
Most accurate Statistical Description of Faint Primordial Galaxies 500 M yrs after Big Bang generated
The University of California, Irvine and Baltimore’s Space Telescope Science Institute team describes its use of a new statistical method to analyze Hubble data of lengthy sky surveys. The method enabled the scientists to parse out signals from the noise in Hubble’s deep-sky images, providing the first estimate of the number of small, primordial galaxies in the early universe. There are close to 10X more of these galaxies than were previously detected in deep Hubble surveys.
The period under investigation is called the “epoch of reionization”, post-Big Bang and a few hundred million years in which a dark universe was dominated by photon-absorbing neutral hydrogen, the epoch of reionization...
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