Alex Bayerle

ORCID: 0000-0002-1084-9724
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About
Contact & Profiles
Research Areas
  • Advanced X-ray Imaging Techniques
  • Advanced Surface Polishing Techniques
  • Particle Detector Development and Performance
  • Astrophysical Phenomena and Observations
  • Thin-Film Transistor Technologies
  • 3D IC and TSV technologies
  • High-pressure geophysics and materials
  • Advanced Fiber Laser Technologies
  • Particle Accelerators and Free-Electron Lasers
  • Advanced optical system design
  • Semiconductor Lasers and Optical Devices
  • Atomic and Subatomic Physics Research
  • Superconducting Materials and Applications
  • Medical Imaging Techniques and Applications
  • Solid State Laser Technologies
  • Adaptive optics and wavefront sensing
  • X-ray Spectroscopy and Fluorescence Analysis
  • Advanced Semiconductor Detectors and Materials
  • Silicon and Solar Cell Technologies
  • Nuclear Physics and Applications
  • Optical Coatings and Gratings
  • Medical Imaging and Pathology Studies

Cosine (Netherlands)
2019-2024

University of Amsterdam
2016

Athena, the largest space-based x-ray telescope to be flown by European Space Agency, uses a revolutionary new modular technology assemble its 2.6 m diameter lens. The lens will consist of several hundreds smaller lenslets, called mirror modules, which each about 70 pairs. Those modules are arranged in circles large optics structure and focus photons with an energy 0.5 10 keV at distance 12 onto detectors Athena. point-spread function (PSF) optic shall achieve half-energy width (HEW) 5" 1...

10.1117/12.2599339 article EN International Conference on Space Optics — ICSO 2020 2021-06-11

Athena is the European Space Agency's next flagship telescope, scheduled for launch in 2030s.Its 2.5 m diameter mirror will be segmented and comprise more than 600 individual Silicon Pore Optics (SPO) modules.Arranged concentric annuli following a Wolter-Schwartzschild design, modules are made of several tens grazing incidence primary-secondary pairs, each silicon, coated to increase effective area system, shaped bring incoming photons common focus 12 away.The mission aims deliver...

10.1117/12.2689003 article EN International Conference on Space Optics — ICSO 2020 2023-07-12

Silicon Pore Optics is the X-ray mirror technology selected for European Space Agency's Athena observatory. We describe testing and characterization cycle that optics are subjected to at PTB's Pencil/Paraller Beam Facility (XPBF) 1 2 beamlines synchrotron radiation facility BESSY II. Individual stacks measured with a pencil beam determine their optical quality orientation of axis. Using metrics based on manufacturing metrology, then paired in primary-secondary Wolter-I-like systems, turn...

10.1117/12.2530977 article EN 2019-09-09

ATHENA, the largest space-based X-ray telescope to be flown by European Space Agency, uses a new modular technology assemble its 2.5 m diameter lens.The lens will consist of several hundreds smaller lenslets, called mirror modules, which each up 76 stacked pairs.Those modules are arranged in circles large optics structure and focus photons with an energy 0.5 10 keV at distance 12 onto detectors ATHENA.The point-spread function (PSF) shall achieve half-energy width (HEW) 5", effective area...

10.1117/12.2593505 article EN 2021-07-30

The mirror modules composing Athena's X-ray optics are made with the Silicon Pore Optics (SPO) technology. SPO is produced as stacks of 38 plates, which paired to form Units (XOUs) following a modified Wolter I geometry. In current design, module composed two confocal XOUs glued in between pair brackets that freeze configuration and provide interfaces structure. Mirror assembled at XPBF2 beamline PTB synchrotron radiation facility BESSY II, using dedicated jigs. this paper we present latest...

10.1117/12.2594171 article EN 2021-07-30

Silicon Pore Optics (SPO) have been invented and developed to enable x-ray optics for space applications that require a combination of high angular resolution while being light-weight allow achieving large mirror surface area. In 2005, the SPO technology development was initiated by European Space Agency (ESA) flagship telescope mission is currently planned as baseline NewATHENA scheduled launch in 2030s. Its more than 2m diameter will be segmented comprises 492 individual grazing-angle...

10.1117/12.2678106 article EN 2023-10-05

The Silicon Pore Optics (SPO) technology has been established as a new type of X-ray optics and will enable future observatories such Athena Arcus. SPO is being developed at cosine Research B.V. together with the European Space Agency (ESA) academic well industrial partners. For Athena, about 150,000 mirror plates are required. With spin-in from semiconductor industry, mass production processes can be employed to manufacture rectangular in high quality, large quantity low cost. Over last...

10.1117/12.2594234 article EN 2021-07-30

The European Space Agency (ESA), cosine and its partners have been developing for 20 years the Silicon Pore Optics (SPO) technology. SPO enables next generation of space x-ray telescopes, with increased sensitivity resolution. NewAthena, New Advanced Telescope High Energy Astrophysics, has just endorsed by ESA as one Lclass mission, to launch around 2037. NewAthena's optic is modular consists up 600 mirror modules that form together a ~2.5 m diameter X-ray focal length 12 an angular...

10.1117/12.3019675 article EN Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray 2024-08-21

The European Space Agency (ESA) is developing the Athena (Advanced Telescope for High ENergy Astrophysics) X-ray telescope, an L-class mission in their current Cosmic Vision cycle long-term planning of space science missions. Silicon Pore Optics (SPO) are a new type optics enabling future observatories such as and being developed at cosine with ESA well academic industrial partners. These high-performance, modular, lightweight yet stiff, high-resolution shall allow missions to reach...

10.1117/12.2530866 article EN 2019-09-09

We present a frequency-shifted feedback (FSF) laser based on tapered amplifier. The operates as coherent broadband source with up to 370GHz spectral width and 2.3us coherence time. If the FSF is seeded by continuous-wave frequency comb spanning output spectrum appears in addition emission. has an power of 280mW center wavelength 780nm. ease flexibility use amplifiers makes our attractive for wide range applications, especially metrology.

10.21468/scipostphys.1.1.002 article EN cc-by SciPost Physics 2016-10-22

Silicon pore optics (SPO) is a novel approach, which has been developed for the European Space Agency X-ray observatory Athena, to achieve high-performance mirrors at low cost and relatively short lead time. The light-weight are manufactured from silicon wafers using mass production semiconductor technology as well custom fully automated robotic assembly systems. A 300 mm IBF machine used further improve by correcting thickness inhomogeneities, specific global gradients reduce initial...

10.1117/12.2687643 article EN 2023-11-22

Silicon direct bonding is a manufacturing process used in the fabrication of electronic, optical and mechanical microsystems. Chemical bonds are providing an intimate surface contact strong structural stiffness that is, for this reason, also suitable large assemblies. Based on knowledge properties X-ray optics, we making mirror imaging systems. The resorts to highest-grade 12 inch silicon wafers with double-sided super polished nearly perfect plan parallel surfaces. With readily available...

10.1149/09804.0135ecst article EN ECS Transactions 2020-09-08

Athena is the European Space Agency's next flagship x-ray telescope, scheduled for launch in 2030s. Its 2.5-m diameter mirror will be segmented and comprise more than 600 individual Silicon Pore Optics (SPO) grazing-incidence-angle imagers, called modules. Arranged concentric annuli following a Wolter-Schwartzschild design, modules are made of several tens primary-secondary pairs, each mono-crystalline silicon, coated to increase collective area system, shaped bring incoming photons common...

10.1117/12.2630775 article EN Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray 2022-08-31
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