AndreaBozzo/ceres-open-data-index huggingface dataset:
Parkes observations for project P1211 semester 2024APRS_17

Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary systems), extremely fast spinning pulsars (e.g., sub-MSPs), and high dispersion measure (DM) pulsars. Such a situation is now changed thanks to the development of next generation radio telescope arrays such as Australian Square Kilometer Array Pathfinder (ASKAP). ASKAP is capable of conducting highly sensitive radio continuum surveys with wide sky coverage (e.g, Evolutionary Map of The Universe survey). One of the solutions is to find pulsar candidates in radio continuum surveys such as ASKAP surveys and then carry out targeted searches. This technique allows us to search over the wide bandwidth with full field of view while avoiding the need for expensive pixel-by-pixel high time resolution searches. In this proposal, we propose to observe 16 pulsar candidates identified in the Galactic plane using new ASKAP EMU images. We found 22 candidates by selecting sources with spectral index steeper than -2.0 and compactness less than 1.2. Among them 13 are known pulsars and a reasonable number of candidates to follow up (9 sources). In total, we have 16 candidates including seven sources from 2023APRS semester. Because of the dense ionised medium in the Galactic Plane, MSPs are likely to be missed by previous pulsar surveys carried out at 1.4 GHz. Here, we propose a targeted pulsar search with the Parkes UWL which allow us to search pulsation at higher frequencies and therefore avoid strong DM smearing and scattering effects.

Organization: CSIRO Data Access Portal
Parkes observations for project P1325 semester 2025APRS_04

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 redback and two black widows. Spider MSPs commonly exhibit frequency-dependent eclipsing, which provides insights into their dense, magnetized plasma environments. We propose to use the Parkes telescope with the UWL receiver in full polar mode to investigate key properties of three spider MSPs, focusing on their eclipse mechanisms and polarization characteristics. Our goals include modeling the eclipse phase spectra using wideband observations to examine the transition from optically thick to thin regimes and exploring the underlying eclipse mechanisms. Additionally, we aim to study the polarization properties of these MSPs, which remain unexplored around 2 GHz, and also to investigate high-frequency eclipses similar to those observed in systems like J1908+2105. Such eclipses suggest the presence of dense and magnetized plasma environments, enabling more precise constraints on parameters like electron column density and magnetic field strengths. Furthermore, we plan to probe magnetic fields by observing potential changes in rotation measure (RM) at eclipse ingress and egress.

Organization: CSIRO Data Access Portal
Parkes observations for project P1325 semester 2025APRS_03

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 redback and two black widows. Spider MSPs commonly exhibit frequency-dependent eclipsing, which provides insights into their dense, magnetized plasma environments. We propose to use the Parkes telescope with the UWL receiver in full polar mode to investigate key properties of three spider MSPs, focusing on their eclipse mechanisms and polarization characteristics. Our goals include modeling the eclipse phase spectra using wideband observations to examine the transition from optically thick to thin regimes and exploring the underlying eclipse mechanisms. Additionally, we aim to study the polarization properties of these MSPs, which remain unexplored around 2 GHz, and also to investigate high-frequency eclipses similar to those observed in systems like J1908+2105. Such eclipses suggest the presence of dense and magnetized plasma environments, enabling more precise constraints on parameters like electron column density and magnetic field strengths. Furthermore, we plan to probe magnetic fields by observing potential changes in rotation measure (RM) at eclipse ingress and egress.

Organization: CSIRO Data Access Portal
Patient Access Coordination Hub (QPACH) ambulance multiagent simulation

As described in Chapter 5 in the report delivered to QPACH titled 'Digital Twin for the Queensland Patient Access Coordination Hub', this web-based application generates ambulance emergency department (ED) admissions for public hospitals in Metro North. 
This is a simulation only, built on agent based modelling on Queensland Ambulance Service (QAS) data. This app is for research purposes only as a proof-of-concept and is not intended for clinical use. 

