Please place any data analysis products related to fitting N132D here, under the appropriate section for each instrument. Please date each entry so we have a log of submissions. JPEG and GIF images can be displayed inline, which other files (PDF, PS, PHA files, event lists) should be included as attachments with a link to the file.
Chandra ACIS
0.35-8.0 keV image from an 89 ks ACIS-S3 observation with the proposed extraction region overlaid. There are about 2.5 million total counts from the SNR in this data set.
Chandra image from a larger region that has been smoothed and contrast enhanced with the XIS extraction region overlaid to determine if there are any bright sources in the XIS extraction region: 
Fit to the ACIS spectrum with the ESAC version 1.0 model for the 2.0-10.0 keV range.
Fit with the ESAC version v1.0 model in the 2.0-4.0 kV range looking for any missing lines, there do not appear to be any line features that the ACIS spectrum would require: 
Chandra HETG
Suzaku XIS
Suzaku/XIS1 full-band image with extraction region in magenta (left) compared to ACIS image and extraction region in green (right).
Suzaku/XIS spectra (black=XIS1, red=XIS0, green=XIS3) from 2010-07-27, with E212_v1.0_20110439.xcm model folded through. A constant normalization factor was allowed to vary for each XIS, but everything else was fixed. Norms are 1.27, 1.31, 1.28 (so ~30% larger than XMM model).
Spectra of Suzaku/XIS N132D obs, with old XMM model folded through
Swift XRT
XMM MOS
Coadded MOS spectra at high energies from 10 observations (processed as of 11-may-2011). Total Exposure ~ 257 ksec. In total there more than
40 observations in the XMM archive.
XMM pn
XMM RGS