Development of an operation plan for observing the Galactic center region with the lobster-eye monitor

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00581946" target="_blank" >RIV/67985815:_____/23:00581946 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/68407700:21230/23:00372556

Výsledek na webu

<a href="https://hdl.handle.net/11104/0350083" target="_blank" >https://hdl.handle.net/11104/0350083</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.31577/caosp.2023.53.4.191" target="_blank" >10.31577/caosp.2023.53.4.191</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Development of an operation plan for observing the Galactic center region with the lobster-eye monitor

Popis výsledku v původním jazyce

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 innthe 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.nnnn

Název v anglickém jazyce

Development of an operation plan for observing the Galactic center region with the lobster-eye monitor

Popis výsledku anglicky

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 innthe 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.nnnn

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10306 - Optics (including laser optics and quantum optics)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2023

Kód důvěrnosti údajů

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

Název periodika

Contributions of the Astronomical Observatory Skalnaté Pleso

ISSN

1335-1842

e-ISSN

1336-0337

Svazek periodika

53

Číslo periodika v rámci svazku

4

Stát vydavatele periodika

SK - Slovenská republika

Počet stran výsledku

7

Strana od-do

191-197

Kód UT WoS článku

001141834600013

EID výsledku v databázi Scopus

2-s2.0-85184744404