Search: id:"swepub:oai:lup.lub.lu.se:f904cee4-902e-4d8c-b162-d56f2fb1b2a9" > Instruments for a E...
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000 | 03909naa a2200397 4500 | |
001 | oai:lup.lub.lu.se:f904cee4-902e-4d8c-b162-d56f2fb1b2a9 | |
003 | SwePub | |
008 | 160404s2004 | |||||||||||000 ||eng| | |
024 | 7 | a https://lup.lub.lu.se/record/5284682 URI |
024 | 7 | a https://doi.org/10.1117/12.5514732 DOI |
040 | a (SwePub)lu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a kon2 swepub-publicationtype |
072 | 7 | a ref2 swepub-contenttype |
100 | 1 | a Russell, Adrian P.4 aut |
245 | 1 0 | a Instruments for a European Extremely Large Telescope: the challenges of designing instruments for 30- to 100-m telescopes |
264 | 1 | b SPIE,c 2004 |
520 | a Designs for Extremely Large Telescopes (ELTs) are quite well advanced,but the requirements of instruments have had limited impact. Sinceprovision of a suitable environment for instruments is a critical aspectof all telescopes, we outline some well-known and some less-appreciatedchallenges of designing instruments for ELTs. A wide-field spectrometer(WFSPEC) with ~10 arcmin field-of-view, probably with AO correction ofground-layer seeing, illustrates the well-known difficulty of matchingmodern detector pixels to large (~0."3) images. The challenges ofexploiting wide-field (1'-2' FOV) high-performance AO systems on ELTsare illustrated by a Multi-Object Multi-field Spectrometer and Imager(MOMSI), which provides imaging and integral-field spectroscopy, atnear-diffraction-limited pixel scales, of targets in approximately 300subfields each. This instrument, roughly equivalent to all theastronomical spectrometers yet built, extracts ~200 times less of theavailable information from the ELT's FOV than near-future instruments on8-m class telescopes will do for their hosts. We emphasise the greatsize of such instruments (40-100 tonnes, 100-200 m3) and the need toaccommodate this size in telescope plans. A third area of challenge isthe exploitation of the potential capabilities of ELTs in the mid-IR,where they would offer powerful complements to JWST and ALMA;low-emissivity telescope designs and, possibly, cryogenic AO, may beneeded. Finally, we outline the potential challenges of correctingatmospheric dispersion effects. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
700 | 1 | a Monnet, Guy4 aut |
700 | 1 | a Quirrenbach, Andreas4 aut |
700 | 1 | a Bacon, Roland4 aut |
700 | 1 | a Redfern, Michael4 aut |
700 | 1 | a Andersen, Torbenu Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science4 aut0 (Swepub:lu)astr-tan |
700 | 1 | a Ardeberg, Arneu Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science4 aut0 (Swepub:lu)astr-aar |
700 | 1 | a Atad-Ettedgui, Eli4 aut |
700 | 1 | a Hawarden, Timothy G.4 aut |
700 | 1 | a Moorwood, Alan F. M.4 edt |
700 | 1 | a Iye, Masanori4 edt |
710 | 2 | a Astronomi - Genomgår omorganisationb Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation4 org |
773 | 0 | t Ground-based instrumentation for astronomy (Proceedings of the SPIE)d : SPIEg 5492, s. 1796-1809q 5492<1796-1809z 0819454249 |
856 | 4 | u http://dx.doi.org/10.1117/12.551473y FULLTEXT |
856 | 4 8 | u https://lup.lub.lu.se/record/528468 |
856 | 4 8 | u https://doi.org/10.1117/12.551473 |
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