Organization: CSIRO Data Access Portal
DSS Disability Employment Services - monthly profile

This report contains key program data for the Disability Employment Services (DES) program, including the two parts Disability Management Service (DMS) and Employment Support Service (ESS). The report provides aggregated data on referrals, commencements, exits, caseload and outcomes for the DES program of the last five years. The report also includes a glossary.

Reports after July 2018 only include 2010 and 2018 DES programs. Please refer to earlier reports for information on the previous programs.

Tags: DES, DMS, Disability, ESS, Employment, Social Services, disability employment services
Organization: Department of Social Services
Parkes observations for project P630 semester 2011APRS_08

We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future and used to search for relativistic binary and millisecond pulsars, RRATs, and extragalactic radio bursts. The survey should discover 100s of new millisecond and normal pulsars and help define the lower limit to pulsar periods, test theories of relativistic gravity, find transients and provide pulsars for gravitational wave detection.

Organization: CSIRO Data Access Portal
Parkes observations for project P630 semester 2011APRS_07

We propose to carry out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using the 20cm multibeam and a new digital filterbank array this survey will create a petabyte digital record of the sky that can be data mined in the future and used to search for relativistic binary and millisecond pulsars, RRATs, and extragalactic radio bursts. The survey should discover 100s of new millisecond and normal pulsars and help define the lower limit to pulsar periods, test theories of relativistic gravity, find transients and provide pulsars for gravitational wave detection.

Organization: CSIRO Data Access Portal
Long-term project observations for project P1101 semester 2025APRS_07

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 the most active FRBs that can be observed with Murriyang, but also shows extreme rotation measure (RM) and dispersion measure (DM) evolution, along with distinctive behavior at 3GHz frequency. This makes the UWL receiver uniquely suited for detailed studies and long-term monitoring of this repeating FRB. Through this program, we anticipate detecting a large sample of bursts from this FRB. In collaboration with FAST, we aim to investigate the time evolution of various properties of FRB 20190520B, enhance our understanding of polarisation across an extremely wide bandwidth with high sensitivity, and gain deeper insights into the local environment and emission mechanisms of FRBs.

Organization: CSIRO Data Access Portal
Compositional dissimilarity data for the National Climate Risk Assessment

Compositional dissimilarity, or the potential degree of ecological change, is the proportion of species at a given location expected to be absent from the same location, and potentially replaced by other species, under a changed climate scenario. Compositional dissimilarity ranges from 0 (no change in species composition) to 1 (100 % change in species composition, Ferrier et al., 2007). 
The data presented here are pixel-based dissimilarities in species composition between the baseline scenario, Australian climate in 1990, and two future climate change scenarios, ACCESS 1.0, and GDFL-ESM2M, at a 2050-centred climate under RCP (Repressentative Concentration Pathway) 8.5 (Harwood et al., 2014). Compositional dissimilarity is estimated in the absence of the effect of land use change by assuming the land is in highest condition, or “reference” condition. As such the expected change in species composition is based on climate change alone.
A model of compositional dissimilarity for vascular plants was fitted using generalized dissimilarity modelling (GDM) (Ferrier et al., 2007) based on 1990-centred species records, climate, and other environmental data (Mokany et al. 2018). Compositional dissimilarity was estimated between 1990 and each of the two climate scenarios, and summarised as the arithmetic mean of the estimated compositional dissimilarity for both climate scenarios (ACCESS 1.0 and GDFL-ESM2M).
For the National Climate Risk Assessment (NCRA) project, the mean model outputs were summarised (arithmetic mean) by various regions (Aggregate Ecosystem Groups (AEGs), and NCRA regions), available in the links below. The AEG and NCRA region data were reprojected to the projection of the dissimilarity raster, and arithmetic mean dissimilarity was calculated per region of the interaction between AEG and NCRA region.

Organization: CSIRO Data Access Portal
Science, Research and Innovation (SRI) Budget Tables

Investment in Australia’s science, research and innovation system is critical to support industry growth, create more jobs and increase our national prosperity.

