CSMStatusUtils
Updated on Fri, 2007-10-19 12:40. Originally created by kocolosk on 2006-11-30 15:56.
Under:
This is CSMStatusUtils, which outputs the status of either calorimeter to text and root status files. Documentation is by Dave Relyea. The code can be found at
StRoot/StEmcPool/CSMStatusUtils
History:
I was given code from both Joanna and Thorsten to figure out the status of the calorimeter towers over all pp production runs. I merged the two sets of code, and and created a package called CSMStatusUtils.
Method:
The first piece of code in CSMSU takes every run and fills a 2-d histogram of ALL channels vs hit number (in ADC counts, from 0 to 150). A second routine then combines these histograms from run subsets into single histograms for each run. From the second routine and on down, the EEMC and BEMC are done entirely separately; the code needs to be run twice, once for each detector.
The code has an algorithm which then takes runs in each fill and combines them until the average number of hits above pedestal for all channels is greater than 100. If runs are left over at the end of a fill, their statistics are added to prior runs in the fill.
For each combined set of runs, the code puts each channel through a series of tests. It finds the pedestal (and writes it out to a file, btw) and determines if the pedestal is abnormally wide, or whether it falls outside acceptable limits (ADC channels 0 to 3, or 147 to 150). It compares all towers' mean number of hits (ten sigma) above pedestal, and then flags towers which have 10x as many hits as the average, or 40x fewer. Finally, it looks for stuck bits (either on or off) in the 1, 2, 4, or 8 position, and flags channels with stuck bits.
The code writes out a table (in text format) for each set of runs with the status of each channel clearly marked. This table is also written in ROOT format, to be read by existing BEMC algorithms. Also written is a hot tower plot, so the hot tower results can be eyeballed. The code can also write out gif files of the spectra of every channel that failed a status test, so long as the number of channels in a given run set that failed the test is less than 25 (**for 2004 pp, gif files were not written out**). Finally, the code creates a nice html file containing links to html subfiles detailing the channel status for each run set, which in turn link to the gif files.
As a final step, the code takes the text files and creates a new series of text status files with the results in differential format, meaning channels whose status didn't change from run set to run set are omitted. However, since some channels fall very near the thresholds of certain status tests (for instance, channels whose pedestals sit at 2.9 ADC counts), I make the requirement that the channel's status must not have changed more than ten percent of the time over all runs sets, excluding runs in which all channels were bad (for nominal production running, this needs to be done, of course!). If it has, it is marked bad once at the beginning, and then does not appear in any of the differential files.
************************************************************************
Running:
To run CSMSU, the first step is to use the FileCatalog to create a list of all the files you wish to analyze. The command I use is typically something like:
get_file_list.pl -keys 'path,filename' -cond 'production=P04ik,tpc=1,emc=1, trgsetupname=productionPP||productionPPnoEndcap||pp||PP,filename~st_physics,filetype=daq_reco_mudst' -onefile -limit 100000 -distinct > allthephysicsfiles
Note that the output format I use is just 'path,filename', and I keep the :: delimiter that the FileCatalog uses. My next step is to call
CSMSU/scripts/analysis0 allthephysicsfiles
PLEASE NOTE: Each minirun will generate about a 200k file. This adds up to ENORMOUS disk space for large runs. The 2004 pp run takes up about 1.4 Gig. The 2004 Au-Au run would be even larger. Thus, I really need to learn how to
use the XML submission scripts.
Next, you want to run the actual status code on the files. The script "analysis2" does this. PLEASE NOTE: this macro requires an x window, as root needs to be able to Draw certain things. I don't know how to do this in batch,
so I always run this interactively. It's not a good solution, but for now, it's a solution.
Finally, you want to generate the ".root" status files and the concatenated status files (to alert you to changes in calorimeter tower status). The script "analysis3" does this.
StRoot/StEmcPool/CSMStatusUtils
History:
I was given code from both Joanna and Thorsten to figure out the status of the calorimeter towers over all pp production runs. I merged the two sets of code, and and created a package called CSMStatusUtils.
Method:
The first piece of code in CSMSU takes every run and fills a 2-d histogram of ALL channels vs hit number (in ADC counts, from 0 to 150). A second routine then combines these histograms from run subsets into single histograms for each run. From the second routine and on down, the EEMC and BEMC are done entirely separately; the code needs to be run twice, once for each detector.
