The photodetector array camera and spectrometer (PACS) for the Herschel Space Observatory

By Albrecht Poglitsch, C. Waelkens, O. Bauer, J. Cepa, H. Feuchtgruber, Th. Henning, C. van Hoof, F. Kerschbaum, D. Lemke, E. Renotte and 3 more. SPIE Astronomical Telescopes + Instrumentation, 2006

248 citations recorded by the source corpus.

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Citations in the corpus

• Herschel-ATLAS: rapid evolution of dust in galaxies over the last 5 billion years (2010, methodology): “H-ATLAS will survey in excess of 550 deg2 in five bands centred on 100, 160, 250, 350 and 500 μm, using the Photodetector Array Camera (PACS; Poglitsch et al. 2010) and Spectral and Photometric Imaging Receiver (SPIRE) instruments (Griffin et al. 2010).”
• Herschel-Planck dust optical-depth and column-density maps - I. Method description and results for Orion (2014, unknown): “1, where Re(ν) is reported for the PACS and SPIRE passbands).”
• Initial highlights of the HOBYS key program, the Herschel imaging survey of OB young stellar objects (2010, methodology): “It will use the SPIRE and PACS cameras (Griffin et al. 2010; Poglitsch et al. 2010) of the Herschel satellite (Pilbratt et al. 2010) to image essentially all of the regions forming OB-type stars at distances less than Herschel is an ESA space observatory with science instruments provided by…”
• THE LESSER ROLE OF STARBURSTS IN STAR FORMATION AT z = 2 (2011, methodology): “The PACS camera (Poglitsch et al. 2010) onboard Herschel (Pilbratt et al. 2010) now allows for the first time to obtain deep far-IR observation probing SFRs down to MS levels for typical galaxies with M∗ ∼ 10 10M⊙ at z ∼ 2, i.e., at the peak epoch of the cosmic SFR density and of the space density…”
• “TNOs are Cool”: A survey of the trans-Neptunian region (2017, unknown): “More recently, Pluto was also observed with the Herschel Space Observatory (Pilbratt et al. 2010) Photodetector Array Camera and Spectrometer (PACS: Poglitsch et al. 2010) and with the Spectral and Photometric Imaging Receiver (SPIRE: Griffin et al. 2010), which provides thermal light curves at six…”
• Lumped Element Kinetic Inductance Detectors (2008, background): “Stressing of arrays of photo-conductors has been demonstrated with the PACS instrument [25] but again is not trivial and it is unlikely that this technology will achieve the required sensitivity specifications for SPICA.”
• Planck 2015 results - XXVIII. The Planck Catalogue of Galactic cold clumps (2015, unknown): “…the PGCC and PH z catalogues, we found 15 common A28, page 19 of 28 The sensitivity and resolution of the Herschel instruments (Pilbratt et al. 2010; Poglitsch et al. 2010; Gri ffi n et al. 2010) enable detailed studies of the structure of the clumps and their interplay with their parent clouds.”