Bibliografías temáticas / Astronomical observatories

Literatura académica sobre el tema "Astronomical observatories"

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Publicado: 4 de junio de 2021
Última modificación: 31 de julio de 2024

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Artículos de revistas sobre el tema "Astronomical observatories"

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Mironov, Α. V. y V. M. Tereshchenko. "Astronomical Observatories in Kazakhstan". Open Astronomy 7, n.º 2 (1 de junio de 1998): 351–54. http://dx.doi.org/10.1515/astro-1998-0219.

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Wolfschmidt, Gudrun. "Cultural heritage of astronomical observatories". Proceedings of the International Astronomical Union 5, S260 (enero de 2009): 229–34. http://dx.doi.org/10.1017/s1743921311002341.

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AbstractWe present the results of the ICOMOS international symposium “Cultural Heritage of Astronomical Observatories (around 1900) – From Classical Astronomy to Modern Astrophysics” (Oct. 2008). The objective of the symposium was to discuss the relevance of modern observatories to the cultural heritage of humankind and to select partner observatories which, due to the date of their construction or to their architectural or scientific importance are comparable to Hamburg Observatory, as international cooperation partners for a serial trans-national application.
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Johnson, Stewart W., Jack O. Burns, Koon Meng Chua, Nebojsa Duric, Walter H. Gerstle y G. Jeffrey Taylor. "Lunar Astronomical Observatories: Design Studies". Journal of Aerospace Engineering 3, n.º 4 (octubre de 1990): 211–22. http://dx.doi.org/10.1061/(asce)0893-1321(1990)3:4(211).

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Tanaka, M., Y. Shirasaki, M. Ohishi, Y. Mizumoto, S. Kawanomoto, N. Yasuda y S. Honda. "Astronomical Research Using Virtual Observatories". Data Science Journal 8 (2010): S113—S121. http://dx.doi.org/10.2481/dsj.igy-018.

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Guoxiang, A. "National Astronomical Observatories in China". Science 293, n.º 5528 (13 de julio de 2001): 214a—214. http://dx.doi.org/10.1126/science.293.5528.214a.

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Swanson, Paul N. y James A. Cutts. "Astronomical observatories on the moon". Advances in Space Research 14, n.º 6 (junio de 1994): 123–27. http://dx.doi.org/10.1016/0273-1177(94)90017-5.

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Dale, Paul-Henri. "A Proposal for Better Cooperation among Libraries of Astronomical Observatories". International Astronomical Union Colloquium 110 (1989): 184–87. http://dx.doi.org/10.1017/s0252921100003341.

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SummaryThe cooperation between libraries of astronomical Observatories remains clearly insufficient despite the numerous means of communication now available. The library of the Royal Observatory of Belgium therefore recommends the establishment of a “subgroup” of users (Libraries of Astronomical Observatories) within the already existing Dobis-Libis Users Group.
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Wenjing, Jin, Jinming Bai y Yongqiang Yao. "The Selection and Protection of Optical Astronomical Observing Sites in China". Proceedings of the International Astronomical Union 10, H16 (agosto de 2012): 748. http://dx.doi.org/10.1017/s1743921314013301.

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Before 1950 there are two observatories, Shanghai and Purple Mountain Astronomical Observatories (SHAO and PMO), and two observing stations, Qingdao and Kunming stations in China. With the requirements of astronomical research, two observatories, Beijing and Shaanxi Astronomical Observatories (BAO and SXAO) and two artificial satellite stations, Urumqi and Changchun, were established about 1960. Based on the current management, now there are 4 observatories, SHAO, PMO, NAOC(National Astronomical Observatories), which was grouped from BAO, YNAO and 2 others, as well as XAO (Xinjiang Astronomical Observatory). The optical 1-2 m class telescopes are being operated at former four observatories. SXAO is changed as National Time Service Center. Because of city expansion as well as the traveling and economic developments, these observatories are suffered severe light pollution. For example, Zo Ce is located at the suburb of Shanghai city. A 40 cm double astrograph was installed in 1900 and a 1.56 m optical reflector have been operated since November 1987. In 1994 the seeing is better than 1 and the night sky brightness in V is about 19 mag/arcsec2, stars fainter than 20 mag with CCD are visibles. In 2007 a large playground was built in Zô Cè area. The light pollution is severe gradually. The night sky brightness has been increased to 15.8 mag/arcsec2. The other observatories have similar situation. New site surveys and found new stations to solve the problem. Except the solar and radio stations of each Astronomical Observatory, now there are 3 optical observing sites at PMO (Hong-He, Xu-Yi and Yaoan), 2 at SHAO (Zô Cè and Tian Huang Ping) and 2 at YNAO (Kunming and Gao-Mei-Gu) as well as 1 optical observing site at BAO (Xing-Long). The best observing site is Gao-Mei-Gu, which is selected as the optical observing site of YNAO and where atmospheric turbulence distribution is 0.11 near ground with heights from 6.5m to 2.7m during night. Sky brightness in B and V band are 22.34 and 21.54. The extinction coefficient K,bv and K,v are 0.298 and 0.135. The seeing measurement is 0.72’,. In the recent years a new 2.4m telescope the second largest telescope in China, was installed there.
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Ellegaard, Ole y Bertil F. Dorch. "The uniqueness of astronomical observatory publications". Proceedings of the International Astronomical Union 15, S367 (diciembre de 2019): 487–88. http://dx.doi.org/10.1017/s1743921321000314.

