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Academic literature on the topic 'And Astronomical Observations'

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Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "And Astronomical Observations"

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Street, R. "Astronomical observations." Physics World 3, no. 5 (May 1990): 15. http://dx.doi.org/10.1088/2058-7058/3/5/11.

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Nikolov, A. S. "An Application of Personal Computers in Astronomy Education." International Astronomical Union Colloquium 105 (1990): 177–78. http://dx.doi.org/10.1017/s0252921100086668.

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Observations play an important role in the process of teaching astronomical knowledge. Practical observations of astronomical phenomena lead to analysis and explanation based on natural laws and so form the basis of cognitive processes in the education. Evidently the observations are an integral part of acquiring astronomical knowledge. Giving up observations, no matter what the reasons, is equivalent to losing quality in the educational process. It decreases the possible influence over the personal development of pupils and students. At the same time, observation and observational results are important for success in education.Carefully planned observational time has a substantial influence on cognitive and educational processes. It leads to considerably more active participation in astronomy lectures.
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Walker, Gordon, Pierre Léna, Daniel J. Schroeder, and Joseph S. Miller. "Astronomical Observations: An Optical Perspective and Observational Astrophysics and Astronomical Optics." Physics Today 42, no. 3 (March 1989): 97. http://dx.doi.org/10.1063/1.2810932.

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Zhang, X. Z., and J. H. Wu. "IPS Observations at Beijing Astronomical Observatory." Highlights of Astronomy 12 (2002): 398. http://dx.doi.org/10.1017/s1539299600013903.

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The radio wave from distant radio sources will be scattered by the irregular structures of the solar wind plasma when propagating through the interplanetary space, resulting into a randomly fluctuating pattern of the radio wave in observation. This pattern is called interplanetary scintillation (IPS). Observation on IPS can give information of the solar wind speed and irregular structures in solar wind plasma. The IPS observations began at Miyun Station, Beijing Astronomical Observatory from the late half of 1999. The properties of the telescope and description of the data analysis can be found in the papers of Wang (1987) and Wu, Zhang and Zheng (2000) respectively.Table 1 summarizes some observational results using IPS source 3C48 in April and May 2000. The Fresnel knees and the first minima in the IPS spectra were used to estimate solar wind speeds. Comparisons of our results with the unpublished data of Hiraiso Solar Terrestrial Research Center obtained from their web site, have been done and good agreement between the two systems was found. Since the collecting area of Miyun telescope is limited, the system noise is relatively high and dominates the high-frequency parts of the spectra. The Miyun IPS observation and data reduction procedures are still under developing and will soon be completed.
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Edberg, Stephen J. "Working with Amateur Astronomers." International Astronomical Union Colloquium 98 (1988): 95–99. http://dx.doi.org/10.1017/s0252921100092307.

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Amateur astronomers have a vast store of talent and expertise in making astronomical observations. When carefully channelled, their enthusiasm coupled with these characteristics can lead to the acquisition of large volumes of high-quality astronomical data. The Amateur Observation Network of the International Halley Watch (IHW) was organized to encourage comet observations by amateurs, standardize techniques whenever possible, and then collect and archive these observations for use by the astronomical community in the near and distant future as part of the whole IHW archive. The lessons learned from this experience will be useful to organizers who plan observation campaigns involving amateur astronomers in the future.
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Klioner, S. A. "Relativistic astrometry and astrometric relativity." Proceedings of the International Astronomical Union 3, S248 (October 2007): 356–62. http://dx.doi.org/10.1017/s174392130801956x.

