LOFT - the Large Observatory For x-ray Timing

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F12%3A00201667" target="_blank" >RIV/68407700:21230/12:00201667 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/67985815:_____/12:00387296 RIV/47813059:19240/12:#0004523 RIV/68407700:21340/12:00201667

Výsledek na webu

<a href="http://arxiv.org/pdf/1209.1497.pdf" target="_blank" >http://arxiv.org/pdf/1209.1497.pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1117/12.926310" target="_blank" >10.1117/12.926310</a>

Jazyk výsledku

angličtina

Název v původním jazyce

LOFT - the Large Observatory For x-ray Timing

Popis výsledku v původním jazyce

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to exploit the diagnostics of rapid X-ray flux and spectral variability that directly probe the motion of matter down to distances very close to black holes and neutron stars, as well as the physical state of ultradense matter. These primary science goals will be addressed by a payload composed of a Large Area Detector (LAD) and a Wide Field Monitor (WFM). The LAD is a collimated (<1 degree field of view) experiment operating in the energy range 2-50 keV, with a 10 m(2) peak effective area and an energy resolution of 260eV at 6 keV. The WFM will operate in the same energy range as the LAD, enabling simultaneous monitoring of a few-steradian wide field of view, with an angular resolution of <5 arcmin. The LAD and WFM experiments will allow us to investig

Název v anglickém jazyce

LOFT - the Large Observatory For x-ray Timing

Popis výsledku anglicky

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is currently planned for between 2022 and 2024. LOFT is designed to exploit the diagnostics of rapid X-ray flux and spectral variability that directly probe the motion of matter down to distances very close to black holes and neutron stars, as well as the physical state of ultradense matter. These primary science goals will be addressed by a payload composed of a Large Area Detector (LAD) and a Wide Field Monitor (WFM). The LAD is a collimated (<1 degree field of view) experiment operating in the energy range 2-50 keV, with a 10 m(2) peak effective area and an energy resolution of 260eV at 6 keV. The WFM will operate in the same energy range as the LAD, enabling simultaneous monitoring of a few-steradian wide field of view, with an angular resolution of <5 arcmin. The LAD and WFM experiments will allow us to investig

Druh

D - Stať ve sborníku

CEP obor

BH - Optika, masery a lasery

OECD FORD obor

—

Projekt

—

Návaznosti

Z - Vyzkumny zamer (s odkazem do CEZ)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2012

Kód důvěrnosti údajů

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

Název statě ve sborníku

SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY

ISBN

978-0-8194-9144-2

ISSN

0277-786X

e-ISSN

—

Počet stran výsledku

16

Strana od-do

—

Název nakladatele

SPIE - The International Society for Optical Engineering

Místo vydání

Washington

Místo konání akce

Amsterdam

Datum konání akce

1. 7. 2012

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000312391600064