SwePub
Sök i LIBRIS databas

  Utökad sökning

WFRF:(Bongiorno L)
 

Sökning: WFRF:(Bongiorno L) > (2010-2014) > 4MOST - 4-metre mul...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00006511naa a2201525 4500
001oai:DiVA.org:uu-195464
003SwePub
008130225s2012 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1954642 URI
024a https://doi.org/10.1117/12.9262392 DOI
040 a (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a kon2 swepub-publicationtype
100a De Jong, R. S.4 aut
2451 0a 4MOST - 4-metre multi-object spectroscopic telescope
264 1b SPIE,c 2012
338 a print2 rdacarrier
500 a Sponsors: The Society of Photo-Optical Instrumentation Engineers (SPIE)
520 a The 4MOST consortium is currently halfway through a Conceptual Design study for ESO with the aim to develop a wide-field (>3 square degree, goal >5 square degree), high-multiplex (>1500 fibres, goal 3000 fibres) spectroscopic survey facility for an ESO 4m-class telescope (VISTA). 4MOST will run permanently on the telescope to perform a 5 year public survey yielding more than 20 million spectra at resolution R∼5000 (λ=390-1000 nm) and more than 2 million spectra at R∼20,000 (395-456.5 nm & 587-673 nm). The 4MOST design is especially intended to complement three key all-sky, space-based observatories of prime European interest: Gaia, eROSITA and Euclid. Initial design and performance estimates for the wide-field corrector concepts are presented. Two fibre positioner concepts are being considered for 4MOST. The first one is a Phi-Theta system similar to ones used on existing and planned facilities. The second one is a new R-Theta concept with large patrol area. Both positioner concepts effectively address the issues of fibre focus and pupil pointing. The 4MOST spectrographs are fixed configuration two-arm spectrographs, with dedicated spectrographs for the high- and low-resolution fibres. A full facility simulator is being developed to guide trade-off decisions regarding the optimal field-of-view, number of fibres needed, and the relative fraction of high-to-low resolution fibres. The simulator takes mock catalogues with template spectra from Design Reference Surveys as starting point, calculates the output spectra based on a throughput simulator, assigns targets to fibres based on the capabilities of the fibre positioner designs, and calculates the required survey time by tiling the fields on the sky. The 4MOST consortium aims to deliver the full 4MOST facility by the end of 2018 and start delivering high-level data products for both consortium and ESO community targets a year later with yearly increments.
653 a eROSITA
653 a Euclid
653 a Facility simulator
653 a Fibre postioner
653 a Gaia
653 a NTT telescope
653 a VISTA telescope
653 a Wide field corrector
653 a Wide-field multi-object spectrograph facility
653 a Multi-object spectrograph
653 a Wide field
653 a Astronomy
653 a Conceptual design
653 a Optical telescopes
653 a Simulators
653 a Spectrographs
653 a Surveys
653 a Telescopes
653 a Fibers
700a Bellido-Tirado, O.4 aut
700a Chiappini, C.4 aut
700a Depagne, É.4 aut
700a Haynes, R.4 aut
700a Johl, D.4 aut
700a Schnurr, O.4 aut
700a Schwope, A.4 aut
700a Walcher, J.4 aut
700a Dionies, F.4 aut
700a Haynes, D.4 aut
700a Kelz, A.4 aut
700a Kitaura, F. S.4 aut
700a Lamer, G.4 aut
700a Minchev, I.4 aut
700a Müller, V.4 aut
700a Nuza, S. E.4 aut
700a Olaya, J. -C4 aut
700a Piffl, T.4 aut
700a Popow, E.4 aut
700a Steinmetz, M.4 aut
700a Ural, U.4 aut
700a Williams, M.4 aut
700a Winkler, R.4 aut
700a Wisotzki, L.4 aut
700a Ansorge, W. R.4 aut
700a Banerji, M.4 aut
700a Solares, E. G.4 aut
700a Irwin, M.4 aut
700a Kennicutt Jr., R. C.4 aut
700a King, D.4 aut
700a McMahon, R.4 aut
700a Koposov, S.4 aut
700a Parry, I. R.4 aut
700a Sun, D.4 aut
700a Walton, N. A.4 aut
700a Finger, G.4 aut
700a Iwert, O.4 aut
700a Krumpe, M.4 aut
700a Lizon, J. -L4 aut
700a Vincenzo, M.4 aut
700a Amans, J. -P4 aut
700a Bonifacio, P.4 aut
700a Cohen, M.4 aut
700a Francois, P.4 aut
700a Jagourel, P.4 aut
700a Mignot, S. B.4 aut
700a Royer, F.4 aut
700a Sartoretti, P.4 aut
700a Bender, R.4 aut
700a Grupp, F.4 aut
700a Hess, H. -J4 aut
700a Lang-Bardl, F.4 aut
700a Muschielok, B.4 aut
700a Böhringer, H.4 aut
700a Boller, T.4 aut
700a Bongiorno, A.4 aut
700a Brusa, M.4 aut
700a Dwelly, T.4 aut
700a Merloni, A.4 aut
700a Nandra, K.4 aut
700a Salvato, M.4 aut
700a Pragt, J. H.4 aut
700a Navarro, R.4 aut
700a Gerlofsma, G.4 aut
700a Roelfsema, R.4 aut
700a Dalton, G. B.4 aut
700a Middleton, K. F.4 aut
700a Tosh, I. A.4 aut
700a Boeche, C.4 aut
700a Caffau, E.4 aut
700a Christlieb, N.4 aut
700a Grebel, E. K.4 aut
700a Hansen, C.4 aut
700a Koch, A.4 aut
700a Ludwig, H. -G4 aut
700a Quirrenbach, A.4 aut
700a Sbordone, L.4 aut
700a Seifert, W.4 aut
700a Thimm, G.4 aut
700a Trifonov, T.4 aut
700a Helmi, A.4 aut
700a Trager, S. C.4 aut
700a Feltzing, S.4 aut
700a Korn, Andreasu Uppsala universitet,Observationell astrofysik4 aut0 (Swepub:uu)ankor103
700a Boland, W.4 aut
710a Uppsala universitetb Observationell astrofysik4 org
773t Proceedings of SPIE - The International Society for Optical Engineeringd : SPIEg , s. 84460T-q <84460T-z 9780819491473
856u http://arxiv.org/pdf/1206.6885
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-195464
8564 8u https://doi.org/10.1117/12.926239

Hitta via bibliotek

Till lärosätets databas

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Stäng

Kopiera och spara länken för att återkomma till aktuell vy