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The scientist on shift has the
responsibility to monitor the quality of the data and to report in
the logbook about changes in the interferometer noise behaviour.
To
follow the ITF behaviour, the scientist can exploit some noise
monitors available on the web under the Last
trend data webpage, under the Reconstruct, Inspiral, Burst
and Noise tabs.
In particular, the scientist has the duty to
perform, every about 2 hours, the following data analysis tasks
Assess the broad-band noise behaviour by checking the evolution of the NS-NS, BH-BH horizon (procedure available here)
Monitor the rate and strength of glitches by checking the outlierMoni behaviour (procedure available here)
Monitor the rate and time-frequency characteristics of burst events by checking the Q-pipeline status (procedure available here)
Check the quality of data for inspiral searches, by looking at the statistics of MBTA events (procedure available here)
Check the quality of data for inspiral searches, by looking at the statistics of Merlino events (procedure available here)