The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources

@article{White2020TheG4,
  title={The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources},
  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 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, +20 authors Lister Staveley-Smith
  • Published 2020
  • Physics
  • arXiv: Astrophysics of Galaxies
  • The entire southern sky (Declination, $\delta $ 4 Jy) in the extragalactic catalogue (Galactic latitude, $|b| >$ 10 deg). We refer to these 1,863 sources as the GLEAM 4-Jy (G4Jy) Sample, and use radio images (of $\leq$ 45-arcsec resolution), and multi-wavelength information, to assess their morphology and identify the galaxy that is hosting the radio emission (where appropriate). Details of how to access all of the overlays used for this work are available at this https URL. Alongside this we… CONTINUE READING

    References

    Publications referenced by this paper.
    SHOWING 1-7 OF 7 REFERENCES

    2015, in The Many Facets of Extragalactic Radio Surveys: Towards New Scientific Challenges

    • C AJackson
    • 2015
    VIEW 11 EXCERPTS
    HIGHLY INFLUENTIAL

    APLpy: Astronomical Plotting Library in Python

    • T. Robitaille, E. Bressert
    • 2012

    SAOImage DS9: A utility for displaying astronomical images in the X11 window environment

    • Smithsonian Astrophysical Observatory
    • 2000