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AbstractAstronomical observatory publications include the work of local astronomers from observatories around the world and are traditionally exchanged between observatories through their libraries. However, large collections of these publications appear to be rare and are often incomplete. In order to assess the unique properties of the collections, we compare observatories present in our own collection from the university at Copenhagen, Denmark with two collections from the USA: one at the Woodman Library at Wisconsin-Madison and another at the Dudley Observatory in Loudonville, New York.
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Lawrence, J. S., M. C. B. Ashley y J. W. V. Storey. "Autonomous observatories for the Antarctic plateau". Proceedings of the International Astronomical Union 8, S288 (agosto de 2012): 6–14. http://dx.doi.org/10.1017/s1743921312016602.

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AbstractAntarctic astronomical site-testing has been conducted using autonomous self-powered observatories for more than a decade (the AASTO at South Pole, the AASTINO at Dome C, and PLATO at Dome A/Dome F). More recently autonomous (PLATO) observatories have been developed and deployed to support small-scale scientific instruments, such as HEAT, a 0.6 m aperture terahertz telescope at Ridge A, and AST3, a 0.5 m optical telescope array at Dome A. This paper reviews the evolution of autonomous Antarctic astronomical observatories, and discusses the requirements and implications for observatories that will be needed for future larger-scale facilities.
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Tesis sobre el tema "Astronomical observatories"

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Shepherd, Harry William. "Turbulence characterisation for astronomical observatories". Thesis, Durham University, 2012. http://etheses.dur.ac.uk/5891/.

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Atmospheric turbulence has two effects in astronomy; (i) the broadening of the point spread function due to phase fluctuations limiting the resolution of imaging and (ii) producing intensity fluctuations known as scintillation. Adaptive Optics (AO) can be installed on telescopes to correct for the effect of phase, and with the push to large telescopes more complex AO systems such as Multi Conjugate AO (MCAO) and Multi Object AO (MOAO) are desired. Operation of these systems requires a detailed profile of the turbulent atmosphere in real time. In this thesis we consider two turbulence profilers, SLOpe Detection And Ranging (SLODAR) and SCIntillation Detection and Ranging (SCIDAR), two cross beam profilers that retrieve data using covariance of phase variations (SLODAR) and intensity variations (SCIDAR). We present a modification of SLODAR to allow an estimate for non resolved turbulence to be made by considering scintillation in the subapertures of a Shack Hartmann wavefront sensor. A new SCIDAR (Stereo--SCIDAR) is described, allowing dynamic re--conjugation to improve altitude resolution. Practical considerations for the implementation of a SLODAR instrument are considered, including a discussion of potential false measurements of non Kolmogorov power spectra in the ground and surface layers of turbulence. Data is presented from SLODAR observing campaigns on La Palma, and at Paranal. Evidence is presented for orographic effects on measured turbulence, including those due to man made structures.
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Copley, Charles Judd. "Temperature dependence of the HartRAO pointing model". Thesis, Rhodes University, 2008. http://hdl.handle.net/10962/d1005277.

