Electro-optical testing of fully depleted CCD image sensors for the large synoptic survey telescope camera

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F14%3A00485396" target="_blank" >RIV/68378271:_____/14:00485396 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1117/12.2056733" target="_blank" >http://dx.doi.org/10.1117/12.2056733</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1117/12.2056733" target="_blank" >10.1117/12.2056733</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Electro-optical testing of fully depleted CCD image sensors for the large synoptic survey telescope camera

Popis výsledku v původním jazyce

The LSST Camera science sensor array will incorporate 189 large format Charge Coupled Device (CCD) image sensors. Each CCD will include over 16 million pixels and will be divided into 16 equally sized segments and each segment will be read through a separate output amplifier. The science goals of the project require CCD sensors with state of the art performance in many aspects. The broad survey wavelength coverage requires fully depleted, 100 micrometer thick, high resistivity, bulk silicon as the imager substrate. Image quality requirements place strict limits on the image degradation that may be caused by sensor effects: optical, electronic, and mechanical. In this paper we discuss the design of the prototype sensors, the hardware and software that has been used to perform electro-optic testing of the sensors, and a selection of the results of the testing to date.n

Název v anglickém jazyce

Electro-optical testing of fully depleted CCD image sensors for the large synoptic survey telescope camera

Popis výsledku anglicky

The LSST Camera science sensor array will incorporate 189 large format Charge Coupled Device (CCD) image sensors. Each CCD will include over 16 million pixels and will be divided into 16 equally sized segments and each segment will be read through a separate output amplifier. The science goals of the project require CCD sensors with state of the art performance in many aspects. The broad survey wavelength coverage requires fully depleted, 100 micrometer thick, high resistivity, bulk silicon as the imager substrate. Image quality requirements place strict limits on the image degradation that may be caused by sensor effects: optical, electronic, and mechanical. In this paper we discuss the design of the prototype sensors, the hardware and software that has been used to perform electro-optic testing of the sensors, and a selection of the results of the testing to date.n

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2014

Kód důvěrnosti údajů

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

Název statě ve sborníku

High Energy, Optical, and Infrared Detectors for Astronomy VI

ISBN

978-0-8194-9622-5

ISSN

0277-786X

e-ISSN

—

Počet stran výsledku

17

Strana od-do

—

Název nakladatele

SPIE

Místo vydání

Bellingham

Místo konání akce

Montreal

Datum konání akce

22. 6. 2014

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000354528900035