000002804 001__ 2804
000002804 005__ 20160701171711.0
000002804 037__ $$aASTROimport-961
000002804 100__ $$aOttensamer, R.
000002804 245__ $$aFishing for Photons: Data Reduction of MESSy PACS Images
000002804 260__ $$c2011
000002804 520__ $$aThe observed targets in the MESS guaranteed time key program for  the Herschel Space Observatory (Groenewegen et al. 2011) typically  consist of a bright central source surrounded by faint dust emission.  We use HIPE for most of the data processing. We need to correct for the correlated noise, without eliminating the extended emission or influencing the photometry of the central star. In addition we carry out deconvolution to make the details in regions close to the central star visible. 
000002804 700__ $$a Luntzer, A.
000002804 700__ $$a Mecina, M.
000002804 700__ $$a Kerschbaum, F.
000002804 700__ $$a Blommaert, J. A. D. L.
000002804 700__ $$a Decin, L.
000002804 700__ $$a Groenewegen, M. A. T.
000002804 700__ $$a Posch, T.
000002804 700__ $$a Vandenbussche, B.
000002804 700__ $$a Waelkens, C.
000002804 773__ $$c625$$pWhy Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants$$v445$$y2011
000002804 85642 $$ahttp://esoads.eso.org/abs/2011ASPC..445..625O
000002804 905__ $$apublished in
000002804 980__ $$aNONREF