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This thesis investigates control aspects of the Hartebeeshoek Radio Astronomy Observatory (HartRAO) antenna. The installation of a new 22 GHz receiver has required the pointing accuracy to be improved to less than 4 mdeg. The effect of thermal conditions on the the HartRAO antenna pointing offset is investigated using a variety of modelling techniques including simple geometric modelling, neural networks and Principal Component Analysis (PCA). Convincing results were obtained for the Declination pointing offset, where applying certain model predictions to observations resulted in an improvement in Declination pointing offset from 5.5 mdeg to 3.2 mdeg (≈50%). The Right Ascension pointing model was considerably less convincing with an improvement of approximately from 5.5 mdeg to 4.5 mdeg (≈20%) in the Right Ascension pointing offset. The Declination pointing offset can be modelled sufficiently well to reduce the pointing offset to less than 4 mdeg, however further investigation of the underlying causes is required for the Right Ascension pointing offset.
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Kenyon, Suzanne Laura Physics Faculty of Science UNSW. "A universe of sky and snow: site-testing for optical astronomy at Dome C, Antarctica". Awarded by:University of New South Wales. Physics, 2007. http://handle.unsw.edu.au/1959.4/40822.

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The unique advantages for astronomy on the Antarctic plateau are now well established. In particular, Dome C, Antarctica is potentially one of the best new sites for optical, infrared and sub-millimeter astronomy, presenting the opportunity to build unique astronomical instruments. Located high on the Antarctic plateau, Dome C offers low wind, clear skies, and negligible precipitation. This thesis addresses three additional properties of the site relevant to optical astronomy-sky brightness, atmospheric extinction and optical turbulence. The sky at an optical astronomy site must be dark, and the atmosphere very clean with minimal light extinction. At present little is known from an astronomer's perspective about the optical sky brightness and atmospheric extinction at most Antarctic sites. The high latitude of Dome C means that the Sun spends a relatively small amount of time far below the horizon, implying longer periods of astronomical twilight and less optical dark time than other sites, especially those close to the equator. We review the contributions to sky brightness at high-latitude sites, and calculate the amount of usable dark time at Dome C. We also explore the implications of the limited sky coverage of high-latitude sites, and review optical extinction data from the South Pole. A proposal to extend the amount of usable dark time through the use of polarising filters is examined, and we present the design and calibration of an instrument (called Nigel) to measure the brightness, spectrum and temporal characteristics of the twilight and night sky. The atmospheric turbulence profile above an astronomical site limits the achievable resolution and sensitivity of a telescope. The atmospheric conditions above high plateau Antarctic sites are different to temperate sites; the boundary layer of turbulence is confined very close to the surface, and the upper atmosphere turbulence very weak. We present the first winter-time turbulence profiles of the atmosphere above Dome C, and characterise the site in terms of the achievable precision for photometry and astrometry, and the isoplanatic angle and coherence time for the adaptive optics.
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Kong, Yuk-ming Simon. "Redevelopment of the Hong Kong Observatory". Hong Kong : University of Hong Kong, 1994. http://sunzi.lib.hku.hk/hkuto/record.jsp?B2594678x.

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Pereira, Jose Miguel Oliveira Cardoso 1959. "Siting an astronomical observatory in an environmentally sensitive area: A multiple criteria location analysis". Thesis, The University of Arizona, 1987. http://hdl.handle.net/10150/276645.

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Mount Graham, in Southern Arizona supports valuable, ecological communities and at least one endangered species, the Mt. Graham red squirrel. The area is managed by the U.S. Forest Service. Elevation, dryness, sky clarity and freedom from light pollution at Mt. Graham make it a desirable site for astronomy. The University of Arizona presented a proposal to the Forest Service for the development of a multi-telescope observatory on the mountain. This has generated much controversy due to the opposition of environmentalists who fear the potential impacts of development on the mountain. Eleven potential sites for astrophysical development have been identified, with varying impacts on the ecosystem. They are ranked according to their suitability for development, using multiple criteria decision making techniques. The results are very consistent and robust, both within and across techniques and can be useful for decision support and conflict management purposes.
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Youthed, Andrew David. "Designing and implementing a new pulsar timer for the Hartebeesthoek Radio Astronomy Observatory". Thesis, Rhodes University, 2008. http://hdl.handle.net/10962/d1005243.

