AndreaBozzo/ceres-open-data-index huggingface dataset:
Building Permit Activity Data 2021

The Victorian Building Authority (VBA) collects information from building surveyors on the number, value and type of building permits issued each month as part of its functions under the Building Act 1993. The Building Permit Activity Data provides information relating to each building permit issued in the State of Victoria and reported to the VBA for the period specified. It includes: - over 40 pieces of information per record - details of what was built (or demolished) - how much it cost - levy paid - when it was built - time series per year In addition, spatial information can be viewed according to: - municipality - Victorian State Regions - Victorian Rural Regions - metropolitan regions - suburb - postal code - street name Please refer to the data quality statement to assist you in determining whether the data meets fitness for purpose tests before use.

Tags: Building, Building Activity, Building Permits, VBA
Organization: Building and Plumbing Commission
Building Permit Activity Data 2025

The Victorian Building Authority (VBA) collects information from building surveyors on the number, value and type of building permits issued each month as part of its functions under the Building Act 1993. The Building Permit Activity Data provides information relating to each building permit issued in the State of Victoria and reported to the VBA for the period specified. It includes: - over 40 pieces of information per record - details of what was built (or demolished) - how much it cost - levy paid - when it was built - time series per year In addition, spatial information can be viewed according to: - municipality - Victorian State Regions - Victorian Rural Regions - metropolitan regions - suburb - postal code - street name Please refer to the data quality statement to assist you in determining whether the data meets fitness for purpose tests before use.

Tags: Building Act 1993, Building Permit Data, Compliance Activity, permit
Organization: Building and Plumbing Commission
Vostronet (Australia) Pty Ltd - Anticipatory notice - 12 February 2024 - Flinders View QLD

Statutory Infrastructure Provider (SIP) - VostroNet Anticipatory Notice Anticipatory notice given 12 February 2024 and the associated project area data for a contract to provide telecommunications network infrastructure. Project area: 10 Astral Court, Flinders View, QLD 4305. Estimated completion date: 31 December 2024. Infrastructure to be installed: FTTP - Fibre to the premises

Tags: SIP, Telecommunications, VostroNet, broadband, statutory infrastructure provider
Organization:  SIP Register - VostroNet (Australia) Pty Ltd
Building Permit Activity Data 2023

The Victorian Building Authority (VBA) collects information from building surveyors on the number, value and type of building permits issued each month as part of its functions under the Building Act 1993. The Building Permit Activity Data provides information relating to each building permit issued in the State of Victoria and reported to the VBA for the period specified. It includes: - over 40 pieces of information per record - details of what was built (or demolished) - how much it cost - levy paid - when it was built - time series per year In addition, spatial information can be viewed according to: - municipality - Victorian State Regions - Victorian Rural Regions - metropolitan regions - suburb - postal code - street name Please refer to the data quality statement to assist you in determining whether the data meets fitness for purpose tests before use.

Tags: Building Act 1993, Building Permit, Building Permit Data, Building Surveyors, VBA
Organization: Building and Plumbing Commission
Building Permit Activity Data 2015

The Victorian Building Authority (VBA) collects information from building surveyors on the number, value and type of building permits issued each month as part of its functions under the Building Act 1993.
The Building Permit Activity Data provides information relating to each building permit issued in the State of Victoria and reported to the VBA for the preiod specified.
It includes:
- over 40 pieces of information per record
- details of what was built (or demolished)
- how much it cost
- levy paid
- when it was built
- time series per year
In addition, spatial information can be viewed according to:
- municipality
- Victorian State Regions
- Victorian Rural Regions
- metropolitan regions
- suburb
- postal code
- street name
Please refer to the data quality statement to assist you in determining whether the data meets fitness for purpose tests before use.

Tags: Building Activity, Building Industry, Building Permit, Building Regulation, Property, VBA, Victorian Building Authority
Organization: Building and Plumbing Commission
Long-term project observations for project P456 semester 2024OCTS_13

The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves
  from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. We are now in an exciting regime where a signal detected in our (and other data sets) has the form expected for a gravitational wave background. We are therefore now attempting to confirm, or deny, this exciting result. With this proposal we aim to maintain our pre-eminent position in the field. Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!

