XIPE the X-ray Imaging Polarimetry Explorer

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00471839" target="_blank" >RIV/67985815:_____/16:00471839 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/47813059:19240/16:N0000139

Výsledek na webu

<a href="http://dx.doi.org/10.1117/12.2233046" target="_blank" >http://dx.doi.org/10.1117/12.2233046</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1117/12.2233046" target="_blank" >10.1117/12.2233046</a>

Jazyk výsledku

angličtina

Název v původním jazyce

XIPE the X-ray Imaging Polarimetry Explorer

Popis výsledku v původním jazyce

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X- ray astronomers with 75% of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.

Název v anglickém jazyce

XIPE the X-ray Imaging Polarimetry Explorer

Popis výsledku anglicky

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X- ray astronomers with 75% of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.

Druh

D - Stať ve sborníku

CEP obor

BH - Optika, masery a lasery

OECD FORD obor

—

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2016

Kód důvěrnosti údajů

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

Název statě ve sborníku

Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray

ISBN

9781510601895

ISSN

—

e-ISSN

—

Počet stran výsledku

20

Strana od-do

"990515/1"-"990515/20"

Název nakladatele

SPIE

Místo vydání

Bellingham

Místo konání akce

Edinburgh

Datum konání akce

26. 6. 2016

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000387731500030