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Letteratura scientifica selezionata sul tema "Telescopes"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 25 luglio 2025

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Articoli di riviste sul tema "Telescopes"

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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Liu, Yi, Changqing Feng, Ingrid-Maria Gregor, et al. "ADENIUM — A demonstrator for a next-generation beam telescope at DESY." Journal of Instrumentation 18, no. 06 (2023): P06025. http://dx.doi.org/10.1088/1748-0221/18/06/p06025.

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Abstract High-resolution beam telescopes for charged particle tracking are one of the most important and equally demanding infrastructure items at test beam facilities. The main purpose of beam telescopes is to provide precise reference track information of beam particles to measure the performance of a device under test (DUT). In this report the development of the ADENIUM beam telescope (ALPIDE sensor based DESY Next test beam Instrument) as a demonstrator and prototype for a next-generation beam telescope is presented. The ADENIUM beam telescope features up to six pixelated reference planes

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Lu, Zhiyi. "Analysis of the Principle and State-of-art Applications of Astronomical Telescope." Highlights in Science, Engineering and Technology 72 (December 15, 2023): 83–89. http://dx.doi.org/10.54097/4kna8f33.

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Astronomical telescopes have been instrumental in enhancing our comprehension of the cosmos since ancient eras. This study explores these remarkable instruments' principles and state-of-art applications, tracing their development from early refracting telescopes to modern space and ground-based telescopes. The primary focus is to analyze the imaging principles of optical and radio telescopes and showcase their significance in capturing high-resolution observations of celestial objects. It also highlights recent achievements made by advanced telescopes, including the James Webb Space Telescope

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Chen, Siyu. "Comparisons of Two Types of Astronomical Telescopes: Terrestrial Telescopes and Space Telescopes." Theoretical and Natural Science 2, no. 1 (2023): 75–80. http://dx.doi.org/10.54254/2753-8818/2/20220166.

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In the field of astrophysics and cosmology, astronomical telescopes are the main and key tool for observing and capturing information of celestial bodies. Generally, there are two types of telescopes, i.e., terrestrial telescopes and space telescopes. This study will be mainly focused on the differences and similarities between the two types mentioned above. According to the analysis, the ground telescope is larger and collect data with processing instead of real picture. The space telescope, on the other hand, is smaller but hard to repair, which is able to send back the real pictures of the

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Kim, Sang Chul. "Paper Productivity of Ground-based Large Optical Telescopes from 2000 to 2009." Publications of the Astronomical Society of Australia 28, no. 3 (2011): 249–60. http://dx.doi.org/10.1071/as11011.

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AbstractWe present an analysis of the scientific (refereed) paper productivity of the current largest (diameter > 8m) ground-based optical (and infrared) telescopes during the ten-year period from 2000 to 2009. The telescopes for which we have gathered and analysed the scientific publication data are the two 10-m Keck telescopes, the four 8.2-m Very Large Telescopes (VLT), the two 8.1-m Gemini telescopes, the 8.2-m Subaru telescope, and the 9.2-m Hobby–Eberly Telescope (HET). We have analysed the numbers of papers published in various astronomical journals produced by using these telescopes

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Xu, Yuchen. "Comparison Of Different Telescopes: James Webb Space, Giant Magellan and Event Horizon." Highlights in Science, Engineering and Technology 112 (August 20, 2024): 101–8. http://dx.doi.org/10.54097/pqj1a442.

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Mankind's obsession with space and the persistence of searching for extraterrestrial life has led to the invention of telescopes as a way to explore the mysterious vastness of the universe. In this paper, the development history of the telescope is studied, as well as the famous events observed by the telescope (black hole, solar structure, etc.), and the structure, environment and interference of the ground-based telescope, space telescope and joint telescope are compared and analyzed. By comparison, it is found that most large telescopes have a variety of research directions and are more res

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Hong, Yiduo. "Working principle of the radio telescope and the study of the sun." Theoretical and Natural Science 12, no. 1 (2023): 172–76. http://dx.doi.org/10.54254/2753-8818/12/20230461.

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Radio telescopes can help people observe celestial bodies far away from people, which is conducive for astronomers to observe and draw the trend of celestial transformations. The use of radio telescopes allows scholars to study and understand celestial bodies to a new height. At present, the more famous are the Webb Space Telescope in the United States, the Hubble Space Telescope and China's Tianyan. In the case of the eye of Heaven in Guizhou, China, the surface of the eye is covered by a metal layer one millimeter thick, so it can not withstand excessive pressure, and the maintenance personn

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Li, Yuqiao. "State-of-art Facilities and Prospect of Radio Telescopes." Highlights in Science, Engineering and Technology 5 (July 7, 2022): 201–7. http://dx.doi.org/10.54097/hset.v5i.743.