Organization: CSIRO Data Access Portal
Parkes observations for project P455 semester 2024OCTS_05

This project is to continue timing and profile studies of the first double-pulsar system, a unique laboratory for gravitational physics. Important results published in our 53-page Phys. Rev. X paper (Kramer et al., Vol 11, October 2021) include the first measurements of higher-order light-propagation effects and of the relativistic deformation of the orbit and highlight the importance of a long term observational campaign, including VLBI observations, for this remarkable system. The main aims of this proposal are to provide the strongest tests to date for general relativity and to measure for the first time the moment-of-inertia of a neutron star. Additionally, we will determine the system geometry, map the pulsar beams via geodetic precession, and search for the reappearance of Pulsar B. We exploit the high sensitivity and broad bandwidth of the UWL receiver. Continuation of this project is vital to provide overlap with MeerKAT timing observations of the Double Pulsar system which commenced recently.

Organization: CSIRO Data Access Portal
AS201 EMU: EMUCAT supermosaic images

EMUCAT generates “supermosaics” by linearly mosaicing together the adjacent EMU tiles within each of EMUCAT’s “source extraction regions”. These supermosaics ensure close to uniform sensitivity in the overlap regions between tiles, and are used to produce unique, de-duplicated, source lists, using Selavy, as the starting point for all subsequent EMUCAT processing and value-added data product generation.

Organization: CSIRO Data Access Portal
Parkes observations for project P885 semester 2024OCTS_16

We propose a reduced even more modest program to continue monitoring 4 of the 6 known radio magnetars, tracking their rotational, flux density, and polarisation properties. The rotational response of 1E 1547.0-5408 to its 2022 'hiccup' in radiative properties is still developing, requiring frequent observations every ~10 days. The cadence and request for Swift J1818.0-1607 is reduced, commensurate with its decreased activity/flux. Observations of XTE J1810-197, and PSR J1622-4950 which ceased emission in 2022, remain at reduced levels. The overall request is 13.5 hours.

Organization: CSIRO Data Access Portal
Parkes observations for project P960 semester 2024OCTS_14

We aim to carry out receiver pointing and characterisation tests of Parkes receivers. Typically, these tests are carried out after the receiver package is installed, but time does not always allow for proper characterisation. Receivers for consideration include UWL, MARS and 13MM packages. In addition to cross-referencing C007 for flux calibration via pointing, we aim to conduct gain-elevation and system temperature experiments using the Moon, to ensure users of the Parkes Observatory have the most accurate information available for calibration purposes.

Organization: CSIRO Data Access Portal
Long-term project observations for project P574 semester 2024OCTS_14

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 disrupts this process, how and why their profiles vary with time, whether they precess or have planetary mass companions, in short all the things that make pulsar timing noisier than the perfect clock. Secondly we want to understand the interstellar medium of our Galaxy through repeated monitoring of dispersion measure, rotation measure and flux density variations in conjunction with scintillation parameters. Finally, we provide these data as a community service both to the high-energy community where we have strong collaborative links (particularly to Fermi) and to the radio pulsar astronomers generally through the CSIRO archive. The project is on-going since 2007, we are (co-)authors on 106 papers arising from the P574 data. The data have contributed to the PhD theses of students from Bordeaux, Manchester, Oxford, Stanford, and Swinburne. We are seeking long-term project status with a view to continuing the project into the SKA era.

Organization: CSIRO Data Access Portal
Parkes observations for project P595 semester 2024OCTS_18

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
SCHISM-WWMIII hydrological and wave model hindcast for Vanuatu

This collection contains netCDF formatted data produced by the SCHSIM-WWMIII hydrological and wave coupled model v5.9 around Vanuatu as part of the VanKIRAP project, described in the Hoeke et al report "National sea level rise and coastal hazard analysis mapping for Vanuatu": https://doi.org/10.25919/7jzw-8y73. 
Files are written monthly for the 41 years from 1980 to 2020, containing hourly data on an unstructured grid (adhering to UGRID1.0 convention) that ranges from 10km resolution offshore down to 50m at the coast. Each file contains variables describing sea surface elevation, significant wave height, mean &amp; peak wave period, peak wave direction, peak directional spreading, and u- and v- components of depth-averaged current. 
The model was forced with: 
- TPXO v9.2 tides
- NOAA CFSR surface winds and Holland vortex model TC winds
- ECMWF ORAS5 water levels and sea level rise (with geodetic correction)
- CAWCR wave hindcast wave spectra. 
The model configuration and tuning is described in the linked project report. 

