QSO J0439+1634, often referred to by just its coordinates, J0439+1634 or J043947.08+163415.7, is a superluminous quasar, and was, until 20 February 2024, (when it was superseded by QSO J0529-4351) considered the brightest quasar in the early universe with a redshift of z = 6.51. It is approximately 12.873 billion light-years away. The brightness of the quasar is equivalent to about 600 trillion luminosities of the Suns with gravitational lensing, without this effect 11 trillion. The quasar-related supermassive black hole has a mass of 700 million solar masses.
Discovery On April 3, 2018, the ACS/WFC observed and photographed gravitational lensing at the location of the quasar, and further research revealed an extremely bright and large quasar there.
References
Further reading "Astronomers Uncover the Brightest Lensed Quasar in the Early Universe – W. M. Keck Observatory". 9 January 2019. Archived from the original on 2021-06-24. Retrieved 2021-06-21. Mara Johnson-Groh 09 January 2019 (9 January 2019). "Ultrabright Quasar Lit Up the Early Universe". livescience.com. Archived from the original on 2021-06-24. Retrieved 2021-06-21.{{cite web}}: CS1 maint: numeric names: authors list (link) "Гравитационное линзирование: квазар J043947.08+163415.7" [Gravitational lensing: Quasar J043947.08+163415.7]. VideoNews | Последние новости с видео (in Russian). VideoNews. 2019-03-24. Archived from the original on 2021-06-24. Retrieved 2021-06-21.



