ATHENA optics technology development

The next generation x-ray observatory ATHENA (advanced telescope for high energy astrophysics) requires an optics with unprecedented performance. It is the combination of low mass, large effective area and good angular resolution that is the challenge of the x-ray optics of such a mission. ATHENA is...

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Main Authors Bavdaz, Marcos, Wille, Eric, Ayre, Mark, Ferreira, Ivo, Shortt, Brian, Fransen, Sebastiaan, Millinger, Mark, Collon, Maximilien J., Vacanti, Giuseppe, Barrière, Nicolas M., Landgraf, Boris, Olde Riekerink, Mark, Haneveld, Jeroen, Start, Ronald, van Baren, Coen, Della Monica Ferreira, Desiree, Massahi, Sonny, Svendsen, Sara, Christensen, Finn, Krumrey, Michael, Handick, Evelyn, Burwitz, Vadim, Pareschi, Giovanni, Salmaso, Bianca, Moretti, Alberto, Spiga, Daniele, Valsecchi, Giuseppe, Vernani, Dervis, Lupton, Paul, Mundon, William, Phillips, Gavin, Schneider, Jakob, Korhonen, Tapio, Sanchez, Alejandro, Heinis, Dominique, Colldelram, Carles, Tordi, Massimiliano, De Lorenzi, Simone, Willingale, Richard
Format Conference Proceeding
LanguageEnglish
Published SPIE 31.08.2022
Online AccessGet full text
ISBN9781510653436
1510653430
ISSN0277-786X
DOI10.1117/12.2629894

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Abstract The next generation x-ray observatory ATHENA (advanced telescope for high energy astrophysics) requires an optics with unprecedented performance. It is the combination of low mass, large effective area and good angular resolution that is the challenge of the x-ray optics of such a mission. ATHENA is the second large class mission in the science programme of ESA, and is currently in a reformulation process, following a design-to-cost approach to meet the cost limit of an ESA L-class mission. The silicon pore optics (SPO) is the mission enabler being specifically developed for ATHENA, in a joint effort by industry, research institutions and ESA. All aspects of the optics are being addressed, from the mirror plates and their coatings, over the mirror modules and their assembly into the ATHENA telescope, to the facilities required to build and test the flight optics, demonstrating performance, robustness, and programmatic compliance. The SPO technology is currently being matured to the level required for the adoption of the ATHENA mission, i.e., the start of the mission implementation phase. The monocrystalline silicon material and pore structure of the SPO provide these optics with excellent thermal and mechanical properties. Benefiting from technology spin-in from the semiconductor industry, the equipment, processes, and materials used to produce the SPO are highly sophisticated and optimised.
AbstractList The next generation x-ray observatory ATHENA (advanced telescope for high energy astrophysics) requires an optics with unprecedented performance. It is the combination of low mass, large effective area and good angular resolution that is the challenge of the x-ray optics of such a mission. ATHENA is the second large class mission in the science programme of ESA, and is currently in a reformulation process, following a design-to-cost approach to meet the cost limit of an ESA L-class mission. The silicon pore optics (SPO) is the mission enabler being specifically developed for ATHENA, in a joint effort by industry, research institutions and ESA. All aspects of the optics are being addressed, from the mirror plates and their coatings, over the mirror modules and their assembly into the ATHENA telescope, to the facilities required to build and test the flight optics, demonstrating performance, robustness, and programmatic compliance. The SPO technology is currently being matured to the level required for the adoption of the ATHENA mission, i.e., the start of the mission implementation phase. The monocrystalline silicon material and pore structure of the SPO provide these optics with excellent thermal and mechanical properties. Benefiting from technology spin-in from the semiconductor industry, the equipment, processes, and materials used to produce the SPO are highly sophisticated and optimised.
Author Collon, Maximilien J.
Vernani, Dervis
Vacanti, Giuseppe
Olde Riekerink, Mark
Phillips, Gavin
Handick, Evelyn
Ferreira, Ivo
Della Monica Ferreira, Desiree
Shortt, Brian
Willingale, Richard
Wille, Eric
Fransen, Sebastiaan
Valsecchi, Giuseppe
Mundon, William
Burwitz, Vadim
Krumrey, Michael
Sanchez, Alejandro
Millinger, Mark
Korhonen, Tapio
Lupton, Paul
Landgraf, Boris
De Lorenzi, Simone
Moretti, Alberto
van Baren, Coen
Spiga, Daniele
Bavdaz, Marcos
Salmaso, Bianca
Haneveld, Jeroen
Start, Ronald
Christensen, Finn
Massahi, Sonny
Svendsen, Sara
Schneider, Jakob
Tordi, Massimiliano
Heinis, Dominique
Colldelram, Carles
Ayre, Mark
Barrière, Nicolas M.
Pareschi, Giovanni
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  givenname: Gavin
  surname: Phillips
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  givenname: Jakob
  surname: Schneider
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  organization: Univ. of Leicester (United Kingdom)
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DOI 10.1117/12.2629894
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Nikzad, Shouleh
Nakazawa, Kazuhiro
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  fullname: Nakazawa, Kazuhiro
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Notes Conference Location: Montréal, Québec, Canada
Conference Date: 2022-07-17|2022-07-23
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