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Next is a sky map showing the whole sky (above the horizon) at the time of the observation, including bright GLEAM sources, other bright sources in the field including the Sun, Moon and Jupiter, and contour lines showing the primary (tile) beam at the centre frequency used in that observation.
To the right of the sky map is the schedule map for that day (described below) - a graphical representation of the MWA schedule covering that 24 hour period.
Next is a table with all log entries referring to that observation.
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The full waterfall plot is divided into three sections, left-right - X pol, X-Y, and Y pol. Each has frequency (0 - 327.68 MHz) on the horizontal axis, time (hours before the time that the plot was generated, most recent times at the top of the plot) on the vertical axis, and colour indicating the PPD power for that tile, at that frequency, at that time. There are tick markers on the inner vertical axes - major ticks every two hours, and minor ticks at the start of each scheduled MWA observation. Clicking inside the plot shows a new page with a graph of the full-spectrum power from that tile, at that instant (which depends where in the plot you click).
Schedule maps:
Graphical maps showing the contents of the MWA schedule are available here: http://telemetry-static.mwa128t.org/schedmap/2018/index.html
The main page shows thumbnail maps of each day, grouped in rows by week, most recent at the top. Clicking on a week date (left column) brings up the maps for all seven days in that week, each showing a 24 hour period.
Inside each plot, UTC time is on the vertical axis, and Right Ascension (in hours) is on the horizontal axis. A diagonal line of black circles shows the RA at the zenith (the Local Sidereal TIme) at that time. A vertical line of yellow circles shows the RA of the Sun at that time. MWA observations in the schedule are shown as horizontal coloured bars. The height of each bar is determined by the length of the observation. The horizontal position and width of the bar is determined by the coordinates of the observation - if the observation was created using Azimuth and Elevation coordinates, then a solid bar is drawn where the centre is at the RA value for that Az/El at that time, and the width is the range of RA values covered by the primary beam width. If the observation was created using RA and Dec values, a solid bar is drawn centred on that RA with a width given by the primary beam size, and a lighter coloured bar is drawn on either side, showing the range of RA values above the horizon at that time, at that declination.
Clicking on the bar representing a single observation in that schedule map brings up a new window showing the observation information page, for that observation.