There is a computer at UofM that is configured to act as a web server for the URL http://www.rotse.net. Once a minute, a PERL script runs on this computer. It queries each ROTSE-III control computer in sequence over a socket connection with the rotsed on each system. It extracts a packet of status variable values and writes them to a local text file in JavaScript format. These variables give information about the state of the entire telescope, which daemons are running, what alarms are currently active, what the weather conditions are, and various header values from the most recent image recorded. The JavaScript files are accessed by the web pages on our site in order to display up-to-the-minute tables of the system status. See Figure 8.4 for an example of what an active display might look like.
Along with the JavaScript status variables, we also copy the thumbnail images that are produced by sexpacman (Section 8.2.1), as well as the analysis status monitor GIF file produced by idlpacman (Section 8.2.2). These images can be accessed through the pushing of buttons on the status display table page, as shown in Figure 8.4. Figure 8.2 shows a typical thumbnail, and Figure 8.3 shows an example of an analysis status image.
Upon receipt of a pager alert message from rotsepager, you may wish to monitor telescope response by periodically reloading http://www.rotse.net/burst_response/, which is automatically updated by software both at the site and on rotse1. These pages will contain tables listing any uncatalogued or highly variable sources near the published GRB position, along with light curve plots and cropped images for each observation. The presence of a candidate GRB counterpart should be immediately obvious from these data. See Sections 8.2.3 and 8.4.1 for more information.
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