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CIAO 4.0 Beta 2 Release Notes
Return to: Version History
(14 Sep 2007) CALDB 3.4.1 has been
released.
The CIAO 4.0 Beta 2 release includes a new, more powerful version of
ChIPS, the CIAO plotting package. It can be used during
data analysis - e.g. to plot a lightcurve - and to create
publication-quality figures. Details and documentation on the
new system is available from the ChIPS
website.
Several bug fixes to the CIAO tools are also included.
Sherpa is not included in CIAO 4.0 Beta 2. It will be
released in Beta 3 (Fall 2007).
This section of the release notes describes how the CALDB 3.4.1
release will affect your analysis. The changes are arranged by
instrument and grating configuration.
ACIS Imaging Data
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Time-dependent ACIS Gain (TGAIN) Files
There are new time-dependent ACIS Gain (TGAIN) files for 01 May
2007 - 31 July 2007 (Epoch 30):
acisD2007-02-01t_gainN0005.fits
acisD2007-02-01t_gainN0006.fits
acisD2007-05-01t_gainN0002.fits
acisD2007-05-01t_gain_biN0002.fits
The files are applicable to -120 C data only.
The acisD2007-05-01t_gain[_bi]N0002.fits files are the
new default proccesing files in the CALDB.
These plots illustrate the degree of change the new files will
produce in comparison with the old files.
Epoch 30
In both of the above figures it is apparent that the T_GAIN
correction at the I3 aimpoint is diminishing over Epochs 28 - 30.
In the S3 case, the general trends with energy and Epoch number
are the same for the CTI and non-CTI cases by comparison, but
with clear differences between them in specific values
particularly above 5 keV. This is normal for recent epochs with
T_GAIN corrections.
Users working with ACIS data taken during this period may wish
to reprocess to improve the TGAIN calibration in their data.
The DATE-OBS header keyword records the observation
start date.
Note that unless you are fitting a spectra with oxygen emission
lines, the gain refinement is unlikely to have an effect on the
spectrum larger than the uncertainties in determining the gain.
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ACIS Blank-Sky Background Files
The newest versions of the ACIS blank-sky background files are now
available in the CALDB.
This set of ACIS background files includes:
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files for -120 C data on ACIS-5 or ACIS-7 with CTI_APP =
PPPPPBPBPP header keyword value (i.e. parallel and serial CTI
applied to the back-illuminated chips)
-
CTI-corrected files for ACIS-8 (ACIS-S4).
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upgrades to the files for chips 1-3, 5-7, and 8 with ACIS-S in
the focal plane. These files include the newest CTI and TGAIN
corrections.
The non-CTI-corrected background files for these chips have
the TGAIN applied. This matches how observational data at
-120 C without the CTI-correction would be processed.
The Using the ACIS "Blank-Sky"
Background Files thread contains instructions on how
to select a file and match it to a specific observation.
ACIS Grating Data
-
Time-dependent ACIS Gain (TGAIN) Files
There are new time-dependent ACIS Gain (TGAIN) files for 01 May
2007 - 31 July 2007 (Epoch 30):
acisD2007-02-01t_gainN0005.fits
acisD2007-02-01t_gainN0006.fits
acisD2007-05-01t_gainN0002.fits
acisD2007-05-01t_gain_biN0002.fits
The files are applicable to -120 C data only.
The acisD2007-05-01t_gain[_bi]N0002.fits files are the
new default proccesing files in the CALDB.
These plots illustrate the degree of change the new files will
produce in comparison with the old files.
Epoch 30
In both of the above figures it is apparent that the T_GAIN
correction at the I3 aimpoint is diminishing over Epochs 28 - 30.
In the S3 case, the general trends with energy and Epoch number
are the same for the CTI and non-CTI cases by comparison, but
with clear differences between them in specific values
particularly above 5 keV. This is normal for recent epochs with
T_GAIN corrections.
Users working with ACIS data taken during this period may wish
to reprocess to improve the TGAIN calibration in their data.
The DATE-OBS header keyword records the observation
start date.
Note that unless you are fitting a spectra with oxygen emission
lines, the gain refinement is unlikely to have an effect on the
spectrum larger than the uncertainties in determining the gain.
-
ACIS Blank-Sky Background Files
The newest versions of the ACIS blank-sky background files are now
available in the CALDB.
This set of ACIS background files includes:
-
files for -120 C data on ACIS-5 or ACIS-7 with CTI_APP =
PPPPPBPBPP header keyword value (i.e. parallel and serial CTI
applied to the back-illuminated chips)
-
CTI-corrected files for ACIS-8 (ACIS-S4).
-
upgrades to the files for chips 1-3, 5-7, and 8 with ACIS-S in
the focal plane. These files include the newest CTI and TGAIN
corrections.
The non-CTI-corrected background files for these chips have
the TGAIN applied. This matches how observational data at
-120 C without the CTI-correction would be processed.
The Using the ACIS "Blank-Sky"
Background Files thread contains instructions on how
to select a file and match it to a specific observation.
HRC-I Imaging and Grating Data
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HRC-I Degap
A new gap lookup table,
hrciD1999-07-22gaplookupN0003.fits, is needed to
improve the off-aimpoint gap map solution for HRC-I at certain
locations.
New observations of Capella from December 2005 -
January 2006 and January 2007 were used to improve the degap
solution for the CRSU=12-13 region, while including a slightly
more optimized solution for other detector positions. The
details of the refinements are presented in the memorandum
HRC-I Degap Lookup from Capella Data - 2007
[http://hea-www.harvard.edu/%7Ejuda/memos/hrci_degap_lookup/capella/degap/2007/degap_lookup.html].
Users must reprocess the data with hrc_process_events
to apply the new calibration, e.g. by following the Create a New
Level=2 Event File thread. The correct file will automatically be
chosen by the tool.
The tool updates in CIAO 4.0 Beta 2 are limited to bug fixes. These
changes will not adversely affect any analysis in progress.
acis_process_events
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Bug fix:
the stop time of afterglow badpixels was not being correctly
used. The afterglow badpixels are now marked as bad (bit
16) until the stop time, not the end of the observation.
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Bug fix:
after a file is reprocessed, the values of PHA_RO are
equal to the summed pulse height of the original, unadjusted
event island (PHAS).
axbary
dmdiff
dmimgthresh
dmmakereg
dmstat
hrc_dtfstats
hrc_process_events
The CIAO 4.0 Beta software establishes a separate local parameter
file directory, ~/cxcds_param_beta. This allows users to
run both CIAO 3.4 and CIAO 4.0 Beta without having to worry about
parameter file conflicts.
ciao.par
Prism
ChIPS Website
Ahelp
Analysis Threads
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The CIAO Science Threads are in the
process of being updated for the CIAO 4.0 Beta 2 release.
Please check the "Last Update" information at the top of each
thread to see if it has been reviewed yet.
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Threads and scripts that were removed at CIAO 4.0 Beta 1 due to
dependencies on ChIPS will be made available shortly as well.
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