AS103 (ASKAP Pilot Survey for POSSUM): reprocessed cubes with off-axis leakage correction

  • Yik Ki Ma (Creator)
  • Tessa Vernstrom (Creator)
  • Takuya Akahori (Creator)
  • Alec J.M. Thomson (Creator)
  • Craig Anderson (Creator)
  • Xiaohui Sun (Creator)
  • Russ Taylor (Creator)
  • Cameron Van Eck (Creator)
  • Lisa Harvey-Smith (Creator)
  • Anthony C. Willis (Creator)
  • Jennifer West (Creator)
  • Jeroen Stil (Creator)
  • Lawrence Rudnick (Creator)
  • Wasim Raja (Creator)
  • Cormac R. Purcell (Creator)
  • Shane P. O'Sullivan (Creator)
  • Naomi McClure-Griffiths (Creator)
  • J Patrick Leahy (Creator)
  • Tom Landecker (Creator)
  • George Heald (Creator)
  • Jamie Farnes (Creator)
  • Ettore Carretti (Creator)
  • Shea D. Brown (Creator)
  • Bryan Gaensler (Creator)
  • Shannon Vanderwoude (Creator)

Dataset

Description

This collection contains post-processed image cubes from the POlarization Sky Survey of the Universe’s Magnetism (POSSUM) Pilot 1 survey. These data products include Stokes IQU cubes and corresponding weight cubes for the 10 Pilot 1 survey ASKAP observations. These data are a combination of 10 separate but contiguous 36-beam observations centered on RA (J2000) 321.815° and Dec (J2000) −54.670°. Each field had an integration time of ten hours and the beams were formed in the closepack36 footprint. The survey was observed at full resolution at the ASKAP mid-band frequency range (1152 – 1439 MHz) and averaged to a 288 MHz bandwidth with 1-MHz channel width. The lower half of the band was discarded due to RFI, leaving only the upper 144 frequency channels (1295 – 1439 MHz). These cubes have been leakage corrected using a source based method that involves stacking the 10 observations beam by beam, and fitting residuals with Zernike polynomials to map intensity as a function of distance from the centre of the beam. The cubes have also been convolved to a common 13”x13” resolution across all channels.
Date made available18 Mar 2024
PublisherCSIRO Publishing

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