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AbstractThe interplay between modern astrometry and gravitational physics is very important for the progress in both these fields. Below some threshold of accuracy, Newtonian physics fails to describe observational data and the Einstein's relativity theory must be used to model the data adequately. Many high-accuracy astronomical techniques have already passed this threshold. Moreover, modern astronomical observations cannot be adequately modeled if relativistic effects are considered as small corrections to Newtonian models. The whole way of thinking must be made compatible with relativity: this starts with the concepts of time, space and reference systems.An overview of the standard general-relativistic framework for modeling of high-accuracy astronomical observations is given. Using this framework one can construct a standard set of building blocks for relativistic models. A suitable combination of these building blocks can be used to formulate a model for any given type of astronomical observations. As an example the problem of four dimensional solar system ephemerides is exposed in more detail. The limits of the present relativistic formulation are also briefly summarized.On the other hand, high-accuracy astronomical observations play important role for gravitational physics itself, providing the latter with crucial observational tests. Perspectives for these astronomical tests for the next 15 years are summarized.
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Šprajc, Ivan. "Astronomical aspects of Group E-type complexes and implications for understanding ancient Maya architecture and urban planning." PLOS ONE 16, no. 4 (April 27, 2021): e0250785. http://dx.doi.org/10.1371/journal.pone.0250785.

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In the 1920s, during the first archaeological excavations at Uaxactún, Petén, Guatemala, an architectural complex named Group E was interpreted as an ancient Maya astronomical observatory, intended specifically for sighting the equinoctial and solstitial sunrises. In the following decades, a large number of architectural compounds with the same configuration have been found, most of them in the central lowlands of the Yucatan peninsula. The multiple hypotheses that have been proposed about the astronomical function of these complexes, commonly designated as E Groups, range from those attributing them a paramount role in astronomical observations to those that consider them merely allegorical or commemorative allusions to celestial cycles, without any observational use. This study, based on quantitative analyses of a reasonably large sample of alignment data, as well as on contextual evidence, shows that many of the previous hypotheses cannot be sustained. I argue that E Groups, although built primarily for ritual purposes, were astronomically functional, but also that they had no specific or particularly prominent role in astronomical observations. Their orientations belong to widespread alignment groups, mostly materialized in buildings of other types and explicable in terms of some fundamental concerns of the agriculturally-based Maya societies. I present the evidence demonstrating that the astronomical orientations initially embedded in E Groups, which represent the earliest standardized form of Maya monumental architecture and whose occurrence in practically all early cities in the central Yucatan peninsula attests to their socio-political significance, were later transferred to buildings and compounds of other types. Therefore, it is precisely the importance of the astronomically and cosmologically significant directions, first incorporated in E Groups, that allows us to understand some prominent aspects of ancient Maya architecture and urbanism.
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Millis, Robert L. "Astronomical observations—an optical perspective." Icarus 74, no. 2 (May 1988): 374–75. http://dx.doi.org/10.1016/0019-1035(88)90052-8.

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Garcia-Piquer, A., J. C. Morales, I. Ribas, J. Colomé, J. Guàrdia, M. Perger, J. A. Caballero, et al. "Efficient scheduling of astronomical observations." Astronomy & Astrophysics 604 (August 2017): A87. http://dx.doi.org/10.1051/0004-6361/201628577.

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Patris, J., and A. Sarkissian. "Astronomical observations with OHP telescopes." Journal de Physique IV (Proceedings) 139, no. 1 (December 2006): 373–90. http://dx.doi.org/10.1051/jp4:2006139024.

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Dissertations / Theses on the topic "And Astronomical Observations"

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Tshenye, Thapelo Obed. "Quality control of astronomical CCD observations." Master's thesis, University of Cape Town, 2007. http://hdl.handle.net/11427/4409.

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Eves, Benjamin Alistair Curtis. "Observations of magnetically driven events in astronomical systems." Thesis, Open University, 2005. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.434234.

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Martin, Didier Dieudonné Elisabeth. "Development of superconducting tunnel junction arrays for astronomical observations." Enschede : University of Twente [Host], 2007. http://doc.utwente.nl/58049.

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Spreitzer, Teresa. "Construction and operation of a cloud detector to assist astronomical observations." Thesis, McGill University, 2003. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=80879.

