Commit 7e719f33 authored by SAPONE Alann's avatar SAPONE Alann

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parent 385a1f97
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keystore
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\BOOKMARK [1][-]{section.1}{Introduction}{}% 1
\BOOKMARK [1][-]{section.2}{Exposure Time}{}% 2
\BOOKMARK [2][-]{subsection.2.1}{DIT - Number of exposures}{section.2}% 3
\BOOKMARK [2][-]{subsection.2.2}{Imaging}{section.2}% 4
\BOOKMARK [2][-]{subsection.2.3}{Spectroscopy}{section.2}% 5
\BOOKMARK [1][-]{section.3}{Signal to Noise Ratio \(SNR\)}{}% 6
\BOOKMARK [2][-]{subsection.3.1}{DIT - Number of exposures}{section.3}% 7
\BOOKMARK [2][-]{subsection.3.2}{Imaging}{section.3}% 8
\BOOKMARK [2][-]{subsection.3.3}{Spectroscopy}{section.3}% 9
\BOOKMARK [1][-]{section.4}{Extra BackgroundNoise}{}% 10
\BOOKMARK [2][-]{subsection.4.1}{No Extra Background Noise}{section.4}% 11
\BOOKMARK [2][-]{subsection.4.2}{Extra Background Noise Profile}{section.4}% 12
\BOOKMARK [1][-]{section.5}{Simulated Background Noise}{}% 13
\BOOKMARK [2][-]{subsection.5.1}{No Simulated Background Noise}{section.5}% 14
\BOOKMARK [2][-]{subsection.5.2}{Background Noise from Flux}{section.5}% 15
\BOOKMARK [2][-]{subsection.5.3}{Slitless Spectrograph}{section.5}% 16
\BOOKMARK [1][-]{section.6}{Extra Signal}{}% 17
\BOOKMARK [2][-]{subsection.6.1}{No Extra Signal}{section.6}% 18
\BOOKMARK [2][-]{subsection.6.2}{Extra Signal Profile}{section.6}% 19
\BOOKMARK [1][-]{section.7}{Simulated Signal}{}% 20
\BOOKMARK [2][-]{subsection.7.1}{No Simulated Signal}{section.7}% 21
\BOOKMARK [2][-]{subsection.7.2}{Signal from Flux}{section.7}% 22
\BOOKMARK [1][-]{section.8}{Wavelength step }{}% 23
\BOOKMARK [2][-]{subsection.8.1}{Imaging}{section.8}% 24
\BOOKMARK [2][-]{subsection.8.2}{Spectroscopy}{section.8}% 25
\BOOKMARK [1][-]{section.9}{Spectral Convolution Kernel Size}{}% 26
\BOOKMARK [2][-]{subsection.9.1}{Imaging}{section.9}% 27
\BOOKMARK [2][-]{subsection.9.2}{Spectroscopy}{section.9}% 28
\BOOKMARK [1][-]{section.10}{Spectral Resolution per Pixel}{}% 29
\BOOKMARK [2][-]{subsection.10.1}{Fixed /pixel}{section.10}% 30
\BOOKMARK [2][-]{subsection.10.2}{Spectral Resolution Profile}{section.10}% 31
\BOOKMARK [1][-]{section.11}{Telescope Area}{}% 32
\BOOKMARK [2][-]{subsection.11.1}{Circular Primary Mirror / Area Obstruction}{section.11}% 33
\BOOKMARK [1][-]{section.12}{Background Flux}{}% 34
\BOOKMARK [2][-]{subsection.12.1}{Ground}{section.12}% 35
\BOOKMARK [2][-]{subsection.12.2}{Space}{section.12}% 36
\BOOKMARK [1][-]{section.13}{Sky Flux}{}% 37
\BOOKMARK [2][-]{subsection.13.1}{No Sky Noise}{section.13}% 38
\BOOKMARK [2][-]{subsection.13.2}{Sky Template}{section.13}% 39
\BOOKMARK [1][-]{section.14}{Zodiacal Flux}{}% 40
\BOOKMARK [2][-]{subsection.14.1}{Flux Template}{section.14}% 41
\BOOKMARK [2][-]{subsection.14.2}{No Zodiacal Noise}{section.14}% 42
\BOOKMARK [1][-]{section.15}{Galactic Flux}{}% 43
\BOOKMARK [2][-]{subsection.15.1}{Flux Template}{section.15}% 44
\BOOKMARK [2][-]{subsection.15.2}{No Galactic Noise}{section.15}% 45
\BOOKMARK [1][-]{section.16}{Sky Area}{}% 46
\BOOKMARK [2][-]{subsection.16.1}{Imaging}{section.16}% 47
\BOOKMARK [2][-]{subsection.16.2}{Slit}{section.16}% 48
\BOOKMARK [2][-]{subsection.16.3}{Fiber}{section.16}% 49
\BOOKMARK [1][-]{section.17}{Atmospheric Transmission}{}% 50
\BOOKMARK [2][-]{subsection.17.1}{Space}{section.17}% 51
\BOOKMARK [2][-]{subsection.17.2}{Absorption and Extinction Profiles}{section.17}% 52
