Evryscope

{{Update|date=July 2021}}

{{Infobox telescope

| coordinates = Cerro Tololo:
{{coord|-30.167778|-70.805278|format=dms|display=inline|region:CL-CO_type:landmark|name=Evryscope-South}}
Mount Laguna:
{{coord|32|50|33|N|116|25|41|W|type:landmark_region:US-CA|display=inline|name=Evryscope-North}}

}}

The Evryscopes are a set of rapid-cadence, gigapixel-scale telescopes. Each instrument contains an array of up to 24 camera units, each consisting of a {{Convert|6.1|cm|in|abbr=on}} telescope (85 mm Rokinon DSLR lens) paired to a thermoelectrically cooled astronomical CCD. The camera units are arranged around a solid fiberglass structure to form a continuous field of view of 9216 sq. deg.

The first instrument (Evryscope-South) was deployed in May 2015 to Cerro Tololo Inter-American Observatory, where it is co-located with the PROMPT Telescopes. The second instrument (Evryscope-North) was deployed in October 2018 to Mount Laguna Observatory.

Evryscope detected the first The First Naked-Eye Superflare Detected from Proxima Centauri. In March 2016, the Evryscope observed the first superflare that was visible to the naked eye from Proxima Centauri. Proxima increased in brightness by a factor of roughly 68 times during the superflare and released a bolometric energy of 10^33.5 erg, about 10 times larger than any previously detected flare from Proxima Centauri.{{Cite web |last=Cowing |first=Keith |date=2018-04-09 |title=The First Naked-Eye Superflare Detected from Proxima Centauri |url=https://astrobiology.com/2018/04/the-first-naked-eye-superflare-detected-from-proxima-centauri.html |access-date=2025-04-01 |website=Astrobiology |language=en-US}}

Evryscope-South is funded by NSF/ATI and NSF/CAREER and was designed and built at the University of North Carolina at Chapel Hill. Evryscope-North is funded in collaboration with San Diego State University.

The Argus Array Pathfinder, a technological successor with 38 cameras, was deployed in December 2022 at PARI, North Carolina. It serves as a prototype for the Argus Array, which will be a 900 camera survey instrument and replace the CCD technology with MOSFET detectors.{{Cite web |title=All-seeing telescope will snap exploding stars, may spy a hidden world |url=https://www.science.org/content/article/all-seeing-telescope-will-snap-exploding-stars-may-spy-hidden-world |access-date=2022-08-29 |website=www.science.org |language=en}}{{Cite web |title=The Argus Array |url=https://evryscope.astro.unc.edu/the-argus-array/ |access-date=2022-08-29 |website=The Argus Array & the Evryscopes |language=en-US}}

See also

References

{{Reflist|refs=

{{cite conference|bibcode=2014SPIE.9145E..0ZL|doi=10.1117/12.2057031|arxiv=1407.0026|chapter=The Evryscope: the first full-sky gigapixel-scale telescope|title=Ground-based and Airborne Telescopes V|volume=9145|pages=91450Z|series=Ground-based and Airborne Telescopes V|year=2014|last1=Law|first1=Nicholas M|last2=Fors|first2=Octavi|last3=Wulfken|first3=Philip|last4=Ratzloff|first4=Jeffrey|last5=Kavanaugh|first5=Dustin}}

{{Cite web| last1 = Law| first1 = Nicholas| title = Northern Evryscope deployed!| work = The Evryscope| accessdate = 2019-03-06| date = 2018-10-27| url = http://evryscope.astro.unc.edu/2018/10/27/northern-evryscope-deployed/}}

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