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The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a ground based gamma ray telescope which studies active galatic nuclei (AGNs). As a ground based experiment, data quality is directly related to atmospheric conditions. This thesis describes the process of verifying the reliability of astronomical weather predictions made by the Canadian Meteorological Service (CMS). This includes a description of the construction, calibration, and operation of a cloud detector at McGill University in Montreal, Canada. Cloud cover data was collected from the beginning of September, 2003, to the beginning of November 2003. These data were compared to cloud cover weather predictions made by the CMS. A blind analysis consisted of scaling the CMS and real data, and calculating the correlation coefficient between these two sets of data. The correlation between the predictions and real sky conditions was 0.4622, well above the 0.1% significance level of 0.1906 Thus the CMS is determined to be a reliable weather predictor, and useful to the STACEE group.
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Hepworth, James Haydn. "Systems Development of a Two-Axis Stabilised Platform to Facilitate Astronomical Observations." Master's thesis, University of Cape Town, 2018. http://hdl.handle.net/11427/29449.

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Inertially Stabilised Platforms (ISPs) aim to control the line-of-sight between a sensor and a target. They perform two distinct operations; keeping track of the target as the sensor host and the target move in inertial space and attenuating rotational disturbances incurred to the sensor by host vehicle motion. This project aimed to develop a two-axis ISP for use in astronomical applications. It represents the initial development of all systems of a low-cost ISP designed for a 3.5” compound telescope. To achieve this, relevant literature describing the various components of an ISP were reviewed to inform the design, implementation and testing cycle which comprised most of the project. A set of system specifications was developed to guide design decisions. The performance of the implemented system was compared against these specifications once the project was complete. During the project, the electro-mechanical structure of the ISP was designed and implemented, including a mechanical assembly designed to mount a camera and inertially and geometrically model the specified telescope. This allowed the ISP to be tested at a lower cost than with the telescope itself. The associated electrical systems were specified and configured. An image processing script capable of detecting and locating the centre of the Moon in the camera field of view was written in Python and implemented on a Raspberry Pi Computer. A complete simulation model for the system was written in the simulation language, Simul_C_EM, and used to design various controllers for the ISP control system and help verify certain estimated system parameters such as gimbal friction. For each gimbal, PI controllers were designed to allow manual orientation control of the telescope, compensated P controllers were designed to achieve target tracking, and compensated PI controllers were designed to reject rotational disturbances. These were implemented in C on an STM32F0 microcontroller tasked with managing the various control and communications tasks required by the system. Finally, a user interface was written in LabVIEW to facilitate intuitive user control of the system and perform datalogging of the system runtime data. Testing of the system showed good correlation between the hardware and the simulated results indicating an accurate simulation model that can be used to test future design developments.
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Travouilon, Tony Physics Faculty of Science UNSW. "Measurements of optical turbulence on the Antarctic Plateau and their impact on astronomical observations." Awarded by:University of New South Wales. Physics, 2005. http://handle.unsw.edu.au/1959.4/20852.