Organization: CSIRO Data Access Portal
Parkes observations for project P1176 semester 2024OCTS_03

Pulsars and their winds are among nature's most powerful particle accelerators, producing particles with energies up to a few PeVatrons. In addition to high-energy radiation from the magnetosphere, the rotational energy of a neutron star is carried away in the form of magnetized ultra-relativistic pulsar winds. Investigation of pulsar wind nebula (PWN) offers an excellent chance to determine the interaction details of relativistic flows with their surroundings that may never be possible in other classes of source. Our recent analyses of ASKAP observations of Galactic Plane uncovered previously known X-ray PWN CXOU J163802.6-471358 (nicknamed Potoroo). Recently, we have successfully detected a pulsar candidate associated with Potoroo with Parkes telescope. It is detected at  3 GHz with a dispersion measure of DM = 1553 pc cm-3 and a rotation period of 65.74 ms. Here we propose to continue timing observations for this young pulsar with the Parkes Ultra-Wideband Low (UWL) receiver. Through pulsar timing, we will be able to obtain precise measurements of the pulsar position and the spin-down of the pulsar which enables us to independently estimate the age of the system. This program will also facilitate our LBA observations to measure proper motions of the pulsar through pulse-phased resolved VLBI experiments.

Organization: CSIRO Data Access Portal
Parkes observations for project P1165 semester 2024OCTS_10

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 to measure "Post-Keplerian" parameters and then measure both neutron star and companion masses.

Organization: CSIRO Data Access Portal
Parkes observations for project P1183 semester 2024OCTS_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 have determined that FRB 20220529 is an extremely active repeater. It exhibits one of the longest activity durations and a potential period. Due to frequent observations scheduled with both Parkes and FAST, we recently observed an abrupt rotation measure (RM) flare in this source. This is the first detection of such an RM flare'' in a fast radio burst (FRB), suggesting that the source is in an environment with occasionally erupting coronal mass ejection. This presents a unique opportunity to study the eruption environment of FRBs and investigate the relation between burst activity and other burst parameters. If confirmed, the periodicity and theRM flare'' of FRB 20220529 would corroborate each other and become a ``smoking gun'' of the binary origin of FRB. In our previous analysis, both Parkes and FAST observations have proven essential. While FAST's higher sensitivity has enabled the capture of many bursts, Parkes' wideband receiver has provided a good burst detection rate even during low-rate phases. Notably, during the RM flare, two high signal-to-noise ratio bursts from Parkes have been crucial in understanding the RM variations. To further investigate FRB 20220529, we have scheduled regular FAST observations every fortnight, monitoring the source for 20 minutes each time. Therefore, we also propose to monitor FRB 20220529 using the Parkes UWL receiver, ensuring high-time resolution and employing full-polarization observations.

Organization: CSIRO Data Access Portal
Parkes observations for project P1054 semester 2024OCTS_14

With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Thirtysix sources have been discovered in targeted observations of Fermi unidentified point sources, two in association with a Supernova Remnant, 14 in the Magellanic Clouds, 94 in Globular Clusters and 81 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including at least one double neutron star system and several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.

Organization: CSIRO Data Access Portal
Parkes observations for project P1101 semester 2024OCTS_09

We propose to continue our fortnightly monitoring of a very active repeater, FRB 20190520B, with the Parkes UWL system. Our current observations show that FRB 20190520B is not only the most active FRB that can be observed with Parkes, but also shows extreme rotation measure (RM) and dispersion measure (DM) evolution and unique behavior at 2 to 3 GHz frequency. This makes UWL the ideal instrument to carry out in-depth studies of this repeating FRB. With this program, we expect to detect a large sample of bursts from FRB 20190520B, and in collaboration with FAST and GBT, we will study its local environment, emission properties, fluence distributions, and polarisation properties over an extremely wide bandwidth with high sensitivity.

