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Status update for MAPS, the MMT AO exoPlanet characterization System 8

Status update for MAPS, the MMT AO exoPlanet characterizatio...

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conference on Adaptive optics systems VIII part of spie Astronomical Telescopes and Instrumentation conference

作者： Montoya, Manny Morzinski, Katie M. Durney, Olivier Gardner, Andrew Mailhot, Emily Vargas, Dan Vaz, Amali West, Grant Patience, Jenny Jannuzia, Buell T. Anugu, Narsireddy Carlson, Jared Chapman, Kim Chen, Shaojie Fellows, Chuck Harrison, Lori Jones, Terry Kulesa, Craig Lamb, Masen Liu, Siqi McCarthy, Don Sivanandam, Suresh Taylor, Jacob Univ Arizona Steward Observ 933 N Cherry Ave Tucson AZ 85721 USA Arizona State Univ Sch Earth & Space Explorat Tempe AZ 85281 USA Georgia State Univ Mt Wilson Observ CHARA Array Mount Wilson CA USA Univ Toronto Dunlap Inst Astron & Astrophys 50 St George St Toronto ON Canada Minnesota Inst Astrophys 116 Church St SE Minneapolis MN 55455 USA

ISBN: (纸本)9781510653528;9781510653511

The MMT Adaptive optics exoPlanet characterization System (MAPS) is an exoplanet characterization program that encompasses instrument development, observational science, and education. The instrument we are developing for the 6.5m MMT observatory is multi-faceted, including a refurbished 336-actuator adaptive secondary mirror (ASM);two pyramid wavefront sensors (PyWFS's);a 1-kHz adaptive optics (AO) control loop;a high-resolution and long-wavelength upgrade to the Arizona infraRed Imager and Echelle Spectrograph (ARIES);and a new-AO-optimized upgrade to the MMT-sensitive polarimeter (MMT-Pol). With the completed MAPS instrument, we will execute a 60-night science program to characterize the atmospheric composition and dynamics of 50-100 planets around other stars. The project is approaching first light, anticipated for Summer/Fall of 2022. With the electrical and optical tests complete and passing the review milestone for the ASM's development, it is currently being tuned. The PyWFS's are being built and integrated in their respective labs: the visible-light PyWFS at the University of Arizona (UA), and the infrared PyWFS at the University of Toronto (UT). The top-level AO control software is being developed at UA, with an on-sky calibration algorithm being developed at UT. ARIES development continues at UA, and MMT-Pol development is at the University of Minnesota. The science and education programs are in planning and preparation. We will present the design and development of the entire MAPS instrument and project, including an overview of lab results and next steps.

关键词： Adaptive optics Adaptive secondary mirror Pyramid wavefront sensor High-resolution spectroscopy Exoplanets Infrared wavefront sensing

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Exploiting metamaterial characteristics for computational imaging

Exploiting metamaterial characteristics for computational im...

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Flat optics: Components to systems, FLAToptics 2021 - part of OSA optical design and Fabrication 2021

作者： Mait, Joseph N. Athale, Ravindra A. van der Gracht, Joseph Euliss, Gary W. MITRE Corporation 7525 Colshire Dr McLeanVA22102 United States

The potential exists for new optical technologies to impact computational sensor design. We consider in a formal manner the potential impact of metamaterials. © OSA 2021.

ISBN: (纸本)9781557528209

The potential exists for new optical technologies to impact computational sensor design. We consider in a formal manner the potential impact of metamaterials. © OSA 2021.

关键词： computational Imaging

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Modal Simulation Framework for the design and Verification of Future Few-Mode Far-Infrared Spectrometers 11

Modal Simulation Framework for the Design and Verification o...

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conference on : Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI

作者： Lap, Bram N. R. Jellema, Willem Withington, Stafford Naylor, David A. Univ Groningen Kapteyn Astron Inst NL-9700 AV Groningen Netherlands SRON Netherlands Inst Space Res NL-9700 AV Groningen Netherlands Cavendish Lab JJ Thomson Ave Cambridge CB3 0HE England Univ Lethbridge Inst Space Imaging Sci Dept Phys & Astron 4401 Univ Dr Lethbridge AB T1K 3M4 Canada

