Impact of Laser Guide Star facilities on neighbouring telescopes: the case of GTC, TMT, VLT, and ELT lasers and the Cherenkov Telescope Array

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F18%3A00546827" target="_blank" >RIV/68378271:_____/18:00546827 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1093/mnras/sty2188" target="_blank" >https://doi.org/10.1093/mnras/sty2188</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1093/mnras/sty2188" target="_blank" >10.1093/mnras/sty2188</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Impact of Laser Guide Star facilities on neighbouring telescopes: the case of GTC, TMT, VLT, and ELT lasers and the Cherenkov Telescope Array

Popis výsledku v původním jazyce

Powerful Laser Guide Star (LGS) systems are standard for the next generation of extremely large telescopes. However, modern earth-based astronomy has gone through a process of concentration on few sites with exceptional sky quality, resulting in those becoming more and more crowded. The future LGS systems encounter hence an environment of surrounding astronomical installations, some of which observing with large fields of view. We derive formulae to calculate the impact of LGS light on the camera of a neighbouring telescope and the probabilities for a laser crossing the camera field of view to occur, and apply these to the specific case of the next very high energy gamma-ray observatory 'Cherenkov Telescope Array' (CTA).

Název v anglickém jazyce

Impact of Laser Guide Star facilities on neighbouring telescopes: the case of GTC, TMT, VLT, and ELT lasers and the Cherenkov Telescope Array

Popis výsledku anglicky

Powerful Laser Guide Star (LGS) systems are standard for the next generation of extremely large telescopes. However, modern earth-based astronomy has gone through a process of concentration on few sites with exceptional sky quality, resulting in those becoming more and more crowded. The future LGS systems encounter hence an environment of surrounding astronomical installations, some of which observing with large fields of view. We derive formulae to calculate the impact of LGS light on the camera of a neighbouring telescope and the probabilities for a laser crossing the camera field of view to occur, and apply these to the specific case of the next very high energy gamma-ray observatory 'Cherenkov Telescope Array' (CTA).

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2018

Kód důvěrnosti údajů

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

Název periodika

Monthly Notices of the Royal Astronomical Society

ISSN

0035-8711

e-ISSN

1365-2966

Svazek periodika

481

Číslo periodika v rámci svazku

1

Stát vydavatele periodika

GB - Spojené království Velké Británie a Severního Irska

Počet stran výsledku

22

Strana od-do

727-748

Kód UT WoS článku

000449651400054

EID výsledku v databázi Scopus

2-s2.0-85055208720