Grating Spectroscopy
If new calibration has been applied to the event file, the grating spectrum should be re-extracted as well. It is then possible to build grating response files (gARF, gRMF) in order to model and fit the data.
- Chandra Grating Analysis Page
- WebGUIDE: Interactive GUIDE for ATOMDB
- Chandra Grating Data Archive and Catalog (TGCat): a browsable interface to analysis-quality spectral products.
-
The chandra_repro script may be
used to easily reprocess Chandra datasets.
Problems with the Zero Order:
HETG/ACIS:
-
HETG/ACIS-S Grating Spectra
(24 Apr 2013)
-
Grating Spectra for Multiple Sources - ACIS
(3 Dec 2012)
-
ACIS-S Grating RMFs
(24 Apr 2013)
-
HETG/ACIS-S Grating ARFs
(24 Apr 2013)
- Grouping a Grating Spectrum
-
HETG/ACIS-S Grating Spectra
LETG/ACIS:
-
LETG/ACIS Grating Spectra
(06 Jan 2012)
-
Grating Spectra for Multiple Sources - ACIS
(3 Dec 2012)
-
ACIS-S Grating RMFs
(24 Apr 2013)
-
LETG/ACIS-S Grating ARFs
(24 Apr 2013)
- Grouping a Grating Spectrum
-
LETG/ACIS Grating Spectra
LETG/HRC-S:
-
LETG/HRC-S Grating Spectra
(24 Apr 2013)
-
Applying Customized Background Regions to LETG/HRC-S Observations
(24 Apr 2013)
- Grating Spectra for Multiple Sources - HRC
- Higher-order Responses for HRC-S/LETG Spectra
-
HRC Grating RMFs
(24 Apr 2013)
-
LETG/HRC-S Grating ARFs
(24 Apr 2013)
- Grouping a Grating Spectrum
-
LETG/HRC-S Grating Spectra
LETG/HRC-I:
-
LETG/HRC-I Grating Spectra
(24 Apr 2013)
- Grating Spectra for Multiple Sources - HRC
-
HRC Grating RMFs
(24 Apr 2013)
-
LETG/HRC-I Grating ARFs
(24 Apr 2013)
- Grouping a Grating Spectrum
-
LETG/HRC-I Grating Spectra
Combining Spectra & Preparation for Fitting:
Modeling & Fitting Grating Data with Sherpa
(from the Sherpa analysis threads):

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