Science, research and innovation are fundamental to the government’s priorities, including rebuilding Australia’s manufacturing capability, supporting home-grown innovation, and securing our long-term productivity, energy security and prosperity. This support extends across government, allowing us to make strategic investments that help researchers do cutting-edge R&D to meet emerging challenges. 

Tags: Innovation, Research, Science, government, investment
Organization: Department of Industry, Science and Resources (DISR)
3PL (Parallel Pipeline Programming Language) compiler

3PL is a "dataflow" parallel programming language for FPGAs which has been explicitly designed to support pipelining.
The name 3PL stands for "Parallel Pipeline Programming Language".
This software is a 3PL compiler, taking 3PL source code and producing a Xilinx "netlist" (EDN) compatible output file.
The EDN file is processed by the Xilinx ISE software suite ultimately producing a "bitfile" that can be loaded into a Xilinx FPGA.

Organization: CSIRO Data Access Portal
Genomator

Genomator is a program which uses a SAT solver to generate synthetic genomic data from an input VCF dataset. The program parses an input file of genomic data for a number of individuals, specified in VCF format, and then generates the genomic data for a number of synthetic individuals, outputting the results as a different VCF formatted file. Genomator formulates SAT problem (boolean SATisfiability problem) which is composed of a (usually) large number of binary variables and a (usually) large number of constraints. In this context the SAT problem is representative of generating new individuals which are sufficiently similar to those in the dataset and yet also sufficiently different from each.

Organization: CSIRO Data Access Portal
Coral Settlement Tile: image analysis

This Python code defines a batch-processing workflow to process raw images and analyse coral larval settlement on tiles. The workflow can be split into two main stages:

ImageProcess: The images need to be prepared for further analysis. The suggested pipeline for image processing includes several steps to ensure a consistent dataset of images:
Cropping: Image cropping ensures that each tile defines the region of interest, removing any background.
Resizing: All images are resized to the exact dimensions.
Histogram Equalisation: If a reference image is provided, the histograms of the images are equalised to match the reference, ensuring uniform lighting and contrast.

Metadata Preservation: The original image metadata and any additional information provided by the user are retained in the processed images, ensuring the dataset maintains the same information as the original images.


Chimera: coral settlement analysis. Once the images are processed, visible recruits can be identified using annotation software (external), like CVAT. Annotated images can then be analysed to study the evolution of the corals, for example, determining the survival rates of chimeras.


The user does not need to follow all the steps sequentially. If the images are already prepared, such as being the same size and adequately cropped around the object of interest around the object of interest (e.g. tiles), they can skip the preparation steps and proceed directly to the recruitment analysis.

Organization: CSIRO Data Access Portal
SnoMAP Starter

SnoMAP Starter is a map from SNOMED CT-AU to ICD 10 AM that is made available as a FHIR Concept Map.
It has been designed to provide a map to meet known and identified requirements of researchers and analysts working with SNOMED encoded patient data collections where their analyses demand conversion to ICD-10-AM for comparability purposes. This could be either for retrospective analyses where only historical ICD-10-AM data is available, or for consolidated patient data collections that contain both SNOMED and ICD-10-AM encoded cases.
This map is a starter map and does not support mandatory reporting for National Minimum Data Standards (NMDS) data, casemix funding, Diagnosis Related Groups (DRG) or Activity Based Funding (ABF). It is not designed to be used in any user facing, point-of-care deployments.

Organization: CSIRO Data Access Portal
Parkes observations for project P595 semester 2025APRS_20

We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the space missions, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.

Organization: CSIRO Data Access Portal
Parkes observations for project P1165 semester 2025APRS_05

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 observations show that they are in circular orbits with massive companions. This suggests that PSR J1849+1001 and J1839+0542 can be classified as the intermediate-mass binary pulsar (IMBP). Their massive companions also make them promising systems to measure "Post-Keplerian" parameters through pulsar timing. These Parkes observations will be combined with regular timing observations with FAST or MeerKAT to measure "Post-Keplerian" parameters and then measure both neutron star and companion masses.

