The Mid-Infrared Instrument for the James Webb Space Telescope, II: Design and Build

The Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) provides measurements over the wavelength range 5 to 28.5 μm. MIRI has, within a single "package," four key scientific functions: photometric imaging, coronagraphy, single-source low-spectral resolving power (R ∼ 1...

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Veröffentlicht in:Publications of the Astronomical Society of the Pacific 2015-07, Vol.127 (953), p.595-611
Hauptverfasser: Wright, G. S., Wright, David, Goodson, G. B., Rieke, G. H., Aitink-Kroes, Gabby, Amiaux, J., Aricha-Yanguas, Ana, Azzollini, Ruymán, Banks, Kimberly, Barrado-Navascues, D., Belenguer-Davila, T., Bloemmart, J. A. D. L., Bouchet, Patrice, Brandl, B. R., Colina, L., Detre, Örs, Diaz-Catala, Eva, Eccleston, Paul, Friedman, Scott D., García-Marín, Macarena, Güdel, Manuel, Glasse, Alistair, Glauser, Adrian M., Greene, T. P., Groezinger, Uli, Grundy, Tim, Hastings, Peter, Henning, Th, Hofferbert, Ralph, Hunter, Faye, Jessen, N. C., Justtanont, K., Karnik, Avinash R., Khorrami, Mori A., Krause, Oliver, Labiano, Alvaro, Lagage, P.-O., Langer, Ulrich, Lemke, Dietrich, Lim, Tanya, Lorenzo-Alvarez, Jose, Mazy, Emmanuel, McGowan, Norman, Meixner, M. E., Morris, Nigel, Morrison, Jane E., Müller, Friedrich, Nø rgaard-Nielson, H.-U., Olofsson, Göran, O'Sullivan, Brian, Pel, J.-W., Penanen, Konstantin, Petach, M. B., Pye, J. P., Ray, T. P., Renotte, Etienne, Renouf, Ian, Ressler, M. E., Samara-Ratna, Piyal, Scheithauer, Silvia, Schneider, Analyn, Shaughnessy, Bryan, Stevenson, Tim, Sukhatme, Kalyani, Swinyard, Bruce, Sykes, Jon, Thatcher, John, Tikkanen, Tuomo, van Dishoeck, E. F., Waelkens, C., Walker, Helen, Wells, Martyn, Zhender, Alex
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Sprache:eng
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Zusammenfassung:The Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) provides measurements over the wavelength range 5 to 28.5 μm. MIRI has, within a single "package," four key scientific functions: photometric imaging, coronagraphy, single-source low-spectral resolving power (R ∼ 100) spectroscopy, and medium-resolving power (R ∼ 1500 to 3500) integral field spectroscopy. An associated cooler system maintains MIRI at its operating temperature of
ISSN:0004-6280
1538-3873
1538-3873
DOI:10.1086/682253