ChangeLog for specgroup
=======================
Version 1.7.1 - 2021-10-04 (EO)
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+ config/specgroup.par: Subparameter groupedset was not well defined
in relation to its parent, overwrite. When groupedset is not entered
in the command line, its default is to output the groups in file
SpecGrp.ds. For this situation, the parent, overwrite, takes also the
default 'no'. However, as soon as groupedset is set in the command
line, the param implicit behaviour would imply to set overwrite to
'yes', as the alternative to its default. This is wrong.
Therefore, the default for groupedset must be changed to '' and the
default for overwrite must be changed to 'yes'. This way, if the
user set groupedset to something, automatically the implicit behaviour
will set overwrite to 'no', which is correct.
Version 1.7 - 2018-02-13 (EO)
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+ This is a new major version of this package including a new GNU
Public License Text disclaimer required to distribute the SAS source
code to the Astronomical Community under the terms of the GNU Public
License. The text as it is shown below is the same that has been
included in all SAS source code files.
ESA (C) 2000-2018
This file is part of ESA's XMM-Newton Scientific Analysis System
(SAS).
SAS is free software: you can redistribute it and/or modify
it under the terms of the GNU General Public License as published by
the Free Software Foundation, either version 3 of the License, or
(at your option) any later version.
SAS is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with SAS. If not, see <http://www.gnu.org/licenses/>.
---------------------------------------------------------------------
Version 1.6 - 2015-11-30 (RDS)
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+ src/Specgroup.cc - Sets file keywords (RESPFILE,
docs/specgroup_description.tex ANCRFILE, BACKFILE) to the command
line values or leaves them set to
the value they had in the input
spectrum (SPR-7295)
Version 1.5 - 2014-05-07 (RDS)
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+ src/Specgroup.cc - Added include for gcc 4.82
Version 1.4 - 2014-05-06 (RDS)
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+ src/WishInterpreter.cc - Flag problem if set bad range
set in keV and no RMF supplied.
Version 1.3 - 2014-04-28 (RDS)
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+ src/Specgroup.cc - Fixed problem when overwrite=yes
was selected
(SPR-7205)
Version 1.2 - 2014-04-09 (RDS)
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+ src/WishInterpreter.cc - Handle the cases of instrument
combinations.
EPIC - use EMOS1,
RGS - use RGS2, CCF settings.
+ doc/specgroup_description.tex - Document changes
(SCR-319 & SCR-7187).
Version 1.1 - 2011-09-27 (RDS)
------------------------------
+ doc/specgroup_description.tex - Add algorithmn (SPR-6664)
+ src/WishInterpreter.cc - Set CAL properly always (SPR-6670)
+ src/Specgroup.cc - Allow grouping to be the same as
+ config/specgroup.par for an input spectrum (SPR-6618)
Version 1.0 - 2011-01-11 (RDS)
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+ doc/specgroup_description.tex - Minor documentation update
Version 0.2.6 - 2010-06-21 (RDS)
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+ src/Specgroup.cc,
+ src/WishInterpreter.cc - Modify the s/n calculation
(SPR-6618)
Version 0.2.5 - 2010-04-13 (RDS)
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+ src/WishInterpreter.cc - If no grouping options have been chosen then
each spectral bin is assigned to its own group.
Version 0.2.4 - 2010-04-12 (RDS)
------------------------------
+ src/Specgroup.cc/h,
src/WishInterpreter.cc/h - Handles the RGS bad channels from
the CCF as integers
Version 0.2.3 - 2010-03-25 (RDS)
------------------------------
+ config/specgroup.par - Included overwrite=yes option
Version 0.2.2 - 2010-03-11 (RDS)
------------------------------
+ src/Specgroup.cc/h,
src/WishInterpreter.cc/h - Made more compatible with RGS.
Reads the lambda and beta values
from the SPECQUAL CCF.
(SPR-6596)
Version 0.2.1 - 2010-03-04 (RDS)
------------------------------
+ src/Specgroup.cc/h,
src/WishInterpreter.cc/h - Made compatible with RGS
Reads the BACKSCAL array and takes
the max value.
Version 0.2 - 2010-02-17 (RDS)
------------------------------
+ src/Specgroup.cc/h,
src/WishInterpreter.cc/h - Added the energy resolution option
'oversample' which ensures that
groups are not too narrow.
Version 0.1 - 2009-11-17 (RDS)
------------------------------
Original version of a task to group spectral data