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  X-ray testing ATHENA optics at PANTER

Burwitz, V., Vacanti, G., Collon, M. J., Barrière, N., Bavdaz, M., Ferreira, I., et al. (2022). X-ray testing ATHENA optics at PANTER. In Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. doi:10.1117/12.2630414.

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 Urheber:
Burwitz, Vadim1, Autor           
Vacanti, Giuseppe, Autor
Collon, Maximilien J., Autor
Barrière, Nicolas, Autor
Bavdaz, Marcos, Autor
Ferreira, Ivo, Autor
Ayre, Mark, Autor
Tipper, Emily, Autor
Eder, Josef1, Autor           
Breunig, Elias, Autor
Hartner, Gisela1, Autor           
Langmeier, Andreas2, Autor           
Müller, Thomas3, Autor           
Rukdee, Surangkhana4, Autor           
Schmidt, Thomas1, Autor           
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              
2MPI for Extraterrestrial Physics, Max Planck Society, ou_159888              
3Center for Astrochemical Studies at MPE, MPI for Extraterrestrial Physics, Max Planck Society, ou_1950287              
4Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              

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 Zusammenfassung: Silicon pore optic (SPO) mirror modules (MMs) are being developed and produced for ESA’s ATHENA mission. The optics have, and will be, tested at MPEs PANTER x-ray test facility. We present the results obtained from tests performed at the PANTER x-ray test facility for the SPO MM-0050 that was produced to verify the latest optical performance (half energy width (HEW), effective area) of SPOs, supporting the ESA reviews of their optical performance.
The preparations are ongoing at PANTER, ESA, cosine and Media Lario to perform complex opto-thermo-mechanical tests of the two full scale 1/6th sectors of the final ATHENA mirror assembly structure produced by the potential ATHENA primes Airbus Defence and Space and Thales Alenia Space. For these tests a set of three SPO MMs have been produced following the flight configuration. The MMs will be incorporated into the full scale 1/6th sectors to measure the impact of thermal gradients on the thermoelastic deformation of the structure and therefore the HEW performance. A description of the tests is presented here.
PANTER is also involved in the development, testing, and fabrication of the mirror adapter structure (MAS) to support the 2.6-m diameter ATHENA mirror assembly module demonstrators (MAMD) during the planned x-ray tests at XRCF. A description of the PANTER tests and results will be presented in this paper together with a short overview of the MAS MGSE for XRCF.

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Sprache(n): eng - English
 Datum: 2022-08-31
 Publikationsstatus: Online veröffentlicht
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: DOI: 10.1117/12.2630414
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Veranstaltung

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Titel: SPIE Astronomical Telescopes + Instrumentation,
Veranstaltungsort: Montréal, Québec, Canada
Start-/Enddatum: 2022-07-17 - 2022-07-23

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Quelle 1

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Titel: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Genre der Quelle: Konferenzband
 Urheber:
Nakazawa, Kazuhiro, Autor
Nikzad, Shouleh , Autor
A. den Herder, Jan-Willem , Autor
Affiliations:
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Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 12181 Artikelnummer: - Start- / Endseite: - Identifikator: -

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Titel: Proceedings of SPIE
Genre der Quelle: Reihe
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Affiliations:
Ort, Verlag, Ausgabe: Bellingham, WA, USA : Society of Photo-Optical Instrumentation Engineers
Seiten: - Band / Heft: - Artikelnummer: 121810Y Start- / Endseite: - Identifikator: ISSN: 0277-786X