NEMX.jl
NEMX.jl is an open source package developed in Julia using JuMP based on PowerModelsACDC.jl that provides physics-based co-optimized electricity and frequency control ancillary... -
Long-term project observations for project P885 semester 2025APRS_11
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 P1356 semester 2025APRS_14
Magnetars are neutron stars with exceptionally high magnetic fields. From the 30 known magnetars, only six have had radio emission detected so far. The remaining 24 magnetars... -
Parkes observations for project P1343 semester 2025APRS_07
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 P1338 semester 2025APRS_50
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... -
OzOat DArTSeq SNP data assets
Single nucleotide polymorphism genotypes for 324 varieties from the OzOat diversity panel generated with DArTSeq technology. Original platform source files are provided. -
Deep sea coral chemical composition data used in Thresher et al. "Southern...
Chemical composition of deep sea corals -
Parkes observations for project P1183 semester 2025APRS_17
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... -
Pathling
Pathling is a set of tools that make it easier to use FHIR® within data analytics, built on Apache Spark. -
Parkes observations for project P1325 semester 2025APRS_07
We request 15 hours of observing time with the Parkes UWL receiver (700-4000 MHz) to investigate frequency-dependent eclipsing in three spider millisecond pulsars (MSPs): one... -
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... -
Parkes observations for project P1325 semester 2025APRS_08
We request 15 hours of observing time with the Parkes UWL receiver (700-4000 MHz) to investigate frequency-dependent eclipsing in three spider millisecond pulsars (MSPs): one... -
Parkes observations for project P1349 semester 2025APRS_04
We propose an investigation of pulsars with interpulse (IP) emissions using the Ultra-wide-bandwidth Low (UWL) receiver at the Parkes (Murriyang) telescope. We aim to explore... -
Parkes observations for project P1349 semester 2025APRS_05
We propose an investigation of pulsars with interpulse (IP) emissions using the Ultra-wide-bandwidth Low (UWL) receiver at the Parkes (Murriyang) telescope. We aim to explore... -
Parkes observations for project P737 semester 2025APRS_04
Instrumental Commissioning -
Parkes observations for project PX600 semester 2020APRS_127
The Galactic Center (GC) is a key target for the radio component of Breakthrough Listen (BL) program. Offering the largest amount of stars in any given direction in the sky, the... -
Parkes observations for project P1211 semester 2024APRS_24
Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary...