Journal of Astronomical Telescopes Instruments and Systems最新文献_第3页

Lessons learned from an NIAC Phase I study for the flat-fabrication of a Dark Ages observatory 从 NIAC 关于黑暗时代天文台平面制造的第一阶段研究中汲取的经验教训

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.024002

Manuel Indaco, Kanak Parmar, Ryan Long, James Whitehead, Russell W. Mailen, Davide Guzzetti

{"title":"Lessons learned from an NIAC Phase I study for the flat-fabrication of a Dark Ages observatory","authors":"Manuel Indaco, Kanak Parmar, Ryan Long, James Whitehead, Russell W. Mailen, Davide Guzzetti","doi":"10.1117/1.jatis.10.2.024002","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.024002","url":null,"abstract":"Flat-fabrication technology may enable the next generation of gigantic deployable architectures devoted to the detection of faint cosmological signals. We assess the applicability of a multifunctional roll-out structure based on shape memory polymer technology for the realization of a large space observatory to measure the cosmological Dark Ages radio signal. Roll-out solutions offer advantageous properties for probe class missions, such as the capability to morph the shape to achieve sufficient structural performance while ensuring high packaging efficiency. We characterize the feasibility of a roll-out observatory in the context of a 5 years-long heliocentric mission scenario. Our preliminary study demonstrates how a four-250 m-long arms architecture with 150 evenly spaced short dipole antennas potentially meets the basic mission requirements dictated by the Dark Ages science case. We conduct a quasi-static structural analysis considering axial and bending loads acting on the arms to assess the structural properties of the proposed architecture, identifying geometric ranges which enable the structure to withstand expected loads while satisfying mass and size constraints. Printable electronics are considered in the design due to the ease of integration with the polymer substrate. In this regard, we explore two distinct electronics configuration options—centralized and decentralized—discussing their benefits in terms of power demand and data management. If successful, such a design may set the stage for future technological development aiming to realize tomographic measurements of the cosmological Dark Ages.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140590038","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Mookodi: multi-purpose low-resolution spectrograph and multi-filter photometric imager for rapid follow-up observations of astronomical transient events Mookodi：用于快速跟踪观测天文瞬变事件的多用途低分辨率摄谱仪和多滤光片测光成像仪

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.025005

Nicolas Erasmus, Iain A. Steele, Andrzej S. Piascik, Stuart D. Bates, Chris. J. Mottram, Kathryn A. Rosie, Carel H. D. R. van Gend, Ulrich Geen, Magaretha L. Pretorius, Stephen B. Potter, Egan Loubser, Willie Koorts, Hitesh Gajjar, Keegan Titus, Hannah L. Worters, Amanda A. Sickafoose, Sunil Chandra, James E. O’Connor, Kgothatso Matlala, Justine Crook-Mansour, Ali Ranjbar, Robert J. Smith, Helen Jermak, Shalom Abiodun, Okwudili D. Egbo

{"title":"Mookodi: multi-purpose low-resolution spectrograph and multi-filter photometric imager for rapid follow-up observations of astronomical transient events","authors":"Nicolas Erasmus, Iain A. Steele, Andrzej S. Piascik, Stuart D. Bates, Chris. J. Mottram, Kathryn A. Rosie, Carel H. D. R. van Gend, Ulrich Geen, Magaretha L. Pretorius, Stephen B. Potter, Egan Loubser, Willie Koorts, Hitesh Gajjar, Keegan Titus, Hannah L. Worters, Amanda A. Sickafoose, Sunil Chandra, James E. O’Connor, Kgothatso Matlala, Justine Crook-Mansour, Ali Ranjbar, Robert J. Smith, Helen Jermak, Shalom Abiodun, Okwudili D. Egbo","doi":"10.1117/1.jatis.10.2.025005","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.025005","url":null,"abstract":"We present Mookodi (meaning “rainbow” in Sesotho), a multipurpose instrument with a low-resolution spectrograph mode and a multi-filter imaging mode for quick-reaction astronomical observations. The instrument, mounted on the 1-m Lesedi telescope at the South African Astronomical Observatory in Sutherland (South Africa), is based on the low-resolution spectrograph for the rapid acquisition of transients (SPRAT) instrument in operation on the 2-m Liverpool Telescope in La Palma (Canary Islands, Spain). Similar to SPRAT, Mookodi has a resolution R≈350 and an operating wavelength range in the visible (∼4000 to 8000 Å). The linear optical design, as in SPRAT, is made possible through the combination of a volume phase holographic transmission grating as the dispersive element and a prism pair (grism), which makes it possible to rapidly and seamlessly switch to an imaging mode by pneumatically removing the slit and grism from the beam and using the same detector as in spectrographic mode to image the sky. This imaging mode is used for auto-target acquisition, but the inclusion of filter slides in Mookodi’s design also provides the capability to perform imaging with a field-of-view ≈10′×10′ (∼0.6″/px) in the complete Sloan Digital Sky Survey filter set.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140805561","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Imaging quality evaluation method for large field-of-view telescope optical systems 大视场望远镜光学系统成像质量评估方法

