Radio continuum sources behind the Large Magellanic Cloud

@article{Filipovic2021RadioCS,
  title={Radio continuum sources behind the Large Magellanic Cloud},
  author={Miroslav D. Filipovi'c and I S Boji{\vc}i{\'c} and Kevin Grieve and Ray P. Norris and Nicholas F. H. Tothill and Devika Shobhana and Lawrence Rudnick and Isabella Prandoni and Heinz Andernach and Natasha Hurley-Walker and Rami Z. E. Alsaberi and C S Anderson and Jordan D Collier and Evan J. Crawford and B-Q For and T J Galvin and F. Haberl and Andrew M. Hopkins and Adriano Ingallinera and Patrick J. Kavanagh and B{\"a}rbel S. Koribalski and R. Kothes and Denis A. Leahy and Howard Leverenz and P Maggi and Chandreyee Maitra and Joshua Marvil and Thomas G. Pannuti and Laurence A. F. Park and Jonathan L. Payne and Clara M. Pennock and Simone Riggi and Gavin Rowell and Hidetoshi Sano and M. Sasaki and Lister Staveley-Smith and Corrado Trigilio and G Umana and Dejan Uro{\vs}evi{\'c} and Jacco Th van Loon and Eleni Vardoulaki},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2021}
}
We present a comprehensive multifrequency catalogue of radio sources behind the Large Magellanic Cloud (LMC) between 0.2 and 20 GHz, gathered from a combination of new and legacy radio continuum surveys. This catalogue covers an area of ∼144 deg2 at angular resolutions from 45 arcsec to ∼3 arcmin. We find 6434 discrete radio sources in total, of which 3789 are detected at two or more radio frequencies. We estimate the median spectral index (α; where Sv ∼ να) of α = −0.89 and mean of −0.88 ± 0… Expand

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