ISBN: (纸本)9781510653627;9781510653610

The next generation of astronomical space-based far-infrared (FIR) missions require ultra-sensitive spectroscopy as a diagnostic tool. These instruments use ultra-sensitive detector technologies to attain unprecedented levels of spectral observing sensitivity. The reception patterns of the individual detectors consist of individually coherent orthogonal field distributions, or equivalently, they are few-mode (5-20), to increase the spectral-spatial coupling to the astronomical source. However, the disadvantage of few-mode detectors is an increase in coupling to external (from the sky or warm telescope optics) and internal (from the instrument itself) straylight, which can greatly affect the measurement of the source spectrum. Therefore, understanding the spectral-spatial few-mode behaviour of these systems in detail, and developing verification and calibration strategies, are crucial to ensure that the science goals of these future mission are met. Since conventional modelling techniques are less suited to address this problem, we developed a modal framework to model, analyse, and address these issues.' In this paper, we use Herschel's Spectral and Photometric Imaging REceiver (SPIRE) as a case study, because its optical design is representative for future FIR missions and illustrative to highlight calibration issues observed in-flight, while including straylight. Our analysis consist out of two part. In the first part, we use our modal framework to simulate the few-mode SPIRE Fourier Transform Spectrometer (FTS). In the second part, we carry out a end-to-end frequency-dependent partially coherent analysis of Herschel-SPIRE. These simulations offer a qualitative explanation for the few-mode behaviour observed in-flight. Furthermore, we use the Herschel-SPIRE case-study to demonstrate how the modelling framework can be used to support the design, verification and calibration of spectrometers for future FIR missions. The modal framework is not only limited to the spec

关键词： astronomical far-infrared spectroscopy few-mode ultra-sensitive detectors modal optics framework development of verification and calibration schemes

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Research Status and Development Trend of optical System design for Infrared Imaging Seeker

Research Status and Development Trend of Optical System Desi...

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conference on AOPC - optical Sensing and Imaging Technology

作者： Zhang, Hao Yu, Chenfei Zhang, Guohua Wan, Zhong Sci & Technol Electroopt Control Lab Luoyang 471000 Peoples R China Luoyang Inst Electroopt Equipment Luoyang 471000 Peoples R China

ISBN: (纸本)9781510650060;9781510650053

Infrared imaging seeker is the main direction of optical imaging seeker technology. Infrared imaging system determines the detection performance and tracking accuracy of the infrared seeker, and it is also the key factor for the miniaturization and lightweight of the seeker. optical structure layout is the design key of infrared optical system. This paper introduces the traditional refractive, reflection, catadioptric optical system layout as well as the new off-axis reflection, hybrid refractive-diffractive, Kuder optical path, free-form surface optical form, and analyses its advantages and disadvantages from weight, volume, image quality, installation and debugging. Fairing is a key part of the optical system of infrared imaging seeker. It plays a high transmittance to the infrared band and protects the seeker from adverse external environment. This paper introduces the common materials of the fairing, the design of the fairing under hypersonic speed and the design method of the conformal optical system. The advance technologies of optical system design are introduced, including binary optics based on light wave diffraction theory, computational optics based on geometric optics, information optics and modern signal processing, micro-optics with great prospects for minimizing the seeker optical system, and adaptive optics which can overcome and compensate for the effects of atmospheric turbulence, and super lens technology using nanotechnology. This paper believes that the optical system of the future seeker should be based on the etching, material and surface design, and the technology of computational optics and signal processing will be widely used in optic design of seeker.

关键词： Infrared imaging seeker optical system Seeker fairing Micro-optics Binary optics Adaptive optics Super lens Free-form surface optical system

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Advanced high-power laser diode combination design for laser scanning applications 6

Advanced high-power laser diode combination design for laser...

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conference on Illumination optics VI held as part of part of spie optical systems design conference

作者： Smeesters, Lien Thienpont, Hugo Meulebroeck, Wendy Vrije Univ Brussel Pl Laan 2 B-1050 Brussels Belgium Flanders Make Dept Appl Phys & Photon Brussels Photon B PHOT Pl Laan 2 B-1050 Brussels Belgium

ISBN: (纸本)9781510645936;9781510645929

Laser cutters and engraving devices traditionally feature a high-power CO 2 laser in combination with a scanning unit. However, within the laser processing industry, a growing interest arose in the use and combination of laser diode sources, enabling a more compact design featuring a longer estimated lifespan. Therefore, we investigate and compare different laser diode combination configurations, while evaluating their applicability in a compact laser scanning configuration. Specifically, as a case study, we target the combination of 4 high-power laser diodes, pursuing a collimated, homogenous and symmetrical output beam, while minimizing light losses. An optimal laser diode combination design was achieved by use of aspherical lenses, knife-edge mirrors and a polarizing beam splitter. Two laser diodes are oriented to emit p-polarized light, while the other emit s-polarized light. In front of each laser diode, an aspherical lens is mounted to collect and collimate the laser beam. The two collimated s-polarized laser beams and the two p-polarized beams are each combined using a knife-edge mirror, after which the s- and p-polarized beam are combined by a polarizing beam splitter, giving rise to a single collimated output beam that can be used as input for the scanning unit. Following the optimization and tolerancing of the design, the laser diode combination system was successfully demonstrated in a proof-of-principle laboratory configuration indicating a homogeneous and collimated illumination beam at the entrance of the scan head, paving the way towards the integration and combination of multiple laser diode sources for use in high-power laser cutting and marking applications.

