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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.

Contents

Parent page for the description of the observatory.

The information for this page should be taken from Chambers et al 2016.  

Details about bad pixel mask should refer to Waters 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.

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