Organization: CSIRO Data Access Portal
Parkes observations for project P1211 semester 2024APRS_20

Traditional pulsar searching techniques are not sensitive enough to extreme pulsars such as millisecond pulsars (MSPs) in compact binaries (e.g., Pulsar-Blackhole binary systems), extremely fast spinning pulsars (e.g., sub-MSPs), and high dispersion measure (DM) pulsars. Such a situation is now changed thanks to the development of next generation radio telescope arrays such as Australian Square Kilometer Array Pathfinder (ASKAP). ASKAP is capable of conducting highly sensitive radio continuum surveys with wide sky coverage (e.g, Evolutionary Map of The Universe survey). One of the solutions is to find pulsar candidates in radio continuum surveys such as ASKAP surveys and then carry out targeted searches. This technique allows us to search over the wide bandwidth with full field of view while avoiding the need for expensive pixel-by-pixel high time resolution searches. In this proposal, we propose to observe 16 pulsar candidates identified in the Galactic plane using new ASKAP EMU images. We found 22 candidates by selecting sources with spectral index steeper than -2.0 and compactness less than 1.2. Among them 13 are known pulsars and a reasonable number of candidates to follow up (9 sources). In total, we have 16 candidates including seven sources from 2023APRS semester. Because of the dense ionised medium in the Galactic Plane, MSPs are likely to be missed by previous pulsar surveys carried out at 1.4 GHz. Here, we propose a targeted pulsar search with the Parkes UWL which allow us to search pulsation at higher frequencies and therefore avoid strong DM smearing and scattering effects.

Organization: CSIRO Data Access Portal
Parkes observations for project P1357 semester 2025APRS_08

MeerKAT has already discovered a number of Galactic transients, which are most likely to be Rotating Radio Transients (RRATs). Previous observations of a few of these sources with the Parkes UWL receiver have proven its utility in follow-up timing observations of MeerKAT discoveries.
  MeerKAT has discovered a few more RRATs in its latest observing cycle and more good quality UWL observations of these sources are required to determine the rotational period and period derivative and also to facilitate the study of their emission properties. Therefore, we request follow-up observations of 5 new sources to achieve this and to further enable spectral and polarization studies of these sources. Given the potential link between RRATs, magnetars, and some fast radio bursts (FRBs) suggested by both observations and theories, this study could reveal more similarities between these different classes of transient sources and significantly advance our understanding of their origins.

Organization: CSIRO Data Access Portal
Parkes observations for project P1356 semester 2025APRS_12

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 are generally only searched for radio emission after an X-ray outburst. This added a strong selection bias to whether magnetars are radio loud or not. From the known six radio loud magnetars, we know that the radio emission changes quickly with time and for the magnetar XTE J1810-197, it has been observed that the radio flux increases strongly without an enhancement in X-ray flux. Thus, it remains unclear whether the radio quiet magnetars are in fact radio quiet and the radio X-ray relation appears to be rather complex.
  In this proposal, we propose a regular monitoring campaign of 4 radio quiet magnetars with bi-weekly observations using the Parkes UWL receiver. For 3 of the sources, we will have accompanying X-ray observations and thus, this will give an unique data set to probe the relation between radio and X-ray independent outbursts. Any detection of radio emission, i.e. single pulses or folded profiles, would be a major discovery and help to constrain the emission mechanisms of magnetars. This will also help to improve the understanding of the emission mechanism of fast radio bursts. However, also a non-detection of radio emission will provide upper limits that serve as a baseline before any future outburst of the observed magnetars as well as allow to constrain the formation process of magnetars in contrast to pulsars.

