Skip navigation
  • INAF logo
  • Home
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects
  • Explore by
    • Research outputs
    • Researchers
    • Organization units
    • Projects
  • Login:
    • My DSpace
    • Receive email
      updates
    • Edit Account details
  • Italian
  • English

  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/32858
Title: X-ray tests of the ATHENA mirror modules in BEaTriX: from design to reality
Authors: SALMASO, Bianca 
Basso, S. 
Ghigo, M. 
SPIGA, Daniele 
Vecchi, G. 
SIRONI, GIORGIA 
COTRONEO, Vincenzo 
Conconi, Paolo 
REDAELLI, Edoardo Maria Alberto 
BIANCO, ANDREA 
PARESCHI, Giovanni 
TAGLIAFERRI, Gianpiero 
Sisana Davide
Pelliciari Carlo
FIORINI, MAURO 
INCORVAIA, SALVATORE 
USLENGHI, MICHELA 
PAOLETTI, Lorenzo 
FERRARI, CLAUDIO 
Lolli R.
Zappettini, A.
Sanchez del Rio, M.
Parodi, G.
Burwitz, V.
Rukdee, S.
Hartner, G
Muller, T.
Schmidt, T.
Langmeier, A.
Ferreira, D.D.
Massahi, S.
Gellert, N.C.
Christensen, F.
Bavdaz, M.
Ferreira, I.
Collon, M.
Vacanti, G.
Barriere, N.
Issue Date: 2022
Volume: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Editors: den Herder, Jan-Willem A.; Nikzad, Shouleh; Nakazawa, Kazuhiro
Series: PROCEEDINGS OF SPIE 
Abstract: The BEaTriX (Beam Expander Testing X-ray) facility is now operative at the INAF-Osservatorio Astronomico Brera (Merate, Italy). This facility has been specifically designed and built for the X-ray acceptance tests (PSF and Effective Area) of the ATHENA Silicon Pore Optics (SPO) Mirror Modules (MM). The unique setup creates a parallel, monochromatic, large X-ray beam, that fully illuminates the aperture of the MMs, generating an image at the ATHENA focal length of 12 m. This is made possible by a microfocus X-ray source followed by a chain of optical components (a paraboloidal mirror, 2 channel cut monochromators, and an asymmetric silicon crystal) able to expand the X-ray beam to a 6 cm × 17 cm size with a residual divergence of 1.5 arcsec (vertical) × 2.5 arcsec (horizontal). This paper reports the commissioning of the 4.5 keV beam line, and the first light obtained with a Mirror Module.
Conference Name: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Conference Place: Montreal, Quebec, Canada
Conference Date: July 17-23, 2022
URI: http://hdl.handle.net/20.500.12386/32858
URL: https://doi.org/10.1117/12.2628227
ISSN: 0277-786X
ISBN: 9781510653436
DOI: 10.1117/12.2628227
Fulltext: open
Appears in Collections:3.01 Contributi in Atti di convegno

Files in This Item:
File Description SizeFormat
121810W.pdfPdf editoriale5.89 MBAdobe PDFView/Open
Show full item record

Page view(s)

38
checked on Sep 25, 2023

Download(s)

22
checked on Sep 25, 2023

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are published in Open Access, unless otherwise indicated.


Explore by
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects

Informazioni e guide per autori

https://openaccess-info.inaf.it: tutte le informazioni sull'accesso aperto in INAF

Come si inserisce un prodotto: le guide a OA@INAF

La Policy INAF sull'accesso aperto

Documenti e modelli scaricabili

Feedback
Built with DSpace-CRIS - Extension maintained and optimized by Logo 4SCIENCE