This page describes the telescope and instruments used to obtain the data in the PS1 survey, including design and construction; the detectors; the filters used; and the observing strategies. The starting point for the PS1 data archive is at The Pan-STARRS1 data archive home page.
Contents
Parent page for the description of the observatory.
The information for this page should be taken from Chambers et al 2016.
Planned contents:
Here is from PS1 dox summary:
The hardware and the survey operations (scheduling) and cadence is described in Chambers 2016.
- Design, construction (UH: Ken Chambers):
- Telescope, location
- FOV
- Image quality
- Site quality (seeing, clarity, backgrounds)
- Detectors: (UH, Tonry?)
- Relation to data quality
- Dynamic range (depth tables)
- Filters: (UH data; Scolnic)
- Illustration
- Compare to others that are nominally the same or similar.
- Observing strategy: (UH)
- Faint- and bright limits.
- Areal coverage versus time
- Distributions of data taking: Numbers of visits; ...
- Surveys (Ken?, Stephen?)
- 3PI. (cut & paste? Smart/Chambers --> DRS)
- Medium Deep Fields.
- 3PI. (cut & paste? Smart/Chambers --> DRS)