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.025003

Chao Chen, Zhengyang Li, Zhixu Wu, Yiming Zhang, Xiangyan Yuan

{"title":"Imaging quality evaluation method for large field-of-view telescope optical systems","authors":"Chao Chen, Zhengyang Li, Zhixu Wu, Yiming Zhang, Xiangyan Yuan","doi":"10.1117/1.jatis.10.2.025003","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.025003","url":null,"abstract":"Large-field telescopes play a significant role in cutting-edge astronomical research fields, such as time-domain astronomy and cosmology. For such telescopes, ensuring symmetrical and uniform imaging across the entire field-of-view (FoV) is pivotal, particularly for areas such as astronomical photometry and astrometry. However, conventional image quality evaluation methods for telescope optical systems have mainly focused on imaging spot size. Other alternative methods, such as ellipticity based methods, also face the challenges of high computational requirements and limited assessment parameters. In addition, establishing a coherent link between the telescope structure and research domains such as photometry has remained a challenge. In response to these challenges, we introduce an assessment approach termed the ray tracing, spot-vector index, and angle (RSVA) approach. This approach offers a fresh perspective on optical systems, prioritizing the depiction of imaging spot shapes. It acts as a valuable supplement to traditional methods and has been effectively employed to analyze four 1-m aperture telescopes with an f-ratio of 3 for a 3 deg FoV. Building on this foundation, the RSVA can be further expanded to explore other research avenues, including exploring the interplay between photometry and telescope systems and guiding large FoV optical design.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140613967","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Far- and Lyman-ultraviolet imaging demonstrator: a rocket-borne pathfinder instrument for high efficiency ultraviolet band selection imaging 远紫外和莱曼紫外成像演示器：火箭搭载的高效紫外波段选择成像探路仪器

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.024001

Nicholas Nell, Nicholas Kruczek, Kevin France, Stefan Ulrich, Patrick Behr, Emily Farr

{"title":"Far- and Lyman-ultraviolet imaging demonstrator: a rocket-borne pathfinder instrument for high efficiency ultraviolet band selection imaging","authors":"Nicholas Nell, Nicholas Kruczek, Kevin France, Stefan Ulrich, Patrick Behr, Emily Farr","doi":"10.1117/1.jatis.10.2.024001","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.024001","url":null,"abstract":"The Far- and Lyman-ultraviolet imaging demonstrator (FLUID) is a rocket-borne arcsecond-level ultraviolet (UV) imaging instrument covering four bands between 92 and 193 nm. FLUID will observe nearby galaxies to find and characterize the most massive stars that are the primary drivers of the chemical and dynamical evolution of galaxies and the co-evolution of the surrounding galactic environment. The FLUID short wave channel is designed to suppress efficiency at Lyman-α (121.6 nm) while enhancing the reflectivity of shorter wavelengths. Utilizing this technology, FLUID will take the first ever images of local galaxies isolated in the Lyman UV (90–120 nm). As a pathfinder instrument, FLUID will employ and increase the technology readiness level of band-selecting UV coatings and solar-blind UV detector technologies, including microchannel plate and solid-state detectors; technologies that are prioritized in the 2022 NASA Astrophysical Biennial Technology Report. These technologies enable high throughput and high sensitivity observations in the four co-aligned UV imaging bands that make up the FLUID instrument. We present the design of FLUID, status on the technology development, and results from initial assembly and calibration of the FLUID instrument.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140590015","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Space interferometer imaging limitations due to Global Positioning System uncertainties and parasitic forces in Low Earth Orbit 低地轨道上全球定位系统的不确定性和寄生力造成的空间干涉仪成像限制

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.025004

Leonid Pogorelyuk, Mason Black, Nicholas Belsten, Eleonora Polini, Jonah T. Hansen, Michael Ireland, John D. Monnier, Kerri Cahoy

