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Development of an operation plan for observing the Galactic center region with the lobster-eye monitor
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SYSNO ASEP 0581946 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Development of an operation plan for observing the Galactic center region with the lobster-eye monitor Tvůrce(i) Šimon, Vojtěch (ASU-R) ORCID, RID
Hudec, René (ASU-R) RID, ORCIDZdroj.dok. Contributions of the Astronomical Observatory Skalnaté Pleso. - : Slovenská akadémia vied - ISSN 1335-1842
Roč. 53, č. 4 (2023), s. 191-197Poč.str. 7 s. Forma vydání Online - E Jazyk dok. eng - angličtina Země vyd. SK - Slovensko Klíč. slova X-rays ; radiation mechanisms ; astronomical instrumentation Obor OECD Optics (including laser optics and quantum optics) Způsob publikování Open access Institucionální podpora ASU-R - RVO:67985815 UT WOS 001141834600013 EID SCOPUS 85184744404 DOI 10.31577/caosp.2023.53.4.191 Anotace Using a CubeSat-like satellite, we show the lobster-eye (LE) monitor’s perspectives and development of an observing plan. This instrument is important because it is able to provide wide-field X-ray imaging. We present the possibilities of monitoring the Galactic center region in the soft X-ray energy (a few keV) bands. The reason is that many X-ray binaries concentrate in
the bulge surrounding the center of our Galaxy. Several such binaries are expected to be present in the monitor’s field of view (typically a square of about 5 × 5 degrees or more) at the same time. We used the planned LE telescope’s 3–6 keV and 6–9 keV band flux. To compare the expected results, we used the data obtained by MAXI/ISS and accommodated these energy bands to assess the object types and their light curves expected to be detected by this LE. We show how such data of GX 5–1 can contribute to this branch.
Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2024 Elektronická adresa https://hdl.handle.net/11104/0350083
Počet záznamů: 1