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The radio telescopes play a crucial role in astrophysical observations; hence it is necessary to discuss about the significance, structure, and applications of radio telescope and analyse the difference between the state-of-art radio telescopes (FAST and SKA) based on present information. Specifically, the background and present conditions as well as the history of radio telescopes will be introduced initially. Subsequently, the significance of radio telescope will be explained, including structure and application of radio telescopes. Subsequently, the doubts on FAST and SKA and strengths of t

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Pech, Miroslav, Justin Albury, Jose A. Bellido, et al. "Simulation of the optical performance of the Fluorescence detector Array of Single-pixel Telescopes." EPJ Web of Conferences 210 (2019): 05014. http://dx.doi.org/10.1051/epjconf/201921005014.

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The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a proposed large-area, next-generation experiment for the detection of ultra-high energy cosmic rays via the atmospheric fluorescence technique. The telescope’s large field-of-view (30 ×30) is imaged by four 200 mm photomultiplier-tubes at the focal plane of a segmented spherical mirror of 1.6 m diameter. Two prototypes are installed and taking data at the Black Rock Mesa site of the Telescope Array experiment in central Utah, USA. We present the process used for optimization of the optical performance of this compact and low

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Porter, F. I., J. M. White, J. Goldberg, J. L. Demer, and A. Koval. "Predicting Successful Low Vision Rehabilitation with Telescopic Spectacles." Journal of Visual Impairment & Blindness 86, no. 1 (1992): 29–32. http://dx.doi.org/10.1177/0145482x9208600116.

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Although telescopic spectacles magnify the retinal image and should improve functional vision, many low vision patients are unable to use them. The authors found that involuntary head movements and the reduction of acuity with imposed head motion differentiated successful from unsuccessful telescope users and that success was related to the age at which telescopes were first used.

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Tesi sul tema "Telescopes"

Mawson, Neil R. "Small telescopes installed at the Liverpool Telescope." Thesis, Liverpool John Moores University, 2013. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.604296.

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The Small Telescopes Installed at the Liverpool Telescope (STILT) have been in operation since March 2009, collecting wide field data from their position, at the Liverpool Telescope on La Palma. The system consists of a set of two wide field imaging cameras, known as SkycamT and SkycamZ. They provide fields of view of 21x210 and Ix 1 0, along with limits of 12th and 18th in R-band magnitude. The work in this thesis describes the methodology used to create an image analysis pipeline and database to store the photometric results contained in the images produced by these cameras. Such a database

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Vaksdal, Birger. "Medium Size Telescopes in the Cherenkov Telescope Array." Thesis, KTH, Fysik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-210238.

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Fernández, Barral Alba. "Extreme particle acceleration in microquasar jets and pulsar wind nebulae with the MAGIC telescopes." Doctoral thesis, Universitat Autònoma de Barcelona, 2017. http://hdl.handle.net/10803/457715.

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A lo largo de toda nuestra historia, los seres humanos nos hemos esforzado por descifrar los misterios con los que el Universo nos desafía. En nuestros humildes comienzos, esta tarea era realizada con nuestros ojos desnudos, mirando las estrellas y los planetas y preguntándonos qué tan lejos estaban y cómo se movían en el cielo nocturno. Durante muchos siglos, sólo el Universo visible fue accesible para nosotros, pero se obtuvieron logros extraordinarios a pesar de las limitadas herramientas: descubrimos, por ejemplo, que nuestro planeta no era el centro del Universo, gracias a las obse

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Witzemann, Amadeus. "Cosmology with next generation radio telescopes." University of the Western Cape, 2019. http://hdl.handle.net/11394/6936.

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Philosophiae Doctor - PhD<br>The next generation of radio telescopes will revolutionize cosmology by providing large three-dimensional surveys of the universe. This work presents forecasts using the technique 21cm intensity mapping (IM) combined with results from the cosmic microwave background, or mock data of galaxy surveys. First, we discuss prospects of constraining curvature independently of the dark energy (DE) model, finding that the radio instrument HIRAX will reach percent-level accuracy even when an arbitrary DE equation of state is assumed. This is followed by a study of the

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O'Dougherty, Stefan, and Stefan O'Dougherty. "Quasi-Optical Spherical Balloon Telescopes." Diss., The University of Arizona, 2018. http://hdl.handle.net/10150/626762.

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Astronomy constantly pushes the limits of technology in order to decipher the workings of the Universe. There is a constant need for higher resolution observations across a wide range of wavelengths, at preferably a minimal cost. The terahertz regime (lambda=100 um to lambda=1000 um) covers a region of the electromagnetic spectrum that is blocked by Earth's atmosphere, which limits observations to high altitude plane and balloon telescopes and space telescopes. These current options limit the resolution achievable due to the size of telescopes that can be launched. This dissertation investigat

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Bou, Cabo Manuel. "Acoustics for underwater neutrino telescopes." Doctoral thesis, Universitat Politècnica de València, 2011. http://hdl.handle.net/10251/10989.

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En esta tesis se tratan diferentes aspectos de la acústica presente en un telescopio submarino de neutrinos, principalmente en dos vertientes: en el sistema de posicionamiento acústico utilizado para la monitorización de las posiciones de los módulos ópticos presentes a lo largo del detector, así como en sistemas para detección acústica de neutrinos, técnica que actualmente está en fase de estudio. Todos los estudios realizados están enmarcados dentro de dos colaboraciones europeas para el diseño, construcción y operación de telescopios submarinos de neutrinos: Antares (en fase de operación)

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Kern, Pierre. "Optique adaptative et grands telescopes." Paris 7, 1990. https://tel.archives-ouvertes.fr/tel-00714946.

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Severement limite par la turbulence atmospherique, les grands telescopes au sol ne sont pas capables d'atteindre leur limite de resolution intrinseque de maniere directe. En fonctionnement normal, ils ne peuvent pas resoudre plus de details, aux longueurs d'ondes du visible et du proche infrarouge qu'un telescope de quelques decimetres de diametre. La technique d'optique adaptative decrite ici, offre l'avantage sur les autres techniques, d'un traitement du front d'onde avant la detection du signal. Lorsque la detection n'est pas limitee par le bruit propre du signal incident ce traitement perm

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Petrushevska, Tanja. "Supernovae seen through gravitational telescopes." Doctoral thesis, Stockholms universitet, Fysikum, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-141633.

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Galaxies, and clusters of galaxies, can act as gravitational lenses and magnify the light of objects behind them. The effect enables observations of very distant supernovae, that otherwise would be too faint to be detected by existing telescopes, and allows studies of the frequency and properties of these rare phenomena when the universe was young. Under the right circumstances, multiple images of the lensed supernovae can be observed, and due to the variable nature of the objects, the difference between the arrival times of the images can be measured. Since the images have taken different pat

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Andersen, Geoff. "Holographic correction of aberrated telescopes /." Title page, abstract and contents only, 1996. http://web4.library.adelaide.edu.au/theses/09PH/09pha544.pdf.

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Thrall, Michael L. "Orbit determination of highly eccentric orbits using a RAVEN telescope." Thesis, Monterey, Calif. : Springfield, Va. : Naval Postgraduate School ; Available from National Technical Information Service, 2005. http://library.nps.navy.mil/uhtbin/hyperion/05Sep%5FThrall.pdf.

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Thesis (M.S. in Space Systems Operations)--Naval Postgraduate School, September 2005.<br>Thesis Advisor(s): Kyle T. Alfriend, Don A. Danielson. Includes bibliographical references (p. 33). Also available online.

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Libri sul tema "Telescopes"

Bender, Lionel. Telescopes. Gloucester Press, 1991.

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Bender, Lionel. Telescopes. Gloucester, 1991.

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Manly, Peter L. Unusual telescopes. Cambridge University Press, 1991.

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English, Neil. Space Telescopes. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-27814-8.

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Chinnici, Ileana, ed. Merz Telescopes. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-41486-7.

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English, Neil. Classic Telescopes. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-4424-4.

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Panel, Anglo-Australian Observatory Schmidt Telescope. The future use of the UK Schmidt Telescope: A report. Anglo-Australian Observatory], 1995.

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Tucker, Wallace H. The cosmic inquirers: Modern telescopes and their makers. Harvard University Press, 1986.

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Kitchin, C. R. Telescopes and techniques: An introduction to practical astronomy. Springer, 1995.

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1934-, Brown Robert A., Ford H. C, Space Telescope Science Institute (U.S.), and United States. National Aeronautics and Space Administration., eds. Report of the HST Strategy Panel: A strategy for recovery : the results of a special study, August-October 1990. Space Telescope Science Institute, 1991.

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Capitoli di libri sul tema "Telescopes"

Gross, Herbert, Fritz Blechinger, and Bertram Achtner. "Telescopes." In Handbook of Optical Systems. Wiley-VCH Verlag GmbH & Co. KGaA, 2015. http://dx.doi.org/10.1002/9783527699247.ch8.