\BOOKMARK [1][-]{section.18}{Source Flux}{}% 53
\BOOKMARK [2][-]{subsection.18.1}{Rest Frame Template}{section.18}% 54
\BOOKMARK [2][-]{subsection.18.2}{Flat Photon Flux}{section.18}% 55
\BOOKMARK [2][-]{subsection.18.3}{Flat Energy Flux}{section.18}% 56
\BOOKMARK [2][-]{subsection.18.4}{Emission Line}{section.18}% 57
\BOOKMARK [2][-]{subsection.18.5}{Black Body}{section.18}% 58
\BOOKMARK [1][-]{section.19}{Normalization Factor}{}% 59
\BOOKMARK [2][-]{subsection.19.1}{Point Source Imaging}{section.19}% 60
\BOOKMARK [2][-]{subsection.19.2}{Point Source Slit}{section.19}% 61
\BOOKMARK [2][-]{subsection.19.3}{Point Source Fiber}{section.19}% 62
\BOOKMARK [2][-]{subsection.19.4}{Extended Source Imaging}{section.19}% 63
\BOOKMARK [2][-]{subsection.19.5}{Extended Source Slit}{section.19}% 64
\BOOKMARK [2][-]{subsection.19.6}{Extended Source Fiber}{section.19}% 65
\BOOKMARK [1][-]{section.20}{Convolution of Surface Brightness Profile with PSF}{}% 66
\BOOKMARK [2][-]{subsection.20.1}{Circularly Symmetric}{section.20}% 67
\BOOKMARK [2][-]{subsection.20.2}{FFT Convolution}{section.20}% 68
\BOOKMARK [2][-]{subsection.20.3}{1D FFT Convolution of projection functions}{section.20}% 69
\BOOKMARK [1][-]{section.21}{Surface Brightness Profile}{}% 70
\BOOKMARK [2][-]{subsection.21.1}{Uniform}{section.21}% 71
\BOOKMARK [2][-]{subsection.21.2}{De Vaucouleurs}{section.21}% 72
\BOOKMARK [2][-]{subsection.21.3}{Exponential}{section.21}% 73
\BOOKMARK [1][-]{section.22}{Number of Pixels}{}% 74
\BOOKMARK [2][-]{subsection.22.1}{Photometry}{section.22}% 75
\BOOKMARK [2][-]{subsection.22.2}{Spectroscopy}{section.22}% 76
\BOOKMARK [1][-]{section.23}{Source Pixel Coverage}{}% 77
\BOOKMARK [2][-]{subsection.23.1}{Symmetric}{section.23}% 78
\BOOKMARK [1][-]{section.24}{Spectral Binning}{}% 79
\BOOKMARK [2][-]{subsection.24.1}{Fiber}{section.24}% 80
\BOOKMARK [2][-]{subsection.24.2}{Slit}{section.24}% 81
\BOOKMARK [2][-]{subsection.24.3}{Slitess}{section.24}% 82
\BOOKMARK [1][-]{section.25}{Spatial Binning}{}% 83
\BOOKMARK [2][-]{subsection.25.1}{Fiber}{section.25}% 84
\BOOKMARK [2][-]{subsection.25.2}{Point Source}{section.25}% 85
\BOOKMARK [2][-]{subsection.25.3}{Extended Source}{section.25}% 86
\BOOKMARK [2][-]{subsection.25.4}{Slit Point Source}{section.25}% 87
\BOOKMARK [2][-]{subsection.25.5}{Slit Extended Source}{section.25}% 88
\BOOKMARK [1][-]{section.26}{PSF Size}{}% 89
\BOOKMARK [2][-]{subsection.26.1}{Symmetric Gaussian}{section.26}% 90
\BOOKMARK [2][-]{subsection.26.2}{Symmetric Double Gaussian}{section.26}% 91
\BOOKMARK [1][-]{section.27}{PSF}{}% 92
\BOOKMARK [2][-]{subsection.27.1}{Diffraction Limited}{section.27}% 93
\BOOKMARK [2][-]{subsection.27.2}{Gaussian Instrument PSF}{section.27}% 94
\BOOKMARK [2][-]{subsection.27.3}{Double Gaussian Instrument PSF}{section.27}% 95
\BOOKMARK [2][-]{subsection.27.4}{Seeing}{section.27}% 96
\BOOKMARK [2][-]{subsection.27.5}{Instruments PSF + Seeing}{section.27}% 97
\BOOKMARK [2][-]{subsection.27.6}{Adaptive Optics}{section.27}% 98
\BOOKMARK [1][-]{section.28}{Wavelength Range}{}% 99
\BOOKMARK [2][-]{subsection.28.1}{Spectroscopy}{section.28}% 100
\BOOKMARK [2][-]{subsection.28.2}{Imaging}{section.28}% 101
\BOOKMARK [1][-]{section.29}{System Efficiency}{}% 102
\BOOKMARK [2][-]{subsection.29.1}{Total Efficiency Profile}{section.29}% 103
\BOOKMARK [1][-]{section.30}{Filter Response}{}% 104
\BOOKMARK [2][-]{subsection.30.1}{NoFilter}{section.30}% 105
\BOOKMARK [2][-]{subsection.30.2}{Filter Transmission Profile}{section.30}% 106
