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arXiv:1805.04317astro-ph.GA

Discovery of the most ultra-luminous QSO using Gaia, SkyMapper and WISE

Christian Wolf, Fuyan Bian, Christopher A. Onken, Brian P. Schmidt, Patrick Tisserand, Noura Alonzi, Wei Jeat Hon, John L. Tonry

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Abstract

We report the discovery of the ultra-luminous QSO SMSS~J215728.21-360215.1 with magnitude $z=16.9$ and W4$=7.42$ at redshift 4.75. Given absolute magnitudes of $M_{145,\rm AB}=-29.3$, $M_{300,\rm AB}=-30.12$ and $\log L_{\rm bol}/L_{\rm bol,\odot} = 14.84$, it is the QSO with the highest unlensed UV-optical luminosity currently known in the Universe. It was found by combining proper-motion data from Gaia DR2 with photometry from SkyMapper DR1 and the Wide-field Infrared Survey Explorer (WISE). In the Gaia database it is an isolated single source and thus unlikely to be strongly gravitationally lensed. It is also unlikely to be a beamed source as it is not discovered in the radio domain by either NVSS or SUMSS. It is classed as a weak-emission-line QSO and possesses broad absorption line features. A lightcurve from ATLAS spanning the time from October 2015 to December 2017 shows little sign of variability.

arXiv comments
6 pages, 4 figures, accepted for publication in PASA
Journal reference
DOI
doi:10.1017/pasa.2018.22
Subjects
astro-ph.GAAstrophysics of Galaxies astro-ph.COCosmology and Nongalactic Astrophysics

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Linked by 1 identifiable commenter in 1 comment across 1 thread, from May 2018 to May 2018. Found in 1 HN submission from May 2018 to May 2018. Open submission discussions.

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    • "Discovery of the most ultra-luminous QSO using Gaia, SkyMapper and WISE" Publications of the Astronomical Society of Australia (PASA) free PDF version: https://arxiv.org/pdf/1805.04317.pdf

      methatswhoView on HNParent context

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