The code has an algorithm which then takes runs in each fill and combines them until the average number of hits above pedestal for all channels is greater than 100. If runs are left over at the end of a fill, their statistics are added to prior runs in the fill.
For each combined set of runs, the code puts each channel through a series of tests. It finds the pedestal (and writes it out to a file, btw) and determines if the pedestal is abnormally wide, or whether it falls outside acceptable limits (ADC channels 0 to 3, or 147 to 150). It compares all towers' mean number of hits (ten sigma) above pedestal, and then flags towers which have 10x as many hits as the average, or 40x fewer. Finally, it looks for stuck bits (either on or off) in the 1, 2, 4, or 8 position, and flags channels with stuck bits.
The code writes out a table (in text format) for each set of runs with the status of each channel clearly marked. This table is also written in ROOT format, to be read by existing BEMC algorithms. Also written is a hot tower plot, so the hot tower results can be eyeballed. The code can also write out gif files of the spectra of every channel that failed a status test, so long as the number of channels in a given run set that failed the test is less than 25 (**for 2004 pp, gif files were not written out**). Finally, the code creates a nice html file containing links to html subfiles detailing the channel status for each run set, which in turn link to the gif files.
As a final step, the code takes the text files and creates a new series of text status files with the results in differential format, meaning channels whose status didn't change from run set to run set are omitted. However, since some channels fall very near the thresholds of certain status tests (for instance, channels whose pedestals sit at 2.9 ADC counts), I make the requirement that the channel's status must not have changed more than ten percent of the time over all runs sets, excluding runs in which all channels were bad (for nominal production running, this needs to be done, of course!). If it has, it is marked bad once at the beginning, and then does not appear in any of the differential files.
************************************************************************
Running:
To run CSMSU, the first step is to use the FileCatalog to create a list of all the files you wish to analyze. The command I use is typically something like:
get_file_list.pl -keys 'path,filename' -cond 'production=P04ik,tpc=1,emc=1, trgsetupname=productionPP||productionPPnoEndcap||pp||PP,filename~st_physics,filetype=daq_reco_mudst' -onefile -limit 100000 -distinct > allthephysicsfiles
Note that the output format I use is just 'path,filename', and I keep the :: delimiter that the FileCatalog uses. My next step is to call
CSMSU/scripts/analysis0 allthephysicsfiles
(YOU NEED TO CHANGE THE HEADER IN THIS FILE TO YOUR OWN OUTPUT DIRECTORY)
which takes the "allthephysicsfiles" file from FileCatalog, splits it up into groups of 20 miniruns, and submits the entire processing job to batch. Note - if I knew how to use the XML submission scripts, I would, but the online documentation for them doesn't mention how to code up your macro (.C) file such that the XML header file will work. No matter.PLEASE NOTE: Each minirun will generate about a 200k file. This adds up to ENORMOUS disk space for large runs. The 2004 pp run takes up about 1.4 Gig. The 2004 Au-Au run would be even larger. Thus, I really need to learn how to
use the XML submission scripts.
(FROM HERE ON, SCRIPT FILES CALL MACROS IN THE MACROS DIRECTORY. YOU NEED TO CHANGE THE DEFAULT ARGUMENTS OF THE MACROS TO YOUR WORKING DIRECTORY. YOU CAN DO THIS IN THE SCRIPT, OR JUST MAKE YOUR OWN SCRIPT, SINCE THEY'RE ALL TRIVIAL ONE LINE SCRIPTS ANYWAY. SORRY ABOUT THE CAPS.)
After all miniruns have been processed, the next step is to combine them into runs. The script "analysis1" does this.Next, you want to run the actual status code on the files. The script "analysis2" does this. PLEASE NOTE: this macro requires an x window, as root needs to be able to Draw certain things. I don't know how to do this in batch,
so I always run this interactively. It's not a good solution, but for now, it's a solution.
Finally, you want to generate the ".root" status files and the concatenated status files (to alert you to changes in calorimeter tower status). The script "analysis3" does this.
»
- Printer-friendly version
- Login or register to post comments