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Proceedings Paper

The PAU camera at the WHT
Author(s): Cristóbal Padilla; Otger Ballester; Laia Cardiel-Sas; Jorge Carretero; Ricard Casas; Javier Castilla; Martin Croce; Manuel Delfino; Martin Eriksen; Enrique Fernández; Pablo Fosalba; Juan García-Bellido; Enrique Gaztañaga; Ferràn Grañena; Cales Hernández; Jorge Jiménez ; Luis Lopez; Pol Martí; Ramon Miquel; Christian Niessner; Cristóbal Pío; Rafael Ponce; Eusebio Sánchez ; Santiago Serrano; Ignacio Sevilla; Nadia Tonello; Juan de Vicente
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Paper Abstract

The PAU (Physics of the Accelerating Universe) project goal is the study of dark energy with a new photometric technique aiming at obtaining photo-z resolution for Luminous Red Galaxies (LRGs) roughly one order of magnitude better than current photometric surveys. To accomplish this, a new large field of view camera (PAUCam) has been built and commissioned at the William Herschel Telescope (WHT). With the current WHT corrector, the camera covers ~1 degree diameter Field of View (FoV). The focal plane consists of 18 2kx4k Hamamatsu fully depleted CCDs, with high quantum efficiency up to 1 μm. To maximize the detector coverage within the FoV, filters are placed in front of the CCD's inside the camera cryostat (made of carbon fiber material) using a challenging movable tray system. The camera uses a set of 40 narrow band filters ranging from ~4400 to ~8600 angstroms complemented with six standard broad-band filters, ugrizY. Here, we describe the camera and its first commissioning results. The PAU project aims to cover roughly 100 square degrees and to obtain accurate photometric redshifts for galaxies down to iAB ~ 22:5 detecting also galaxies down to iAB ~ 24 with less precision in redshift. With this data set we will obtain competitive constraints in cosmological parameters using both weak lensing and galaxy clustering as main observational probes.

Paper Details

Date Published: 4 August 2016
PDF: 12 pages
Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 99080Z (4 August 2016); doi: 10.1117/12.2231884
Show Author Affiliations
Cristóbal Padilla, Institut de Física d'Altes Energies (Spain)
Otger Ballester, Institut de Física d'Altes Energies (Spain)
Laia Cardiel-Sas, Institut de Física d'Altes Energies (Spain)
Jorge Carretero, Port d'Informació Científica (Spain)
Ricard Casas, Institut de Ciències de l'Espai (Spain)
Javier Castilla, Port d'Informació Científica (Spain)
Martin Croce, Institut de Ciències de l'Espai (Spain)
Manuel Delfino, Port d'Informació Científica (Spain)
Martin Eriksen, Institut de Ciències de l'Espai (Spain)
Enrique Fernández, Institut de Física d'Altes Energies (Spain)
Pablo Fosalba, Institut de Ciències de l'Espai (Spain)
Juan García-Bellido, Univ. Autónoma de Madrid (Spain)
Enrique Gaztañaga, Institut de Ciències de l'Espai (Spain)
Ferràn Grañena, Institut de Física d'Altes Energies (Spain)
Cales Hernández, Institut de Física d'Altes Energies (Spain)
Jorge Jiménez , Institut de Física d'Altes Energies (Spain)
Luis Lopez, Institut de Física d'Altes Energies (Spain)
Pol Martí, Institut de Física d'Altes Energies (Spain)
Ramon Miquel, Institut de Física d'Altes Energies (Spain)
Institució Catalana de Recerca i Estudis Avançats (Spain)
Christian Niessner, Port d'Informació Científica (Spain)
Cristóbal Pío, Institut de Física d'Altes Energies (Spain)
Rafael Ponce, Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain)
Eusebio Sánchez , Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain)
Santiago Serrano, Institut de Ciències de l'Espai (Spain)
Institut d'Estudis Espaciales de Catalunya (Spain)
Ignacio Sevilla, Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain)
Nadia Tonello, Port d'Informació Científica (Spain)
Juan de Vicente, Ctr. de Investigaciones Energéticas, Medioambientales y Tecnológicas (Spain)


Published in SPIE Proceedings Vol. 9908:
Ground-based and Airborne Instrumentation for Astronomy VI
Christopher J. Evans; Luc Simard; Hideki Takami, Editor(s)

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