{"title":"Space interferometer imaging limitations due to Global Positioning System uncertainties and parasitic forces in Low Earth Orbit","authors":"Leonid Pogorelyuk, Mason Black, Nicholas Belsten, Eleonora Polini, Jonah T. Hansen, Michael Ireland, John D. Monnier, Kerri Cahoy","doi":"10.1117/1.jatis.10.2.025004","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.025004","url":null,"abstract":"Space interferometers could, in principle, exploit the relatively stable space environment and ease of baseline reconfiguration to collect measurements beyond the limitations of ground-based interferometers. In particular, a two-element interferometer could provide excellent uv-plane coverage over a few tens of low Earth orbits. One of the challenges for free-flying interferometers is controlling the optical path distance with subwavelength accuracies despite the collectors flying up to hundreds of meters apart. We consider two approaches: an artificial in-orbit laser guide star (LGS) that provides a phase reference for the space interferometer and fringe tracking on the science target itself. The two approaches (LGS versus no LGS) would require different image processing techniques. In this work, we explore image processing with LGS phase residuals due to global positioning system (GPS) uncertainties. We use GPS uncertainties from the Gravity Recovery and Climate Experiment Follow-On mission to simulate image retrieval with a 300-m baseline laser-guided space interferometer. This is done by fitting the slowly varying phase errors of complex visibility measurements. We also consider a 40-m baseline interferometer with visibility(-modulus)-only measurements. In this case, we simulate the bias in visibility due to fringe tracking in the presence of parasitic forces acting on the spacecraft. We then use a modified version of the hybrid input–output phase retrieval algorithm for image reconstruction. We conclude that under our optimistic assumptions, both approaches could enable general imaging of a few large stars even with CubeSats, although an LGS would significantly improve the best resolution obtainable.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140635169","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Laboratory demonstration of a Photonic Lantern Nuller in monochromatic and broadband light 单色光和宽带光下的光子灯笼无效器实验室演示

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.025001

Yinzi Xin, Daniel Echeverri, Nemanja Jovanovic, Dimitri Mawet, Sergio Leon-Saval, Rodrigo Amezcua-Correa, Stephanos Yerolatsitis, Michael P. Fitzgerald, Pradip Gatkine, Yoo Jung Kim, Jonathan Lin, Barnaby Norris, Garreth Ruane, Steph Sallum

{"title":"Laboratory demonstration of a Photonic Lantern Nuller in monochromatic and broadband light","authors":"Yinzi Xin, Daniel Echeverri, Nemanja Jovanovic, Dimitri Mawet, Sergio Leon-Saval, Rodrigo Amezcua-Correa, Stephanos Yerolatsitis, Michael P. Fitzgerald, Pradip Gatkine, Yoo Jung Kim, Jonathan Lin, Barnaby Norris, Garreth Ruane, Steph Sallum","doi":"10.1117/1.jatis.10.2.025001","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.025001","url":null,"abstract":"Photonic lantern nulling (PLN) is a method for enabling the detection and characterization of close-in exoplanets by exploiting the symmetries of the ports of a mode-selective photonic lantern (MSPL) to cancel out starlight. A six-port MSPL provides four ports where on-axis starlight is suppressed, while off-axis planet light is coupled with efficiencies that vary as a function of the planet’s spatial position. We characterize the properties of a six-port MSPL in the laboratory and perform the first testbed demonstration of the PLN in monochromatic light (1569 nm) and in broadband light (1450 to 1625 nm), each using two orthogonal polarizations. We compare the measured spatial throughput maps with those predicted by simulations using the lantern’s modes. We find that the morphologies of the measured throughput maps are reproduced by the simulations, though the real lantern is lossy and has lower throughputs overall. The measured ratios of on-axis stellar leakage to peak off-axis throughput are around 10−2, likely limited by testbed wavefront errors. These null-depths are already sufficient for observing young gas giants at the diffraction limit using ground-based observatories. Future work includes using wavefront control to further improve the nulls, as well as testing and validating the PLN on-sky.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140590014","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Analyzing the atmospheric dispersion correction of the Gemini Planet Imager: residual dispersion above design requirements 分析双子座行星成像仪的大气色散校正：超出设计要求的残余色散

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.025002

Malachi Noel, Jason J. Wang, Bruce Macintosh, Katie Crotts, Christian Marois, Eric L. Nielsen, Robert J. De Rosa, Katie Scalzo, Kent Wallace