\contentsline {section}{\numberline {1}Introduction}{4}{section.1}
\contentsline {section}{\numberline {2}Exposure Time}{4}{section.2}
\contentsline {subsection}{\numberline {2.1}DIT - Number of exposures}{4}{subsection.2.1}
\contentsline {subsection}{\numberline {2.2}Imaging}{5}{subsection.2.2}
\contentsline {subsection}{\numberline {2.3}Spectroscopy}{5}{subsection.2.3}
\contentsline {section}{\numberline {3}Signal to Noise Ratio (SNR)}{5}{section.3}
\contentsline {subsection}{\numberline {3.1}DIT - Number of exposures}{6}{subsection.3.1}
\contentsline {subsection}{\numberline {3.2}Imaging}{6}{subsection.3.2}
\contentsline {subsection}{\numberline {3.3}Spectroscopy}{6}{subsection.3.3}
\contentsline {section}{\numberline {4}Extra BackgroundNoise}{6}{section.4}
\contentsline {subsection}{\numberline {4.1}No Extra Background Noise}{6}{subsection.4.1}
\contentsline {subsection}{\numberline {4.2}Extra Background Noise Profile}{7}{subsection.4.2}
\contentsline {section}{\numberline {5}Simulated Background Noise}{7}{section.5}
\contentsline {subsection}{\numberline {5.1}No Simulated Background Noise}{7}{subsection.5.1}
\contentsline {subsection}{\numberline {5.2}Background Noise from Flux}{7}{subsection.5.2}
\contentsline {subsection}{\numberline {5.3}Slitless Spectrograph}{8}{subsection.5.3}
\contentsline {section}{\numberline {6}Extra Signal}{8}{section.6}
\contentsline {subsection}{\numberline {6.1}No Extra Signal}{9}{subsection.6.1}
\contentsline {subsection}{\numberline {6.2}Extra Signal Profile}{9}{subsection.6.2}
\contentsline {section}{\numberline {7}Simulated Signal}{9}{section.7}
\contentsline {subsection}{\numberline {7.1}No Simulated Signal}{9}{subsection.7.1}
\contentsline {subsection}{\numberline {7.2}Signal from Flux}{9}{subsection.7.2}
\contentsline {section}{\numberline {8}Wavelength step $\Delta \lambda $}{10}{section.8}
\contentsline {subsection}{\numberline {8.1}Imaging}{10}{subsection.8.1}
\contentsline {subsection}{\numberline {8.2}Spectroscopy}{10}{subsection.8.2}
\contentsline {section}{\numberline {9}Spectral Convolution Kernel Size}{10}{section.9}
\contentsline {subsection}{\numberline {9.1}Imaging}{11}{subsection.9.1}
\contentsline {subsection}{\numberline {9.2}Spectroscopy}{11}{subsection.9.2}
\contentsline {section}{\numberline {10}Spectral Resolution per Pixel}{11}{section.10}
\contentsline {subsection}{\numberline {10.1}Fixed $\Delta \lambda _{/pixel}$}{11}{subsection.10.1}
\contentsline {subsection}{\numberline {10.2}Spectral Resolution Profile}{12}{subsection.10.2}
\contentsline {section}{\numberline {11}Telescope Area}{12}{section.11}
\contentsline {subsection}{\numberline {11.1}Circular Primary Mirror / Area Obstruction}{12}{subsection.11.1}
\contentsline {section}{\numberline {12}Background Flux}{12}{section.12}
\contentsline {subsection}{\numberline {12.1}Ground}{13}{subsection.12.1}
\contentsline {subsection}{\numberline {12.2}Space}{13}{subsection.12.2}
\contentsline {section}{\numberline {13}Sky Flux}{13}{section.13}
\contentsline {subsection}{\numberline {13.1}No Sky Noise}{13}{subsection.13.1}
\contentsline {subsection}{\numberline {13.2}Sky Template}{13}{subsection.13.2}
\contentsline {section}{\numberline {14}Zodiacal Flux}{14}{section.14}
\contentsline {subsection}{\numberline {14.1}Flux Template}{14}{subsection.14.1}
\contentsline {subsection}{\numberline {14.2}No Zodiacal Noise}{14}{subsection.14.2}
\contentsline {section}{\numberline {15}Galactic Flux}{14}{section.15}
