Stellar intensity interferometric capabilities of IACT Arrays

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00553120" target="_blank" >RIV/68378271:_____/18:00553120 - isvavai.cz</a>

Result on the web

<a href="https://pos.sissa.it/301/828/pdf" target="_blank" >https://pos.sissa.it/301/828/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.301.0828" target="_blank" >10.22323/1.301.0828</a>

Result language

angličtina

Original language name

Stellar intensity interferometric capabilities of IACT Arrays

Original language description

Sub-milliarcsecond imaging of nearby main sequence stars and binary systems can provide critical information on stellar phenomena such as rotational deformation, accretion effects, and the universality of starspot (sunspot) cycles. Achieving this level of resolution in optical wavelength bands (U/V) requires use of a sparse array of interferometric telescopes with kilometer scale baseline separations. Current ground based VHE gamma-ray observatories, such as VERITAS, HESS, and MAGIC, employ arrays of > 10 m diameter optical Imaging Atmospheric Cherenkov Telescopes (IACTs) with >80 m telescope separations, and are therefore well suited for sub-milliarcsecond astronomical imaging in the U/V bands using Hanbury Brown and Twiss (HBT) interferometry.n

Czech name

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Czech description

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Type

D - Article in proceedings

CEP classification

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OECD FORD branch

10303 - Particles and field physics

Project

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Continuities

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Publication year

2018

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Proceedings of Science

ISBN

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ISSN

1824-8039

e-ISSN

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Number of pages

8

Pages from-to

1-8

Publisher name

Sissa Medilab srl

Place of publication

Trieste

Event location

Busan

Event date

Jul 10, 2017

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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