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Atmospheric turbulence results taken on the Antarctic plateau are presented in this thesis. Covering two high sites: South Pole and Dome C, this work describes their seeing and meteorological conditions. Using an acoustic sounder to study the turbulence profile of the first kilo- metre of the atmosphere and a Differential Image Motion Monitor (DIMM) to investigate the integrated seeing we are able to deduce important at- mospheric parameters such as the Fried parameter (r0) and the isoplanatic angle (??0). It was found that at the two sites, the free atmosphere (above the first kilometer) was extremely stable and contributed between 0.2" and 0.3" of the total seeing with no evidence of jet or vortex peaks of strong turbulence. The boundary layer turbulence is what differentiates the two sites. Located on the Western flank of the plateau, the South Pole is prone to katabatic winds. Dome C on the other hand is on a local maximum of the plateau and the wind conditions are amongst the calmest in the world. Also linked to the topography is the vertical extent of the temperature in- version that is required to create optical turbulence. At the South Pole the inversion reaches 300 m and only 30 m at Dome C. This difference results in relatively poor seeing conditions at the South Pole (1.8") and excellent at Dome C (0.27"). The strong correlation between the seeing and the ground layer meteorological conditions indicates that even better seeing could be found at Dome A, the highest point of the plateau. Having most of the turbulence near the ground is also incredibly ad- vantageous for adaptive optics. The isoplanatic angle is respectively 3.3" and 5.7" for the South Pole and Dome C. This is significantly larger than at temperate sites where the average isoplanatic angle rarely exceeds 2". This means that wider fields can be corrected without the complication of conjugation to specific layers. For such purpose the potential is even more interesting. We show that ground conjugated adaptive optics would decrease the natural seeing to 0.22" for a wide field of 10 and 0.47" for a field of 1" at the South Pole. At Dome C the results are less impressive due to the already excellent seeing, but a gain of 0.1"e can still be achieved over 1"e. These results show that high angular resolution observations can be done better on the Antarctic plateau than any other known site.
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Carvalho, Fernando Pedro. "'Powellsnakes' : a fast Bayesian approach to discrete object detection in multi-frequency astronomical data sets." Thesis, University of Cambridge, 2014. https://www.repository.cam.ac.uk/handle/1810/245147.

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In this work we introduce a fast Bayesian algorithm designed for detecting compact objects immersed in a diffuse background. A general methodology is presented in terms of formal correctness and optimal use of all the available information in a consistent unified framework, where no distinction is made between point sources (unresolved objects), SZ clusters, single or multi-channel detection. An emphasis is placed on the necessity of a multi-frequency, multi-model detection algorithm in order to achieve optimality. We have chosen to use the Bayes/Laplace probability theory as it grants a fully consistent extension of formal deductive logic to a more general inferential system with optimal inclusion of all ancillary information [Jaynes, 2004]. Nonetheless, probability theory only informs us about the plausibility, a ‘degree-of-belief ’, of a proposition given the data, the model that describes it and all ancillary (prior) information. However, detection or classification is mostly about making educated choices and a wrong decision always carries a cost/loss. Only resorting to ‘Decision Theory’, supported by probability theory, one can take the best decisions in terms of maximum yield at minimal cost. Despite the rigorous and formal approach employed, practical efficiency and applicability have always been kept as primary design goals. We have attempted to select and employ the relevant tools to explore a likelihood form and its manifold symmetries to achieve the very high computational performance required not only by our ‘decision machine’ but mostly to tackle large realistic contemporary cosmological data sets. As an illustration, we successfully applied the methodology to ESA’s (European Space Agency) Planck satellite data [Planck Collaboration et al., 2011d]. This data set is large, complex and typical of the contemporary precision observational cosmology state-of-the-art. Two catalogue products are already released: (i) A point sources catalogue [Planck Collaboration et al., 2011e], (ii) A catalogue of galaxy clusters [Planck Collaboration et al., 2011f]. Many other contributions, in science products, as an estimation device, have recently been issued [Planck et al., 2012; Planck Collaboration et al., 2011g,i, 2012a,b,c]. This new method is called ‘PowellSnakes’ (PwS).
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Isaak, Katherine Gudrun. "Low-noise instrumentation and astronomical observations of high-redshift objects in submillimetre wavelengths." Thesis, University of Cambridge, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.364389.

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Rojas, Folkers Eduardo. "Evaluation, design, and construction of the Wallace Astrophysical Observatory Camera for astronomical observations." Thesis, Massachusetts Institute of Technology, 2009. http://hdl.handle.net/1721.1/54464.

