PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RELEASE_ID = 0001 REVISION_ID = 0000 OBJECT = TEXT PUBLICATION_DATE = 2003-12-04 NOTE = "Description of XSM delivered software included in the SOFTWARE directory" END_OBJECT END SOFTWARE directory of XSM PDS archive ======================================= SOFTWARE directory contains XSM software necessary to produce input data for XSPEC spectral fitting applications. This software is delivered as a compressed file. The SOFTWARE directory contains the following files: File Name File Contents ---------------- -------------------------------------------------------- SOFTINFO.TXT Description of the contents of this directory. This file. XSM_SOFT.ZIP Compressed file containing the DG.PRO and RA.PRO applications and MU_SI.FITS auxiliary data table required to produce input data for XSPEC. XSM_SOFT.LBL Detached PDS label describing the XSM_SOFT.ZIP file. DESCRIPTION OF THE S/W PROGRAMS NEEDED TO ANALYZE XSM SPECTRAL DATA =================================================================== List of all S/W programs(=ASCII files in this directory) needed to reduce the 1 b level data up to level 3b data. (NOTE: Run IDL by entering ".r RA.PRO" or ".r DG.PRO"!) LIST OF S/W PROGRAMS: 1. DG.PRO 2. RA.PRO 1.DG.PRO (IDL) This program generates FITS-formetted XSPEC applicable spectral data files. Input: Delivered data table of level 1 b e.g. CCYY-MM-DDThh:mm:ss_1.DAT Output: XSM_NNNN.DAT, N's are ascending numbers from 0 to 9999 e.g row numbers in the DATA TABLE CCYY-MM-DDThh:mm:ss_1.DAT 2.RA.PRO (IDL) This program generates FITS-formetted XSPEC applicable Ancillary Response files (ARF) and FITS-formetted XSPEC applicable Redistribution Matrix Files (RMF). Input: Delivered data table of level 1 b e.g. CCYY-MM-DDThh:mm:ss_1.DAT Output: XSM_NNNN.ARF, N's are ascending numbers from 0 to 9999 e.g row numbers in the DATA TABLE CCYY-MM-DDThh:mm:ss_1.DAT. As a default this program generates just one RMF (=YYYY_MM_DDThh_mm.RMF), which has gain and offset are calculaetd as mean values of start and end calibrations. A log file is also generated automatically. Take a closer look at this log file after running RA.PRO! You can generate a specific RMF for each spectrum by adjusting the NX value to correspond to the row number, i.e. spectrum in the data file. This is recommendated when the gain shift between the start and end of the observation is greater that 20 eV. AUXILIARY DATA TABLE: 1. MU_SI.FITS This file includes silicon mass attenuation cofficiects between 0.03 and 20 keV. It is needed to compute the Response Matrix File. It is input table of the program RA.PRO.