PAU camera

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PAU survey• The main goal of the PAU survey is to study cosmology/darkenergy characterising the geometry and growth of structure of theuniverse• Large volumes and moderately accurate redshifts are needed forthis purpose• The idea is to use a large field of view camera and narrow bandfilters to achieve both• The survey will use ~40 narrow band filters (~100 A wide)covering from 4500 to 8500 A supplemented by wide band filtersto image the sky and measure the position and distance (usingphotometric redshift techniques) to millions of galaxies
PAU survey• The PAU survey collaboration is in the process of building anew large field-of-view camera to be installed in the current primefocus of the WHT reaching an etendue of ~7 to carry a large areasurvey
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 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
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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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