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Title: ETC and per<strong>for</strong>mance analysis Reference: MUSE-MEM-SCI-051 Issue: 1.3 Date: 28/01/04 Page: 51/14 15.1.3.2 Line emission source ( ( ) EE spa λ ) K Obj ( λ) := K O FracE spec k spec , ( ), 1, 1 , λ, AM ( ) K Sky ( λ) := K S k spec ⋅∆ spec , k spa_poor ⋅∆ WFspa , λ K RN K DC 2 := k spa_poor ⋅ kspec := K RN ( ) LimFLineWFgenI poor ( λ) := F O SN lim , n exp , t exp , F Sky ( λ) , RN CCD , DN CCD , K Obj ( λ) , K Sky ( λ) , K RN , K DC 2 . 10 18 1.37 . 10 18 LimFLineWFgenI poor ( λ) erg⋅s − 1 ⋅cm − 2 7.33 . 10 19 1 .10 19 0.4 0.5 0.6 0.7 0.8 0.9 1 λ µm LimVFLineWFgenI poori := LimFLineWFgenI poor ⎛ λ MUSEi ⎞ ⎝ ⎠ i := 0.. 4 ⎛ ⎜ 2.109× 10 − 18 ⎛ "B" ⎜ 6.908× 10 − 19 ⎟ ⎜ "V" ⎜ ⎟ LimVFLineWFgenI poor ⎜ 4.596× 10 − 19 ⎟ erg⋅s − 1 cm − 2 ⎜ = ⋅ Band MUSE = ⎜ "R" ⎜ ⎟ ⎜ 4.177× 10 − 19 ⎜ "I" ⎟ ⎜ ⎜ 5.293× 10 − 19 ⎝ "z" ⎝ ⎞ ⎠ ⎞ ⎟ ⎟ ⎟ ⎠ back ( ) FN( λ) := FNoise LimFLineWFgenI poor ( λ) , n exp , t exp , F Sky ( λ) , RN CCD , DN CCD , K Obj ( λ) , K Sky ( λ) , K RN , K DC FN( λ V ) ⎛ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎝ 9.05× 10 − 3 0.752 ⎞ ⎟ ⎟ = 0.201 FN λ ⎟ R 0.038 ⎟ 0.239 ⎠ ( ) ⎛ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎝ 8.661× 10 − 3 0.772 = 0.184 FN λ ⎟ z 0.035 ⎟ 0.219 ⎞ ⎟ ⎟ ⎠ ( ) = ⎛ ⎜ ⎜ ⎜ ⎜ ⎜ ⎝ 0.012 0.537 0.379 0.071 0.45 ⎞ ⎟ ⎟ ⎟ ⎠ back
Title: ETC and per<strong>for</strong>mance analysis Reference: MUSE-MEM-SCI-051 Issue: 1.3 Date: 28/01/04 Page: 52/14 15.1.4 AO Gen I, good seeing conditions back i := 0.. 4 ( ) EE spa ( λ) := EEgenI good λ , k spa_good 0.7 EE spa ( λ) 0.6 0.5 0.4 0.5 0.6 0.7 0.8 0.9 1 λ µm 15.1.4.1 Continuum source back ( ) K Obj ( λ) := K O 1, EE spa ( λ) , ∆ spec , 1 , λ, AM ( ) K Sky ( λ) := K S ∆ spec , k spa_good ⋅∆ WFspa , λ 2 K RN := k spa_good 2 K DC := k spa_good ( ) LimFContWFgenI good ( λ) := F O SN lim , n exp , t exp , F Sky ( λ) , RN CCD , DN CCD , K Obj ( λ) , K Sky ( λ) , K RN , K DC 4 .10 19 LimFContWFgenI 3 .10 19 good ( λ) erg⋅s − 1 ⋅cm − 2 ⋅A − 1 2 .10 19 1 .10 19 0.4 0.5 0.6 0.7 0.8 0.9 1 λ µm ⎛ LimMagContWFgenI goodi := Flux2AB LimFContWFgenI good λ MUSEi , ⎝ ⎠ λ MUSE ⎝ i ⎛ ⎞ ⎞ ⎠
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SCIENCE DOCUMENTS SECTION Title Ver
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The median descendant mass of galax
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with the slicer development for NIR
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Science Case Coordinator : R. Bacon
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Title: Science Case Reference: MUSE
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Keck Telescope (Rhoads et al. 2000)
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Assuming that most of the black hol
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5. Solar system Title: Science Case
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Page 120 and 121: ANNEX - ETC mathcad sheet Roland Ba
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