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Thematische Bibliographien / IUCAA 2 M telescope

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Auswahl der wissenschaftlichen Literatur zum Thema „IUCAA 2 M telescope“

Autor: Grafiati

Veröffentlicht am 18. Mai 2024

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Zeitschriftenartikel zum Thema "IUCAA 2 M telescope"

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Srivastava, Mudit K., A. N. Ramaprakash, Hillol K. Das, Mahesh P. Burse, Pravin A. Chordia, Abhay A. Kohok und Chaitanya V. Rajarshi. „Design and development of an optical-fibre-based Integral Field Unit (IFU) on the IUCAA 2-m telescope“. Monthly Notices of the Royal Astronomical Society 418, Nr. 2 (20.10.2011): 1127–37. http://dx.doi.org/10.1111/j.1365-2966.2011.19560.x.

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2

Anandaram, Mandayam N., B. A. Kagali und S. P. Bhatnagar. „Design of a Small Automated Telescope for Indian Universities“. Transactions of the International Astronomical Union 24, Nr. 3 (2001): 303–6. http://dx.doi.org/10.1017/s0251107x00000973.

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AbstractWe have constructed a computer controlled telescope using a 0.36-m f/11 Celestron optical tube assembly for teaching and research applications. We have constructed a heavy duty fork-type equatorial mount fitted with precision machined 24 inch drive disks for both axes. These are friction driven by stepper motors through one inch rollers. We have used an open loop control system triggerable by an ST-4 CCD camera to acquire and track any target object. Our telescope can home in on any target within a range of two arc-minutes. We have employed a commercial stepper motor controller card for which we have written a user friendly pc based telescope control software in C. Photometry using a solid state photometer, and imaging by an ST-6 CCD camera are possible.We consider that this project is suitable for those wishing to construct some parts of a telescope and understand the principles of operation. A simpler model of this telescope could use DC motors instead of stepper motors. We shall be happy to send our design diagrams and details to those interested. This project was funded by the DST, and was assisted by IUCAA, Pune.

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Geyl, R., und H. Gashut. „A 2-m robotic telescope project“. Astronomische Nachrichten 325, Nr. 6-8 (Oktober 2004): 665–66. http://dx.doi.org/10.1002/asna.200410320.

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4

Takato, N., T. Ichikawa, F. Uraguchi, R. Lundock, C. Murata, Y. Taniguchi, H. Motoyama, K. Fukui und M. Taguchi. „A 2-m class Telescope at Dome Fuji“. EAS Publications Series 33 (2008): 271–74. http://dx.doi.org/10.1051/eas:0833038.

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5

Getov, R. G. „Photographic Surface Photometry of Bright Galaxies in the M 81 Group“. Symposium - International Astronomical Union 161 (1994): 594–95. http://dx.doi.org/10.1017/s0074180900048154.

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A programme for the surface photometry of bright galaxies has been underway at the Rozhen Observatory since 1991. In a series of papers we shall explore the optical morphology, photometric properties and some peculiarities suggestive of galaxy-galaxy interactions of the bright galaxies NGC 2976, NGC 3031, NGC 3034 and NGC 3077 in the M 81 group. Most of the plates were taken with the 2 m Rozhen Ritchey-Chrétien telescope, but at our disposal there are plates from the 6 m BTA and 2 m Tautenburg Schmidt telescope. Here we discuss some preliminary results for the optical morphology on the basis of two B-plates from the 2 m Tautenburg Schmidt telescope. It shows the edge-on like face of NGC 2976, the grand-designed spiral structure of NGC 3031 and the filament-jet peculiarities in NGC 3034 and NGC 3077.

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Mirzoyan, Razmick. „Status of the 17 m diameter MAGIC telescope“. European Physical Journal C 33, S1 (03.02.2004): s938—s940. http://dx.doi.org/10.1140/epjcd/s2004-03-1630-2.

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7

DENG Yong-ting, 邓永停, 李洪文 LI Hong-wen, 王建立 WANG Jian-li und 陈. 涛. CHEN Tao. „Main axes AC servo control system for 2 m telescope“. Optics and Precision Engineering 25, Nr. 1 (2017): 163–71. http://dx.doi.org/10.3788/ope.20172501.0163.

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8

Xia Peipei, 夏培培, 邓永停 Deng Yongting, 王志乾 Wang Zhiqian, 李洪文 Li Hongwen und 王显军 Wang Xianjun. „Model identification for K mirror turntable of 2 m telescope“. Infrared and Laser Engineering 47, Nr. 3 (2018): 318001. http://dx.doi.org/10.3788/irla201847.0318001.

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9

Silva-Cabrera, José Sergio, Joel Humberto Castro-Chacón, Mauricio Reyes-Ruiz, Matthew J. Lehner, Carlos Alberto Guerrero, Chung-Kai Huang, Fernando Iván Alvarez-Santana et al. „2018 August 15 stellar occultation by minor planet (134340) Pluto“. Monthly Notices of the Royal Astronomical Society 511, Nr. 4 (08.03.2022): 5550–59. http://dx.doi.org/10.1093/mnras/stac401.

