ChangeLog for especplot ======================= Version 2.10 - 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 . --------------------------------------------------------------------- Version 2.9 - 2004-03-19 (NW) ------------------------------- Included binning by minimum number of counts per channel. Version 2.8 - 2002-07-25 (NW) ------------------------------- Updated the DEPEND file. It now includes a dependence on sas. Version 2.7 - 2002-06-03 (NW) ---------------------- Made the updates necessary for the new version of param Version 2.6.1 - 22-05-01 ---------------------- The documentation has been updated to include an example of how to run especplot and to include the columns required in the spectrum header extension of the input files. Version 2.6 - 06-04-01 ---------------------- The test harness has been changed to be variable for Linux or Unix, because the environment variables are different. In this way, the test can be passed on Linux or Unix. Version 2.5 - 23-03-01 ---------------------- The environment variables for `pgplot' were different to those at the `static build' and hence the test was not passed, as the output files were different to the comparison files. The environment variables for `pgplot' are now changed, so the output files of the `static build' should pass the test. Also, essential keywords are now read from the header extension, rather than the primary header, so that files generated by `evselect' can be read. `Especplot' no longer uses the CAL to determine the energy value of each data bin, but uses 1PI=1eV, a fundamental convention adopted in the pipeline. Version 2.4 - 20-12-00 ---------------------- Changed the test harness so that it no longer calls gs Version 2.3.1 - 02-11-00 ---------------------- Revised the documentation and updated the GROUPS description Version 2.3 - 03-10-00 ---------------------- Upgrade the version number as required for the SAS V5 Version 2.2.2 - 26-09-00 ------------------------ Update the .info file Version 2.2.1 - 27-06-00 ------------------------ - SSC-SPR-1824 especplot (version 2.2) : Update documentation to remove non existant links Version 2.2 - 22-05-00 ---------------------- add especplot.info in the config directory Version 2.1 - 18-04-00 ---------------------- The following SPRs have been fixed (1661) - SSC-SPR-1661 especplot (version 2.0): wrong format for errors and warnings in documentation Version 2.0 - 07-03-00 ---------------------- The following SPRs have been fixed (1512 was irelevant) - SSC-SPR-1514 especplot (version 1.11): The existing output file is deleted for SAS_CLOBBER=0 and for SAS_CLOBBER=1 - SSC-SPR-1513 especplot: There is no parameter layout file - SSC-SPR-1512 especplot (version 1.11): srcspectrumset should be a mandatory parameter - SSC-SPR-1511 especplot (version 1.11): useautobinning should be a boolean parameter and not a string one. - SSC-SPR-1510 especplot (version 1.11): The documentation does not follow "hello" document conventions . Version 1.11 - 26-11-99 ----------------------- - Test spectra must now have 4096 channels (it was 4095 earlier). This depends on the CAL. Version 1.10 - 7-10-99 ---------------------- -Fixed SSC-SPR-1267 especplot (version 1.8): Task hangs when binsize=2.0 or 1.0 -Fixed SSC-SPR-1268 especplot (version 1.8): Source and background plots have different energy ranges. Version 1.9 - 28-09-99 ---------------------- -Fixed SSC-SPR-1266 especplot (version 1.8): task looks for incorrect attributes in header Version 1.8 - 22-09-99 ---------------------- -Fixed SPR (1241) Version 1.6 - 08-06-99 ---------------------- - Update of DEPEND file (cal 3.0) - Change also the fits files for the test (now has 4095 channels) Version 1.5 - 11-05-99 ---------------------- - DEPEND now contains taskmain (SPR 989) - Make test harness sentivitive to the existence of the executable Version 1.4 - 03-05-99 ---------------------- - EXTERNALS = pgplot (in src/Makefile) - Fix cal version dependency (update DEPEND) - Test harness check on whether the output file exists Version 1.3 - 23-06-98 ----------------------- - Closed SSC-SPR-[0360/0362] Version 1.2 - 26-05-98 ----------------------- - Closed SSC-SPR-[0155/0160] Open SPRs : SSC-SPR-0360 : function change_case duplicated in other tasks SSC-SPR-0361 : remove the additions in especplot.tex SSC-SPR-0362 : test harness only test running-to-completion Version 1.1 - 22-04-98 ----------------------- - Initial version for SAS v1 integration Open SPRs : SSC-SPR-0155 : Use empty default values SSC-SPR-0156 : Require .par instead of .prm SSC-SPR-0157 : Require ghostview SSC-SPR-0158 : Make test waits for STDIN SSC-SPR-0159 : Task contains postscript files SSC-SPR-0160 : Documentation version number incorrect