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| Paper: |
Herschel/PACS Image Data Processing |
| Volume: |
497, Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time |
| Page: |
559 |
| Authors: |
Mečina, M.; Mayer, A.; Ottensamer, R.; Luntzer, A.; Kerschbaum, F. |
| Abstract: |
With the end of the mission of the Herschel Space Observatory
in May 2013, a rich archive of data is ready to be analysed. Data
reduction pipelines have progressed to give good results for most
types of observations, but for other, more specialised programs,
improved image reconstruction tools and methods need to be applied
to fully exploit the telescope's unique sensitivity and spatial
resolution. This is the case for post-main-sequence objects
(typically bright stars surrounded by faint dust emission) observed
with Herschel/PACS as part of the MESS sample. We compare six
standard map-making tools for Herschel observations and further
show how improved astrometry can enhance image quality. |
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