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GN-z11 is a high-redshift galaxy found in the constellation Ursa Major.It is among the farthest known galaxies from Earth ever discovered. [5] [6] The 2015 discovery was published in a 2016 paper headed by Pascal Oesch and Gabriel Brammer (Cosmic Dawn Center).
JADES-GS-z13-0 is the most distant galaxy.. This article documents the most distant astronomical objects discovered and verified so far, and the time periods in which they were so classified.
JADES-GS-z14-0 is a high-redshift Lyman-Break galaxy in the constellation Fornax that was discovered in 2024 using NIRcam as part of the JWST Advanced Deep Extragalactic Survey (JADES) program. [1] [2] It has a redshift of 14.32, making it the most distant galaxy and astronomical object ever discovered.
JADES-GS-z13-0 is a high-redshift Lyman-break galaxy discovered by the James Webb Space Telescope (JWST) during NIRCam imaging for the JWST Advanced Deep Extragalactic Survey (JADES) on 29 September 2022.
MACS1149-JD1 (also known as JD1 and PCB2012 3020) is a young galaxy that is known for being one of the farthest known galaxies from Earth. It was discovered in 2014 and confirmed in 2018. [ 6 ] The JD1 galaxy is at a redshift of about z=9.11, [ 1 ] or about 13.28 billion ly (4.07 billion pc ) away from Earth meaning that it formed when the ...
GRB 090423 was a gamma-ray burst (GRB) detected by the Swift Gamma-Ray Burst Mission on April 23, 2009, at 07:55:19 UTC whose afterglow was detected in the infrared and enabled astronomers to determine that its redshift is z = 8.2, making it one of the most distant objects detected at that time with a spectroscopic redshift (GN-z11, discovered ...
MACS0647-JD is a galaxy with a redshift of about z = 10.7, equivalent to a light travel distance of 13.26 billion light-years (4 billion parsecs).If the distance estimate is correct, it formed about 427 million years after the Big Bang.
The galaxy was observed in August and September 2009. [2] [8] The image data was released to the scientific community, which led to the galaxy's detection by the teams of Bouwens, [1] Bunker [5] and McLure, [6] and subsequent spectroscopic campaign by the team of Lehnert and colleagues. [citation needed]