\contentsline {subsection}{\numberline {15.1}Flux Template}{14}{subsection.15.1}
\contentsline {subsection}{\numberline {15.2}No Galactic Noise}{15}{subsection.15.2}
\contentsline {section}{\numberline {16}Sky Area}{15}{section.16}
\contentsline {subsection}{\numberline {16.1}Imaging}{15}{subsection.16.1}
\contentsline {subsection}{\numberline {16.2}Slit}{15}{subsection.16.2}
\contentsline {subsection}{\numberline {16.3}Fiber}{16}{subsection.16.3}
\contentsline {section}{\numberline {17}Atmospheric Transmission}{16}{section.17}
\contentsline {subsection}{\numberline {17.1}Space}{16}{subsection.17.1}
\contentsline {subsection}{\numberline {17.2}Absorption and Extinction Profiles}{16}{subsection.17.2}
\contentsline {section}{\numberline {18}Source Flux}{17}{section.18}
\contentsline {subsection}{\numberline {18.1}Rest Frame Template}{17}{subsection.18.1}
\contentsline {subsection}{\numberline {18.2}Flat Photon Flux}{18}{subsection.18.2}
\contentsline {subsection}{\numberline {18.3}Flat Energy Flux}{18}{subsection.18.3}
\contentsline {subsection}{\numberline {18.4}Emission Line}{18}{subsection.18.4}
\contentsline {subsection}{\numberline {18.5}Black Body}{19}{subsection.18.5}
\contentsline {section}{\numberline {19}Normalization Factor}{19}{section.19}
\contentsline {subsection}{\numberline {19.1}Point Source Imaging}{20}{subsection.19.1}
\contentsline {subsection}{\numberline {19.2}Point Source Slit}{20}{subsection.19.2}
\contentsline {subsection}{\numberline {19.3}Point Source Fiber}{21}{subsection.19.3}
\contentsline {subsection}{\numberline {19.4}Extended Source Imaging}{22}{subsection.19.4}
\contentsline {subsection}{\numberline {19.5}Extended Source Slit}{23}{subsection.19.5}
\contentsline {subsection}{\numberline {19.6}Extended Source Fiber}{24}{subsection.19.6}
\contentsline {section}{\numberline {20}Convolution of Surface Brightness Profile with PSF}{24}{section.20}
\contentsline {subsection}{\numberline {20.1}Circularly Symmetric}{25}{subsection.20.1}
\contentsline {subsection}{\numberline {20.2}FFT Convolution}{25}{subsection.20.2}
\contentsline {subsection}{\numberline {20.3}1D FFT Convolution of projection functions}{25}{subsection.20.3}
\contentsline {section}{\numberline {21}Surface Brightness Profile}{25}{section.21}
\contentsline {subsection}{\numberline {21.1}Uniform}{25}{subsection.21.1}
\contentsline {subsection}{\numberline {21.2}De Vaucouleurs}{26}{subsection.21.2}
\contentsline {subsection}{\numberline {21.3}Exponential}{26}{subsection.21.3}
\contentsline {section}{\numberline {22}Number of Pixels}{26}{section.22}
\contentsline {subsection}{\numberline {22.1}Photometry}{26}{subsection.22.1}
\contentsline {subsection}{\numberline {22.2}Spectroscopy}{26}{subsection.22.2}
\contentsline {section}{\numberline {23}Source Pixel Coverage}{27}{section.23}
\contentsline {subsection}{\numberline {23.1}Symmetric}{27}{subsection.23.1}
\contentsline {section}{\numberline {24}Spectral Binning}{27}{section.24}
\contentsline {subsection}{\numberline {24.1}Fiber}{28}{subsection.24.1}
\contentsline {subsection}{\numberline {24.2}Slit}{28}{subsection.24.2}
\contentsline {subsection}{\numberline {24.3}Slitess}{28}{subsection.24.3}
\contentsline {section}{\numberline {25}Spatial Binning}{28}{section.25}
\contentsline {subsection}{\numberline {25.1}Fiber}{28}{subsection.25.1}
\contentsline {subsection}{\numberline {25.2}Point Source}{29}{subsection.25.2}
\contentsline {subsection}{\numberline {25.3}Extended Source}{29}{subsection.25.3}
