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. 

Put one or more images or figures at the top of this column. Novices may simply "Insert" an "Image" here. Experts should create first go to the "Media Repository" page and "Create" a new "PS1 image information" page for the new image. The image information page provide a mechanism for capturing metadata and including alternate versions of the figure.

Include an infobox below the picture. Summarize key facts in the infobox. The infobox helps users quickly assess the content of the article.