PAU camera

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Requirements for cosmology survey• sample large volumes• sample enough (many) objects• measure distances (how accurate?)
The trick<strong>PAU</strong> survey• Use photometry to obtain redshifts• Many cosmological applications need only “rough”spectroscopic precision (~10 Mpc/h)• Broad band imaging does not provide enough resolution• Need sufficient spectral resolution as to obtain good photometricredshifts => narrow band imaging• Previously: Combo-17, Alhambra, COSMOS, Subaru,…• Simulations: MICE
Page 1 and 2: Cosmology with AccuratePhotometric
Page 3: Survey requirements• The precisio
Page 7 and 8: Requirements on Redshift Precisions
Page 10 and 11: Lensing Magnification• Lensing ef
Page 12 and 13: PAU survey• The main goal of the
Page 14 and 15: The PAU CameraO. Ballester(2), L. C
Page 16 and 17: The PAU CameraTelescopio William He
Page 18 and 19: The PAU CameraTelescopio William He
Page 20 and 21: The PAU CameraCamara efficiency•F
Page 22 and 23: The PAU CameraDistribution22
Page 24 and 25: The PAU CameraFilters40 narrow band
Page 26 and 27: The PAU CameraFilter TraysNeed to b
Page 28 and 29: The PAU CameraElectronicsMonsoon a
Page 30 and 31: The PAU Camera30
Page 32: PAU survey• The PAU survey collab
Page 35 and 36: PAU survey• The PAU collaboration
Page 37 and 38: • Galaxy evolutionPAU SurveyAltho
Page 39: DES landscape• If and when LSST o

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