The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue

@article{White2020TheG4,
  title={The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue},
  author={Sarah V. White and Thomas M. O. Franzen and Chris J. Riseley and O. Ivy Wong and Anna D. Kapi'nska and Natasha Hurley-Walker and Joseph Russell Callingham and Kshitij Thorat and Chen Wu and Paul J. Hancock and Richard W. Hunstead and Nick Seymour and Jesse G. Swan and Randall B. Wayth and John Morgan and Rajan Thapa Chhetri and Carole Jackson and Stuart Weston and Martin Bell and B. For and Bryan M. Gaensler and Melanie Johnston-Hollitt and Andr'e Offringa and Lister Staveley-Smith},
  journal={arXiv: Astrophysics of Galaxies},
  year={2020}
}
  • Sarah V. White, Thomas M. O. Franzen, +21 authors Lister Staveley-Smith
  • Published 2020
  • Physics
  • arXiv: Astrophysics of Galaxies
  • The Murchison Widefield Array (MWA) has observed the entire southern sky (Declination, $\delta $ 10 deg) to define the GLEAM 4-Jy (G4Jy) Sample. This is a complete sample of the 'brightest' radio-sources ($S_{\mathrm{151MHz}} >$ 4 Jy), the majority of which are active galactic nuclei with powerful radio-jets. Crucially, low-frequency observations allow the selection of such sources in an orientation-independent way (i.e. minimising the bias caused by Doppler boosting, inherent in high-frequency… CONTINUE READING

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