Timeline
11/07/03:
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11/06/03:
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11/05/03:
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11/04/03:
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11/03/03:
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- 12:58 Changeset [2453] by
- Independent reference time for each telescope.
- 12:49 Changeset [2452] by
- Bug fixed in MFadc::Pedestal() and in print out.
- 12:44 Changeset [2451] by
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- We add a function member to set seed of rundom numbers.
10/31/03:
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10/30/03:
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10/29/03:
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- New constructot added to decouple the StarResponse from MARS.
- 19:13 Changeset [2443] by
- New constructor needed to decouple StarResponse from MARS.
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- 13:23 Changeset [2439] by
- Added write permission for 'marcos'
10/28/03:
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10/27/03:
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10/26/03:
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- 20:18 Changeset [2433] by
- Now it writes in the screen its cahracteristiques while the constructor is called.
- 20:12 Changeset [2432] by
- The compilation option -fno-rtti -fno-exceptions has been removed.
- 20:03 Changeset [2431] by
- A define VERSIONSR has been introduced, now it is 1000.0
- 20:01 Changeset [2430] by
- A check of the StarResponse version has been introduced. If the one used for the generation of the database and the one of the current software used is not the same, the camera program will stop. Current verion 1000.0
- 19:51 Changeset [2429] by
- Header file for creadparam.cxx version 1.25
- 19:45 Changeset [2428] by
- The write_all_data input card command has been removed.
- 19:43 Changeset [2427] by
- - The screen output information has been improved to prevent some non-desired running conditions just looking at the output screen. - One MMcEvt for each Telscope is stored in the output file. - 500 empty events are simualted to get a more precise estimation of the pedestal Sigma for each pixel.
10/24/03:
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10/23/03:
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10/22/03:
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10/21/03:
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- A factor 2.35 to transform the fwhm into the sigma of gaussian was missing in the storing of FADC single hpe pulse determination.
10/20/03:
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- 13:06 Changeset [2401]
- This commit was manufactured by cvs2svn to create tag 'Mars_V0-8-1'.
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10/17/03:
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- 20:40 Changeset [2391] by
- The gain ratio between the high and low FADC gain is controlled from the input card.
- 20:39 Changeset [2390] by
- Factor used for the NSB scaling for several qe files is defined.
- 20:38 Changeset [2389] by
- Now the camera program will stop if a undefined Geometry is required. The NSB is internally scaled for any camera geometry and qe. The seeds in the input card are used to initilize the random numbers. The Amplitud stored in the MMcFadcHeader is the amplitud of the sphe reponse. The Pedestal rms is simualted in a artificail empty event.
10/15/03:
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