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Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Nuclear Science and Engineering, June 2009.
"May 2008." Cataloged from PDF version of thesis.
Includes bibliographical references (p. 53-54).
The goal of this thesis is to upgrade the scientific capabilities of the 24" Cassegrain reflector telescope at the George R. Wallace, Jr. Astrophysical Observatory (Wallace Observatory), part of Massachusetts Institute of Technology (MIT). The upgrade consists of evaluating, designing and constructing the Wallace Astrophysical Observatory Camera (WAOcam), optimized for 24" telescope. A full 3D model of the 24" telescope and dome was created to find the size restrictions for WAOcam. An optical model was also developed to maximize the field of view of the camera detector. WAOcam was designed using SolidWorks (3D modeling Software), the parts files from the designing process were also used to machine the instrument. The manufacturing of the WAOcam involved using the following: Computer Numerical Control (CNC) lathe, CNC mill, drill press, and a Waterjet (cutting machine). The manufacturing process also required learning of Omax (software for the Waterjet) and MasterCam 9.1 (software for the CNC lathe and CNC mill). The resulting product is WAOcam, which consists of three modules: 1) vacuum dewar (houses a CCD detector), 2) shutter (controls when light hits the camera detector), and 3) filter wheel (modifies the light before hitting the detector). The remaining work left on the WAOcam is the installation of two additional modules: 1) a four port instrument rotator and 2) a field rotator. This upgrade will allow for occultation observations, strip scanning surveys, and Kuiper Belt Object (KBOs) astrometry to be obtained using the 24" telescope.
by Folkers Eduardo Rojas.
S.B.
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PENNING, WILLIAM ROY. "INVESTIGATIONS OF LONG-PERIOD DQ HERCULIS STARS." Diss., The University of Arizona, 1986. http://hdl.handle.net/10150/188161.

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The magnetic rotator model has long been the favored explanation for coherent photometric modulations in the DQ Herculis class of cataclysmic variables. However, to date, all evidence supporting this model has been of the indirect variety. Unlike their synchronously rotating cousins, the AM Herculis objects, DQ Herculis stars have not yet been discovered to emit polarized radiation. Therefore, in light of this crucial lack, the evidence used to place these objects in the magnetic cataclysmic variable category has been strictly circumstantial, based primarily on the coherence of the photometric periodicities. In this work, time-resolved spectroscopy of four long-period DQ Herculis stars is performed. In addition, two of the same objects are observed with a new, sensitive circular polarimeter. Chapters II and III describe these observations and the results of each. To summarize, coherent variations in the wavelength of emission lines were found with the spectroscopic observations. A model is put forth, explaining this phenomenon as being due to varying illumination from a bright spot on the primary. This, of course, adds strength to the magnetic rotator model. Secondly, circular polarization was definitely found in one object studied, and possibly in a second. Therefore, for the first time, there is direct evidence of the magnetic nature of these binaries. In Chapter IV, the model of the rotating bright spot illuminating the disk is explored in further detail, including modeling with a minicomputer. Afterward, a problem brought out by the low polarization coupled with large amplitude photometric variations and a cool spectrum is investigated, namely, is it possible to produce large amounts of cyclotron radiation without producing large amounts of circular polarization? The results tend to show that, for a large emitting area, the answer is yes. Chapter V is a summary of the rest of the work.
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Books on the topic "And Astronomical Observations"

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Walker, Gordon. Astronomical observations: An optical perspective. Cambridge: Cambridge University Press, 1987.

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Astronomical observations: An optical perspective. Cambridge [Cambridgeshire]: Cambridge University Press, 1987.

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Appenzeller, I., H. J. Habing, and P. Léna, eds. Evolution of Galaxies Astronomical Observations. Berlin, Heidelberg: Springer Berlin Heidelberg, 1989. http://dx.doi.org/10.1007/3-540-51315-9.

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Polarization of light and astronomical observations. Amsterdam: Gordon & Breach, 2000.

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Dobbins, Thomas A. Introduction to observing and photographing the solar system. Richmond, Va., U.S.A: Willmann-Bell, 1988.

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Meteorological, astronomical, and seismological observations from ancient Korea. Seoul: Korea Meteorological Administration, 2013.