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This thesis outlines the design and implementation of a single channel, dual polarization pulsar timing instrument for the Hartebeesthoek Radio Astronomy Observatory (HartRAO). The new timer is designed to be an improved, temporary replacement for the existing device which has been in operation for over 20 years. The existing device is no longer reliable and is di±cult to maintain. The new pulsar timer is designed to provide improved functional- ity, higher sampling speed, greater pulse resolution, more °exibility and easier maintenance over the existing device. The new device is also designed to keeping changes to the observation system to a minimum until a full de-dispersion timer can be implemented at theobservatory. The design makes use of an 8-bit Reduced Instruction Set Computer (RISC) micro-processor with external Random Access Memory (RAM). The instrument includes an IEEE-488 subsystem for interfacing the pulsar timer to the observation computer system. The microcontroller software is written in assembler code to ensure optimal loop execution speed and deterministic code execution for the system. The design path is discussed and problems encountered during the design process are highlighted. Final testing of the new instrument indicates an improvement in the sam- pling rate of 13.6 times and a significant reduction in 60Hz interference over the existing instrument.
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Chin, Eu-Jeen. "High performance vibration isolation techniques for the AIGO gravitational wave detector". University of Western Australia. School of Physics, 2007. http://theses.library.uwa.edu.au/adt-WU2007.0159.

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[Truncated abstract] Interferometric gravitational wave detectors are being built around the world with continually improving measurement sensitivities. Noise levels from sources that are intrinsic to these detectors must be reduced to a level below the gravita- tional wave signal. Seismic noise in the low frequency range, which is within the gravitational wave detection bandwidth, is a concern for earth-based detectors. This thesis presents research and development of a high performance vibration isolation system that is designed to attenuate seismic noise. The final design will be used as part of a fully working interferometer at the Australian International Gravitational Observatory (AIGO). Pendulums and springs are conventionally used for the horizontal and vertical vibration isolation components respectively. A complete system comprises of a cascade of these components, each stage dramatically improving the level of isola- tion. The residual motion at the test mass level is thus reduced but is dominated by the normal mode resonances of the chain. A simple and effective method to reduce residual motion further is to add ultra-low frequency pre-isolation stages which suspend the chain. The Roberts Linkage is a relatively new and simple geometrical structure that is implemented in the pre-isolation stages. Here we present experimental results of improving isolation based on mathematical mod- elling. The attenuation of seismic noise in the vertical direction is almost as important as that in the horizontal direction, due to cross-coupling between the two planes. To help improve the vertical performance a lightweight Euler spring that stores no static energy was implemented into the AIGO suspension system. ... Theoretical and experimental results are presented and discussed. Currently the AIGO laboratory consists of two 80 m length arms. They are aligned along the east and south directions. One of AIGO's top priorities is the installation of two complete vibration isolators in the east arm to form a Fabry-Perot cavity. Assembling two suspension systems will enable more accurate performance measurements of the tuned isolators. This would significantly reduce the measurement noise floor as well as eliminate the seismic noise spectrum due to referencing with the ground motion. The processes involved in preparing such a task is presented, including clean room preparation, tuning of each isolator stage, and local control schematics and methods. The status of the AIGO site is also presented.
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江育明 y Yuk-ming Simon Kong. "Redevelopment of the Hong Kong Observatory". Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1994. http://hub.hku.hk/bib/B31982013.

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Pollard, Lloyd Wayne 1936. "Design of a flexure mount for optics in dynamic and cryogenic environments". Thesis, The University of Arizona, 1988. http://hdl.handle.net/10150/276741.

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The design of the flexure mount recently submitted to NASA Ames for the structural support of the primary mirror of the Space Infrared Telescope Facility (SIRTF) is presented. The flexure system must passively accommodate the differential thermal contraction between the glass mirror and the aluminum structure of the telescope during cryogenic cooldown. Further, it must support the one meter diameter, 116 kilogram (258 pound) primary mirror during a severe launch to orbit. Procedures used to establish the required radial compliance using computer programs NASTRAN and FRINGE are discussed. The parametric design program developed to study early concepts is presented. Methods of combining modal responses resulting from a displacement response spectrum analysis are discussed, and a combination scheme called MRSS, Modified Root of Sum of Squares, is presented. Modal combination schemes using MRSS, SRSS, and ABS are compared to the results of a Modal Frequency Response analysis.
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Lee, Benjamin H. "Advanced test mass suspensions and electrostatic control for AIGO". University of Western Australia. School of Physics, 2007. http://theses.library.uwa.edu.au/adt-WU2007.0187.