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Redfern, Gregory I. "Telescopes." In The Patrick Moore Practical Astronomy Series. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-45943-7_4.

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Bennett, Jim. "Telescopes." In A Companion to the History of Science. John Wiley & Sons, Inc., 2016. http://dx.doi.org/10.1002/9781118620762.ch37.

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Dire, James. "Telescopes." In The Patrick Moore Practical Astronomy Series. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-65346-9_1.

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Schilizzi, Richard T., Ronald D. Ekers, Peter E. Dewdney, and Philip Crosby. "Large Radio Telescopes and the Emergence of the SKA, 1957–1993." In The Square Kilometre Array. Springer International Publishing, 2024. http://dx.doi.org/10.1007/978-3-031-51374-9_2.

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AbstractThe SKA is the culmination of radio telescope design development in the decades prior to 1990. This chapter surveys the earlier telescopes and traces the origins of the ideas behind the SKA design.

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Mullaney, James. "Refracting Telescopes." In The Patrick Moore Practical Astronomy Series. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-8733-3_4.

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Mullaney, James. "Reflecting Telescopes." In The Patrick Moore Practical Astronomy Series. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-8733-3_5.

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Mullaney, James. "Catadioptric Telescopes." In The Patrick Moore Practical Astronomy Series. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-8733-3_6.

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Phillips, Thomas G., Stephen Padin, and Jonas Zmuidzinas. "Submillimeter Telescopes." In Planets, Stars and Stellar Systems. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-5621-2_7.

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EkersCSIRO Fellow, Ron, and Thomas L. Wilson. "Radio Telescopes." In Planets, Stars and Stellar Systems. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-5621-2_8.

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Atti di convegni sul tema "Telescopes"

Conan, R., K. Vogiatzis, and H. Fitzpatrick. "Characterization of the Dome Seeing of the Giant Magellan Telescope with Computational Fluid Dynamics Simulations." In Propagation Through and Characterization of Atmospheric and Oceanic Phenomena. Optica Publishing Group, 2024. http://dx.doi.org/10.1364/pcaop.2024.pth1e.1.

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The image quality of ground based telescopes is limited by atmospheric turbulence. The turbulence inside the dome of the telescopes, or dome seeing, accounts for a significant fraction of the image degradation. The Giant Magellan Telescope (GMT) is using extensively computational fluid dynamics simulations, to investigate GMT dome seeing for a large set of environmental conditions.

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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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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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Iye, Masanori, and Eiji Nishihara. "Differential Dome Seeing Monitor." In Adaptive Optics for Large Telescopes. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/aolt.1992.amd1.

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The evaluation and control of atmospheric turbulence in the upper atmosphere and around the telescope environment are growing concerns, since these are the last limiting factors in improving the imaging quality of large ground based telescopes. The adaptive optics is naturally a recent topical dynamic approach to control the optical wavefront aberration using a real time servo system. Another line of pains-taking efforts have been made to improve the thermal environment more favorable to telescopes. They are, for example, 1) reducing the thermal mass and thermal time constant of mirrors, teles

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Merkle, Fritz, and Norbert Hubin. "Adaptive Optics for the ESO Very Large Telescope." In Adaptive Optics for Large Telescopes. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/aolt.1992.atua4.

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Adaptive optics is one of the main features of the Very Large Telescope (VLT) of the European Southern Observatory (ESO). The VLT consists of an array of four 8 meter telescopes arranged in a quadrilateral configuration (see Figure 1). These four telescopes can be operated individually, in a so-called incoherent combined mode (mainly for high resolution spectroscopy), and in a coherently combined mode as a long baseline interferometer to achieve highest spatial resolution in the milliarcsecond range. In order to increase the performance and flexibility in use of the VLT in the interferometric

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Kim, Daewook, Jonathan W. Arenberg, Yuzuru Takashima, Art Palisoc, and Christopher Walker. "SALTUS Probe Class Space Mission: Enabled by 20-m Inflatable Mirror." In CLEO: Applications and Technology. Optica Publishing Group, 2022. http://dx.doi.org/10.1364/cleo_at.2022.aw4i.2.

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SALTUS (Single Aperture Large Telescope for Universe Studies) is a mid/far-infrared telescope concept utilizing a 20-m scale inflatable mirror antenna. The light-weight mirror utilizes a membrane architecture that has been developed and characterized specifically for space-based applications. The telescope's end-to-end optical design and optimization process unleashes the unprecedented photon collecting power of a large space aperture. A series of inflatable mirror prototypes have been designed, manufactured, and tested. These tests confirmed the optical performance of the apertures under spac

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Beckers, Jacques M. "Requirements for Adaptive Optics in Large Astronomical Telescopes." In Adaptive Optics for Large Telescopes. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/aolt.1992.atua1.

