Bibcode
Poglitsch, Albrecht; Waelkens, Christoffel; Bauer, Otto H.; Cepa, Jordi; Henning, Thomas; van Hoof, Chris; Katterloher, Reinhard; Kerschbaum, Franz; Lemke, Dietrich; Renotte, Etienne; Rodriguez, Louis; Royer, Pierre; Saraceno, Paolo
Bibliographical reference
In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A. Wilson. ESA SP-577, Noordwijk, Netherlands: ESA Publications Division, ISBN 92-9092-855-7, 2005, p. 11 - 16
Advertised on:
1
2005
Citations
1
Refereed citations
0
Description
The Photodetector Array Camera and Spectrometer (PACS) is one of the
three science instruments for ESA's far infrared and submillimetre
observatory, Herschel. It employs two Ge:Ga photoconductor arrays
(stressed and unstressed) with 16×25 pixels, each, and two filled
Si bolometer arrays with 16×32 and 32×64 pixels,
respectively, to perform imagiung line spectroscopy and imaging
photometry in the 57-210μm wavelength band. In photometry mode, it
will simultaneously image two bands, 60-85μm or 85-130μm and
130-210μm, over a field of view of ~1.75'×3.5', with full beam
sampling in each band. In spectroscopy mode, it will image a field of
~50"×50", resolved into 5×5 pixels, with an instantaneous
spectral coverage of ~600-2500 km/s and a spectral resolution of ~75-300
km/s. In both modes background-noise limited performance is expected,
with sensitivities (5σ in 1h) of ~3 mJy or
3-20×10-18W/m2, respectively.