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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: 35/14 Noise Statistics ( ) := V O ← K O ⋅F O FNoise F O , n, t, F S , RN, DC, K O , K S , K RN , K DC ⋅n⋅ t V S ← K S ⋅F S ⋅n⋅ t V RN ← nK ⋅ RN ⋅RN 2 V DC ← nK ⋅ DC ⋅DC⋅ t V CCD ← V RN + V DC V Tot ← V O + V S + V CCD ⎛ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎜ ⎝ V O V Tot V S V Tot V RN V Tot V DC V Tot V CCD V Tot ⎞ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎟ ⎠ This function give the fraction of noise due to object (line 1), sky (line 2), readout (line 3), dark current (line 4), detector (ie readout + drak current, line 5) back
Title: ETC and per<strong>for</strong>mance analysis Reference: MUSE-MEM-SCI-051 Issue: 1.3 Date: 28/01/04 Page: 36/14 13. ETC parameters SN lim := 5 Signal to Noise t exp := 1⋅hour Exposure time n exp := 80 Number of summed exposures AM := 1 Air mass of observations F Sky ( λ) Flux SkyNoOH ( λ) := Sky flux is taken outside OH lines back
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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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Page 92 and 93: Title: Science Case Reference: MUSE
Page 96 and 97: 5. Solar system Title: Science Case
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Page 120 and 121: ANNEX - ETC mathcad sheet Roland Ba
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Reference: MUSE-MEM-SCI-054 Issue:
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