<?xml version="1.0" encoding="utf-8"?>
<export-example>
  <doc>
    <id>2049</id>
    <completedYear>2022</completedYear>
    <publishedYear/>
    <thesisYearAccepted/>
    <language>eng</language>
    <pageFirst>1</pageFirst>
    <pageLast>2</pageLast>
    <pageNumber>2</pageNumber>
    <edition/>
    <issue>123</issue>
    <volume>2022</volume>
    <type>conferenceobject</type>
    <publisherName>DGaO</publisherName>
    <publisherPlace/>
    <creatingCorporation>Technische Universität Prag</creatingCorporation>
    <contributingCorporation>TH Aschaffenburg</contributingCorporation>
    <belongsToBibliography>0</belongsToBibliography>
    <completedDate>2022-09-07</completedDate>
    <publishedDate>2022-09-06</publishedDate>
    <thesisDateAccepted>--</thesisDateAccepted>
    <title language="eng">Effective areas of astronomical X-ray optics for cubesats and rocket experiments</title>
    <abstract language="eng">The effective area is one of the main telescope parameters when justifying real space application. We discuss the estimation of the effective collecting area of an X-ray telescope by two different methods, an analytical method and a simulation algorithm, and then compare the results. The Lobster Eye type telescopes considered here are designed for rocket experiments and CubeSat flights.</abstract>
    <parentTitle language="eng">DGaO Proceedings</parentTitle>
    <identifier type="issn">1614-8436</identifier>
    <identifier type="url">https://www.dgao-proceedings.de/download/123/123_p12.pdf</identifier>
    <enrichment key="copyright">1</enrichment>
    <enrichment key="opus.source">publish</enrichment>
    <enrichment key="opus.doi.autoCreate">false</enrichment>
    <enrichment key="opus.urn.autoCreate">false</enrichment>
    <licence>Keine Lizenz - es gilt das deutsche Urheberrecht</licence>
    <author>Rene Hudec</author>
    <author>Florian Gille</author>
    <author>Elzear Guimbelot</author>
    <author>Vladimir Tichy</author>
    <author>Thorsten Döhring</author>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>X-ray</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>telescope</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>satellite</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>effective area</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>Lobster Eye</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Röntgenteleskop</value>
    </subject>
    <collection role="institutes" number="">Internationales Technisches Vertriebsmanagement (Bachelor)</collection>
    <collection role="forschungsschwerpunkte" number="">Material Testing &amp; Sensor Technology</collection>
    <file>https://opus4.kobv.de/opus4-h-ab/files/2049/123_p12.pdf</file>
  </doc>
  <doc>
    <id>2014</id>
    <completedYear>2022</completedYear>
    <publishedYear/>
    <thesisYearAccepted/>
    <language>eng</language>
    <pageFirst>1</pageFirst>
    <pageLast>1</pageLast>
    <pageNumber>1</pageNumber>
    <edition/>
    <issue/>
    <volume/>
    <type>other</type>
    <publisherName>DGaO</publisherName>
    <publisherPlace/>
    <creatingCorporation>TH Aschaffenburg</creatingCorporation>
    <contributingCorporation>CVUT Prague</contributingCorporation>
    <belongsToBibliography>0</belongsToBibliography>
    <completedDate>2022-06-21</completedDate>
    <publishedDate>--</publishedDate>
    <thesisDateAccepted>--</thesisDateAccepted>
    <title language="eng">Effective areas of astronomical X-ray optics for cubesats and rocket experiments</title>
    <abstract language="eng">We address the problem of estimation the sensitivity of  astronomical X-ray telescopes of Lobster Eye type , with emphasis on calculation of effective areas for telescopes designed for rocket and CubeSat flights. This parameter is one of the principal parameters when  justifying the real space application. Indeed, the larger the effective area is, the more efficient the optical system is, able to provide images of fainter and more distant celestial  targets. We discuss the estimation of  the effective collecting area of a X-ray telescope by two different methods and then compare the results: the analytical method and then the simulation algorithm.</abstract>
    <abstract language="deu">Poster</abstract>
    <enrichment key="copyright">1</enrichment>
    <enrichment key="opus.source">publish</enrichment>
    <licence>Keine Lizenz - es gilt das deutsche Urheberrecht</licence>
    <author>Rene Hudec</author>
    <author>Florian Gille</author>
    <author>Elzear Guimbelot</author>
    <author>Vladimir Tichy</author>
    <author>Thorsten Döhring</author>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>CubeSat</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>rocket</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>X-ray</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>telescope</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>effective area</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Röntgenteleskop</value>
    </subject>
    <collection role="institutes" number="">Internationales Technisches Vertriebsmanagement (Bachelor)</collection>
    <collection role="forschungsschwerpunkte" number="">Innovative Material Processing</collection>
    <file>https://opus4.kobv.de/opus4-h-ab/files/2014/PosterHudec-PforzheimV2.pdf</file>
  </doc>
</export-example>
