- ... determined2.1
- In fact,
the satellite orbit is monitored at ground stations of
JAXA/TKSC. JAXA/TKSC determines the Suzaku orbit, and delivers the orbit files to
ISAS regularly.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... 1993)3.1
- See
http://heasarc.gsfc.nasa.gov/docs/journal/ogip_fortran3.html.
This is ANSI Fortran77 with some extensions. The extension includes the following:
(1) Both upper and lower case letter are allowed.
(2) END DO are allowed. (3) DO WHILE loops are allowed. (4) INCLUDE statements are allowed.
(5) INTEGER*2 data type is allowed. (6) Variable can be up to 31 character long.
(7) IMPLICIT NONE is allowed.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... tasks4.1
- atFunctions has been used also for ASCA.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
respectively4.2
- On the Unix platforms. For other platforms, the names will
be different.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... planning5.1
- See the MAKI home page
http://heasarc.gsfc.nasa.gov/Tools/maki/maki.html
for detail.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... Plug-In''5.2
- The LHEA Plug-In is developed at LHEA at NASA/GSFC. It is
a web plug-in that lets users use interactive astronomy
tools via the simple interface of users' browser.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... ``SkyView''5.3
- SkyView is a ``Virtual Observatory'' on the Net generating images of any part of the sky at wavelengths
in all regimes from Radio to Gamma-Ray.
See
http://skyview.gsfc.nasa.gov/skyview.html
for details. MAKI can launch from the SkyView output page if ``Advanced'' interface is selected.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...http://heasarc.gsfc.nasa.gov/docs/software/tools/pimms.html5.4
- The WWW version of PIMMS, WebPIMMS is also developed and available
at
http://heasarc.gsfc.nasa.gov/Tools/w3pimms.html.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
spectra5.5
- The WWW version of the XSPEC spectral simulation, WebSpec,
is available at
http://heasarc.gsfc.nasa.gov/webspec/webspec.html.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...xissim5.6
-
the xissim software package can be downloaded from
http://heasarc.gsfc.nasa.gov/docs/astroe/prop_tools/xissim/xissim_usage.html
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... (ICD)6.1
- http://heasarc.gsfc.nasa.gov/docs/suzaku/archive/astroe_icd_sdc_v1.2.pdf
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... center,6.2
- The ISAS data center manages data
from all past and current ISAS missions.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... processing6.3
- The ASCA pipeline processing took
almost 4 years
to implement the automated data screening, extraction and response generation
into the pipe-line processing.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... available.6.4
- The flookup implemented on gisclean is used for screening ASCA GIS data,
with the discrimination criteria on the PHA vs. Rise Time plane.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... files.6.5
-
The ASCA pipeline processing scripts was developed at GSFC ADF and ran only at GSFC.
It contains over 14,000 lines of ksh code.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... (CALDB)7.1
- See
http://heasarc.gsfc.nasa.gov/docs/heasarc/caldb/caldb_intro.html.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...Suzaku7.2
- The XRS gain history was one.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... instrument7.3
- Either xrs, xis, xi0, xi1, xi2, xi3,
hxd.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
examples.7.4
-
In the case of ASCA SIS, RDD (Residual Dark-current Distribution)
and echo parameters are also variable, and time history of
these parameters are also saved in the individual calibration files.
RDD should not be present for XIS.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... SegmentD.1
- Each of the four XIS sensors has a
single CCD chip, and a single chip is divided into four Segments.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... directionD.2
- Satellite Z-axis points the
telescope direction, and Y direction is toward the solar paddle.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... givenD.3
- There are several
projection methods, such as -TAN, -SIN, -ARC and -STG.
See http://www.cv.nrao.edu/fits/documents/wcs/wcs.all.ps for details. The
tangential projection (-TAN) is widely used, and will be adopted for
Suzaku event files too.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.