Telescope Optical Design - inaoe

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Wide-field 0.8 FoV
WFCAM (UKIDSS) ‣ 3.8 m UK InfraRed <strong>Telescope</strong> ‣ Started operations in May 2005 ‣ Built by the ATC (Edinburgh) ‣ 4 2048 2 Rockwell detectors (0.4”/pixel) ‣ 0.21 square degree/exposure ‣ ZYJHK filters ‣ Data release 3 (2007)
Page 1 and 2: Synoptic All-Sky Infrared Survey Te
Page 3 and 4: SASIR dedicated telescope A new lar
Page 5 and 6: SPM-Twin: Competitiveness based on
Page 7 and 8: FWHM ["] FWHM ["] SPM-Twin: 1.5°-2
Page 9 and 10: Diameter [mm] SPM-Twin: WF Telescop
Page 11 and 12: SPM-Twin: WFT Atmospheric Dispersio
Page 13 and 14: 100 cm S P M 6.5m f/4.5 WFT Effecti
Page 15 and 16: Infrared emission Mauna Kea atmosph
Page 17: SASIR pre-conceptual design Tels ex
Page 23: Normal Field 9’ FoV (0.075)
Page 27: f/2.5
Page 32 and 33: Relevant issues to cover by the opt
Page 34 and 35: Thanks!
Page 36 and 37: ‣ Input from the community (diver
Page 38 and 39: Resolving power SPM-Twin: Wide-Fiel
Page 40 and 41: Sitios privilegiados para el visibl
Page 42 and 43: Algunos de los primarios de hoy 67t
Page 44 and 45: Basic Survey ‣ ~ 20 sec dithered
Page 46: Technical Concept (Detectors)
Page 49 and 50: M US$ 1 st order estimate Need IR-C
Page 51 and 52: Detectors ‣ The cost of large for
Page 53 and 54: Cost [FY2008 $Million] Telescopios
Page 57 and 58: Cost [FY2008 $Million] Very LargeTe
Page 61 and 62: Cost [FY2008 $Million] Cost-Apertur
Page 63 and 64: Previous work $ ~ D 2.6 (Smith-Kale
Page 65 and 66: Cost [FY2008 $Million] 1000.0 100.0
Page 67 and 68: Distribución de costos de inversi
Page 69: Operación ‣ Varían entre el 7%

Telescope Optical Design - inaoe

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