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This thesis presents the research done towards the development of the final mirror suspension stage for the high power test facility at AIGO, Western Australia. One of the goals of the facility is to test advanced suspension methods that may be useful in future gravitational wave detectors. An in depth study of current mirror suspension techniques is presented and areas of possible improvement are highlighted. The extension of an existing suspension modelling toolkit written in Mathematica is also presented, where added functions allow one to include the violin modes of a suspension into their analysis. Through this tool, new suspension geometries boasting a lower number of violin modes with lower Q factors where developed. The orthogonal ribbon suspension and the thin tube suspension boast a lower number of lower Q violin modes compared to typical ribbon suspensions. For the latter, a reduction in the number of violin modes below 5kHz down to 5 and peak thermal noise amplitude by approximately 30dB is predicted. Presented also is the affect that such suspension geometries have on pendulum mode dilution factor and overall suspension thermal noise. It is seen that the violin mode improvement comes at a cost of a small increase in thermal noise above approximately 50Hz. A theoretical analysis of the AIGO cavity locking control scheme is also given. Issues of sensor noise and dynamic range are considered to produce a possible hierarchical locking method that would be compatible with advanced detectors. The resulting actuator force range requirements for AIGO at each actuation location on the vibration isolation system are given. Requirements of local controls before achieving cavity lock are also discussed. Finally, the suspension of a dummy sapphire mirror using removable modular niobium ribbons is presented. The design and performance of an electrostatic actuator and sensor for suspended mirror control is given. Initial experimental results of positioning and control of the final stage suspension through a digital interface is also included.
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Libros sobre el tema "Astronomical observatories"

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Moore, Patrick, ed. Small Astronomical Observatories. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0.

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Moore, Patrick, ed. More Small Astronomical Observatories. London: Springer London, 2002. http://dx.doi.org/10.1007/978-1-4471-0213-7.

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Inc, World Book, ed. Observatories in space. Chicago, IL: World Book, 2010.

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Inc, World Book, ed. Observatories on Earth. Chicago: World Book, 2010.

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World Book, Inc. Observatories on Earth. Chicago: World Book, 2010.

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Mojzes, Imre. A kalocsai Haynald Obszervatórium története. Budapest: Magyar Tudományos Akadémia Csillagászati Kutató Intézete, 1986.

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Lukac, Marie R. List of active professional observatories. Washington, D.C: United States Naval Observatory, 2000.

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Hutchins, Roger. British university observatories, 1772-1939. Burlington, VT: Ashgate Pub. Co., 2007.

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Müller, Peter. Sternwarten in Bildern: Architektur und Geschichte der Sternwarten von den Anfängen bis ca. 1950. Berlin: Springer-Verlag, 1992.

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Paolantonio, Santiago. Uranometría argentina: Historia del Observatorio Nacional Argentino. Córdoba, Argentina: Universidad Nacional de Córdoba, Secretaría de Ciencia y Tecnología, Observatorio Astronómico, 2001.

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Capítulos de libros sobre el tema "Astronomical observatories"

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Powell, Jonathan. "Astronomical Observatories". En Astronomers' Universe, 163–214. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-31688-4_10.

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Mobberley, Martin. "Observatories". En Astronomical Equipment for Amateurs, 223–37. London: Springer London, 1999. http://dx.doi.org/10.1007/978-1-4471-0583-1_11.

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Allen, Dennis. "A Practical Roll-off Roof Observatory in Michigan, USA". En Small Astronomical Observatories, 1–12. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_1.

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Kitchin, C. R. "The University of Hertfordshire Observatory in Bayfordbury, England". En Small Astronomical Observatories, 93–102. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_10.

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Johnson, Ron. "An Amateur Observatory with a Glass Fibre Dome". En Small Astronomical Observatories, 103–14. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_11.

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Manning, B. G. W. "A Glass Fibre Dome for a 260mm, 1.9m Focal Length Reflecting Telescope". En Small Astronomical Observatories, 115–24. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_12.

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Sizer, A. J. "Chigwell School Observatory in Chigwell, England". En Small Astronomical Observatories, 125–34. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_13.

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Reid, David y C. Lintott. "The Torquay Boys’ Grammar School Observatory". En Small Astronomical Observatories, 135–43. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_14.