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The incorporation of adaptive optics in large astronomical telescopes to provide diffraction limited imaging promises to revolutionize ground based optical astronomy in the next decade. The gains are especially impressive for large aperture telescopes where the large increase in diameter D results both in a decrease of the area of the telescope point spread function proportional to D2 and in an increase in collected photons within that smaller area of D2. The availability of adaptive optics will thus pay off handsomely in many astronomical uses of large telescopes.

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Martin, H. M. "Innovative Optics for Giant Telescopes." In Optical Fabrication and Testing. Optica Publishing Group, 1996. http://dx.doi.org/10.1364/oft.1996.ofd.1.

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The present decade is an unprecedented period of expansion in the collective power of ground-based optical and infrared telescopes worldwide. No fewer than 13 telescopes between 6.5 m and 10 m in diameter--all larger than the most powerful telescope available before 1990--will be completed by roughly the year 2000. Some of these telescopes are designed with specific scientific goals in mind, such as high-resolution infrared imaging and spectroscopy, while others are multi-purpose instruments designed to serve the needs of an astronomical community whose observations have been limited by collec

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Miao, C. H. "Design of Array Systems Using Shared Symmetry." In International Lens Design. Optica Publishing Group, 1990. http://dx.doi.org/10.1364/ild.1990.lwb4.

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The design of multiple aperture array systems intended to cover a relatively wide field of view requires the appropriate combination of individual telescopes feeding a central collecting telescope system. In addition, specific aberration correction and scaling relations between the individual telescopes and the collecting telescope must be maintained. Of necessity there are at lease two optical axes that must be considered in such designs, with rotated symmetries dependent upon the position of each telescope in the array, practical systems should contain a minimum number of components in order

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Leviton, Douglas B., Geraldine A. Wright, Roger J. Thomas, Joseph M. Davila, and Gabriel L. Epstein. "Performance comparison of two Wolter Type II telescopes in the vacuum ultraviolet." In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/soa.1991.mf8.

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The SERTS-A and SERTS-C solar telescopes are examples of Wolter Type II glancing incidence telescopes built for flight1,2 on sounding rockets to study active regions on the sun in the extreme ultraviolet wavelength range 24-45 nm. Improvements in computer-controlled polishing technology at GSFC have led to the SERTS-C telescope which has substantially improved throughput and angular resolution in that wavelength range over the earlier SERTS-A. While both telescopes are diffraction-limited in the visible, preventing an obvious selection of the better telescope for flight, laboratory results in

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Rapporti di organizzazioni sul tema "Telescopes"

Halyo, Valerie. Diamond Pixel Luminosity Telescopes. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1166638.

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Hyde, R. A. ,. LLNL. Large aperture Fresnel telescopes/011. Office of Scientific and Technical Information (OSTI), 1998. http://dx.doi.org/10.2172/304513.

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Swanson, W. P. Aperture of two-counter telescopes. Office of Scientific and Technical Information (OSTI), 1988. http://dx.doi.org/10.2172/5997515.

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Ma, Binzhong. Research on Large Astronomical Telescopes,. Defense Technical Information Center, 1995. http://dx.doi.org/10.21236/ada297609.

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Baltz, E. Kaluza-Klein Dark Matter, Electrons and Gamma Ray Telescopes. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/839776.

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Pollard, Eric L., and Christopher H. Jenkins. Shape Memory Alloy Deployment of Membrane Mirrors for Spaceborne Telescopes. Defense Technical Information Center, 2005. http://dx.doi.org/10.21236/ada443511.

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Jefferies, Stuart M., and Douglas A. Hope. Advancing the Surveillance Capabilities of the Air Force's Large-Aperature Telescopes. Defense Technical Information Center, 2014. http://dx.doi.org/10.21236/ada605833.

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Anheier, Norman C., and Cliff S. Chen. A New Approach to Space Situational Awareness using Small Ground-Based Telescopes. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1171901.

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Marois, C. High Resolution Imaging of Satellites with Ground-Based 10-m Astronomical Telescopes. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/1036840.

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Lloyd-Hart, M., and T. McMahon. Adaptive Optics for the 6.5 m MMT Conversion, Development of Very High Resolution Imaging with Adaptive Optics for Large Telescopes, and Advanced Adaptive Optics for the World's Largest Telescopes. Defense Technical Information Center, 2001. http://dx.doi.org/10.21236/ada387632.

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