K. Taylor, A. Marin-Franch, R. Laporte, F. G. Santoro, L. Marrara, J. Cepa, A. J. Cenarro, S. Chueca, D. Cristobal-Hornillos, A. Ederoclite, N. Gruel, M. Moles, F. Rueda, S. Rueda, J. Varela, A. Yanes, N. Benitez, R. Dupke, A. Fernandez-Soto, P. Jorden, G. Lousberg, A. Molino Benito, I. Palmer, C. Mendes de Oliveira, L. Sodre Jr
JPCam is a 14-CCD mosaic camera, using the new e2v 9k-by-9k 10microm-pixel 16-channel detectors, to be deployed on a dedicated 2.55m wide-field telescope at the OAJ (Observatorio Astrofisico de Javalambre) in Aragon, Spain. The camera is designed to perform a Baryon Acoustic Oscillations (BAO) survey of the northern sky. The J-PAS survey strategy will use 54 relatively narrow-band (~13.8nm) filters equi-spaced between 370 and 920nm plus 3 broad-band filters to achieve unprecedented photometric red-shift accuracies for faint galaxies over ~8000 square degrees of sky. The cryostat, detector mosaic and read electronics is being supplied by e2v under contract to J-PAS while the mechanical structure, housing the shutter and filter assembly, is being designed and constructed by a Brazilian consortium led by INPE (Instituto Nacional de Pesquisas Espaciais). Four sets of 14 filters are placed in the ambient environment, just above the dewar window but directly in line with the detectors, leading to a mosaic having ~10mm gaps between each CCD. The massive 500mm aperture shutter is expected to be supplied by the Argelander-Institut fur Astronomie, Bonn. We will present an overview of JPCam, from the filter configuration through to the CCD mosaic camera. A brief outline of the main J-PAS science projects will be included.
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http://arxiv.org/abs/1301.4175
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