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Moore, Patrick. "Patrick Moore’s Observatory in Selsey, England". En Small Astronomical Observatories, 145–52. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_15.

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Newton, Jack. "A Deep-Sky Observatory". En Small Astronomical Observatories, 153–62. London: Springer London, 1996. http://dx.doi.org/10.1007/978-1-4471-0999-0_16.

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Actas de conferencias sobre el tema "Astronomical observatories"

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Rozelot, Jean-Pierre. "Lunar-based astronomical observatories". En Metal Mirrors, editado por Richard G. Bingham y David D. Walker. SPIE, 1993. http://dx.doi.org/10.1117/12.158740.

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Wainscoat, Richard, Ronald Theil y Robert Billingsley. "LIGHTING REQUIREMENTS NEAR ASTRONOMICAL OBSERVATORIES". En CIE 2017 Midterm Meetings and Conference on Smarter Lighting for Better Life. International Commission on Illumination, CIE, 2018. http://dx.doi.org/10.25039/x44.2017.po97.

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Colome, Josep, Pau Colomer, Josep Guàrdia, Ignasi Ribas, Jordi Campreciós, Thierry Coiffard, Lluis Gesa, Francesc Martínez y Florian Rodler. "Research on schedulers for astronomical observatories". En SPIE Astronomical Telescopes + Instrumentation, editado por Alison B. Peck, Robert L. Seaman y Fernando Comeron. SPIE, 2012. http://dx.doi.org/10.1117/12.926899.

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Johnson, Stewart W., Koon M. Chua, Jack O. Burns y Frederic A. Slane. "Lunar dust: implications for astronomical observatories". En Orlando '91, Orlando, FL, editado por Pierre Y. Bely y James B. Breckinridge. SPIE, 1991. http://dx.doi.org/10.1117/12.46725.

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Peterson, Karla A., Marty Eckert, Nancy R. Evans, Paul Hilton, Beth Perriello, Bryce A. Roberts, Evan Smith y Peg Stanley. "Coordinating multiwavelength campaigns between observatories". En Astronomical Telescopes and Instrumentation, editado por Peter J. Quinn. SPIE, 2000. http://dx.doi.org/10.1117/12.392503.

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Pinigin, Gennadiy, Magda Stavinschi, Vasile Mioc, Cristiana Dumitrache y Nedelia A. Popescu. "Bucharest-Nikolaev Astronomical Observatories’ Collaboration in Astronomy". En EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993704.

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Tordi, Massimiliano, Alessandro Colovini, Matteo Spinola, Francesco Rampini, Francois Dury y Cristina Battistel. "New scaling clamshells for distributed astronomical observatories". En Ground-based and Airborne Telescopes IX, editado por Heather K. Marshall, Jason Spyromilio y Tomonori Usuda. SPIE, 2022. http://dx.doi.org/10.1117/12.2630304.

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Emde, Peter y Pierre Chapus. "Operational support and service concepts for observatories". En SPIE Astronomical Telescopes + Instrumentation, editado por Alison B. Peck, Chris R. Benn y Robert L. Seaman. SPIE, 2014. http://dx.doi.org/10.1117/12.2056333.

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Kubánek, Petr, Alberto J. Castro-Tirado, Antonio de Ugarte Postigo, Ronan Cunniffe, Michael Prouza, Jan Štrobl, Hendrik van Heerden et al. "Operating a global network of autonomous observatories". En SPIE Astronomical Telescopes + Instrumentation, editado por Nicole M. Radziwill y Alan Bridger. SPIE, 2010. http://dx.doi.org/10.1117/12.857222.

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Walker, Arthur B. C., J. Gethyn Timothy, Richard B. Hoover y Troy W. Barbee. "Astronomical EUV/x-ray observatories on the moon". En Astrophysics from the Moon. AIP, 1990. http://dx.doi.org/10.1063/1.39321.

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Informes sobre el tema "Astronomical observatories"

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Galvis, H. D., D. Galeano y E. Quintero. Space Weather Monitoring from Observatorio Astronomico of the Universidad Tecnologica de Pereira. Balkan, Black sea and Caspian sea Regional Network for Space Weather Studies, marzo de 2020. http://dx.doi.org/10.31401/sungeo.2019.02.10.

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