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Please
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place
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any
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data
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analysis
...
products
...
related
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to
...
fitting
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N132D
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here,
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under
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the
...
appropriate
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section
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for
...
each
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instrument.
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Please
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date
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each
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entry
...
so
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we
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have
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a
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log
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of
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submissions.
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JPEG
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and
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GIF
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images
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can
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be
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displayed
...
inline,
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which
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other
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files
...
(PDF,
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PS,
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PHA
...
files,
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event
...
lists)
...
should
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be
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included
...
as
...
attachments
...
with
...
a
...
link
...
to
...
the
...
file.
...
...
...
Anchor | ||||
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Chandra ACIS
0.35-8.0
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keV
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image
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from
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an
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89
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ks
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ACIS-S3
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observation
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with
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the
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proposed
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extraction
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region
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overlaid.
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There are about 2.5
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million
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total
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counts
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from
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the
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SNR
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in
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this
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data
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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
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keV
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range.
Fit with the ESAC version v1.0 model in the 2.0-4.0
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kV
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range
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looking
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for
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any
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missing
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lines,
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there
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do
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not
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appear
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to
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be
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any
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line
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features
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that
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the
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ACIS
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spectrum
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would
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require:
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Chandra HETG
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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,
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with
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E212_v1.0_20110439.xcm
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model
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folded
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through.
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A
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constant
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normalization
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factor
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was
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allowed
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to
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vary
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for
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each
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XIS,
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but
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everything
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else
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was
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fixed.
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Norms
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are
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1.27,
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1.31,
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1.28
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(so
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~30%
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larger
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than
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XMM
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model).
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Spectra of Suzaku/XIS
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N132D
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obs,
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with
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old
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XMM
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model
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folded
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through
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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).
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Total
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Exposure
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~
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257
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ksec.
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In
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total
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there
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more
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than
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40
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observations
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in
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the
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XMM
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archive.
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XMM pn
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XMM RGS
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Attachments:
Attachments |
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