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

Author(s):  
Albrecht Poglitsch ◽  
Christoffel Waelkens ◽  
Otto H. Bauer ◽  
Jordi Cepa ◽  
Helmut Feuchtgruber ◽  
...  
2004 ◽  
Author(s):  
Albrecht Poglitsch ◽  
Christoffel Waelkens ◽  
Otto H. Bauer ◽  
Jordi Cepa ◽  
Thomas F. Henning ◽  
...  

2008 ◽  
Author(s):  
Albrecht Poglitsch ◽  
Christoffel Waelkens ◽  
Otto H. Bauer ◽  
Jordi Cepa ◽  
Helmut Feuchtgruber ◽  
...  

2007 ◽  
Vol 4 (4) ◽  
pp. 136-144
Author(s):  
Hilmar H. Richter ◽  
Michael Harr ◽  
Peter Dinges ◽  
Heribert Krüger ◽  
Alexandra Todisco ◽  
...  

The high- and low-stressed photodetector array camera and spectrometer (PACS) modules (linear 16-pixel arrays) are the basic constituents of the 16 × 25 pixel far-infrared (57–220 μm) PACS cameras aboard the Herschel satellite. The essentials for the stress application and the pixel stacking technique originate from detectors aboard the Infrared Space Observatory (ISO, 1995–1998) and for the field imaging far infrared line spectrometer (FIFI-LS) aboard the Stratospheric Observatory for Infrared Astronomy (SOFIA). To meet the mass budget of the cameras and provide the required high tensile strength, the only usable material for the module body turned out to be an aluminum alloy (AL 7075 T651). Especially challenging was the tight thermal budget for the PACS modules. Compared to FIFI-LS, in the case of the PACS module the heat dissipation from the front end electronics (FEE) and harness substrates at about 4 K to the module body containing the pixel stack at about 2 K had to be reduced drastically. A genuine suspension concept and packaging for the respective substrates was developed and successfully applied, allowing reliable electrical wiring from the harness over the FEE on to the pixels. The FEE with the cryogenic readout electronics (CRE) is contributed by the Interuniversity Microelectronics Centre (IMEC).


2003 ◽  
Author(s):  
Ian Pain ◽  
Brian Stobie ◽  
Gillian S. Wright ◽  
T. A. Paul ◽  
Colin R. Cunningham

Author(s):  
E. Varga-Verebélyi ◽  
L. Dobos ◽  
T. Budavári ◽  
Cs. Kiss

AbstractWe created the Herschel1 Footprint Database and web services for the Herschel Space Observatory imaging data. For this database we set up a unified data model for the PACS and SPIRE Herschel instruments, from the pointing and header information of each observation, generated and stored sky coverages (footprints) of the observations in their exact geometric form. With this tool we extend the capabilities of the Herschel Science Archive by providing an effective search tool that is able to find observations for selected sky locations (objects), or even in larger areas in the sky.


2010 ◽  
Vol 518 ◽  
pp. L2 ◽  
Author(s):  
A. Poglitsch ◽  
C. Waelkens ◽  
N. Geis ◽  
H. Feuchtgruber ◽  
B. Vandenbussche ◽  
...  

2011 ◽  
Vol 20 (3) ◽  
Author(s):  
Maarten Baes ◽  
Jacopo Fritz ◽  
Naseem Rangwala ◽  
Pasquale Panuzzo ◽  
Christine D. Wilson ◽  
...  

AbstractThe FIR/submm window is one of the least-studied regions of the electromagnetic spectrum, yet this wavelength range is absolutely crucial for understanding the physical processes and properties of the ISM in galaxies. The advent of the Herschel Space Observatory has opened up the entire FIR/submm window for spectroscopic studies. We present the first FIR/submm spectroscopic results on both nearby and distant galaxies obtained in the frame of two Herschel key programs: the Very Nearby Galaxies Survey and the Herschel ATLAS.


2012 ◽  
Author(s):  
Guillaume Dovillaire ◽  
Yong Wang ◽  
Rémy Toth ◽  
Raphael Porcar-Guézénec

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