MACS 1423-z7p64

MACS 1423-z7p64 is a galaxy listed in the MAssive Cluster Survey (MACS), and announced (doi:10.1038/s41550-017-0091) on 10 April 2017 in the journal Nature Astronomy,[1] as being the most distant galaxy known at this time, with a redshift z = 7.640 ± 0.001 (lookback time >13.1 Gyr), in the time of Reionization.

Discovery

MACS 1423-z7p64 was discovered through gravitational lensing by MACS J1423.8+2404 (z = 0.545), a cluster that magnified its brightness by a factor of 10. To identify the galaxy, the astronomers used the slitless grism spectrograph of the Wide Field Infrared Survey Telescope on the Hubble Space Telescope, and to determine its distance the Multi-Object Spectrometer for Infra-Red Exploration (MOSFIRE) detector of the Keck Observatory .[1][2]

Nature received the paper on 27 October 2016.)[1]

Importance

With a redshift z = 7.640 ± 0.001, and being an order of magnitude lower in intensity than the four other Lyman-α emitters currently known at z > 7.5, it is probably the most distant representative source of reionization found to date.[1] This is from a time when the universe was around 700 million years old.[2]

References

  1. 1 2 3 4 Spectroscopic confirmation of an ultra-faint galaxy at the epoch of reionization, Austin Hoag et al, Nature, 2017-04-10
  2. 1 2 Astronomers detect ultra-faint galaxy from the very early universe, Genelle Weule, ABC News Online, 2017-04-11
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