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 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: Image Added
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: Image Added

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Suzaku XIS

0.5-2 keV image of N132D from the XIS. The green box shows the FOV.
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Suzaku/XIS1 full-band image with extraction region in magenta (left) compared to ACIS image and extraction region in green (right).
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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).
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Spectra of Suzaku/XIS N132D obs, with old XMM model folded through
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Update 2020-12-01

Eric's work simultaneously fitting the NXB+CXB background to Suzaku XIS (FI CCD) observations of N132D.

Presentation to IACHEC 2020 Symposium:  PDF  Video

Tarball of data and XSPEC command files showing example fit procedure: suzaku_background_fit_example.tar.gz

Update 2021-05-12

Comparison of v2.13 empirical model and 'n132d_afoster_suzuki_vrnei_20210420' physical model: miller_n132d_suzaku_20210512.pdf0.5-2 keV image of N132D from XIS, showing the extraction region.
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Swift XRT

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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.
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XMM pn

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XMM RGS

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NICER XTI

NICER has ~21 ksec good data, taken between 2018-01-29 and 2018-02-23.  All 52 operating detectors were enabled.

Data were screened for undershoots in 0-40 ct/s/FPM range and overshoots in the 0-2 ct/s/FPM range, plus an additional cut on high energy X-ray counts (>2 keV, 0-4.5 ct/s/FPM cut).

This is a fit using the v2.11 model, only allowing the overall norm and NICER SCORPEON background terms to vary.

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The NICER norm is 0.993.  The backgrounds are pretty reasonable, although the "LEEL" background component would indicate a slightly rare condition.  Without "LEEL", the fit demands an additional high energy background component in the 2-10 keV range.

Using the v2.14 model, the NICER situation is considerable worse.

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NICER is not particularly sensitive to emission in the Fe K region.

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