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OWL IR MOS study

OWL IR MOS study. Study lead : Jean-Gabriel Cuby LAM (Marseille), CRAL (Lyon), OPM (Meudon), ONERA ESO: M.Casali. Search for Reionization at z=8-19 Ly α in J to K  IR ~ 100 AGN/Quasars per OWL field  MOS Detect Orion at Z=3 abundances/gradients  IFU. 1. Why an IR MOS ?.

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OWL IR MOS study

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  1. OWL IR MOS study Study lead : Jean-Gabriel Cuby LAM (Marseille), CRAL (Lyon), OPM (Meudon), ONERA ESO: M.Casali

  2. Search for Reionization at z=8-19 Ly α in J to K  IR ~ 100 AGN/Quasars per OWL field  MOS Detect Orion at Z=3 abundances/gradients  IFU 1. Why an IR MOS ?

  3. 2. Field information MCAO Strehl>80% at K over 5 arcminutes TelescopeRes elements/field OWL 7 x 108 at K Schmidt plate 5 x 108  massive instrumentation challenge to use the photons gathered

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