关键词： laser cutting laser diode array illumination design beam shaping beam collimation laser diode circularization knife-edge mirror polarizing beam combiner

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HARMONI at ELT: development of the High-Contrast module 8

HARMONI at ELT: development of the High-Contrast module

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conference on Adaptive optics systems VIII part of spie Astronomical Telescopes and Instrumentation conference

作者： Jocou, Laurent Rabou, Patrick Moulin, Thibaut Magnard, Yves Hours, Adrien Pancher, Fabrice Guieu, Sylvain Carlotti, Alexis Delboulbe, Alain Verove, Maxime Stadler, Eric Maurel, Didier Sylvain, Rochat Henault, Francois Dohlen, K. Thatte, N. Neichel, B. Vola, P. Clarke, F. Melotte, D. Tecza, M. Schnetler, H. Univ Grenoble Alpes CNRS IPAG 414 Rue Piscine St Martin Dheres France Aix Marseille Univ CNRS Marseille France Univ Oxford Dept Phys Oxford OX1 3RH England UKATC Royal Observ Edinburgh Blackford Hill Edinburgh EH9 3HJ Midlothian Scotland

ISBN: (纸本)9781510653528;9781510653511

HARMONI is the first light near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. It can operate in two Adaptive optics (AO) modes - Single Conjugated AO ( SCAO - including a High-Contrast capability) and Laser Tomography AO (LTAO) - or without AO (NOAO). The project is preparing for Final design Reviews. In addition of the SCAO mode, the instrument includes a high-contrast imaging capability working in H and K band. This sub-system will be essential to spectrally characterize young giant exoplanets with contrast down to 1e-6 and a separation from 0.1 to 0.3 arc second (goal: 0.05-0.3 '') from their host star. It will also be used to characterize young circumstellar disks. The High-Contrast Module (HCM) is based on an apodized pupil coronagraph which lowers the intensity of the diffracted starlight to a planet-star contrast compatible with the dynamic range of the scientific detector. A dedicated Zernike wavefront sensor will internally calibrate non-common path aberrations at a 0.1Hz rate. This paper therefore recalls the driver requirements before describing the optical, mechanical and control system designs. We then shortly describe the operation of the HCM. Section 3 addresses the main aspects of the system analysis while the last section is dedicated to the AIT aspects.

关键词： HARMONI High contrast ELT Adaptive optics

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Photonics Applications and Web Engineering - WILGA 2021

Photonics Applications and Web Engineering - WILGA 2021

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conference on Photonics Applications in Astronomy, Communications, Industry, and High Energy Physics Experiments

作者： Romaniuk, Ryszard S. Smolarz, Andrzej Wojcik, Waldemar Warsaw Univ Technol Inst Elect Syst Warsaw Poland Lublin Univ Technol Fac Elect Engn & Comp Sci Lublin Poland

ISBN: (数字)9781510649569

ISBN: (纸本)9781510649569;9781510649552

Wilga 2021 Summer Symposium on Photonics Applications and Web Engineering was the 48th edition of the research and technical meetings series [1,2]. Traditionally, the whole week lasting annual series of technical conferences and topical sessions was scheduled to be held on 26 May - 02 June 2020 in Wilga resort near Warsaw, owned by the Warsaw University of Technology. Nearly 150 participants took part in all of the Wilga 2021 events, most of them being young researchers active in all aspects of photonics, electronics and ICT science and technology. Wilga Symposium also embraces hardware and software technologies associated with photonics like optics, optical engineering, optoelectronics, electronics and electrical engineering, mechatronics, chemical and material engineering, applied physics, industrial solutions and applications. Around 100 papers were presented during Wilga 2021, oral and poster. Out of this number, some papers chosen by authors are published in this volume of Proc. spie mostly related to photonics. The major change was that during Wilga 2020 and 2021 Symposia, during summer editions, no traditional large young researcher sessions at large were possible to be organized

关键词： quantum optics material science and engineering optics optical engineering photonics optoelectronics teaching photonics and electronics photonic system design photonic-electronic integration photonic-electronic co-design advanced electronic and photonic systems sensors sensor fusion software engineering instrumentation for large research experiments photonics in quantum computing and artificial intelligence systems

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Laser modulation to reduce the dependence on natural guide star for focus sensing: simulations and preliminary results 8

Laser modulation to reduce the dependence on natural guide s...