Organization: CSIRO Data Access Portal
Hydrodynamic and sediment observations in Fitzroy Estuary QLD and Cassady Creek (Hinchinbrook, QLD) 2024-2025:  CSIRO Tidal Inundation project

This dataset compiles field observations collected as part of CSIRO’s Tidal Inundation project, 2024-2025. The field campaign deployed oceanographic and tide level sensors in two Queensland estuaries: the Fitzroy Estuary and Cassady Creek (Hinchinbrook Shire). Additional project information, deployment details, site maps and quality control notes are provided in the data_summary pdf and time_series_summary spreadsheets. 
Geophysical survey data collected during this study, including multibeam sonar bathymetry and aerial LiDAR surveys, are not included in this dataset but are available in a separate data collection associated with the Tidal Inundation project (see related links below).
Periodic field trips were undertaken during the 12-month study to scout, deploy, maintain and retrieve instrumentation at several fixed stations. Instrumentation consisted of tide level sensors, acoustic doppler current profilers (ADCPs), and wave monitoring buoys with pressure and temperature sensors. Additionally, 38 discrete samples of surface sediments were collected by manual grabs to quantify grain size throughout the Fitzroy Estuary and its distributary (Casuarina Creek). 
This data collection includes brief quality control reports prepared after retrieval of each ADCP, with additional QC notes included in the data summary document. Data in this repository are grouped by instrument type and location. All timestamps are in local time (GMT +10), unless otherwise noted.

Organization: CSIRO Data Access Portal
Geomorphic change detection between 2018 and 2024 for the Bowen region of the Burdekin River Basin Queensland Australia

This dataset shows geomorphic change (erosion and deposition) in the Bowen-Broken catchment of the Burdekin River Basin Queensland, Australia. The change is determined by the difference in elevation in the overlapping areas of two co-registered airborne laser scanning (ALS) point cloud datasets, collected in 2018 and 2024. 
The change is measured in metres for each 0.5 m x 0.5 m grid cell across the study area. Negative values indicate erosion and positive values indicate deposition.

Organization: CSIRO Data Access Portal
MyPort Pty Ltd-Anticipatory Notice- 7 August 2025-Browns Plains

MyPort Pty Ltd-Anticipatory Notice given on 7 August 2025 Ref ED25/86369 for

Project area: The Plains Stage 3 at 806-810 Wembley Rd, Browns Plains QLD, 
Australia

Estimated completion date: 30 June 2028
Contract date: 4 Aug 2025
Network Type: FTTP



Tags: Broadband, MyPort, SIP, Telecommunications, statutory infrastructure provider
Organization: SIP Register - Myport Pty Ltd
MyPort Pty Ltd - ANticipatory Notice - 7 August 2025-Upper Mt Gravatt

MyPort Pty Ltd - ANticipatory Notice given on 7 August 2025 Ref ED25/86365 for project area
32 Hertford Street, Upper Mount Gravatt QLD

Estimated completion date: 1/7/26
Contract date: 4/8/25
Network Type: FTTP

Tags: Broadband, MyPort, SIP, Telecommunications, statutory infrastructure provider
Organization: SIP Register - Myport Pty Ltd
MyPort Pty Ltd - Anticipatory Notice-7 August 2025-Melbourne

MyPort Pty Ltd - Anticipatory Notice given on 7 August 2025 for project area Novus on Bowen	
 at 2 Bowen Crescent, Melbourne VIC 3004; 
Estimated completion date: 31 July 2026
Contract signded: 31 July 2025
Network Type: FTTB


Tags: Broadband, MyPort, SIP, Telecommunications, statutory infrastructure provider
Organization: SIP Register - Myport Pty Ltd
MyPort Pty Ltd - Anticipatory Notice- 7 August 2025-South Melbourne

MyPort Pty Ltd - Anticipatory Notice given on 7 August 2025 Ref ED25/86361 for 
Project areas Local South Melbourne at 245 Normanby Road, South Melbourne VIC
Estimated completion date: 31/10/25
Contract date: 5/8/25
Network: FTTB

Tags: Broadband, MyPort, SIP, Telecommunications, statutory infrastructure provider
Organization: SIP Register - Myport Pty Ltd