| step | purpose | What you have to do |
| setup | have your own data_rep on your account. Follow the E2E-F setup advice. | |
| setenv COMMONLOGFILE mylog.txt | define a logfile | If you want to have a log file, set it now. To unset it later just type "unsetenv COMMONLOGFILE" |
| emacs dols.txt | create a list of SCWs | Here is one example for a valid list of one SCW: dols.txt. Please have a look on the list of usable E2E-F data. Be aware that during E2E-F the detector was not cooled and the high voltage was not switched on, thus imaging can be performed but will give strange results. |
| og_create idxSwg="dols.txt" ogid="obs_id" baseDir="." | create the OG | give a (up to now not existing!) name for the obs-branch (obs_id). |
| cd obs/obs_id | go to your obs branch. | |
| spi_science_analysis (if you want to avoid the GUI, unsetenv DISPLAY before starting spi_science_analysis !) |
do the analysis | start with spi_science_analysis, fill in the parameters for the analysis (either off-line using an editor, or by using the GUI which will appear on the screen). The following parameter file can be a basis for your analysis: spi_science_analysis_e2ef.par (if you want to use it, copy it to your $PFILES/spi_science_analysis.par). For different sets of detectors you need different response (IRF). You can get a detector list if you are not familiar with our pseudo-detector scheme. Which IRFs do you want to use? Begin with small numbers of energy bins! Read also the user manuals of spihist, spiskymax, and spiros.. |
| fv spi/source_res.fits ... |
output check | read the log file, check the images, events table and so on. If it is failing - check for missing/wrong input parameters first. |
| spi_science_analysis | step back and repeat parts of the analysis | Run spi_science_analysis again in the level range you like. E.g. start from binning again up to the imaging/spectra level by using StartLevel = BIN_I and EndLevel = IMA. |
