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0.2” Optics +Tracking +Diffraction +Det Perturbations +Lens Perturbations +Mirror Perturbations +Detector +Dome Seeing +Low Altitude +Mid Altitude +High Altitude +Pixelization Atmosphere Atmosphere Atmosphere 38
0.2” Optics +Tracking +Diffraction +Det Perturbations +Lens Perturbations +Mirror Perturbations +Detector +Dome Seeing +Low Altitude +Mid Altitude +High Altitude +Pixelization Atmosphere Atmosphere Atmosphere 39
Page 1 and 2: Simulating the Large Synoptic Surve
Page 3 and 4: Future Measurements in Cosmology N
Page 5 and 6: 5) Weak Gravitational Lensing High
Page 7 and 8: How does LSST do this? Etendue Eten
Page 9 and 10: LSST Site
Page 11: LSST Camera
Page 14 and 15: COSMO- LOGICAL SIMULATOR: Synthetic
Page 16 and 17: Optical Photon Monte Carlo Simulati
Page 18 and 19: Very important physics PSF size, s
Page 20 and 21: Monte Carlo Efficiency Basically do
Page 22 and 23: Catalog Constructor Connolly, Krugh
Page 24 and 25: Draw Photons Direction: Direction
Page 26 and 27: Atmosphere Model Photons accumulate
Page 28 and 29: Atmosphere Opacity 1) Cloud model 2
Page 30 and 31: Raytracing through Telescope & Came
Page 32 and 33: Every optical surface & CCD has an
Page 34 and 35: After 1 micron After 10 microns Ras
Page 36 and 37: Background Model Two components: Ai
Page 40 and 41: Entire focal plane 3 gigapixels 1
Page 42: Central chip 15’ x 15’ 42
Page 45 and 46: ImSim Description 45
Page 47 and 48: 4 Major LSST Data Challenges so far
Page 49: Validation!

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