The Mid-Infrared Instrument for theJames Webb Space Telescope, V: Predicted Performance of the MIRI Coronagraphs-Reference-Cited by-同舟云学术

The Mid-Infrared Instrument for theJames Webb Space Telescope, V: Predicted Performance of the MIRI Coronagraphs

Published:2015-07 Issue:953 Volume:127 Page:633-645
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:Publications of the Astronomical Society of the Pacific

Author:

Boccaletti A.,Lagage P.-O.,Baudoz P.,Beichman C.,Bouchet P.,Cavarroc C.,Dubreuil D.,Glasse Alistair,Glauser A. M.,Hines D. C.,Lajoie C.-P.,Lebreton J.,Perrin M. D.,Pueyo L.,Reess J. M.,Rieke G. H.,Ronayette S.,Rouan D.,Soummer R.,Wright G. S.

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference29 articles.

1. The Limiting Effects of Dust in Brown Dwarf Model Atmospheres

2. Feasibility of the Four‐Quadrant Phase Mask in the Mid‐Infrared on theJames Webb Space Telescope

3. The Four‐Quadrant Phase Mask Coronagraph. IV. First Light at the Very Large Telescope

4. VLT/NACO coronagraphic observations of fine structures in the disk ofβ Pictoris

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