VLASS Quick Look and Single Epoch CatalogsWebpage Last Updated - 2023-09-30

The catalogs provided here are based on the VLASS quick look (QL) and the single epoch (SE) imaging completed as of September 2022. All three catalogs consist of a Component Table, a Host ID Table, and a Subtile Information Table that provides metadata on the images used to produce the catalog. In addition, the DRAGNHunter table is available for the QL epoch 1 data. The production of these catalogs, the data models, and the known data quality issues are detailed in the Catalog User Guide, which we strongly urge users to read prior to using the catalogs. The main issues with the data quality include a non-homogeneous on-sky distribution of the rms noise.
Data Limitations/Caveats:

  • A systematic ≈15% underestimation of flux measurements is present for the QL catalogs. We have corrected the astrometric errors that were previously present in the QL epoch one catalog. Consequently, the catalogs are useful for generating source samples and target lists but should be used with extreme caution for further applications.
  • Essential data quality flagging is included, and we recommend that in most cases, people will want to use catalog entries satisfying Duplicate_flag < 2 and Quality_flag == (0 | 4) and S_code!='E' from the Component Table, and P_Host > 0.8 and Source_reliability_flag == 0 from the Host ID Table.
  • The single epoch component table contains spectral index information along with errors revised from those produced by NRAO and independent quality flags to select sources with reliable spectral index values. We encourage users to set Alpha_quality_flag == 1 (read Section 3.2 of the Catalog User Guide) while using the spectral index values provided in the SE catalog.

What's New?

  • Value-added catalog of DRAGNHunter
    We have produced a value-added catalog of Double Radio sources associated with Active Galactic Nuclei (DRAGNs) and single-component radio sources using the VLASS component catalogs. Where possible the likely AllWISE counterpart has been identified for these sources and redshifts have been obtained by querying a number of different optical surveys. The DRAGNs are identified using an automated algorithm DRAGNhunter and, as with all automated algorithms, this introduces some false positive detections into the catalog. Contamination from these spurious DRAGNs is < 3% when using the provided quality flag (and up to 11% without). The data are available as two tables (described below) that can be downloaded below or queried via CADC's TAP service. If you make use of this data or the DRAGNhunter code in your research, we ask that you please cite the journal article A Quick look at the 3GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey (Y. A. Gordon et al., 2023) which describes the methodology and data in full. The table DRAGNhunter_sources contains information on all radio sources identified by DRAGNhunter (single-component and DRAGNs) as well as IR host ID information from AllWISE and redshift information where available. For Epoch 1 this consists of 595,375 radio sources. Of these ≈247,000 have host IDs, > 87,000 with redshifts. The table DRAGNhunter_dragns provides additional information specific to the DRAGNs -- a subset of Table 1. In VLASS Epoch 1 > 17,000 DRAGNs are identified.

  • Morphological annotations using Self-Organizing Map (SOM). With the latest release, we provide the machine learning classifications of each component in the QL 2 and SE catalog based on their morphology using a Self-Organizing Map (SOM). Although the primary goal was to add data quality flags and understand the probability of a component being a sidelobe, these classifications can serve as a valuable resource for users interested in the morphology of VLASS sources. Samples based on morphology can be compiled using the Best Matching Neuron columns in the component catalog. Please refer to the SOM image and sections 3.5 and 3.6 in the Catalog User Guide. Make sure to read 5.3 and 5.4 to learn about issues when selecting a sample.

Catalog User Guide - read before accessing data
A full description of the catalog production, data models and known data quality issues. Users of this catalog are strongly urged to read this document in full prior to accessing the catalog.

The VLASS Catalogs can be accessed via the following routes.

CatalogEpochVersion(catalog, DRAGNHunter)DescriptionComponent TableHost ID TableSubtile Information tableDRAGNHunter Catalog
QL13,1Quick Look epoch 1 catalog of the entire skyData ( ~1 GB )Data( ~110 MB )Data ( ~5 MB ) DRAGNHunter_sources (~ 150 MB) ::- -:: DRAGNHunter_dragns (~ 6 MB)
QL22,1Quick Look epoch 2 catalog of the entire skyData ( ~1 GB)Data ( ~120 MB )Data ( ~5 MB ) DRAGNHunter_sources (~ 120 MB) ::- -:: DRAGNHunter_dragns (~ 5 MB)
SE22,1~1000 sq.deg with ~0.1M rowsData ( ~34 MB )Data ( ~4 MB )Data ( ~150 KB ) DRAGNHunter_sources (~ 880 KB) ::- -:: DRAGNHunter_dragns (~ 43 KB)

Column Definitions

SOM Resources

We provide two ways to access the cutouts.

Software used to produce these catalogs can be used as pipelines in sequence. The links to the software are available at: Link to software

References:

October 2020, Gordon et al.:A Catalog of very Large Array Sky Survey Epoch 1 Quick Look Components, Sources, and Host identifications

August 2021, Gordon et al.:A Quick Look at the 3 GHz Radio Sky 1. Source Statistics from the Very Large Array Sky Survey

March 2023, Gordon et al.:A Quick Look at the 3GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey

Version History for Quick Look epoch2 and Single Epoch data

  • Version 2 (30-Sep-2023): Sidelobe probabilities and the best-matching neurons are now present in the component catalogs.
  • Version 1 (07-Feb-2023): The first version of both Single Epoch and Quick Look epoch 2 component catalogs does not contain sidelobe probabilities. Note: To access version 1 of the QL2 and SE2 catalog, click here.

Version History for DRAGNHunter

  • Version 1 (30-Sep-2023): First version

  • Version History for Quick Look epoch1 data

    • Version 3 (30-Sep-2023): Older versions of the VLASS images contained astrometric errors of up to 1". These images have now been corrected for the astrometric offsets. In addition, some subtiles were re-imaged to remove ghosts. The entire VLASS pipeline was re-run on the corrected images to produce the corrected versions of the component, subtile, and host ID tables.
    • Version 2 (13-Jul-2021): There are some quality control metrics based on our analysis of the data. Table 1 has been updated to correct an unforeseen issue with the data in columns QL_image_RA and QL_image_DEC, referring to the center of the VLASS tile observed - this is distinct from the component RA and DEC, which were unaffected. Only QL_image_RA and QL_image_DC in Table 1 were affected, and all other data presented were accurate. For most users, we recommend using components with Duplicate_flag < 2 and Quality_flag == (0 | 4), which returns approximately 1.8M rows. This includes sidelobe information added to the component table. Four columns were added to the table. We also have additional files generated. Note: To access the older versions of the catalogs click here.
    • Version 1 (06-Jan-2021): The first catalog published contains 3.3M rows.


    Whilst the major problems with the data quality are known and detailed in the Catalog User Guide, this is unlikely to be a comprehensive list of potential issues. Should you encounter problems with this website or data problems beyond what are described in the Catalog User Guide then please reach out to Biny (Biny.Sebastian@umanitoba.ca) or Susan (Susan.Xu@utoronto.ca).