OWL IR MOS study
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OWL IR MOS study OWL IR MOS study Study lead : Jean-Gabriel Study lead : Jean-Gabriel Cuby Cuby LAM (Marseille), CRAL (Lyon), LAM (Marseille), CRAL (Lyon), OPM (Meudon), ONERA OPM (Meudon), ONERA ESO: M.Casali ESO: M.Casali
description
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 ?. - PowerPoint PPT Presentation
Transcript of OWL IR MOS study
OWL IR MOS studyOWL IR MOS study
Study lead : Jean-Gabriel CubyStudy lead : Jean-Gabriel Cuby
LAM (Marseille), CRAL (Lyon), LAM (Marseille), CRAL (Lyon), OPM (Meudon), ONERAOPM (Meudon), ONERA
ESO: M.CasaliESO: M.Casali
1. Why an IR MOS ?1. Why an IR MOS ?
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
2. Field information 2. Field information
MCAO Strehl>80% at K over 5 MCAO Strehl>80% at K over 5 arcminutesarcminutes
TelescopeTelescope Res Res elements/fieldelements/field
OWLOWL 7 x 107 x 1088 at K at K
Schmidt plateSchmidt plate 5 x 105 x 1088 massive instrumentation challenge to use the photons gathered
