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Long-term project observations for project P1101 semester 2025APRS_05
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 P1165 semester 2025APRS_02
We recently discovered two new pulsars J1849+1001 (35.1 ms) and J1839+0542 (57.9 ms) in a FAST pulsar survey at intermediate Galactic latitudes (PT2020_0141). Follow-up timing... -
Parkes observations for project P1196 semester 2023APRS_04
We request observing time at the Parkes telescope for observing three millisecond pulsars (MSPs): J1242-4712, J2101-4800, and J2144-5237. These MSPs were discovered with the... -
Parkes observations for project P1183 semester 2025APRS_07
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 P1185 semester 2023APRS_45
Ultra-long period neutron stars (ULPNSs) are an emerging class of objects that have sparked interest and curiosity in the fast transient community. Along with standard... -
Global terrestrial plant nitrogen stable isotope ratio samples: 30m centroid...
Annual global maps of foliar δ15N during 1984-2022, produced based on the method described in detail in Yang et al. (in review) . The maps could inform the improvement of... -
Parkes observations for project P1171 semester 2025APRS_03
The origin of Fast Radio Bursts (FRBs) is still unclear with a plethora of theoretical models for their origin. Several models predict associated multi-wavelength emission, but... -
Parkes observations for project P1219 semester 2025APRS_04
Magnetic fields are fundamental in regulating star formation and the evolution of molecular clouds. Zeeman splitting offers a unique method to directly measure line-of-sight... -
Parkes observations for project P1211 semester 2024APRS_13
Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary... -
Long-term project observations for project P1321 semester 2025APRS_05
The atomic interstellar medium shows tiny-scale optical depth fluctuations on the scale of 0.1~10,000 AU, whose origin and nature are poorly understood. The existence of this... -
Parkes observations for project P1325 semester 2025APRS_02
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 P1328 semester 2025APRS_13
Fast radio bursts are peculiar micro-millisecond duration transients, which have been seen to be extragalactic in origin. Since their discovery, a dichotomy has emerged in their... -
Tropical Cyclone Potential Intensity (TCPI)
This data collection consists of Tropical Cyclone (TC) Potential Intensity (PI) calculated from the ERA5 reanalysis dataset (1979 to 2023) and a selection of global climate... -
Parkes observations for project P1344 semester 2025APRS_06
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_31
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 P1348 semester 2024OCTS_04
We have discovered 6 candidate eclipsing binary millisecond pulsar (BMSPs) systems via image-plane searches for steep-spectrum radio sources with periodic variability. The radio... -
Long-term project observations for project P1361 semester 2025APRS_04
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 P1356 semester 2025APRS_09
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 P1345 semester 2025APRS_08
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 P574 semester 2025APRS_05
We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what...