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Proximal grain composition of 240 globally diverse chickpea lines
The proximal composition (starch, protien, soluble sugars, lipid, insoluble fiber, and moisture) of 240 varieties of chickpea (Cicer arietinum) sourced from the ICRISAT... -
Parkes pulsar observations with undefined project IDs for 2025APRS_01
Parkes pulsar observations with undefined project IDs for 2025APRS. This collection contains observations from project IDs P999 and PX135. -
Parkes observations for project PX500 semester 2025APRS_09
This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries. As the observing time has been... -
LBA observations for project V642 semester 2024APRS
With supreme timing stabilities, millisecond pulsars (MSPs) have been used to test gravitational theories, and to collectively probe the stochastic gravitational-wave background... -
LBA observations for project V653 semester 2024APRS
Roughly 1 in 10 O stars have been found to harbour extremely stable, ordered (usually dipolar) magnetic fields, which are of ~kG strength. The presence of such organized surface... -
LBA observations for project V646 semester 2024APRS
This proposal aims to measure the parallax of pulsar B1055-52. PSR B1055-52 is particularly important for studying neutron star properties. Bright at radio and gamma-rays, the... -
LBA observations for project V651 semester 2024APRS
We propose an LBA pilot phase-referenced observation at 8.4GHz of a pulsar J1638-4713 associated with a bow shock pulsar wind nebula. The estimated velocity of 1500 km/s for the... -
LBA observations for project V636 semester 2023OCTS
To improve the link accuracy between the bright Gaia-CRF and ICRF, we request four 8-hour epochs using all available LBA antennas for phase-reference observations of five radio... -
LBA observations for project V626 semester 2024APRS
ASASSN-14ko is a transient source in the ESO 253-G003 galaxy system, which is in the process of merging. It was discovered by the ASAS-SN survey in 2014, and it periodically... -
LBA observations for project V603 semester 2024APRS
The energetics and central engines of Fast Radio Bursts (FRBs) are still mysterious, and it is unclear whether the subset of repeating FRBs are a function of their host... -
LBA observations for project V645 semester 2024APRS
Traditionally searches for techno-signatures have utilised raw voltage data from single-dish radio telescopes or beam-formed data from radio arrays with relatively short... -
LBA observations for project V650 semester 2024APRS
We request 8 GHz LBA observations of a nearby radio galaxy hosted by an active and likely unstable lenticular galaxy that may have underwent a minor merger in the past. Based on... -
LBA observations for project V652 semester 2024APRS
Relativistic outflows from cosmic explosions are some of the most extreme environments in the Universe, providing a natural laboratory to study the physics of jets, radiative... -
LBA observations for project V629 semester 2023OCTS
The Evolutionary Map of the Universe (EMU) survey is currently underway using the Australian Square Kilometre Array Pathfinder (ASKAP) telescope. This survey will catalogue up... -
Parkes observations for project P1338 semester 2025APRS_15
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... -
RV Investigator Voyage IN2025_V01 End of Voyage (EOV) Archive
This record describes the End of Voyage (EOV) data archive from the Marine National Facility (MNF) RV Investigator voyage IN2025_V01, titled "Collaborative Australian... -
Parkes observations for project P1338 semester 2025APRS_16
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 P1356 semester 2025APRS_04
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 P1219 semester 2025APRS_02
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 P1171 semester 2025APRS_02
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...