\contentsline {subsection}{\numberline {25.4}Slit Point Source}{29}{subsection.25.4}
\contentsline {subsection}{\numberline {25.5}Slit Extended Source}{30}{subsection.25.5}
\contentsline {section}{\numberline {26}PSF Size}{30}{section.26}
\contentsline {subsection}{\numberline {26.1}Symmetric Gaussian}{30}{subsection.26.1}
\contentsline {subsection}{\numberline {26.2}Symmetric Double Gaussian}{31}{subsection.26.2}
\contentsline {section}{\numberline {27}PSF}{31}{section.27}
\contentsline {subsection}{\numberline {27.1}Diffraction Limited}{31}{subsection.27.1}
\contentsline {subsection}{\numberline {27.2}Gaussian Instrument PSF}{32}{subsection.27.2}
\contentsline {subsection}{\numberline {27.3}Double Gaussian Instrument PSF}{32}{subsection.27.3}
\contentsline {subsection}{\numberline {27.4}Seeing}{33}{subsection.27.4}
\contentsline {subsection}{\numberline {27.5}Instruments PSF + Seeing}{33}{subsection.27.5}
\contentsline {subsection}{\numberline {27.6}Adaptive Optics}{33}{subsection.27.6}
\contentsline {section}{\numberline {28}Wavelength Range}{34}{section.28}
\contentsline {subsection}{\numberline {28.1}Spectroscopy}{34}{subsection.28.1}
\contentsline {subsection}{\numberline {28.2}Imaging}{34}{subsection.28.2}
\contentsline {section}{\numberline {29}System Efficiency}{34}{section.29}
\contentsline {subsection}{\numberline {29.1}Total Efficiency Profile}{35}{subsection.29.1}
\contentsline {section}{\numberline {30}Filter Response}{35}{section.30}
\contentsline {subsection}{\numberline {30.1}NoFilter}{35}{subsection.30.1}
\contentsline {subsection}{\numberline {30.2}Filter Transmission Profile}{35}{subsection.30.2}
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\BOOKMARK [1][-]{section.4}{Observing parameters}{}% 17
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\contentsline {section}{\numberline {1}Instruments}{2}{section.1}
\contentsline {subsection}{\numberline {1.1}Telescope}{2}{subsection.1.1}
\contentsline {subsubsection}{\numberline {1.1.1}Aperture}{2}{subsubsection.1.1.1}
\contentsline {subsubsection}{\numberline {1.1.2}PSF}{2}{subsubsection.1.1.2}
\contentsline {subsubsection}{\numberline {1.1.3}Transmission}{2}{subsubsection.1.1.3}
\contentsline {subsection}{\numberline {1.2}Detector}{2}{subsection.1.2}
\contentsline {subsection}{\numberline {1.3}Type}{3}{subsection.1.3}
\contentsline {subsubsection}{\numberline {1.3.1}Imaging}{3}{subsubsection.1.3.1}
\contentsline {subsubsection}{\numberline {1.3.2}Spectrograph}{3}{subsubsection.1.3.2}
\contentsline {section}{\numberline {2}Sites}{3}{section.2}
\contentsline {subsection}{\numberline {2.1}Location}{3}{subsection.2.1}
\contentsline {subsection}{\numberline {2.2}Confusion noise}{4}{subsection.2.2}
\contentsline {section}{\numberline {3}Sources}{4}{section.3}
\contentsline {subsection}{\numberline {3.1}Magnitude}{4}{subsection.3.1}
\contentsline {subsection}{\numberline {3.2}Spatial Distribution}{5}{subsection.3.2}
\contentsline {subsection}{\numberline {3.3}Spectral Distribution}{5}{subsection.3.3}
\contentsline {section}{\numberline {4}Observing parameters}{5}{section.4}
\contentsline {subsection}{\numberline {4.1}Time sample}{5}{subsection.4.1}
\contentsline {subsection}{\numberline {4.2}Fixed parameter}{6}{subsection.4.2}
\contentsline {subsection}{\numberline {4.3}Spectral Quantum}{6}{subsection.4.3}
\contentsline {section}{\numberline {5}Simulation outputs}{6}{section.5}
\contentsline {subsection}{\numberline {5.1}Final results}{6}{subsection.5.1}
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