| 1 | camera 0.5
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| 2 | input_file /home/magic/RawData/Proton_20_1_370to379.rfl
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| 3 | #
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| 4 | # Reflector format file that gives the NSB from the stars
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| 5 | #starfield_file /home/magic/RawData/CrabNebula.rfl
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| 6 | #
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| 7 | # Center of the FOV for stars light, right information should
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| 8 | # be here since it is no checked in the Camera program (RA and DEC)
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| 9 | #starfield_center 5 34 32 22 00 55
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| 10 | #
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| 11 | # Output file with a brief summary about trigger
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| 12 | data_file test.dat
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| 13 | #
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| 14 | # Root file with the output information
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| 15 | root_file test.root
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| 16 | #
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| 17 | # Information about the telescope
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| 18 | ct_file ../Data/magic.def
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| 19 | #
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| 20 | # Directory to look for the NSB database (it should finish with /)
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| 21 | nsb_directory /tmp/Starlight/
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| 22 | #
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| 23 | # Diskriminator and response properties (gate_lentgh, minimum overlaping time,
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| 24 | # amplitude and fwhm) needed for the trigger studies
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| 25 | trigger_prop 6.0 0.25 1.0 2.0
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| 26 | #
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| 27 | # Trig electronic noise (the width of the gaussian noise is that times
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| 28 | # the amplitude of the single phe response for the trigger)
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| 29 | trig_noise 0.3
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| 30 | #
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| 31 | # Fadc properties (amplitude and fwhm) needed for the fadc simulation
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| 32 | fadc_prop 4.0 5.0
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| 33 | #
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| 34 | # Fadc electronic noise (width of the gaussian on top of FADC signal)
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| 35 | fadc_noise 2.0
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| 36 | #
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| 37 | # Trigger loop mode (theshold, multiplicity and topology)
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| 38 | #trigger_loop 4 7 4 4 2 2
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| 39 | #
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| 40 | # Single trigger mode (theshold, multiplicity and topology)
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| 41 | trigger_single 3 4 2
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| 42 | #
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| 43 | # Pixels with special trigger threshold (one line for each pixel)
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| 44 | #pixel_thres 37 7.0
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| 45 | #
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| 46 | # Write also images that do not trigger
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| 47 | #write_all_images
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| 48 | #
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| 49 | # Do not write Mc information
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| 50 | #nowrite_McEvt
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| 51 | #
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| 52 | # Write Mc trigger information
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| 53 | write_McTrig
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| 54 | #
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| 55 | # Write Mc fadc information
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| 56 | write_McFadc
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| 57 | #
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| 58 | # Analised pixels
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| 59 | ana_pixels 577
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| 60 | #
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| 61 | # Switch off the Electronic Noise
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| 62 | #elec_noise_off
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| 63 | #
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| 64 | # Switch on NSB
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| 65 | #nsb_on
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| 66 | #
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| 67 | # Switch off NSB
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| 68 | nsb_off
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| 69 | # Number of photons from the diffuse NSB and
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| 70 | # minmum number of phe from shower required to simulate NSB
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| 71 | nsb_mean 0.09 10
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| 72 | #
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| 73 | # Show signal of diskriminator on the screen
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| 74 | #trigger_scan
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| 75 | #
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| 76 | # Show signal of FADC on the screen
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| 77 | #fadc_scan
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| 78 | #
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| 79 | # Select Energy of particles
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| 80 | #select_energy 0 10000000000
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| 81 | #
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| 82 | # Skip showers (interactive)
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| 83 | #skip
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| 84 | #
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| 85 | #Data from STDIN
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| 86 | #data_from_stdin
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| 87 | #
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| 88 | # Seeds for random numbers
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| 89 | seeds 69184 10406
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| 90 | #
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| 91 | # Axis of the telescope while running the reflector simualtion
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| 92 | # 200 400 means that the telescope axis is always paralel to the
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| 93 | # shower axis
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| 94 | telescope_axis 20 90
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| 95 | #
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| 96 | # Distance from source position to camera center (Theta, phi)
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| 97 | source_offset 0.0 0.0
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| 98 | #
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| 99 | # Version of the Corsika, the actual version*1000
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| 100 | corsika_vers 5200
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| 101 | #
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| 102 | # End of steercards
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| 103 | end_file
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| 104 |
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| 105 |
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