These are the results of a fast quick look analysis on site, i.e. they are preliminary.
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The quick look analysis includes all data, i.e. no data selection done.
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NO data check is included in the analysis.
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The shown curves are not fluxes but excess rates (number of excess events per effective ontime), \n";
-echo "i.e. there is a dependence on trigger threshold and zenith distance of the observation (with the current \n";
-echo "analysis for zenith distance > 40 degree and trigger threshold > 500 DAC counts).
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-//echo "i.e. a dependence on trigger threshold and zenith distance of the observation is expected ";
-//echo "for zenith distance larger than 40 degree and very strong moon light.";
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NO corrections for the dependence on zenith distance and trigger threshold of the observation are applied so far.
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This webpage shows the excess rates (black), i.e. number of excess events ";
-//echo "(signal minus background in the signal region) devided by the ontime of the observation, ";
-//echo "and the background rates (blue), i.e. number of background events devided by ontime.
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The curves are provided with 20 min binning and nightly binning.
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In case, you need further details about the data or a different binning, please do not hesitate to contact us.
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QLA results are available for the data since 12.12.2012. For older data, please contact us.
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New software versions were introduced at the following dates: 24.5.2014
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-echo "If you intend to use the data or information from this website, please let us know for reference. \n";
-echo "Please cite this webpage and the ";
-echo "FACT design paper\n ";
-echo "when using information from this webpage or any FACT data.\n";
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\n \n ";
-echo "Reference FACT Design Paper: H. Anderhub et al. JINST 8 P6008 ADS\n ";
-echo "open access\n \n";
-echo "Reference FACT Performance Paper: A. Biland et al. JINST 9 P10012 ADS\n ";
-echo "open access\n
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-echo "Contact: Daniela Dorner dorner<at>astro.uni-wuerzburg.de. ";
-//echo "You acknowledge these regulations by clicking on the 'Show' button.