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Adam Aurisano

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06/13/2019

03:43 PM NOvA-ART Revision 36899 (svn): Now correctly filling SpillData::isRHC instead of just SpillData::hornI.

03/28/2019

12:13 PM NOvA-ART Revision 35971 (svn): Fixed debug message to only print the appropriate number of ADC values for a given nanoslice version. This should fix the errors seen in the FD miniproduction tests using single point runs.

03/12/2019

12:17 PM NOvA-ART Revision 35715 (svn): This is the ray tracing package I developed to construct the photon collection templates used by ImprovedTransport. Instructions on how to use this package are in the included README file.

01/16/2019

03:16 PM NOvA-ART Revision 34900 (svn): Based on discussions at the conveners and DetSim meetings, I've removed the randomization of pixel gains. Instead, each pixel is assigned the mean of the gain distribution for that pixel position. This accounts for the fact that pixels have systematically different gains depending on their position on the APD without injecting excess variation that the currrent calibration procedure can not remove.

12/18/2018

04:17 PM NOvA-ART Revision 34467 (svn): Updated the FD and ND attenuation profiles to match average functions derived from fiber stringing data, as shown in docdb-34702.
04:16 PM NOvA-ART Revision 34466 (svn): Changed Birks constant to 0.01155 as found in bench measurements shown in docdb-34223.
04:14 PM NOvA-ART Revision 34465 (svn): Turned on Robert's code that models the time structure of the NuMI beam.
04:13 PM NOvA-ART Revision 34464 (svn): If the flux is dk2nu, SpillData is now filled from the flux metadata. This should allow for reco to be able to tell whether a file is FHC or RHC.

11/28/2018

03:08 PM NOvA-ART Revision 34241 (svn): Changing the random gain generation procedure sample different distributions based on pixel position. Since CMap isn't initialized at BeginRun, gains are now redrawn each event. This shouldn't matter for any practical purpose.

09/13/2018

03:04 PM NOvA-ART Revision 33445 (svn): First commit of scripts to tune light levels and Cherenkov parameters.

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