ChangeLog for rgslccorr
=======================

Version 0.57.2 - 2023-03-28 (AI) 
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	+ GTI and EXPOSU inconsistency warning text modified. SOC-SPR-7685

Version 0.57.1 - 2019-04-05 (AI) 
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	+ Cross-check, before count rate is calculated, if the frame 
	is empty or does not exists. In this case, a NaN is propagated 
	for this particular frame and the final count rate for the bin 
	is properly calculated.

Version 0.57 -  2018-03-23 (AI) 
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	+ Fatal error thrown if the number of rows in the GTI and EXPOSU
	extension are different. This problem should be solved at ODF
	level and is probably due to a frame jump in the AUX and SPE RGS files.
	+ Documentation updated

Version 0.56 - 2018-02-13 (EO)
------------------------------
	+ 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 0.55 -  2016-09-16 (AI) 
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	+ (src/rgslccorr.cc) Output keyword SRCNUM now contains the correct 
	source identifier value.

Version 0.54 -  2015-05-12 (AI) 
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	+ Brackground rate and error column added to the background corrected light curve.
	+ Obs id, exp id, ra_obj and dec_obj keywords added to the output 
	file to make it compatible with elcplot.
	+ error when filtering with single CCDs fixed.
	
Version 0.52.1 -  2012-06-08 (AI) 
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	+ Attribute keyword HDUCLAS2 changed to NET in case bkg subtraction is applied.
	
Version 0.52 -  2010-07-21 (AI) 
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	+ Bug fixed when only order 2 is selected and the wavelength filtering is enabled.
	SOC-SPR-6623 fixed
	
Version 0.51.4 -  2009-09-02 (AI) 
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	+ Fixes to make rgslccorr gcc-4.3 compliant.
	
Version 0.51.3 -  2009-05-29 (AI) 
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	+ Error producing empty bkg light curves when "withbkgsubtraction" 
	is desabled fixed. SOC-SPR-6539 fixed 
	
Version 0.51.2 -  2009-05-22 (AI) 
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	+ Bug related to ccd selection and SOC-SPR-6535 fixed.
	
Version 0.51.1 -  2009-05-21 (AI) 
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	+ Bug in rgslccorr.cc expression creation fixed. SOC-SPR-6535 fixed
	
Version 0.51 -  2009-04-23 (AI) 
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	+ doc updated
	
Version 0.5 -  2009-04-23 (AI) 
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	+ Selection in energy implemented

Version 0.4 -  2009-04-22 (AI) 
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	+ New CCD selection and wavelength filtering functionalities added.
	+ New file for background light curve created
	+ withbackground subtraction parameter added
	+ withccdselection parameter added
	+ withwavelength filtering parameter added 
	+ doc updated

Version 0.3 -  2009-02-02 (AI) 
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	+ (src/Lightcurve.cc) New background count rate, error background
	count rate, source counts, background counts and fracexp columns added to 
	the output file. Weigthed mean BACKSCALE keyword added. (SOC-SCR-270)

Version 0.2.2 -  2008-06-17 (AI) 
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	+ (config/rgslccorr.info) Set VISIBLE to yes
	
Version 0.2.1 -  2007-10-31 (AI) 
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	+ (src/rgslccorr.cc) bug related to order selection fixed. 
	
Version 0.2 -  2007-10-30 (AI) 
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	+ (src/LightCurve.cc) bug related to binzise values similar to 
	RGS frame time resolution fixed. SOC-SPR-2731 Closed.
	
Version 0.1.1 -  2007-07-04 (AI) 
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	+ First experimental version.
	+ Dead time correction applied.
	+ Area scale correction applied.
	
Version 0.1 -  2007-05-25 (AI) 
-----------
	+ First skeleton version for development 
	of rgs light curve correction.