The year-long keogram is constructed from daily keograms, where each daily keogram takes the central pixel column of the all-sky images of each successive image to show motion in the sky. This video shows the all-sky images for a 24h time span and the resulting keogram shown below.

Zooming in on the daily keograms, the motion of celestial objects becomes clear. These daily keograms from January 16th to February 2nd 2024 show the Moon moving across the sky. It starts at sunset near first quarter, culminates around full moon, and ends at sunrise near last quarter.

Similarly, the stars move across the sky. During June, when the nights on the Northern hemisphere are short and the sky does not fully darken, the bright star Vega is high in the sky. Over these 12 daily keograms, we see Vega moving slowly left by 4 minutes every day.

During 2024 there were two nights with Northern Lights that were relatively clear. The keograms of those nights captured the colors and motion of the Aurora Borealis. Keograms were specifically designed to study the Aurora: https://victoriaweather.ca/keogram.php.

The all-sky camera consists of a ZWO ASI178MC color camera with a 2.5mm F/1.2 fish-eye lens. A small Raspberry Pi computer operates the camera and sets the exposure time and camera gain based on the sky brightness. It also controls a dew heater and a fan to prevent condensation on the acrylic dome.