{"title":"Analyzing the atmospheric dispersion correction of the Gemini Planet Imager: residual dispersion above design requirements","authors":"Malachi Noel, Jason J. Wang, Bruce Macintosh, Katie Crotts, Christian Marois, Eric L. Nielsen, Robert J. De Rosa, Katie Scalzo, Kent Wallace","doi":"10.1117/1.jatis.10.2.025002","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.025002","url":null,"abstract":"The atmospheric dispersion corrector (ADC) of the Gemini Planet Imager (GPI) corrects the chromatic dispersion caused by differential atmospheric refraction (DAR), making it an important optic for exoplanet observation. Despite requiring <5 mas of residual DAR to avoid potentially affecting the coronagraph, the GPI ADC averages ∼7 and ∼11 mas of residual DAR in H and J band, respectively. We analyzed GPI data in those bands to find explanations for the underperformance. We found the model GPI uses to predict DAR underestimates humidity’s impact on incident DAR, causing on average a 0.54 mas increase in H band residual DAR. Additionally, the GPI ADC consistently undercorrects in H band by about 7 mas, causing almost all the H band residual DAR. J band does not have such an offset. Perpendicular dispersion induced by the GPI ADC, potentially from a misalignment in the prisms’ relative orientation, causes 86% of the residual DAR in J band. Correcting these issues could reduce residual DAR, thereby improving exoplanet detection. We also made an approximation for the index of refraction of air from 0.7 to 1.36 microns that more accurately accounts for the effects of humidity.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140590044","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Gamma-ray burst studies with wide-field X-ray detectors on a SmallSat platform 利用小卫星平台上的宽视场 X 射线探测器进行伽马射线暴研究

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.026003

Jared E. Fuchs, Peter Veres, Michael S. Briggs, Peter Jenke

引用次数: 0

Radiation effects on scientific complementary metal-oxide-semiconductor detectors for x-ray astronomy: II. Total ionizing dose irradiation 用于 X 射线天文学的科学互补金属氧化物半导体探测器的辐射效应：II.总电离剂量辐照

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.026001

Mengxi Chen, Zhixing Ling, Mingjun Liu, Qinyu Wu, Chen Zhang, Jiaqiang Liu, Zhenlong Zhang, Weimin Yuan, Shuang-Nan Zhang

{"title":"Radiation effects on scientific complementary metal-oxide-semiconductor detectors for x-ray astronomy: II. Total ionizing dose irradiation","authors":"Mengxi Chen, Zhixing Ling, Mingjun Liu, Qinyu Wu, Chen Zhang, Jiaqiang Liu, Zhenlong Zhang, Weimin Yuan, Shuang-Nan Zhang","doi":"10.1117/1.jatis.10.2.026001","DOIUrl":"https://doi.org/10.1117/1.jatis.10.2.026001","url":null,"abstract":"Complementary metal-oxide-semiconductor (CMOS) detectors are a competitive choice for current and upcoming astronomical missions. To understand the performance variations of CMOS detectors in the space environment, we investigate the total ionizing dose effects on custom-made large-format X-ray CMOS detectors. Three CMOS detector samples were irradiated with a Co60 source with a total dose of 70 and 105 krad. We test and compare the performance of these detectors before and after irradiation. After irradiation, the dark current increases by roughly 20∼100 times, and the readout noise increases from 3 e− to 6 e−. The bias level at 50 ms integration time decreases by 13 to 18 digital number (DN) at −30°C. The energy resolution increases from ∼150 to ∼170 eV at 4.5 keV at −30°C. The conversion gain of the detectors varies for <2% after the irradiation. Furthermore, there are about 50 pixels in which bias at 50 ms has changed by more than 20 DN after the exposure to the radiation and about 30 to 140 pixels in which the readout noise has increased by over 20 e− at −30°C at 50 ms integration time. These results demonstrate that the performances of large-format CMOS detectors do not suffer significant degeneration in space environment.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":2.3,"publicationDate":"2024-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140590117","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Optical ray tracing of echelle spectrographs applied to the wavelength solution for precise radial velocities 应用于精确径向速度波长求解的埃歇尔摄谱仪的光学射线追踪

IF 2.3 3区工程技术

Journal of Astronomical Telescopes Instruments and Systems Pub Date : 2024-04-01 DOI: 10.1117/1.jatis.10.2.028001

Marcelo Tala Pinto, Adrian Kaminski, Andreas Quirrenbach, Mathias Zechmeister

引用次数: 0