The following image is a mosaic of a region of the sky 2.5 degrees on a side. Two separate sweeps of the sky (called Run 32 and Run 36) were made on successive nights with the 2.5-meter telescope and its mosaic camera. The 6 columns of CCDs in the camera collect data from 6 scanlines on the sky separated by small gaps. By offseting the telescope a small amount between the two runs, the scanlines from the two runs can be interleaved as indicated by the headings in the table to form a seamless map of a complete section of the sky.
Click on any portion of the mosaic to see a zoomed-in view in the frame below.
| Run 32 | Run 36 | Run 32 | Run 36 | Run 32 | Run 36 | Run 32 | Run 36 | Run 32 | Run 36 | Run 32 | Run 36 |
| Col 1 | Col 1 | Col 2 | Col 2 | Col 3 | Col 3 | Col 4 | Col 4 | Col 5 | Col 5 | Col 6 | Col 6 |
