ChangeLog for omgrismplot ========================= Version 1.8.7 - 2024-09-23 (RDS) --------------------- + Fixed error in ax.imshow(... norm=LogNorm()...) within omgrismplot_graph.py (SPR-7759) Version 1.8.6 - 2023-04-03 (RDS) --------------------- + Improved documentation Version 1.8.5 - 2023-03-06 (RDS) --------------------- + Fixed axis labels and improved naming convention of temporary files. (SPR-7673) - currently produces PDF and postscript output. PGPLOT code has not been removed. Version 1.8.4 - 2022-05-24 (AG) --------------------- + Fixed a typo in the documentation. + Added support for plotting regions alongside the rotated image in Python (omgrismplot_graph.py). + Added pysasplot_utils to DEPEND. Version 1.8.3 - 2022-05-09 (AG) --------------------- + Fixed an issue related to the ChangeLog entry for version 1.8.2. Version 1.8.2 - 2022-05-09 (AG) --------------------- + Fixed a bug in which the DATE-END keyword could not be found. + Made some changes in the appearance to match the original PGPlot task. Version 1.8.1 - 2022-02-03 (AG) --------------------- + Fixed a bug in which if the plotting device was set to /XW, an empty pdf file would be created. Now it's deleted after the plots are displayed to the user. Version 1.8 - 2022-02-01 (AG) ----------------------- + Added omgrismplot_graph.py in order to make the plots in Python. Old PGPlot plots are still created in order to make the testing parts easier. Version 1.7 - 2018-12-18 (RDS) ----------------------------- + src/omgrismplot_mod.f90 - Added the sensitivity correction factor onto the plot (SCR-7504) Version 1.6 - 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 1.5.3 - 2011-02-21 (VNY) +(src/omgrismplot_mod.f90) Reshaped to reduce the number of subroutine calls (as the previos fix of SSC-SPR-6649 did not work). Version 1.5.2 - 2011-02-16 (VNY) +(src/omgrismplot_mod.f90) String manipulation is modified in the subroutine create_labels to avoid a crash in the 64-bit mode (SSC-SPR-6649) Version 1.5.1 - 2009-11-25 (VNY) +(src/omgrismplot_mod.f90) A bug related to the memory deallocation problem is fixed (SSC-SPR-6579) Version 1.5 - 2009-04-06 (VNY) +(DEPEND) the previouse change was unmade and the dependency on ssclib-4.6 is included as the task uses one of the routines from this library. Version 1.4 - 2009-04-05 (VNY) +(DEPEND) the dependency from ssclib is removed to avoid build failure. Version 1.3 - 2008-05-01 (VNY) +(src/omgrismplot_mod.f90) introducing the capability to generate a postscript file showing the spectra extraction regions on the grism rotated image Version 1.2.1 - 2005-11-15, 2005-05-23 (VNY) +(src/omgrismplot_mod.f90) The X- and Y- coordinates are introduced into the plot header; strange symbols at the top of the plot are eliminated (this version is not uploaded yet - VNY 15.11.2005) Version 1.2 - 2005-10-18 (VNY) +(src/omgrismplot_mod.f90) A small bug introduced during the previous upload is fixed Version 1.1 - 2005-10-18 (VNY) +(src/omgrismplot_mod.f90) A warning message is included in the case of no spectral data in the input file (fixed SSC-SPR-3526) Version 1.0.6 - 2005-06-03 (VNY) +(src/omgrismplot_mod.f90) A bug is fixed (SSC-SPR-3436) which was leading to the task failure in the Full-Frame Low-Resolution mode when extracting field spectra. The failure was cause by some unexplicable manipulation of memory by the Fortran compiler: coding the same thing in slightly different way has fixed the problem. Version 1.0.5 - 2004-10-02 (VNY) +(src/omgrismplot_mod.f90) The contaminating sources are masked to avoid the excessive scale of the plot in the vertical axis when some zero-order images overlap the target spectrum (SPR-3396) Version 1.0.4 - 2004-07-15 (VNY) +(src/omgrismplot_mod.f90) The target plot is labelled with ``Object: target'' to distinguish it from the other sources (SSC-SPR-3356) Version 1.0.3 - 2004-05-13 (VNY) +(src/omgrismplot_mod.f90) Information bout the used spectrum extraction mode is inserted into the title of the output plot (SSC-SPR-3321) Version 1.0.2 - 2004-03-04 (VNY) +(src/omgrismplot_mod.f90) the bug causing crushing of the task on some data set is fixed (SSC-SPR-3267) Version 1.0.1 - 2004-02-03 (VNY) +(src/omgrismplot_mod.f90), +(config/omgrismplot.par) The parameters plotflux and scalebkgplot are activeted. The spectra ID's are inserted into the plots (SSC-SPR-3242) Version 1.0 - 2003-12-04 (VNY) +(src/omgrismplot_mod.f90) plotting of undetected spectra in included Version 0.5 - 2003-11-21 (VNY) +(src/omgrismplot_mod.f90) wrong warning messages are corrected Version 0.4 - 2003-11-20 (VNY) +(config/omgrismplot.par) the parameter plotdevise is set to the default value /PS since /VC is not recognised in some machines Version 0.3 - 2003-11-19 (VNY) +(config/omgrismplot.par) the parameter plotdevice is set to produce the portrait orientation of the output plot by default; +(src/omgrismplot_mod.f90): the plot labels are improved Version 0.2 - 2003-11-07 (VNY) +(src/omgrismplot_mod.f90) a new parameter (plotflux) is introduced Version 0.1 - 2003-10-27 (VNY) Created as a new task for plotting OM grism spectra, SAS-SCR-116