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Volumn , Issue 577, 2005, Pages 3-10

Herschel mission: Status and observing opportunities

Author keywords

Galaxies: evolution, formation ISM; Infrared: galaxies, stars; ISM: jets and outflows, molecules; Space vehicles: instrumentation, cryostat; Stars: early type, formation, late type, pre main sequence, winds, outflows; Submillimetre

Indexed keywords

ASTRONOMY; DECISION MAKING; GALAXIES; JETS; LAUNCHING; SCHEDULING; SPACE APPLICATIONS; SPECTROMETERS;

EID: 23844492905     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper
Times cited : (5)

References (15)
  • 2
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    • The Herschel HIFI instrument
    • in The Dusty and Molecular Universe, A. Wilson, ed. (this volume)
    • T. de Graauw and the HIFI Consortium, 'The Herschel HIFI Instrument', in The Dusty and Molecular Universe, A. Wilson, ed., ESA. SP-577 (this volume)
    • ESA , vol.SP-577
    • De Graauw, T.1
  • 3
    • 33645361037 scopus 로고    scopus 로고
    • The Herschel SPIRE instrument
    • The Dusty and Molecular Universe, A. Wilson, ed. (this volume)
    • M.J. Griffin and the SPIRE Consortium, 'The Herschel SPIRE Instrument' in The Dusty and Molecular Universe, A. Wilson, ed., ESA. SP-577 (this volume)
    • ESA , vol.SP-577
    • Griffin, M.J.1
  • 4
    • 33645373184 scopus 로고    scopus 로고
    • ESA/SPC(97)22, rev.1; approved by the SPC in August 1997; available online
    • 'Herschel Science Management Plan', ESA/SPC(97)22, rev.1; approved by the SPC in August 1997; available online
    • Herschel Science Management Plan
  • 5
    • 10044277583 scopus 로고    scopus 로고
    • Herschel/HSC/ DOC/0369; v1.1; available online
    • 'Herschel Observing Programmes', Herschel/HSC/ DOC/0369; v1.1, 2004; available online
    • (2004) Herschel Observing Programmes
  • 8
    • 0009715924 scopus 로고    scopus 로고
    • Orion proplyds and the Eagle's eggs
    • Herbig-Haro Flows and the Birth of Stars, B. Reipurth, C. Bertout, eds
    • M.J. McCaughrean, 'Orion Proplyds and the Eagle's Eggs', in Herbig-Haro Flows and the Birth of Stars, B. Reipurth, C. Bertout, eds, Proc. IAU Symp. 182, pp. 551-560, 1997
    • (1997) Proc. IAU Symp. , vol.182 , pp. 551-560
    • McCaughrean, M.J.1
  • 9
    • 0038739404 scopus 로고    scopus 로고
    • The current status of the Herschel/Planck programme
    • IR Space Telescope and Instruments, J.C. Mather, ed.
    • T. Passvogel, J.-J. Juillet, 'The current status of the Herschel/Planck programme', in IR Space Telescope and Instruments, J.C. Mather, ed., Proc. SPIE 4850 pp. 598-605, 2003
    • (2003) Proc. SPIE , vol.4850 , pp. 598-605
    • Passvogel, T.1    Juillet, J.-J.2
  • 12
    • 33645341853 scopus 로고    scopus 로고
    • The Photodetector Array Camera and Spectrometer (PACS) for the Herschel space observatory'
    • The Dusty and Molecular Universe, A. Wilson, ed. (this volume)
    • A. Poglitsch and the PACS Consortium, "The Photodetector Array Camera and Spectrometer (PACS) for the Herschel Space Observatory', in The Dusty and Molecular Universe, A. Wilson, ed., ESA. SP-577 (this volume)
    • ESA , vol.SP-577
    • Poglitsch, A.1
  • 13
    • 0038401234 scopus 로고    scopus 로고
    • A 3.5 m diameter SiC telescope for the Herschel mission
    • IR Space Telescopes and Instruments, J.C. Mather, ed.
    • E. Sein, Y. Toulemont, F. Safa, M. Duran, P. Deny, D. de Chambure, G.L. Pilbratt, 'A 3.5 m diameter SiC telescope for the Herschel mission', in IR Space Telescopes and Instruments, J.C. Mather, ed., Proc. SPIE 4850 pp. 606-618, 2003
    • (2003) Proc. SPIE , vol.4850 , pp. 606-618
    • Sein, E.1    Toulemont, Y.2    Safa, F.3    Duran, M.4    Deny, P.5    De Chambure, D.6    Pilbratt, G.L.7
  • 14
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    • Cosmic vision, the new ESA plan for space science
    • IR Space Telescopes and Instruments, J.C. Mather, ed.
    • S. Volonte, 'Cosmic Vision, the new ESA plan for Space Science', in IR Space Telescopes and Instruments, J.C. Mather, ed., Proc. SPIE 4850, pp. 1-11, 2003
    • (2003) Proc. SPIE , vol.4850 , pp. 1-11
    • Volonte, S.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.