Soft X-ray observing the cosmic sources by the ESA-CAS satellite SMILE

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00586887" target="_blank" >RIV/67985815:_____/24:00586887 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68407700:21230/24:00373349

Výsledek na webu

<a href="https://doi.org/10.1016/j.jheap.2024.02.005" target="_blank" >https://doi.org/10.1016/j.jheap.2024.02.005</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.jheap.2024.02.005" target="_blank" >10.1016/j.jheap.2024.02.005</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Soft X-ray observing the cosmic sources by the ESA-CAS satellite SMILE

Popis výsledku v původním jazyce

This paper describes the scientific potential of a Soft X-ray Imager (SXI) onboard the ESA-CAS satellite SMILE for investigating cosmic X-ray sources of various types. We show that this instrument, albeit 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. Regarding sufficiently luminous X-ray sources with continuous spectra to be observable by the X-ray monitor MAXI/ISS to assess the object types and their light curves that are expected to be detected by SXI/SMILE, the compact sources accreting matter are promising targets for evaluating the possibilities of SXI.

Název v anglickém jazyce

Soft X-ray observing the cosmic sources by the ESA-CAS satellite SMILE

Popis výsledku anglicky

This paper describes the scientific potential of a Soft X-ray Imager (SXI) onboard the ESA-CAS satellite SMILE for investigating cosmic X-ray sources of various types. We show that this instrument, albeit 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. Regarding sufficiently luminous X-ray sources with continuous spectra to be observable by the X-ray monitor MAXI/ISS to assess the object types and their light curves that are expected to be detected by SXI/SMILE, the compact sources accreting matter are promising targets for evaluating the possibilities of SXI.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2024

Kód důvěrnosti údajů

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

Název periodika

Journal of High Energy Astrophysics

ISSN

2214-4048

e-ISSN

2214-4056

Svazek periodika

41

Číslo periodika v rámci svazku

March

Stát vydavatele periodika

NL - Nizozemsko

Počet stran výsledku

9

Strana od-do

97-105

Kód UT WoS článku

001210961100001

EID výsledku v databázi Scopus

2-s2.0-85186678510