Organization: CSIRO Data Access Portal
Parkes observations for project P1189 semester 2024OCTS_09

The solar wind and space weather events have a significant impact on the solar system and can pose hazards to both space and Earth-based technologies. Understanding the origins of the solar wind and space weather is therefore essential to comprehend how these events are driven and to enhance space weather prediction efforts. Magnetic structures such as coronal holes, helmet streamers, and prominences in the lower corona are believed to be key drivers of the winds and coronal mass ejections (CMEs). However, there are very few observational constraints on the solar wind and space weather events at low solar altitudes (&lt; 20 solar radii), as this region is inaccessible to space probes. In this proposal, we aim to monitor a set of pulsars as they pass within 5.7 degrees of the Sun. Using the UWL receiver on the Parkes Radio Telescope, we will make precision measurements of the dispersive group delay and Faraday rotation of the pulses. This will enable us to investigate the densities and magnetic fields of the coronal structures driving the wind and to observe approximately $6 \pm 4$ CMEs as they pass by the pulsars serendipitously. We will integrate this data with complementary efforts to study the solar wind via interplanetary scintillation, constraints from space probes, and simulations. This approach provides an exciting opportunity to develop a comprehensive understanding of the solar wind and space weather.

Organization: CSIRO Data Access Portal
Parkes observations for project P1185 semester 2023APRS_42

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 magnetars, they have been theorised to be potential progenitors of the enigmatic fast radio bursts (FRBs). The MeerTRAP project at the MeerKAT radio telescope is uncovering several magnetar and ultra-long period neutron star candidates, an example of which is PSR J0901-4046 with a period of 76s. Continued long-term monitoring of PSR J0901-4046 has shown it to be potentially transitioning into radio quiescence. The proposed observations will enable us to continue to monitor and characterise the decline in flux density. We have also discovered two new candidates MTP0027 and MTP0068 with periods of ~10 seconds and ~5 seconds respectively. Both sources exhibit magnetar-like pulse morphology and have only been detected in one epoch with MeerKAT. We propose to continue monitoring these sources to re-detect pulses and study their spectro-temporal-polarimetric properties.

Organization: CSIRO Data Access Portal
Parkes observations for project P1219 semester 2023OCTS_29

The magnetic field potentially regulates the process of star formation and the evolution of molecular clouds. It is inherently difficult to measure interstellar magnetic field strengths, with the measurement of Zeeman splitting a unique method to estimate the magnetic field strength along the line of sight directly. Despite the detection of Zeeman splitting in other mediums, there are as yet no Zeeman detections against compact background sources in quiescent molecular clouds or the cold neutral medium. Pulsars with extremely small solid angles and relatively high transverse velocities are ideal background sources to study the magnetic field in molecular clouds, providing a distinct signal to measure splitting against. There are four pulsars with OH absorption detections, namely PSR B1849+00, B1641-45, B1718-35, and B1749-28. We propose to utilize these four pulsars to explore the properties of the magnetic field and its variations within molecular clouds through both the Zeeman splitting of OH absorption and rotation measure estimations, between epochs. If a detection is confirmed, it will open a new window on the hard-to-measure magnetic fields in molecular clouds, independent of interpretation, thus shedding light on the physics of star formation and the interstellar medium.

Organization: CSIRO Data Access Portal
Parkes observations for project P1281 semester 2024OCTS_19

The physical origin of fast radio bursts (FRBs) has been hotly debated over the past decade until the discovery of bright radio bursts from the Galactic magnetar in 2020. The discovery of galactic FRBs has demonstrated that at least some faint FRBs can originate from normal magnetars. So far, only two active FRB repeaters are confirmed to be associated with persistent radio sources, which are normally interpreted as magnetar wind nebulae by theorists. From the most recent observations with the FAST and Parkes telescopes, we observed a particular radio source, VT 1137-0337, and we found several suspicious short-duration single pulse candidates whose dispersion measurements were very close. Notably, the signal found in the Parkes UWL data has a typical pulse width of 1 ms and exhibits an apparent broadband feature. We strongly request continuing to monitor this source with the Parkes UWL receiver, aiming to detect a significant FRB and directly reveal the nature of the active FRB repeaters.

Organization: CSIRO Data Access Portal
VostroNet (Australia) Pty Ltd - Anticipatory notice -13 October 2023 -Docklands VIC (Declared 30 Aug 24)

Statutory Infrastructure Provider (SIP) VostroNet (Australia) Pty Ltd Anticipatory notice given 13 October 2023 and the associated project area data for a contract to provide telecommunications network infrastructure.

Project area: 7-23 Spencer Street, Docklands VIC 3008 

Infrastructure to be installed: FTTP

Estimated completion date: 30 June 2024

Tags: SIP, VostroNet, broadband, statutory infrastructure provider, telecommunications
Organization:  SIP Register - VostroNet (Australia) Pty Ltd