Scheduling in Targeted Transient Surveys and a New Telescope for CHASE

Figure 6

Approximate transmission curves for the filters implemented in our future 50 cm telescope. “Open” corresponds to no filters, and includes the effects of atmospheric extinction, mirror reflectivity and CCD quantum efficiency. The supernova search will be likely performed in “Open” mode or with a clear filter, but for the follow-up program we will use the filters shown here. It is possible that in the future we will include additional filters.