SCORPIO field's study with ASKAP Virtual Observatory Resource

Authors
  1. Umana G.
  2. Trigilio C.
  3. Ingallinera A.
  4. Riggi S.
  5. Cavallaro F.
  6. Marvil J.,Norris R.P.
  7. Hopkins A.M.
  8. Buemi C.S.
  9. Bufano F.
  10. Leto P.
  11. Loru S.,Bordiu C.
  12. Bunton J.D.
  13. Collier J.D.
  14. Filipovic M.
  15. Franzen T.M.O.,Thompson M.A.
  16. Andernach H.
  17. Carretti E.
  18. Dai S.
  19. Kapinska A.,Koribalski B.S.
  20. Kothes R.
  21. Leahy D.
  22. McConnell D.
  23. Tothill N.,Michalowski M.J.
  24. Published by
    CDS
Abstract

In the broad context of the Australian Square Kilometer Array Pathfinder (ASKAP) early-science phase and preparation for the related surveys, we report the first radio observations towards the Galactic plane. The targeted field was chosen to encompass the entire SCORPIO survey, one of the several pathfinder projects for the Evolutionary Map of the Universe survey planned with the ASKAP. The observations were carried out in 2018 January at a central frequency of 912 MHz, with 15 operational antennas, and covered a total area of about 40 square degrees in three different pointings. The final image has a resolution of 24.1 * 21.1 arcsec^2^ and a median rms of 541 {mu}Jy/beam. We were able to extract 3545 candidate sources, 75 per cent of them point sources. For a preliminary validation, a comparison with the 843 MHz Molonglo Galactic Plane Survey is presented. Although the present observations were obtained with the ASKAP only partially deployed, its unique capability to map complex sources, such as those inhabiting the Galactic plane, at different angular scales, is highlighted. Within the SCORPIO field all the previously classified H II regions, Planetary Nebulae (PNe), and supernovae remnants (SNRs), previously known to be radio sources, were detected. We also report new radio detections from several H II regions previously classified as 'candidates' or 'radio quiet' and from half of all the PNe in the SCORPIO field with robust classification. Most notably, we find numerous unclassified, extended sources which constitute a promising sample of candidates H II regions and SNRs.

Keywords
  1. milky-way-galaxy
  2. planetary-nebulae
  3. supernova-remnants
  4. h-ii-regions
  5. galaxy-planes
  6. radio-sources
  7. photometry
Bibliographic source Bibcode
2021MNRAS.506.2232U
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/506/2232
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/506/2232

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/506/2232
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/506/2232
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/506/2232
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/506/2232/table2?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/506/2232/table2?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/506/2232/table2?

History

2024-06-24T13:31:07Z
Resource record created
2024-06-24T12:34:25Z
Updated
2024-06-24T13:31:07Z
Created

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr