PAU camera

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<strong>PAU</strong> survey• some cosmological probes do not require accurate spectroscopicredshift• exploit this with a narrow band survey delivering good photo-z’s• building a new <strong>camera</strong> for the WHT• probes: BAO (area), z-space distortions, magnification bias• sampling the galaxy power spectrum will not be limited by shotnoiseand could be traced with several tracers
DES landscape• If and when LSST operates, DECam will be out-dated• DESpec role• If DESpec is delayed or cannot happen, using narrow band filtersmay be an option for DECam
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 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: • Galaxy evolutionPAU SurveyAltho

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