Changeset 8653 for trunk/MagicSoft
- Timestamp:
- 07/29/07 11:46:33 (17 years ago)
- Location:
- trunk/MagicSoft/Mars
- Files:
-
- 3 edited
Legend:
- Unmodified
- Added
- Removed
-
trunk/MagicSoft/Mars/Changelog
r8652 r8653 25 25 - removed conc1-spark cut 26 26 - changed cut coefficients to new algorithm 27 28 * mars.rc, star.rc: 29 - switched to use new image cleaning 27 30 28 31 -
trunk/MagicSoft/Mars/NEWS
r8650 r8653 58 58 - mars: There are two new heckboxes which allow to switch off 59 59 the calculated image parameters 60 61 - callisto: was broken for MCs... fixed. 62 63 - callisto: improved calculation of spline coefficients a lot. This 64 leads to a further improvement of the event rate calibrating MUX 65 data of about 15% (175evt/s instead of 150evt/s) 66 67 - callisto: finally the raw data we read is now real 16bit (with 68 10bit precision) for MUX data and not a stripped 8bit number 69 anymore. Due to scaling of the numbers (without precision loss 70 into an [0-256[ range, the final numbers for pedestal, pedestalrms 71 and extacted signal don't change. However, at all places where 72 raw data is directly accessed (eg. saturation and variation 73 limits in the signal- and pedestal-extraction) the numbers 74 refer still to the data's 16bit range. 75 76 - callisto: The maximum arrival time difference used in the bad 77 pixel treatment is now in units of nanoseconds, which leads to 3.0ns 78 for both, old FADC and MUX-FADC, data. 79 80 - callisto: Be aware that callisto is now calibrating the arrival time 81 in nanoseconds rather than time slices. Also all following tasks 82 have been changed to assume ns units now. If you star data 83 calibrated with an older version it might be necessary to adapt 84 some timimng parameters (Muon Analysis and MFSoftwareTrigger) 85 to obtain optimal results. The plot in the PulsePos tab 86 will now be in ns, too. This might also mean that the Muon 87 analysis in star might not work as perfect as expected as long 88 as old files read in. 89 90 - star: For speed reasons events suitable for the muon analysis 91 are now also preselected by fConcCOG<0.1 which seems to be a very 92 good preselector for muons. 93 94 - star: is now calculating a new timing parameter the Slope along 95 the major and minor axis of the shower. Therefore a numerical 96 solution of a line-fit is used. To use MHillasExt.fSlopeLong 97 and MHillasExt.fSlopeTrans don't forget to multiply it with 98 the sign stored in MHillasSrc.fCosDeltaAlpha as usual. 99 100 - star: The parameters fInnerSize, fInnerLeakage1 and fInnerLeakage2 101 have been removed from MNewImagePar. They have never been good for 102 anything. 60 103 61 104 - star: Implemented a new recursive algorithm which is supposed to be … … 89 132 + PostCleanType: 3 90 133 91 - callisto: was broken for MCs... fixed.92 93 - callisto: improved calculation of spline coefficients a lot. This94 leads to a further improvement of the event rate calibrating MUX95 data of about 15% (175evt/s instead of 150evt/s)96 97 - callisto: finally the raw data we read is now real 16bit (with98 10bit precision) for MUX data and not a stripped 8bit number99 anymore. Due to scaling of the numbers (without precision loss100 into an [0-256[ range, the final numbers for pedestal, pedestalrms101 and extacted signal don't change. However, at all places where102 raw data is directly accessed (eg. saturation and variation103 limits in the signal- and pedestal-extraction) the numbers104 refer still to the data's 16bit range.105 106 - callisto: The maximum arrival time difference used in the bad107 pixel treatment is now in units of nanoseconds, which leads to 3.0ns108 for both, old FADC and MUX-FADC, data.109 110 - callisto: Be aware that callisto is now calibrating the arrival time111 in nanoseconds rather than time slices. Also all following tasks112 have been changed to assume ns units now. If you star data113 calibrated with an older version it might be necessary to adapt114 some timimng parameters (Muon Analysis and MFSoftwareTrigger)115 to obtain optimal results. The plot in the PulsePos tab116 will now be in ns, too. This might also mean that the Muon117 analysis in star might not work as perfect as expected as long118 as old files read in.119 120 - star: For speed reasons events suitable for the muon analysis121 are now also preselected by fConcCOG<0.1 which seems to be a very122 good preselector for muons.123 124 - star: is now calculating a new timing parameter the Slope along125 the major and minor axis of the shower. Therefore a numerical126 solution of a line-fit is used. To use MHillasExt.fSlopeLong127 and MHillasExt.fSlopeTrans don't forget to multiply it with128 the sign stored in MHillasSrc.fCosDeltaAlpha as usual.129 130 - star: The parameters fInnerSize, fInnerLeakage1 and fInnerLeakage2131 have been removed from MNewImagePar. They have never been good for132 anything.133 134 134 135 - ganymed: The old hadronness and size cuts have gotten new indices … … 169 170 "nearest position" trick) 170 171 171 - ganymed: From XXXX on a real starguider calibration with a real172 pointing model for the starguider is done.173 174 172 - ganymed: From 85340 (19.3.2006) on a real starguider calibration 175 173 with a real pointing model for the starguider is done, calibrated … … 186 184 the Area-Cut (parameters 2,3,4) and the theta-sq cut (parameter 1) 187 185 should be optimized. All other values should be kept as they are. 186 If you want to do an anylsis without timing a parameters, you can 187 switch off the timing cuts by seeting parameter 7 to a very small 188 value (eg. -99). To remove the slope parameter from the disp 189 paremtrization set parameter 8 to 0. 190 191 - ganymed: IMPORTANT - The spark cuts have been removed from the 192 resource files because there is currently no proper known 193 cut. Whenever you do an analysis you have to find proper cuts 194 yourself! 188 195 189 196 - optim, sponde: should now properly support three off-regions. -
trunk/MagicSoft/Mars/star.rc
r8310 r8653 46 46 # Setup the image cleaning here 47 47 # ------------------------------------------------------------------------- 48 MImgCleanStd.CleanLevel1: 8.5 49 MImgCleanStd.CleanLevel2: 4.0 50 MImgCleanStd.CleanMethod: Absolute 51 #MImgCleanStd.CleanRings: 1 52 #MImgCleanStd.KeepSinglePixels: No 48 MImgCleanStd.CleanMethod: absolute 49 #MImgCleanStd.CleanLevel0: 6.0 50 MImgCleanStd.CleanLevel1: 6.0 51 MImgCleanStd.CleanLevel2: 3.0 52 MImgCleanStd.TimeLevel1: 1.75 53 MImgCleanStd.TimeLevel2: 1.75 54 MImgCleanStd.PostCleanType: 3 55 56 #MImgCleanStd.CleanRings: 3 57 #MImgCleanStd.KeepIsolatedPixels: Yes 58 #MImgCleanStd.RecoverIsolatedPixles: Yes 53 59 54 60 # -------------------------------------------------------------------------
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