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> Suzaku
> Data Analysis
Suzaku Data Analysis (for v2.x data)
The Suzaku pipeline processing was major updated from
v1.x to v2.x on 2007-08-14, and all observations
will be re-processed with the new pipeline. Users are
requested to use the latest Suzaku software (version 6
released as a part of Headas-6.3.1) to analyze the v2.x data.
Appropriate combinations of data and software are summarized
in the table below.
| Observation date |
Processing version |
Suzaku Software |
| Before 2007-06-14 |
V1.x.x.x |
Version 4 (Headas-6.2) |
| Before 2007-06-14 |
V2.x.x.x |
Version 6 (Headas-6.3.1) |
| After 2007-06-15 |
V2.x.x.x |
Version 6 (Headas-6.3.1) |
If you need to upgrade v1.x data into "v2.x equivalent" by yourself,
please consult this page.
The distributed Suzaku data are already applied
with the latest calibration (only the exception is the energy
scale of GSO) and the clean events are screened with the standard
criteria. From these event files, images, spectra, and light curves
can be created using the standard multi-mission software,
HEAsoft package. Mission-specific software, which are
necessary for the standard analysis, are also released as
a part of the HEAsoft. In the early stage of the mission,
some additional files or tools prepared by the instrument teams
may be provided via the web page, in addition to the HEAsoft.
Manuals
Information and data supplied by the instrument teams
Suzaku Help Desk
ISAS/JAXA Department of High Energy Astrophysics

Last Modified: Wednesday, 26-Nov-2008 20:55:52 JST
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