\n";
-//echo "The official release of this webpage will take place on 1.9.2013.
";
-
+echo "
FACT Quick Look Analysis - Download Area
\n";
+//echo "\n";
+echo "
Data Usage Policy
\n";
+
+if ($expert=="yes")
+{
+ echo "As a member or associated member of the FACT Collaboration, you have access to internal information. \n";
+ echo "Any publication using FACT internal information has to have the full FACT author list.
\n";
+}
+else
+{
+ echo "Using data from the FACT Quick Look Analysis, you agree to cite the ";
+ echo "FACT design paper\n ";
+ echo "and the quick look analysis.\n";
+ echo "
FACT Design Paper: H. Anderhub et al. JINST 8 P6008 ADS\n ";
+ echo "open access\n
\n";
+ echo "
FACT Performance Paper: A. Biland et al. JINST 9 P10012 ADS\n ";
+ echo "open access\n
\n";
+ echo "
Information on the Quick Look Analysis: D. Dorner et al. Proceedings Fermi Symposium 2014 ADS\n ";
+ echo "open access\n
\n";
+ echo "
\n";
+}
+
+
+echo "If you intend to use data or information from this website, please let us know for reference. \n";
+
+
+//echo "\n";
echo "\n";
-echo " \n";
-echo "REMARKS: ";
-echo "
";
-//echo "
The results shown on this page are PRELIMINARY.
";
-echo "
These are the results of a fast quick look analysis on site, i.e. they are preliminary.
\n";
-echo "
The quick look analysis includes all data, i.e. no data selection done.
\n";
-//echo "
NO data check is included in the analysis.
";
-echo "
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).
\n";
-//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.";
-//echo "
NO corrections for the dependence on zenith distance and trigger threshold of the observation are applied so far.
";
-//echo "
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.
";
-echo "
The curves are provided with 20 min binning and nightly binning.
\n";
-echo "
In case, you need further details about the data or a different binning, please do not hesitate to contact us.
\n";
-echo "
QLA results are available for the data since 12.12.2012. For older data, please contact us.
\n";
-echo "
New software versions were introduced at the following dates: 24.5.2014
\n";
-echo "
";
-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";
-echo "
\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 \n";
-echo "Information on the Quick Look Analysis: D. Dorner et al. Proceedings Fermi Symposium 2014 ADS\n ";
-echo "open access\n
The correction formula to correct the excess rate for the effects of zd and threshold are not yet final.
\n";
+ echo "
The CU conversion is currently only valid for QLA and until summer 2016.
\n";
+ echo "
The data quality selection based on the artificial trigger rate R750 might not work for all data (effect of lidar).
\n";
+ //echo "\n";
+ echo "
";
+}
+else
+{
+ echo "
\n";
+ //echo "
The results shown on this page are PRELIMINARY.
";
+ echo "
These are the results of a fast quick look analysis on site, i.e. they are preliminary.
\n";
+ echo "
The quick look analysis includes all data, i.e. no data selection done.
\n";
+ //echo "
NO data check is included in the analysis.
";
+ echo "
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).
\n";
+ //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.";
+ //echo "
NO corrections for the dependence on zenith distance and trigger threshold of the observation are applied so far.
";
+ //echo "
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.
";
+ echo "
The curves are provided with 20 min binning and nightly binning.
\n";
+ echo "
In case, you need further details about the data or a different binning, please do not hesitate to contact us.
\n";
+ echo "
QLA results are available for the data since 12.12.2012. For older data, please contact us.
\n";
+ echo "
New software versions were introduced at the following dates: 24.5.2014
\n";
+ echo "
\n";
+ echo "In case you are interested in more than the public data, please contact us.\n";
+}
+
+echo "
Contact
";
+echo "Daniela Dorner dorner<at>astro.uni-wuerzburg.de ";
//echo "You acknowledge these regulations by clicking on the 'Show' button.