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Astronomical observations: Astronomy and the study of deep space. New York, NY: Britannica Educational Pub. in association with Rosen Education Services, 2010.

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Rendtel, Jürgen. Handbook for photographic meteor observations. Potsdam: International Meteor Organization, 1993.

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Marett-Crosby, Michael. Twenty-Five Astronomical Observations That Changed the World. New York, NY: Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-6800-4.

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Observational astrophysics. 3rd ed. Heidelberg: Springer, 2012.

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Book chapters on the topic "And Astronomical Observations"

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Pearse, Colonel Thomas D. "Astronomical Observations." In Representing India, 57–121. London: Routledge, 2023. http://dx.doi.org/10.4324/9781003101789-2.

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Ciyuan, Liu. "Historical Chinese Astronomical Observations." In Earth’s Rotation from Eons to Days, 27–32. Berlin, Heidelberg: Springer Berlin Heidelberg, 1990. http://dx.doi.org/10.1007/978-3-642-75587-3_4.

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Ziółkowski, Mariusz, and Jacek Kościuk. "Astronomical Observations at Machu Picchu: Facts, Hypothesis and Wishful Thinking." In Machu Picchu in Context, 167–236. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-92766-0_5.

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AbstractThe aim of this text has been the evaluation of the hypotheses, formulated by various authors, on the possible astronomical function of seven structures and architectural ensembles located in the Llaqta of Machu Picchu and its immediate vicinity: the Temple of the Sun, the Room of the Mortars, the cave of Intimachay, the Temple of Condor, the Intihuatana, the Mirador de Inkaraqay, the River Intihuatana as well as the site of Llactapata. Apart from the Room of the Mortars, whose astronomical function was revealed to be dubious, the remaining six ensembles present well-documented evidence of astronomical alignments, with a marked preference for orientations towards sunrise on the June Solstice, and the demarcation of a fixed number of days around this phenomenon. Two structures, namely Intimachay and the Mirador de Inkaraqay, meet instrument requirements for precision observations, but of different types. The latter structure, provided with two observation tubes, a unique case in Inca architecture, seems to have been designed for observations of the Pleiades and Venus at its maximum elongation, in the frame of a multiannual cycle. Intimachay, on the other hand, was used for observations of the cycles of the Sun and the Moon.
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Escribano, Rafael, and Guillermo M. Muñoz Caro. "Introduction to Spectroscopy and Astronomical Observations." In Laboratory Astrophysics, 27–47. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-90020-9_3.

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Kimeswenger, S., and C. Kienel. "Strategy of Denis Observations." In Science with Astronomical Near-Infrared Sky Surveys, 23–24. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0946-8_4.

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Kaspi, V. M. "Observations of Millisecond Pulsars on Time Scales from 10 Nanoseconds to 10 Years." In Astronomical Time Series, 25–36. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-015-8941-3_3.

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Boisson, C. "Near-Infrared Observations of AGN." In Science with Astronomical Near-Infrared Sky Surveys, 233–36. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0946-8_49.

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Strano, Giorgio. "Galileo’s telescope: history, scientific analysis, and replicated observations." In 400 Years of Astronomical Telescopes, 15–29. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-90-481-2233-2_2.

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Sarre, Peter J. "Observations of PAHs and Nanodiamonds with UKIRT." In Thirty Years of Astronomical Discovery with UKIRT, 207–12. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7432-2_19.

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Tanvir, Nial. "Observations of Gamma-Ray Bursts at UKIRT." In Thirty Years of Astronomical Discovery with UKIRT, 259–68. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7432-2_24.

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Conference papers on the topic "And Astronomical Observations"

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Jones, Lewis R., J. E. Spragg, and B. M. Smith. "Automated scheduling of astronomical observations." In 1994 Symposium on Astronomical Telescopes & Instrumentation for the 21st Century, edited by David L. Crawford and Eric R. Craine. SPIE, 1994. http://dx.doi.org/10.1117/12.176785.

