TY - GEN
T1 - The James Webb space telescope
T2 - 2nd International Conference on Space Technology, ICST 2011
AU - Greenhouse, Matthew A.
AU - Mather, John C.
AU - Clampin, Mark
AU - Doyon, Rene
AU - Flanagan, Kathryn A.
AU - Franx, Marijn
AU - Hammel, Heidi B.
AU - Hutchings, John B.
AU - Jakobsen, Peter
AU - Lilly, Simon J.
AU - Lunine, Jonathan I.
AU - McCaughrean, Mark J.
AU - Mountain, Matt
AU - Rieke, George H.
AU - Rieke, Marcia J.
AU - Sonneborn, George
AU - Stiavelli, Massimo
AU - Windhorst, Rogier
AU - Wright, Gillian S.
PY - 2011
Y1 - 2011
N2 - The James Webb Space Telescope (JWST) is the infrared successor to the Hubble Space Telescope. It is a cryogenic infrared space observatory with a 25 m2 aperture (6 m class) telescope yielding diffraction limited angular resolution at a wavelength of 2 um. The science instrument payload includes three passively cooled near-infrared instruments providing broad- and narrow-band imagery, coronagraphy, as well as multi-object and integral-field spectroscopy over the 0.6 < λ < 5.0 um spectrum. An actively cooled mid-infrared instrument provides broad-band imagery, coronagraphy, and integral-field spectroscopy over the 5.0 < λ < 29 um spectrum. The JWST is being developed by NASA, in partnership with the European and Canadian Space Agencies, as a general user facility with science observations to be proposed by the international astronomical community in a manner similar to the Hubble Space Telescope. Technology development and mission design are complete, and construction is underway in all areas of the program.
AB - The James Webb Space Telescope (JWST) is the infrared successor to the Hubble Space Telescope. It is a cryogenic infrared space observatory with a 25 m2 aperture (6 m class) telescope yielding diffraction limited angular resolution at a wavelength of 2 um. The science instrument payload includes three passively cooled near-infrared instruments providing broad- and narrow-band imagery, coronagraphy, as well as multi-object and integral-field spectroscopy over the 0.6 < λ < 5.0 um spectrum. An actively cooled mid-infrared instrument provides broad-band imagery, coronagraphy, and integral-field spectroscopy over the 5.0 < λ < 29 um spectrum. The JWST is being developed by NASA, in partnership with the European and Canadian Space Agencies, as a general user facility with science observations to be proposed by the international astronomical community in a manner similar to the Hubble Space Telescope. Technology development and mission design are complete, and construction is underway in all areas of the program.
UR - http://www.scopus.com/inward/record.url?scp=82055188340&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=82055188340&partnerID=8YFLogxK
U2 - 10.1109/ICSpT.2011.6064655
DO - 10.1109/ICSpT.2011.6064655
M3 - Conference contribution
AN - SCOPUS:82055188340
SN - 9781457718748
T3 - 2nd International Conference on Space Technology, ICST 2011
BT - 2nd International Conference on Space Technology, ICST 2011
Y2 - 15 September 2011 through 17 September 2011
ER -