PAU camera

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The <strong>PAU</strong> CameraCamara efficiency•Fill the available field of view as densely populated as possiblewith CCD detectors•Use CCD with the highest QE available in the whole wavelengthrange accessible•Size: 2048 x 4096 pixelsPixel size: 15 µm•Scale: 0.26 arcsec/pix20
The <strong>PAU</strong> CameraDetectors• Hamamatsu21
Page 1 and 2: Cosmology with AccuratePhotometric
Page 3 and 4: Survey requirements• The precisio
Page 5 and 6: The trickPAU survey• Use photomet
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 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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