Novel X-ray imaging instrumentation for astrophysics

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00645236" target="_blank" >RIV/67985815:_____/25:00645236 - isvavai.cz</a>

Výsledek na webu

<a href="https://pos.sissa.it/482/067/pdf" target="_blank" >https://pos.sissa.it/482/067/pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.482.0067" target="_blank" >10.22323/1.482.0067</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Novel X-ray imaging instrumentation for astrophysics

Popis výsledku v původním jazyce

The recent progress in innovative X-ray imaging instrumentation for astrophysics is briefly discussed. The capabilities of the novel instrumentation for investigating celestial X-ray sources are also discussed, along with recent technological progress. We have developed and tested advanced novel Kirkpatrick Baez, Lobster-Eye (LE), and Hybrid X-ray optics mirror technologies, including the calibration and testing of the ongoing developments of this optic. We presented the possibilities of monitoring the objects in the Galactic center region in the soft X-ray energy band by a small LE telescope on a CubeSat-like satellite platform. Even some instruments not designed for astronomy are suitable for investigating the X-ray activity of cosmic sources. E.g., a Soft Xray Imager (SXI) (LE telescope observing in a soft X-ray band) onboard the ESA-CAS satellite SMILE (designed for X-ray imaging of solar wind Charge eXchange of the magnetosheath and the cusps) is also essential for astrophysics because it is able to provide wide-field imaging of the sky in the soft X-ray region and can be used for investigating the activity of cosmic X-ray sources.

Název v anglickém jazyce

Novel X-ray imaging instrumentation for astrophysics

Popis výsledku anglicky

The recent progress in innovative X-ray imaging instrumentation for astrophysics is briefly discussed. The capabilities of the novel instrumentation for investigating celestial X-ray sources are also discussed, along with recent technological progress. We have developed and tested advanced novel Kirkpatrick Baez, Lobster-Eye (LE), and Hybrid X-ray optics mirror technologies, including the calibration and testing of the ongoing developments of this optic. We presented the possibilities of monitoring the objects in the Galactic center region in the soft X-ray energy band by a small LE telescope on a CubeSat-like satellite platform. Even some instruments not designed for astronomy are suitable for investigating the X-ray activity of cosmic sources. E.g., a Soft Xray Imager (SXI) (LE telescope observing in a soft X-ray band) onboard the ESA-CAS satellite SMILE (designed for X-ray imaging of solar wind Charge eXchange of the magnetosheath and the cusps) is also essential for astrophysics because it is able to provide wide-field imaging of the sky in the soft X-ray region and can be used for investigating the activity of cosmic X-ray sources.

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

2025

Kód důvěrnosti údajů

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

Název statě ve sborníku

Proceedings of Science

ISBN

—

ISSN

1824-8039

e-ISSN

—

Počet stran výsledku

8

Strana od-do

067

Název nakladatele

Sissa Medilab srl

Místo vydání

Trieste

Místo konání akce

Palermo

Datum konání akce

9. 9. 2024

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

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