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conference on Adaptive optics systems VIII part of spie Astronomical Telescopes and Instrumentation conference

作者： Krishna, Sowmya Hassan Rey, Noelia Martinez Rigaut, Francois Hart, John Roberts, Lyle d'Orgeville, Celine Australian Natl Univ Adv Instrumentat Technol Ctr Res Sch Astron & Astrophys Mt Stromlo Observ Cotter Rd Weston ACT 2611 Australia Australian Natl Univ Res Sch Phys Ctr Gravitat Astrophys Bldg 38ASci Rd Canberra ACT 2601 Australia

ISBN: (纸本)9781510653528;9781510653511

The adaptive optics (AO) system requires natural guide stars (NGS) to differentiate the focus error generated due to vertical shift in the sodium centroid altitude together with atmospheric turbulence. This dependency on NGS restricts achieving useable sky coverage and AO operation during dawn. One of the proposed approaches to distinguish these two focus errors is to monitor continuously the region of the sodium layer where the LGS is generated. The classical approaches used for this task, direct imaging, and LIDAR technology, have limitations. The technique of continuously amplitude modulating the guidestar laser (GSL) according to the pseudo-random binary sequence (PRBS) has the potential to overcome the limitations of classical approaches and reduce the dependency of the AO system on the NGS. The focus error is the major issue in large telescopes;therefore, we extended the PRBS technique to one of the large telescopes, the Gaint Magellan Telescope through numerical simulations. The study shows that modulation strength of 0.47 is required to fulfil the requirements during high sodium column density. Previously, it was intended to experimentally verify the technique with an LGS facility installed at the 1.8 m EOS telescope, Mount Stromlo, Canberra, Australia. Due to unavoidable circumstances, we now intend to perform the experiment with the LGS facility at the 2.3 m ANU telescope, Siding Spring Observatory (SSO), Coonabarabran, Australia. The paper presents the numerical simulations conducted with parameters of SSO, hardware selection for the experiment based on the system requirements, and preliminary test results from the laboratory.

关键词： Sodium Laser Guide Star Adaptive optics Sodium Centroid Altitude LGS WFS Focus Error Pseudo Random Binary Sequence Laser Amplitude Modulation Large Telescopes.

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Current status of PAPYRUS : the pyramid based adaptive optics system at LAM/OHP 2

Current status of PAPYRUS : the pyramid based adaptive optic...

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conference on optical Instrument Science, Technology, and Applications II held as part of spie optical System design conference

作者： Muslimov, E. Levraud, N. Chambouleyron, V Boudjema, I Lau, A. Caillat, A. Pedreros, F. Otten, G. El Hadi, K. Joaquina, K. Maxime, M. El Morsy, M. Martin, Beltramo O. Fetick, R. Ke, Z. Sauvage, J-F Neichel, B. Fusco, T. Schmitt, J. Suu, Le Van A. Charton, J. Schimpf, A. Martin, B. Dintrono, F. Esposito, S. Pina, E. Lab Astrophys Marseille Marseille France Univ Paris Saclay ONERA DOTA F-91123 Palaiseau France NOVA Opt IR Instrumentat Grp Dwingeloo Netherlands Observ Haute Provence St Michel Lobservatoire France ALPAO Montbonnot St Martin France INAF Osservatorio Astrofis Arcetri Florence Italy

ISBN: (数字)9781510645974

ISBN: (纸本)9781510645974;9781510645967

The Provence Adaptive optics Pyramid Run System (PAPYRUS) is a pyramid-based Adaptive optics (AO) system that will be installed at the Coude focus of the 1.52m telescope (T152) at the Observatoire de Haute Provence (OHP). The project is being developed by PhD students and Postdocs across France with support from staff members consolidating the existing expertise and hardware into an R&D testbed. This testbed allows us to run various pyramid wavefront sensing (WFS) control algorithms on-sky and experiment on new concepts for wavefront control with additional benefit from the high number of available nights at this telescope. It will also function as a teaching tool for students during the planned AO summer school at OHP. To our knowledge, this is one of the first pedagogic pyramid-based AO systems on-sky. The key components of PAPYRUS are a 17 Chi 17 actuators Alpao deformable mirror with a Alpao RTC, a very low noise camera OCAM2k, and a 4-faces glass pyramid. PAPYRUS is designed in order to be a simple and modular system to explore wavefront control with a pyramid WFS on sky. We present an overview of PAPYRUS, a description of the opto-mechanical design and the current status of the project.

关键词： Adaptive optics Pyramid sensor

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Meta-optical computational imaging systems for large aperture, aberration-free imaging

Meta-optical computational imaging systems for large apertur...

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Flat optics: Components to systems, FLAToptics 2021 - part of OSA optical design and Fabrication 2021

作者： Majumdar, Arka Department of Electrical and Computer Engineering University of Washington SeattleWA98195 United States Department of Physics University of Washington SeattleWA98195 United States

By exploiting computational backend, coupled with a designer meta-optics we demonstrate high-quality imaging using a single meta-optics. The aperture is currently 0.5-2mm, but can be extended to 10cm. © OSA 2021

ISBN: (纸本)9781557528209

关键词： computational Imaging

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