País 2009Operações (M US$)Instrumentação (M SU$) US UK CA AU BR AR
GMT Technical Overview January GMT Instruments Instrument Conceptual Design RFPsAO modeλ (μm) 1High Contrast IR AO ImagerAO Near-IR High Resolution SpectrographAO & NS High Resolution Visible SpectrographNS High Resolution Near-IR ImagerAO Wide-Field Multi-Object Near-IR SpectrographGLAO Wide-Field Multi-Object Visible SpectrographNS Near-IR Integral Field SpectrographAO Precision Radial Velocity SpectrographNS Facility Multi-Object Fiber SystemNS NIRMOS GMTNIRS GMACS Conceptual design requests for proposals issued June 15. Proposals received 30 October Conceptual design reviews in 2011 Mode: AO= adaptive optics, NS = natural seeing, GLAO = ground layer AO
TMT Early Light Instrument Suite
Critérios: área, localização: Chile e 2 hemisférios, modo fila, instrumentação, custo GMT 24m Chile $ 700M, sem queue, 7M$/ano, 2.6M$/ano oper. 10% TMT 30m Hawaii $1000M, sem queue, 7M$/ano, 3.2M$/ano oper. 10% E-ELT 42m Chile $1300M, queue, 7M$/ano, 3.2M$/ano oper. 5% ESO 42m+4x8m+Alma $185M entrada: (14M$+9M$ oper.)/ano Gemini 2x8m $7M/ano oper. 25% k$/m^2/ano ESO = 21 a 32M$/ano/[(42m)^2+4x(8m)^2] 11.6 k$/m^2/ano 10% E-ELT = 20.4 M$/ano/(42m)^ k$/m^2/ano 10% TMT = 10.2 M$/ano/(30m)^ k$/m^2/ano 10% GMT = 9.6M$/ano/(24m)^ k$/m^2/ano 10% Gemini = 2.8M$/ano/[2x(8m)^2] Comparação