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

Result code in 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>
Alternative codes found
RIV/68407700:21230/24:00373349
Result on the web
<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>

Result language
angličtina
Original language name
Soft X-ray observing the cosmic sources by the ESA-CAS satellite SMILE
Original language description
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.
Czech name
—
Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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