<?xml version="1.0" encoding="utf-8"?>
<export-example>
  <doc>
    <id>1972</id>
    <completedYear>2021</completedYear>
    <publishedYear/>
    <thesisYearAccepted/>
    <language>deu</language>
    <pageFirst>1</pageFirst>
    <pageLast>2</pageLast>
    <pageNumber>2</pageNumber>
    <edition/>
    <issue>122</issue>
    <volume>2021</volume>
    <type>conferenceobject</type>
    <publisherName>DGaO</publisherName>
    <publisherPlace/>
    <creatingCorporation>TH Aschaffenburg</creatingCorporation>
    <contributingCorporation>Max-Planck Institut für Extraterrestrische Physik</contributingCorporation>
    <belongsToBibliography>0</belongsToBibliography>
    <completedDate>2021-12-04</completedDate>
    <publishedDate>2021-12-01</publishedDate>
    <thesisDateAccepted>--</thesisDateAccepted>
    <title language="deu">Charakterisierung von Weitwinkel-Röntgenteleskopen in der Testanlage PANTER</title>
    <abstract language="deu">Im Rahmen einer bayerisch-tschechischen Kooperation entstanden zwei Röntgenteleskope, bestückt mit Gold- und Iridium-beschichteten Planspiegeln. Deren Charakterisierung erfolgte an der Röntgentestanlage PANTER, welche parallel auf die Teleskope einfallendes Sternenlicht simuliert. Die Teleskope haben eine Winkelauflösung von ca. 4 Bogenminuten und eine Brennweite von rund 2 Metern.</abstract>
    <parentTitle language="deu">DGaO Proceedings</parentTitle>
    <identifier type="issn">1614-8436</identifier>
    <identifier type="url">https://www.dgao-proceedings.de/download/122/122_p2.pdf</identifier>
    <enrichment key="copyright">1</enrichment>
    <enrichment key="opus.source">publish</enrichment>
    <licence>Keine Lizenz - es gilt das deutsche Urheberrecht</licence>
    <author>Thorsten Döhring</author>
    <author>Veronika Stieglitz</author>
    <author>Vadim Burwitz</author>
    <author>Gisela Hartner</author>
    <author>Thomas Müller</author>
    <author>Thomas Schmidt</author>
    <author>Surangkhana Rukdee</author>
    <author>Peter Friedrich</author>
    <author>Fatih Sahin</author>
    <author>Rene Hudec</author>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Röntgenstrahlung</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Teleskop</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Iridium</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Beschichtung</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Astronomie</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Röntgenteleskop</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Iridium</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Spiegelteleskop</value>
    </subject>
    <collection role="forschungsschwerpunkte" number="">Innovative Material Processing</collection>
    <collection role="forschungsschwerpunkte" number="">Material Testing &amp; Sensor Technology</collection>
    <file>https://opus4.kobv.de/opus4-h-ab/files/1972/122_p2.pdf</file>
  </doc>
  <doc>
    <id>1937</id>
    <completedYear>2021</completedYear>
    <publishedYear/>
    <thesisYearAccepted/>
    <language>deu</language>
    <pageFirst>1</pageFirst>
    <pageLast>1</pageLast>
    <pageNumber>1</pageNumber>
    <edition/>
    <issue/>
    <volume>2021</volume>
    <type>other</type>
    <publisherName/>
    <publisherPlace/>
    <creatingCorporation>TH Aschaffenburg</creatingCorporation>
    <contributingCorporation>Max-Plack-Institut für extraterrestrische Physik</contributingCorporation>
    <belongsToBibliography>0</belongsToBibliography>
    <completedDate>2021-09-24</completedDate>
    <publishedDate>2021-09-21</publishedDate>
    <thesisDateAccepted>--</thesisDateAccepted>
    <title language="deu">Charakterisierung von Weitwinkel-Röntgenteleskopen in der Testanlage PANTER</title>
    <abstract language="deu">Im Rahmen einer bayerisch-tschechischen Kooperation entstanden zwei mechanisch baugleiche Röntgenteleskope, bestückt mit Gold- und Iridium-beschichteten Planspiegeln. Die Charakterisierung der nach dem ägyptischen Gott HORUS benannten Teleskope erfolgte an der Röntgentestanlage PANTER des Max-Plack-Instituts für extraterrestrische Physik. Diese Vakuum-Testanlage simuliert parallel auf die Teleskope einfallendes Sternenlicht, wobei hier die Strahlung aus einer Röntgenquelle in 120 Metern Abstand stammt. Die Messungen selbst fanden in einer daran angebauten 12 Meter langen Testkammer von 3,5 Metern Durchmesser statt. Im März 2021 sahen die HORUS-Teleskope zum erstem Mal Röntgenlicht. Während der Testkampagne von ca. 54 Stunden Dauer wurden 536 Einzelmessungen an den beiden Teleskopen durchgeführt, bei denen Photonenenergien und Einfallswinkel variiert wurden. Von einer empfindlichen CCD-Kamera, einem Prototyp der eROSITA-Satellitenkamera, wurden hierbei insgesamt 11.153.574 Röntgenphotonen individuell detektiert, analysiert und digital verarbeitet. Die beiden Weitwinkel-Röntgenteleskope haben eine Winkelauflösung von circa 4 Bogenminuten und eine Brennweite von rund zwei Metern.</abstract>
    <abstract language="mul">Poster</abstract>
    <parentTitle language="deu">DGaO Jahrestagung</parentTitle>
    <identifier type="url">https://dgao.de/jahrestagung/</identifier>
    <enrichment key="copyright">1</enrichment>
    <enrichment key="opus.source">publish</enrichment>
    <licence>Keine Lizenz - es gilt das deutsche Urheberrecht</licence>
    <author>Thorsten Döhring</author>
    <author>Veronika Stieglitz</author>
    <author>Vadim Burwitz</author>
