Versions Compared

Key

  • This line was added.
  • This line was removed.
  • Formatting was changed.


Excerpt

The Pan-STARRS telescopes are located at Haleakala Observatories on the island of Maui. The first telescope built, the Pan-STARRS1 Telescope (PS1), is an alt-az telescope with an 1.8m diameter mirror. With a field-of-view diameter of 3 degrees, it can observe a 7 square degree are on the sky with every exposure. The PS1: GPC1 camera, which uses 60 Orthogonal Transfer Arrays devices, is mounted in its focal plane. The PS1 observations are obtained through a set of five broadband filters, designated as grizyP1. Under certain circumstances PS1 observations are obtained with a sixth, “wide” filter designated as wP1 that essentially spans the gri bands. The PS1 Observing strategy was optimized for detecting moving objects as well as a uniform coverage of the 3pi survey (see PS1 Description of the surveys).

 


The starting point for the PS1 data archive is at Pan-STARRS1 data archive home page.

The information on the pages below is  taken from Chambers et al 2016, "The Pan-STARRS1 Surveys" and this paper should be cited when information is used. 

This page describes the telescope and instruments used to obtain the PanSTARRS data, including design and construction; the detectors; the filters used; and the observing strategies.

 

Tip
iconfalse
titleContents

Table of Contents
maxLevel2
indent20px

Parent page for the description of the observatory.

Planned contents:

Excerpt
  • Facility design and construction
    • The telescope, location, FOV
    • Site quality
  • Detectors
    • Description, numbering scheme
    • Bad pixel masks
    • Evolution of detectors over the survey period
    • Unique qualities and relation to observing strategy and data quality
    • Dynamic range
  • Filters
    • Selection criteria
    • Throughput curves
    • Comparison to nominally similar other filters
  • Seeing - distribution function by filter
Alignalignleft