Gotowe bibliografie tematyczne / Cassegrain telescope

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  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji

Gotowa bibliografia na temat „Cassegrain telescope”

Autor: Grafiati
Data publikacji: 3 czerwca 2025
Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Cassegrain telescope"

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Liu, Xuan, Junhong Deng, King Fai Li, et al. "Optical telescope with Cassegrain metasurfaces." Nanophotonics 9, no. 10 (2020): 3263–69. http://dx.doi.org/10.1515/nanoph-2020-0012.

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AbstractThe Cassegrain telescope, made of a concave primary mirror and a convex secondary mirror, is widely utilized for modern astronomical observation. However, the existence of curved mirrors inevitably results in bulky configurations. Here, we propose a new design of the miniaturized Cassegrain telescope by replacing the curved mirrors with planar reflective metasurfaces. The focusing and imaging properties of the Cassegrain metasurface telescopes are experimentally verified for circularly polarized incident light at near infrared wavelengths. The concept of the metasurface telescopes can
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BAQUERO, N., W. A. HERNANDEZ, and R. A. RINCON. "Diseño y construcción de un telescopio Cassegrain clásico." Orinoquia 10, no. 2 (2006): 7–12. http://dx.doi.org/10.22579/20112629.209.

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Titulo en ingles: Design and construction of a telescope classic CassegrainRESUMEN: Se presenta los resultados del trabajo de investigación aplicada y desarrollo tecnológico llevado a cabo en el taller de óptica de UNILLANOS: Diseño y construcción de un telescopio Cassegrain clásico, de 150 mm de diámetro, f/D= 20; como instrumento óptico para la observación astronómica.Palabras clave: Diseño óptico, telescopio CassegrainABSTRACT: Next are shown the scientific results of the applied investigation work and technology development accomplished in the optic laboratory of UNILLANOS: Design and cons
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Yue, Song, Zhe Zhang, Kunpeng Zhang, et al. "Design and Numerical Analysis of an Infrared Cassegrain Telescope Based on Reflective Metasurfaces." Nanomaterials 11, no. 11 (2021): 2904. http://dx.doi.org/10.3390/nano11112904.

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Reflective imaging systems such as Cassegrain-type telescopes are widely utilized in astronomical observations. However, curved mirrors in traditional Cassegrain telescopes unavoidably make the imaging system bulky and costly. Recent developments in the field of metasurfaces provide an alternative way to construct optical systems, possessing the potential to make the whole system flat, compact and lightweight. In this work, we propose a design for a miniaturized Cassegrain telescope by replacing the curved primary and secondary mirrors with flat and ultrathin metasurfaces. The meta-atoms, cons
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Sobirin, Farhan Fatwa, Satia Nugraha, Fauzia Haz, and Peberlin Sitompul. "Study of Cassegrain-type antenna for radio telescope." Journal of Physics: Conference Series 2214, no. 1 (2022): 012028. http://dx.doi.org/10.1088/1742-6596/2214/1/012028.

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Abstract There are many critical parameters in the design of a radio telescope, such as antenna gain and antenna resolution. In telecommunications, radar, and radio telescopes, an antenna is a very important component. There are many designs of the antenna, such as dipole array and parabolic antenna. Parabolic antennas also have many sub-reflector and antenna methods that control the radio wave, such as the Cassegrain type. A Cassegrain-type antenna is a parabolic antenna in which the feed antenna is mounted at or behind the surface of the main parabolic reflector dish. For the transmitter sys
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Haider, Y. Hammod*1 Saaid F. Hassan2 Intisar A. Naseef3. "DESIGN AND ANALYSISA ZOOM CASSEGRAIN TELESCOPE COVER MIDDLE IR REGION USING ZEMAX PROGRAM." INTERNATIONAL JOURNAL OF ENGINEERING SCIENCES & RESEARCH TECHNOLOGY 6, no. 8 (2017): 178–85. https://doi.org/10.5281/zenodo.839159.

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The goal of the project is to find an optimal design of zoom -Cassegrain telescope which is popular for amateur astronomers. Also,the objective function of the optical design is to reduce the aberrations to provide aclear image. Cassegrain telescope has been designing and analysis by using (Zemax) software. The full field of view of the objective lens angle to 0.383°, the focal length to 747,748,750 and751mm, Back focal distance BFD 41 mmand Entrance pupil diameter 218.The system consists of a fixed focal length of the objective lens, zoom eyepiece. The eyepiece continuous zoom the zoom telesc
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Tokunaga, A. T., C. Ftaclas, J. R. Kuhn, and P. Baudoz. "High Dynamic Range and the Search for Planets." Symposium - International Astronomical Union 211 (2003): 487–96. http://dx.doi.org/10.1017/s0074180900211200.

