Authors
Albrecht Poglitsch, Christoffel Waelkens, Norbert Geis, Helmut Feuchtgruber, Bart Vandenbussche, Louis Rodriguez, Oliver Krause, Etienne Renotte, Christiaan Van Hoof, P Saraceno, J Cepa, F Kerschbaum, P Agnese, B Ali, B Altieri, P Andreani, J-L Augueres, Z Balog, L Barl, OH Bauer, N Belbachir, Milena Benedettini, N Billot, O Boulade, H Bischof, J Blommaert, E Callut, C Cara, R Cerulli, D Cesarsky, A Contursi, Y Creten, W De Meester, V Doublier, E Doumayrou, L Duband, K Exter, R Genzel, J-M Gillis, U Grözinger, T Henning, J Herreros, R Huygen, M Inguscio, G Jakob, Claude Jamar, C Jean, J De Jong, R Katterloher, C Kiss, U Klaas, D Lemke, D Lutz, S Madden, Benoit Marquet, J Martignac, A Mazy, P Merken, Francis Montfort, LORENZO Morbidelli, T Müller, M Nielbock, K Okumura, R Orfei, R Ottensamer, Stefano Pezzuto, P Popesso, J Putzeys, S Regibo, V Reveret, P Royer, M Sauvage, J Schreiber, J Stegmaier, D Schmitt, J Schubert, E Sturm, M Thiel, G Tofani, R Vavrek, M Wetzstein, E Wieprecht, E Wiezorrek
Publication date
2010/7/1
Journal
Astronomy & astrophysics
Volume
518
Pages
L2
Publisher
EDP Sciences
Description
The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments on ESA's far infrared and submillimetre observatory. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16×25 pixels, each, and two filled silicon bolometer arrays with 16×32 and 32×64 pixels, respectively, to perform integral-field spectroscopy and imaging photometry in the 60–210 μm wavelength regime. In photometry mode, it simultaneously images two bands, 60–85 μm or 85–125 μm and 125–210 μm, over a field of view of ~1.75'× 3.5', with close to Nyquist beam sampling in each band. In spectroscopy mode, it images a field of 47” × 47”, resolved into 5×5 pixels, with an instantaneous spectral coverage of ~1500 km s-1 and a spectral resolution of ~175 km s-1. We summarise the design of the instrument, describe observing modes, calibration, and data analysis methods, and …
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