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Testing of lobster-eye type telescopes with X-rays and visible light

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F23%3A00374357" target="_blank" >RIV/68407700:21230/23:00374357 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1117/12.2665429" target="_blank" >http://dx.doi.org/10.1117/12.2665429</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1117/12.2665429" target="_blank" >10.1117/12.2665429</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Testing of lobster-eye type telescopes with X-rays and visible light

  • Original language description

    Reflective coatings for astronomical X-ray optics were developed at the “Aschaffenburg Competence Center for Astronomical and Space Instrumentation” (ACCASI) since several years. As part of a Bavarian-Czech cooperation between the Technical University of Aschaffenburg and the Czech Technical University of Prague, now two mechanically identical telescopes were built. One telescope optic was equipped with conventional gold-coated mirrors, manufactured by the Czech project partners. The 34 X-ray mirrors of the second telescope use an innovative coating system made of chromium and iridium, which was applied at the Aschaffenburg coating laboratory. Both telescopes are designed according to the bionic principle of a reflecting lobster eye. The optics works with two consecutive reflections on mutually perpendicular mirror surfaces. This enables a large field of view with many square degrees in diameter, which, however, comes at the price of a reduced angular resolution. An extensive X-ray characterization of these telescopes was carried out at the PANTER test facility of MPE, which simulates parallel starlight incident on the telescopes. The telescopes have an angular resolution of about 4 arc minutes in X-rays and a focal length of about 2 meters. Furthermore, the used X-ray mirrors reflect and focus visible light as well and this functionality in the optical regime was checked in laboratory tests. Now another test campaign was done to examine the telescope resolution for real objects of the visible sky and the imaging properties for star constellations. Such functional tests by observing astronomical objects of the visible sky may simplify and accelerate the development of X-ray telescopes for satellite applications.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    R - Projekt Ramcoveho programu EK

Others

  • Publication year

    2023

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    EUV and X-ray Optics: Synergy between Laboratory and Space VIII 2023

  • ISBN

    9781510662728

  • ISSN

    0277-786X

  • e-ISSN

  • Number of pages

    22

  • Pages from-to

  • Publisher name

    SPIE

  • Place of publication

    Bellingham

  • Event location

    Prague

  • Event date

    Apr 26, 2024

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article