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General arguments for optimized coronagraphy in the search for planets are presented. First, off-axis telescopes provide the best telescopic platforms for use with coronagraphy, and telescope fabrication technology now allows the fabrication of such telescopes with diameters of up to 6.5 m. We show that in certain circumstances a smaller telescope with an off-axis primary has a signal-to-noise advantage compared with larger Cassegrain telescopes. Second, to fully exploit the advantages of the coronagraph for suppressing stray light, it is necessary to use a high Strehl ratio adaptive optics sy
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Wang, Honghao, Jianli Wang, Yuyan Cao, Tao Chen, and Hongwen Li. "Optical Pupil Shift Correction Method for Large Ground-Based Optical Telescopes." Applied Sciences 13, no. 24 (2023): 13173. http://dx.doi.org/10.3390/app132413173.

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Cassegrain telescopes with larger apertures suffer significant optical pupil shifting errors caused by gravity and temperature gradients. This study constructs an optical model of a large Cassegrain telescope and a method to calculate and compensate its shifting error. First, the optical structure is simplified by incorporating only the most relevant telescope components, and the system optics is modeled using ray tracing. A computer-aided mounting-based method for calculating the misalignment error of primary and secondary mirrors is proposed, with the spatial position change of secondary mir
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Tan, Alfred Yong Liang. "High-resolution solar imaging for citizen science." EPJ Web of Conferences 240 (2020): 01002. http://dx.doi.org/10.1051/epjconf/202024001002.

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High-resolution solar imaging, essential for research into the Sun is usually limited to high-end expensive telescopes found in professional observatories using adaptive optics technology. However, a Schmidt-Cassegrain Telescope (SCT) or a refractor telescope equipped with a narrow-band energy rejection filter and a suitable solar spectrum filter, employing appropriate data acquisition and post-processing techniques can provide an amateur astronomer a costeffective means to high-resolution solar imaging.
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Xiaodong Hu, Xiaodong Hu, Weike Wang Weike Wang, Qiang Hu Qiang Hu, et al. "Design of CASSEGRAIN telescope baffles with honeycomb entrance." Chinese Optics Letters 12, no. 7 (2014): 072901–72904. http://dx.doi.org/10.3788/col201412.072901.

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Stavroudis, Orestes N. "Principal surface of a Cassegrain telescope." Journal of the Optical Society of America A 11, no. 4 (1994): 1253. http://dx.doi.org/10.1364/josaa.11.001253.

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Rozprawy doktorskie na temat "Cassegrain telescope"

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Benli, Ozturk Esra. "A Practical Alignment Algorithm For Cassegrain Type Telescopes." Master's thesis, METU, 2012. http://etd.lib.metu.edu.tr/upload/12614573/index.pdf.

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Focal plane corrected Cassegrain type optical systems have been widely used in various fields. The axial alignment of complex optical systems is not easy and a practical alignment method is needed for such systems. Tilts, decenters and axial motion of elements or group of elements in the system are the typical alignment parameters. Interferometric measurement is an effective way to see the errors caused by the misalignment of each element in an optical system. In this thesis, alignment of a Cassegrain type telescope will be examined by using interferometric measurements and modulation transfer
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Chan, Yat-ping Carl, and 陳一平. "Installation of direct-vision prism spectroscopy into a 32CM cassegrain telescope." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1998. http://hub.hku.hk/bib/B31220472.

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Chan, Yat-ping Carl. "Installation of direct-vision prism spectroscopy into a 32CM cassegrain telescope /." Hong Kong : University of Hong Kong, 1998. http://sunzi.lib.hku.hk/hkuto/record.jsp?B20357680.

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Hosseini, Sona, and Walter Harris. "Khayyam: progress and prospects of coupling a spatial heterodyne spectrometer (SHS) to a Cassegrain telescope for optical interferometry." SPIE-INT SOC OPTICAL ENGINEERING, 2016. http://hdl.handle.net/10150/622529.

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In the temporal study of faint, extended sources at high resolving power, Spatial Heterodyne Spectrometer (SHS) can offer significant advantages about conventional dispersive grating spectrometers. We describe here a four-year continuous progress in Mt. Hamilton, Lick Observatory, toward development of a prototype reflective Spacial Heterodyne Spectrometer, Khayyam, instrument-telescope configuration to combine all of the capabilities necessary to obtain high resolving power visible band spectra of diffuse targets from small aperture on-axis telescopes where significant observing time can be o
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Choi, Narak. "Image degradation due to surface scattering in the presence of aberrations." Doctoral diss., University of Central Florida, 2012. http://digital.library.ucf.edu/cdm/ref/collection/ETD/id/5165.