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ABSTRACT We present photometric light curves of the stellar occultation event of the star UCAC4 341-187633 on 2018 August 15 by the minor planet (134340) Pluto. Photometric observations were carried out using the 2.1-m telescope at the San Pedro Mártir Observatory and the 1.3-m telescopes at Sites 2 and 3 of the Trans-Neptunian Automated Occultation Survey (TAOS II) project, and using a portable 0.4-m telescope from Bahía Asunción, Baja California Sur, Mexico. Different filters were used with the 2.1-m telescope and the TAOS II telescopes, whilst observations with the portable system were performed with no filter. The resulting light curves from the San Pedro Mártir Observatory show clear structures, with at least two bright spikes observed on ingress and one more observed on egress as the star traverses the atmosphere of the dwarf planet. The light curve from the portable telescope (440 km away) measured a longer duration for the occultation event, because the shadow of Pluto was observed at a lower latitude. Normalized light curves were created for the 2.1-m telescope, the Site 3 telescope of the TAOS II and the portable telescope. These normalized light curves show a difference in amplitude.

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Akabane, Kenji, Shozo Tsunekawa, Makoto Inoue, Ryohei Kawabe, Nagayoshi Ohashi, Osamu Kameya, Masato Ishiguro und Yoshiaki Sofue. „Millimeter-Wave Continuum Around NGC 7538-IRS1, IRS2, and IRS3“. International Astronomical Union Colloquium 140 (1994): 258–59. http://dx.doi.org/10.1017/s0252921100019692.

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Millimeter-wave continuum sources in NGC 7538 region were observed with the NRO 45-m telescope and Nobeyama Millimeter Array. NRO 45-m telescope observations showed that the compact region which includes IRS1, IRS2, and IRS3 has a strong millimeter-wave intensity excess, cf. figures 1, and 2.

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Dissertationen zum Thema "IUCAA 2 M telescope"

1

Paul, Jyotirmay. „Design and development of adaptive optics system in visible and near infra-red-band for IUCAA 2 M Telescope“. Thesis, University of North Bengal, 2019. http://ir.nbu.ac.in/handle/123456789/4041.

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Bücher zum Thema "IUCAA 2 M telescope"

1

Inter-University Centre for Astronomy and Astrophysics., Hrsg. The IUCAA telescope: A new technology telescope of 1.5 m diameter for use of the universities and colleges : a project report. Pune: [The Centre], 1995.

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Buchteile zum Thema "IUCAA 2 M telescope"

1

Stavrev, K. Y., und I. S. Barzova. „Direct-Photography Observations with the 2 M RCC Telescope at Nao-Rozhen: Catalogue of Plates and Archive-Data Analysis“. In Astronomy from Wide-Field Imaging, 371–75. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1146-1_79.

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2

„II. ESO, La Silla, the 3.6-m Telescope, Other Telescope Projects in Europe“. In Europe's Quest for The Universe, 25–42. EDP Sciences, 2020. http://dx.doi.org/10.1051/978-2-7598-0167-1.c006.

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3

„II. ESO, La Silla, the 3.6-m Telescope, Other Telescope Projects in Europe“. In Europe's Quest for The Universe, 25–42. EDP Sciences, 2020. http://dx.doi.org/10.1051/978-2-7598-0167-1-006.

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4

Smith, Victoria Anne, Graham Appleby, Marek Ziebart und Jose Rodriguez. „Twelve Years of High Frequency Absolute Gravity Measurements at the UK’s Space Geodesy Facility: Systematic Signals and Comparison with SLR Heights“. In International Association of Geodesy Symposia. Berlin, Heidelberg: Springer Berlin Heidelberg, 2021. http://dx.doi.org/10.1007/1345_2021_129.

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AbstractAbsolute gravity measurements taken on a near-weekly basis at a single location is a rarity. Twelve years of data at the UK’s Space Geodesy Facility (SGF) provides evidence to show that the application of results from international comparisons of absolute gravimeters should be applied to data and are critical to the interpretation of theSGF gravity time series of data from 2007 to 2019. Though residual biases in the data are seen. The SGF time series comprises near weekly data, with exceptions for manufacturer services and participation in international instrument comparisons. Each data set comprises hourly data taken over 1 day, with between 100 and 200 drops per hour. Environmental modelling indicates that the annual groundwater variation at SGFof some 2 m influences the gravity data by 3.1 μGal, based upon some measured and estimated soil parameters. The soil parameters were also used in the calculation of the effect of an additional telescope dome, built above the gravity laboratory, and have been shown to be realistic. Sited in close proximity to the long-established satellite laser ranging (SLR) system and the global navigation satellite systems (GNSS) the absolute gravimetry (AG) measurements provide a complimentary geodetic technique, which is non space-based. The SLR-derived height time series provides an independent measurement of vertical motion at the site which may be used to assess the AG results, which are impacted by ground motion as well as mass changes above and below the instruments.