    <author>Gisela Hartner</author>
    <author>Thomas Müller</author>
    <author>Thomas Schmidt</author>
    <author>Surangkhana Rukdee</author>
    <author>Peter Friedrich</author>
    <author>Fatih Sahin</author>
    <author>Rene HUdec</author>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Röntgenstrahlung</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Spiegel</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Teleskop</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Satellit</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>uncontrolled</type>
      <value>Iridium</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Röntgenstrahlung</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Spiegelteleskop</value>
    </subject>
    <collection role="forschungsschwerpunkte" number="">Innovative Material Processing</collection>
    <collection role="forschungsschwerpunkte" number="">Material Testing &amp; Sensor Technology</collection>
    <file>https://opus4.kobv.de/opus4-h-ab/files/1937/DGaO_Poster_P2_Roentgenteleskop.pdf</file>
  </doc>
  <doc>
    <id>1866</id>
    <completedYear>2021</completedYear>
    <publishedYear/>
    <thesisYearAccepted/>
    <language>eng</language>
    <pageFirst>1177605-1</pageFirst>
    <pageLast>1177605-8</pageLast>
    <pageNumber>8</pageNumber>
    <edition/>
    <issue>11776</issue>
    <volume>2021</volume>
    <type>conferenceobject</type>
    <publisherName>SPIE</publisherName>
    <publisherPlace/>
    <creatingCorporation>Czech Technical University in Prague</creatingCorporation>
    <contributingCorporation>TH Aschaffenburg</contributingCorporation>
    <belongsToBibliography>0</belongsToBibliography>
    <completedDate>2021-05-24</completedDate>
    <publishedDate>2021-04-18</publishedDate>
    <thesisDateAccepted>--</thesisDateAccepted>
    <title language="eng">Lobster eye type X-ray telescope with chromium-iridium coated tri-layer mirrors</title>
    <abstract language="eng">For space-born astronomical X-ray telescopes, iridium-based reflective layer systems are known as highly effective&#13;
mirrors coatings. During the recent years, Aschaffenburg University of Applied Sciences and the Czech Technical&#13;
University in Prague jointly developed stress compensated chromium-iridium coatings for this application. To overcome the disturbing reflectivity reduction of the iridium absorption edge around 2 keV photon energy, thin overcoat layers of chromium were applied in addition. Now a prototype of a wide-field, imaging X-ray telescope&#13;
of Lobster Eye type is assembled at the company RIGAKU. For this purpose a small series of 34 mirrors based on 100 x 50 mm semiconductor grade silicon substrates has been coated at Aschaffenburg University. The applied tri-layer system consists of a stack of 40 nm chromium, which act as adhesive layer and compensates layer stress, a 30 nm iridium thick reflective layer, and an additional overcoat layer of 6 nm chromium. This layer system&#13;
have been analysed by AFM and TEM images. The mirrors are assembled into an aluminium frame to build a 2D Lobster Eye type telescope. The designed focal length of this wide field X-ray telescope is two meter. To study the performance of the tri-layer coating system, a twin LE telescope with convenient gold coatings was manufactured also. Performance measurements of both telescopes and under same conditions are planned at the PANTER test facility at the Max-Planck Institute for Extraterrestrial Physics. First experimental results,&#13;
their comparison with theoretical simulations and the comparison between both models will be presented in this contribution.</abstract>
    <parentTitle language="eng">Proceedings of SPIE</parentTitle>
    <identifier type="doi">https://doi.org/10.1117/12.2589266</identifier>
    <enrichment key="copyright">1</enrichment>
    <enrichment key="opus.source">publish</enrichment>
    <licence>Keine Lizenz - es gilt das deutsche Urheberrecht</licence>
    <author>Veronika Stehlikova</author>
    <author>Thorsten Döhring</author>
    <author>Manfred Stollenwerk</author>
    <author>Johannes Stadtmüller</author>
    <author>Veronika Marsikova</author>
    <author>Rene Hudec</author>
    <author>Dennis Flachs</author>
    <author>Vadim Burwitz</author>
    <author>Gisela Hartner</author>
    <author>Surangkhana Rukdee</author>
    <author>Thomas Müller</author>
    <author>Thomas Schmidt</author>
    <author>Adolf Inneman</author>
    <author>Mariana Klementova</author>
    <author>Sebastian Zeising</author>
    <author>Andreas Langmeier</author>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>telescope</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>Lobster Eye</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>X-ray</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>mirror</value>
    </subject>
    <subject>
      <language>eng</language>
      <type>uncontrolled</type>
      <value>iridium</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Röntgenteleskop</value>
    </subject>
    <subject>
      <language>deu</language>
      <type>swd</type>
      <value>Röntgenspiegel</value>
    </subject>
    <collection role="forschungsschwerpunkte" number="">Innovative Material Processing</collection>
    <collection role="forschungsschwerpunkte" number="">Material Testing &amp; Sensor Technology</collection>
  </doc>
</export-example>
