1 / 3

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 ?.

curt
Download Presentation

OWL IR MOS study

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  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

More Related