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DTSTAMP:20261112T104901Z
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DTSTART:20261130T110000
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DESCRIPTION:The Lyman alpha forest provides a rich probe of the intergalact
 ic medium (IGM) during the late stages of the Epoch of Reionization (EoR).
   Regardless of the model used\, recent analyses have shown that the fores
 t data require a late end to the EoR and a very slow evolution of the ioni
 zing emissivity at z<~6.  These requirements are very difficult to satisfy
  without: (i) reionization driven by faint galaxies\; and (ii) a recombina
 tion-regulated ending (so-called "soft-landing"). Despite early claims to 
 the contrary\, these implications from the Lyman alpha forest are actually
  consistent with the latest analysis of Lyman alpha emitters from Subaru\,
  as well as the UV luminosity functions and angular correlation functions 
 from JWST.\n
LOCATION:ETH Zürich\, Hönggerberg HIT J 43.1
ORGANIZER:Andrei Albert Mesinger 
SUMMARY:What we know about cosmic reionization and the galaxies that drove 
 it
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