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The Pan-STARRS wide-field optical/NIR imaging survey
Abstract
Pan-STARRS is a highly cost-effective, modular and scalable approach to wide-field optical/NIR imaging. It uses 1.8m telescopes with very large (7 square degree) field of view and revolutionary1.4 billion pixel CCD cameras with low noise and rapid read-out to provide broad-band imaging from 400-1000nm wavelength. The first single telescope system, PS1, has been deployed on Haleakala on Maui, and has been collecting science quality survey data for approximately six months. PS1 will be joined by a second telescope PS2 in approximately 18 months. A four aperture system is planned to become operational following the end of the PS1 mission. This will be able to scan the entire visible sky to approximately 24th magnitude in less than a week, thereby meeting the goals set out by the NAS 2000 decadal review for a "Large Synoptic Sky Telescope". Here we review the technical design, and give an update on the progress that has been made with the PS1 system.
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“We note that the Pan-STARRS project ( Kaiser et al. 2002, 2010 ) , with similar science goals to LSST, envisions a distributed aperture design, where the total system étendue is a sum of étendue values for an array of small 1.8 m telescopes.”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Kaiser et al. 2010
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Metadata
- Authors
- Kaiser, N., Burgett, W., Chambers, K., Denneau, L., Heasley, J., Jedicke, R., Magnier, E., Morgan, J., Onaka, P., & Tonry, J.
- Affiliations
- University of Hawaiʻi at Mānoa (US)
- Venue
- SPIE Proceedings
- Publisher
- SPIE
- Published
- 2010-07-16
- Volume
- 7733
- Pages
- 77330E
- ISSN
- 0277-786X (ISSN-L)
- OpenAlex
- W2079595033
- Cited by
- 508
- References
- 0
- Citations by year
- 2026: 11 · 2025: 21 · 2024: 30 · 2023: 19 · 2022: 25 · 2021: 22 · 2020: 36 · 2019: 44 · 2018: 52 · 2017: 54 · 2016: 65 · 2015: 41 · 2014: 32 · 2013: 29 · 2012: 22
- FWCI
- 22.66
- Type
- conference paper
- Language
- en
- Open access
- closed
- Locations
- Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Adaptive optics and wavefront sensing
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astronomical Observations and Instrumentation
- Keywords
- Pan-STARRS, wide-field optical imaging, near-infrared imaging, CCD detector, Haleakala, telescope design, sky survey
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
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