peak star-formation epoch
(peak epoch, peak epoch of star formation, peak star-formation era, cosmic high noon, cosmic noon)
(around 10 billion years ago when star formation peaked)
The peak epoch of star formation
(aka cosmic high noon and other variants of these phrases)
on the order of 10 billion years ago (lookback time)
at a redshift on the order of 2,
is the time when star formation across the
universe was at its highest,
i.e., the peak in a star-formation-history graph.
Terms regarding galaxies such as peak galaxy-formation epoch
mean basically the same thing, the term used being a matter of
preference of the writer.
The peak epoch is determined by surveying the star formation rate across
the sky, across redshifts, using normal star formation rate estimation
methods adjusted for redshift. Much of the star formation in this
epoch appears within the disks of galaxies.
(cosmology,star formation,galaxies,star formation rate)
Further reading:
https://ui.adsabs.harvard.edu/abs/2014ARA%26A..52..415M/abstract
https://sese.asu.edu/sites/default/files/erb_asu_colloq.pdf
https://ned.ipac.caltech.edu/level5/March14/Madau/Madau5.html
Redshift | Parsecs /Distance | Lightyears /Lookback Years | | |
2 | 3.43Gpc | 11.18Gly | | peak star-formation epoch |
|
Referenced by pages:
accretion rate
Balmer-break galaxy (BBG)
epoch of galaxy formation
globular cluster (GC)
star formation history (SFH)
star formation rate (SFR)
star-formation rate stellar-mass ratio
Index