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Konferenzberichte zum Thema "IUCAA 2 M telescope"

1

Shafer, David. „Rich man’s 2-m telescope“. In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1985. http://dx.doi.org/10.1364/oam.1985.thi2.

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At the last OSA annual meeting, I showed how the coma of a classical Cassegrain telescope can be fixed by adding a very weak meniscus lens next to the secondary mirror. The mirrors were not touched, so the design could be used with or without the lens in place. The distinctly less popular classical Gregorian telescope has a parabolic primary mirror and an elliptical concave secondary. This paper is about a simple way to fix both the coma and astigmatism of the Gregorian, again in such a way that the design can be used with or without the “fix” in place. Here, however, the “fix” is very small—a fraction of the secondary diameter. A small single lens is all that is added, in one version. A slightly more complex all-reflective component, equally small, is added in a different version. Performance numbers are given for a 2-m aperture example, with an f/1.5 primary mirror.

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2

Geyl, Roland, und Hadi Gashut. „A 2-m robotic telescope project“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Jacobus M. Oschmann, Jr. SPIE, 2004. http://dx.doi.org/10.1117/12.553805.

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3

Cui, Xiangqun, Yongheng Zhao, Yanan Wang und Guoping Li. „2-m LAMOST-type telescope for the Antarctic“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Larry M. Stepp. SPIE, 2006. http://dx.doi.org/10.1117/12.671265.

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4

Eaton, Joel A., und Michael H. Williamson. „Control of the TSU 2-m automatic telescope“. In SPIE Astronomical Telescopes + Instrumentation. SPIE, 2004. http://dx.doi.org/10.1117/12.549451.

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5

Medrano-Cerda, Gustavo A., Robert D. Lett und Paul Rees. „H-Infinity motion control system for a 2 m telescope“. In Astronomical Telescopes and Instrumentation, herausgegeben von J. Anthony Tyson und Sidney Wolff. SPIE, 2002. http://dx.doi.org/10.1117/12.457003.

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6

Aruga, T., T. Itabe, N. Hiromoto, W. S. Smith und J. E. Kimbrell. „Multipurpose 1.5-m telescope system“. In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1989. http://dx.doi.org/10.1364/oam.1989.tuu18.

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A new optical system with a 1.5-m diam telescope was designed and constructed in the CRL. The distinctive feature of the new telescope system is its flexibility as well as its capability for fast and accurate tracking. The system is flexible, that is, applicable to multiple studies. These are (1) satellite tracking (including geostationary satellites), (2) space optical communication, (3) laser ranging, (4) astronomy (IR/ visible), (5) laser radar, and (6) radiometry (remote sensing of planetary atmospheres). There are many foci, i.e., Nasmith (two), bent-Cassegrain (two), Cassegrain (usually not used due to tertiary mirror installation), and coude (instrument selection is avail able in four directions). Azimuth/elevation encoder resolution is 0.0001° and fast tracking (up to Az 15°/sec, El 5°/sec) is possible. The subsystems which have been integrated include a high sensitivity CCD camera and an image intensification tube camera for spacecraft tracking, point- ahead/fine-tracking assembly for space optical communication, 110-mJ/70-ps Nd:YAG laser for satellite ranging, 124 × 124 element IR camera and FT spectrometer for astronomy, and several CO2 and isotope lasers as well as heterodyne receiver for lidar and radiometer.

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Gomboc, Andreja. „Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope“. In INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP, 2005. http://dx.doi.org/10.1063/1.2130231.

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8

Staguhn, Johannes G., Dominic J. Benford, Christine A. Allen, S. Harvey Moseley, Elmer H. Sharp, Troy J. Ames, Walter Brunswig et al. „GISMO: a 2-millimeter bolometer camera for the IRAM 30 m telescope“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Jonas Zmuidzinas, Wayne S. Holland, Stafford Withington und William D. Duncan. SPIE, 2006. http://dx.doi.org/10.1117/12.671970.

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9

Zhao, Fu, Ping Wang, Yuejin Zhao, Li Zhang, Hongbing Xin und Liang Lv. „Finite element analysis of the mirror room of the 2-m telescope“. In 2nd International Symposium on Advanced Optical Manufacturing and Testing Technologies, herausgegeben von Yudong Zhang, Wenhan Jiang und Myung K. Cho. SPIE, 2006. http://dx.doi.org/10.1117/12.674108.

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10

Moiseev, A. S., M. Yu Fokin und V. V. Komarov. „Power Supply at the Nasmyth-2 Focus of the 6-m Telescope“. In Groud-Based Astronomy in Russia. 21st Century. Специальная астрофизическая обсерватория РАН, 2020. http://dx.doi.org/10.26119/978-5-6045062-0-2_2020_123.

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