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This dissertation focuses on the scattering phenomena by well-polished optical mirror surfaces. Specifically, predicting image degradation by surface scatter from rough mirror surfaces for a two-mirror telescope operating at extremely short wavelengths (9nm~30nm) is performed. To evaluate image quality, surface scatter is predicted from the surface metrology data and the point spread function in the presence of both surface scatter and aberrations is calculated. For predicting the scattering intensity distribution, both numerical and analytic methods are considered. Among the numerous analyti
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Giulietti, Marika. "Telescopi ottici, radio, X: principi e differenze." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/12353/.

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Lo scopo di questo elaborato è la descrizione dei principi su cui si basano i telescopi ottici, radio e x nell'osservazione dei corpi celesti, la loro meccanica di funzionamento e le relative differenze. Un telescopio è uno strumento fisico volto a raccogliere radiazione proveniente da oggetti molto distanti in una grande regione di cielo facendola convogliare su un'area ristretta. Questo avviene tramite l'utilizzo ad esempio di specchi, lenti o antenne, in modo da ottenere la massima risoluzione possibile. I fotoni raccolti vengono poi fatti convogliare in dei rilevatori come un obietti
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Książki na temat "Cassegrain telescope"

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Mollise, Rod. Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4.

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Fazio, Giovanni G. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy. Smithsonian Institution, Astrophysical Observatory, 1986.

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Fazio, Giovanni G. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy. Smithsonian Institution, Astrophysical Observatory, 1986.

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Mollise, Rod. Choosing and using a new CAT: Getting the most from your Schmidt Cassegrain or any catadioptric telescope. Springer, 2009.

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Fazio, Giovanni G. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy: Semiannual status report no. 2 for the period 1 March 1984 through 31 August 1984. Smithsonian Institution, Astrophysical Observatory, 1985.

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Observatory, Smithsonian Astrophysical, and United States. National Aeronautics and Space Administration, eds. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy: Semiannual status report no. 2 for the period 1 March 1984 through 31 August 1984. Smithsonian Institution, Astrophysical Observatory, 1985.

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Observatory, Smithsonian Astrophysical, and United States. National Aeronautics and Space Administration, eds. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy: Semiannual status report no. 4 for the period 1 March 1985 through 31 August 1985. Smithsonian Institution, Astrophysical Observatory, 1985.

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Fazio, Giovanni G. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy: Semiannual status report no. 2 for the period 1 March 1984 through 31 August 1984. Smithsonian Institution, Astrophysical Observatory, 1985.

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1942-, Burnside Walter Dennis, and Langley Research Center, eds. A Cassegrain reflector system for compact range applications. National Aeronautics and Space Administration, Langley Research Center, 1986.

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Center, Langley Research, ed. Beam scanning offset Cassegrain reflector antennas by subreflector movement. National Aeronautics and Space Administration, Langley Research Center, 1994.

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Części książek na temat "Cassegrain telescope"

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Hickey, David. "Construction of a 32cm Cassegrain Photoelectric Telescope." In Instrumentation and Research Programmes for Small Telescopes. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-010-9433-7_17.

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Mollise, Rod. "Why a CAT?" In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_1.

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Mollise, Rod. "The Advanced CAT: Imaging and Computers." In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_10.

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Mollise, Rod. "Afterword: 25 Years with a CAT — How to Keep Going." In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_11.

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Mollise, Rod. "What’s a CAT?" In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_2.

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Mollise, Rod. "Inside a CAT." In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_3.

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Mollise, Rod. "Which CAT?" In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_4.

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Mollise, Rod. "The SCT Out-of-Box Experience: Initial Telescope Assembly and Checkout." In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_5.

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Mollise, Rod. "Accessories for your CAT." In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_6.

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Mollise, Rod. "From That Very First Night: Field Setup, Checkout and Observing." In Choosing and Using a Schmidt-Cassegrain Telescope. Springer London, 2001. http://dx.doi.org/10.1007/978-1-4471-0227-4_7.

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Streszczenia konferencji na temat "Cassegrain telescope"

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Oldenettel, Jerry R. "Mirror and dome seeing measurements at AMOS." In Adaptive Optics for Large Telescopes. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/aolt.1992.amc5.

