Evaluation of scientific complementary metal-oxide-semiconductor sensors for sky survey applications

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F19%3A00522114" target="_blank" >RIV/68378271:_____/19:00522114 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1002/asna.201913669" target="_blank" >https://doi.org/10.1002/asna.201913669</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1002/asna.201913669" target="_blank" >10.1002/asna.201913669</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Evaluation of scientific complementary metal-oxide-semiconductor sensors for sky survey applications

Popis výsledku v původním jazyce

Scientific complementary metal–oxide–semiconductor (CMOS) image sensors are a modern alternative for typical charge‐coupled device detectors, as they offer low read‐out noise, large sensitive area, and high frame rates. All these make them promising devices for a modern wide‐field sky surveys. However, the peculiarities of CMOS technology have to be properly taken into account when analyzing the data. In order to characterize these, we performed extensive laboratory testing of Andor Marana scientific CMOS (sCMOS) camera. Here, we report its results, especially on the temporal stability and linearity, and compare it with the previous versions of Andor sCMOS cameras. We also present the results of an on‐sky testing of this sensor connected to a wide‐field lens and discuss its applications for astronomical sky surveys.n

Název v anglickém jazyce

Evaluation of scientific complementary metal-oxide-semiconductor sensors for sky survey applications

Popis výsledku anglicky

Scientific complementary metal–oxide–semiconductor (CMOS) image sensors are a modern alternative for typical charge‐coupled device detectors, as they offer low read‐out noise, large sensitive area, and high frame rates. All these make them promising devices for a modern wide‐field sky surveys. However, the peculiarities of CMOS technology have to be properly taken into account when analyzing the data. In order to characterize these, we performed extensive laboratory testing of Andor Marana scientific CMOS (sCMOS) camera. Here, we report its results, especially on the temporal stability and linearity, and compare it with the previous versions of Andor sCMOS cameras. We also present the results of an on‐sky testing of this sensor connected to a wide‐field lens and discuss its applications for astronomical sky surveys.n

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/EF15_003%2F0000437" target="_blank" >EF15_003/0000437: Kosmologie, gravitace a temný sektor vesmíru</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2019

Kód důvěrnosti údajů

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

Název periodika

Astronomische Nachrichten

ISSN

0004-6337

e-ISSN

—

Svazek periodika

340

Číslo periodika v rámci svazku

7

Stát vydavatele periodika

DE - Spolková republika Německo

Počet stran výsledku

8

Strana od-do

638-645

Kód UT WoS článku

000493339600014

EID výsledku v databázi Scopus

2-s2.0-85074274241