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Ashmore Reef Marine Park Terrestrial Ecosystem Characterisation and...
Ashmore Reef Marine Park is located 630km north of Broome and has four vegetated islands that support significant biodiversity values. These values are under threat from non-... -
Parkes observations for project P1090 semester 2020OCTS_08
We propose to search for millisecond pulsars (MSPs) in an annular region around Blazar OJ 287, the most promising candidate to host a nano-Hz gravitational wave (GW) emitting... -
Wynarka 2024 Long Coleoptile Wheat Trial: Effects of Sowing Depth,...
This dataset captures results from a 2024 field experiment conducted at Wynarka, South Australia, to investigate the interaction between sowing depth, fertiliser placement, and... -
Parkes observations for project P1321 semester 2024APRS_08
We propose to search for temporal variations in HI absorption spectra seen against background pulsars to characterise Tiny Scale Atomic Structure (TSAS) in the Milky Way... -
Parkes observations for project P1321 semester 2024APRS_01
We propose to search for temporal variations in HI absorption spectra seen against background pulsars to characterise Tiny Scale Atomic Structure (TSAS) in the Milky Way... -
Parkes observations for project P1321 semester 2024APRS_02
We propose to search for temporal variations in HI absorption spectra seen against background pulsars to characterise Tiny Scale Atomic Structure (TSAS) in the Milky Way... -
Digital soil mapping of several soil properties: Forest Hill Agricultural...
A soil survey was conducted at CSIRO’s “Forest Hill” research farm to support scientific research, land management, infrastructure planning, and development activities. This... -
Long-term project observations for project P1321 semester 2025OCTS_03
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... -
Long-term project observations for project P1321 semester 2025APRS_11
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... -
Long-term project observations for project P1321 semester 2025APRS_12
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... -
Long-term project observations for project P1321 semester 2025APRS_13
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... -
Long-term project observations for project P1321 semester 2025APRS_14
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... -
Long-term project observations for project P1321 semester 2025APRS_15
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... -
Long-term project observations for project P1321 semester 2025APRS_16
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_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... -
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... -
Long-term project observations for project P1321 semester 2025APRS_17
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... -
Long-term project observations for project P1321 semester 2025APRS_18
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... -
Long-term project observations for project P1321 semester 2025APRS_19
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... -
Long-term project observations for project P1321 semester 2025APRS_20
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...