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While the effect of mirror and dome temperatures on seeing quality has been the subject of several recent laboratory experiments (1,2,3), no data from working telescope systems has been published. In this paper, I present data collected on telescopes of two different designs located at the Maui Space Surveillance Site located near the 10,000 foot summit of Haleakala Volcano on Maui, HI. The 1.6 meter aperture AMOS telescope is a closed tube Cassegrain design which tends to trap mirror generated turbulence and channel it along the telescope line of site. The 1.2 meter aperture MOTIF telescope i
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Renero-C., Francisco-J., Octavio Cardona-N., Roberto Cardona-N., et al. "Fabrication of the SubReflector for the Large Millimeter Telescope (Gran Telescopio Milimétrico)." In Optical Fabrication and Testing. Optica Publishing Group, 1998. http://dx.doi.org/10.1364/oft.1998.otuc.5.

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Astronomers use telescopes to study the universe in the different spectrum regions. The dimensions of telescopes, to research in the millimeter region, are too big. Thus, fabrication of such instruments is a challenge work. The “Gran Telescopio Milimétrico (Large Millimeter Telescope, which will be called LMT) is a Cassegrain Telescope, which diameter of the primary reflector is 50 meters and the subreflector is a hyperbolic surface which diameter is 2.57 meters, and it is been developed to observe in the millimeter region. The subrelector surface must be fabricated with an accuracy of 13 µm (
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Close, Laird M., Francois Roddier, Claude Roddier, Malcolm Northcott, and J. Elon (Buzz) Graves. "Bubbles, Disks, and Planets: Science with the University of Hawai’i AO System." In Adaptive Optics. Optica Publishing Group, 1996. http://dx.doi.org/10.1364/adop.1996.atub.1.

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The Adaptive Optics system, built at the Institute for Astronomy (University of Hawai’i), has been making unique scientific observations since 1993. During that period this versatile AO system has been mounted at both Cassegrain and coude feeds at the 3.6m CFH telescope and the bent Cassegrain at the 3.8m UKIRT telescope. The instrument is now permanently a Cassegrain instrument which has enjoyed 24 nights of 4m class observing at Manua Kea.
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Ho, Cheng-Fang, and Shenq-Tsong Chang. "Baffle design for a Cassegrain telescope." In International Conference on Optical Instrumentation and Technology, edited by Yongtian Wang, Yunlong Sheng, and Kimio Tatsuno. SPIE, 2009. http://dx.doi.org/10.1117/12.838089.

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Shafer, David R. "Unusual binary-optics telescope design." In OSA Annual Meeting. Optica Publishing Group, 1993. http://dx.doi.org/10.1364/oam.1993.wcc.4.

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Walker, A. B. C., T. W. Barbee, R. B. Hoover, and J. F. Lindblom. "Soft X-Ray Images of the Solar Corona With a Normal-Incidence Cassegrain Multilayer Telescope." In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Optica Publishing Group, 1988. http://dx.doi.org/10.1364/soa.1988.wb3.

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High resolution images of the sun in the soft x-ray/extreme ultraviolet (XUV) regime have been obtainec with normal-incidence Cassegrain multilayer telescopes for the first time. The inherent energy selective property of multilayer-coated optics allowed distinct groups of emission lines to be isolated in the solar corona and the transition region. The sounding rocket borne soft x-ray telescopes [1] were launched on October 23, 1987. In addition to the Cassegrain telescopes, which provided images in bands centered at 173 Å and 256 Å, the payload contained concave spherical mirror multilayer tel
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Zhang, Xiaoming, Hongbin Chen, Jihong Wang, and Bo Qi. "Computer aided alignment for a Cassegrain telescope." In 6th International Symposium on Advanced Optical Manufacturing and Testing Technologies (AOMATT 2012), edited by Yudong Zhang, Libin Xiang, and Sandy To. SPIE, 2012. http://dx.doi.org/10.1117/12.970392.

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Moore, Kenneth E., and Tina Valente. "Numerical Method For Cassegrain Telescope Baffle Design." In 33rd Annual Techincal Symposium, edited by Daniel Vukobratovich. SPIE, 1989. http://dx.doi.org/10.1117/12.962944.

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Rail, Zdenek, Pavel Pintr, Tomas Thor, David Vápenka, and Zbyněk Melich. "All-spherical Cassegrain telescope with a Volosov corrector." In Optics and Measurement 2019 International Conference, edited by Jana Kovačičinová. SPIE, 2019. http://dx.doi.org/10.1117/12.2542703.

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Kimura, K., H. Ogawa, H. Ujihara, et al. "ASTRO-G/VSOP-2 off-set cassegrain telescope." In 2008 IEEE Antennas and Propagation Society International Symposium and USNC/URSI National Radio Science Meeting. IEEE, 2008. http://dx.doi.org/10.1109/aps.2008.4619071.

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