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Franchini, Mariagrazia, and Carlo Morossi. "Modeling of spectroscopic astronomical observations." In 1994 Symposium on Astronomical Telescopes & Instrumentation for the 21st Century, edited by David L. Crawford and Eric R. Craine. SPIE, 1994. http://dx.doi.org/10.1117/12.176802.

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Ebizuka, N., T. Okamoto, M. Takeda, T. Hosobata, Y. Yamagata, M. Sasaki, T. Kamizuka, et al. "Novel gratings for astronomical observations." In International Conference on Space Optics - ICSO 2018, edited by Nikos Karafolas, Zoran Sodnik, and Bruno Cugny. SPIE, 2019. http://dx.doi.org/10.1117/12.2536144.

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Noordam, Jan E. "Self-calibration of radio astronomical observations." In Astronomical Telescopes and Instrumentation, edited by Harvey R. Butcher. SPIE, 2000. http://dx.doi.org/10.1117/12.390429.

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Ueno, Munetaka. "PtSi infrared camera for astronomical observations." In Aerospace/Defense Sensing and Controls, edited by Bjorn F. Andresen and Marija S. Scholl. SPIE, 1996. http://dx.doi.org/10.1117/12.243452.

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Ebizuka, Noboru, Takayuki Okamoto, Yutaka Yamagata, Minoru Sasaki, Ichi Tanaka, Takashi Hattori, Yusuke Nakauchi, et al. "Novel gratings for astronomical observations II." In International Conference on Space Optics — ICSO 2021, edited by Zoran Sodnik, Bruno Cugny, and Nikos Karafolas. SPIE, 2021. http://dx.doi.org/10.1117/12.2600051.

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Haig, Douglas J., Peter A. R. Ade, James E. Aguirre, James J. Bock, Samantha F. Edgington, Melissa L. Enoch, Jason Glenn, et al. "Bolocam: status and observations." In SPIE Astronomical Telescopes + Instrumentation, edited by Jonas Zmuidzinas, Wayne S. Holland, and Stafford Withington. SPIE, 2004. http://dx.doi.org/10.1117/12.553154.

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Klvaňa, Miroslav, Michal Sobotka, and Michal Švanda. "Optimisation of solar synoptic observations." In SPIE Astronomical Telescopes + Instrumentation, edited by Alison B. Peck, Robert L. Seaman, and Fernando Comeron. SPIE, 2012. http://dx.doi.org/10.1117/12.925317.

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Goodwin, Michael, Charles Jenkins, Peter Conroy, and Andrew Lambert. "Observations of ground-layer turbulence." In SPIE Astronomical Telescopes + Instrumentation, edited by Norbert Hubin, Claire E. Max, and Peter L. Wizinowich. SPIE, 2008. http://dx.doi.org/10.1117/12.787732.

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Ma, Yongzheng, Xiaomeng Lu, Zhengyi Shao, Hongwei Yang, and Kai Nan. "Towards a collaboration cloud for astronomical observations." In 2012 IEEE 2nd International Conference on Cloud Computing and Intelligence Systems (CCIS). IEEE, 2012. http://dx.doi.org/10.1109/ccis.2012.6664422.

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Reports on the topic "And Astronomical Observations"

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McAlister, Harold A. Astronomical Observations by Speckle Interferometry. Fort Belvoir, VA: Defense Technical Information Center, June 1986. http://dx.doi.org/10.21236/ada170069.

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Dundon, Luke R. Physical Properties of Near-Earth Objects: Optical and Infrared Astronomical Observations. Fort Belvoir, VA: Defense Technical Information Center, April 2003. http://dx.doi.org/10.21236/ada416078.

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Frohlich, Carla. The Origin of Chemical Elements: Connecting Laboratory Nuclear Astrophysics with Astronomical Observations through Nucleosynthesis Modeling. Office of Scientific and Technical Information (OSTI), February 2019. http://dx.doi.org/10.2172/1496039.

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