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1. First CCD Observations of Asteroids from Armagh
... Down), have conducted astrometric observations of main-belt and near-Earth asteroids using the Observatory's ST-7 CCD camera attached to the Armagh Planetarium's 10-inch Meade Schmidt-Cassegrain telescope. Three main-belt asteroids were observed, namely (304)Olga, (849)Ara and (1146)Biarmia. ... It is believed that these observations were also the first Earth-approaching near-Earth asteroid to be observed with the Faulkes Telescope (see http://star.arm.ac.uk/press/2000PH5.html). ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2004/node20.html -- 6.0 Кб -- 19.04.2005
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2. Australia-Japan Collaborative Workshops
... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Australia Telescope Online Archive (ATOA) . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/projects/mnrf1996/austjap.html -- 48.3 Кб -- 08.04.2016
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3. http://www.naic.edu/vscience/schedule/2015Spring/FonsecatagP2945.pdf
Proposal Identification No.: ... Begin ­ End Interval­Interval 00:00 ­ 01:00 15:30 ­ 16:30 16:30 ­ 17:30 20:00 ­ 21:00 Days Needed at This Interval 26 26 26 26 2 Time Constraints (Must Be Justified in the Prop osal Text) As we discuss in our attached proposal, we prefer to observe five radio pulsars, each for one hour per observing epoch, for 26 epochs during each semester for each source or 52 epochs for the whole observing year (52 x 5 = 260 hours total for all five sources). ...
[ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/2015Spring/FonsecatagP2945.pdf -- 62.5 Кб -- 09.09.2014
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4. Astrophysical Research Consortium Small Aperture Telescope
The Astrophysical Research Consortium Small Aperture Telescope (ARCSAT) is a 0.5-m (or 20") Classical Cassegrain telescope, formerly known as the SDSS Photometric Telescope (PT). ... Chief Telescope Engineer : Bill Ketzeback (bketzeba/apo.nmsu.edu) . Remote Operations Upgrade Project Manager : Joe Huehnerhoff (jwhueh/apo.nmsu.edu) . ... SurveyCam PI : Dmitry Bizyaev (dmbiz/apo.nmsu.edu) . FlareCam PI : Joe Huehnerhoff ( jwhueh/apo.nmsu.edu ) . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/index.html -- 4.9 Кб -- 09.01.2015
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5. The SMS Survey
... The SMS program is a critical endeavor to investigate whether the predictions of standard cold dark matter cosmology are consistent with the observed matter distribution in the Milky Way halo. It is the deepest, most extended search for optically elusive dwarf satellite galaxies and tidal streams to date, covering the entire Southern hemisphere. ... However only a few dwarf satellites have been found around the Milky Way to date - 22 dwarfs compared to 500-10,000 predicted by theory (Klypin et al. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/SMS_Survey.html -- 12.0 Кб -- 09.04.2016
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6. ESO - Observing Facilities
... Science . ... Science Users Information > Observing Facilities . ... La Silla Paranal Observatory . ... Paranal Telescopes . ... Observing with ESO Telescopes . ... Today, ESO operates the La Silla Paranal Observatory , providing some of the world's largest and most advanced observational facilities at three sites in Northern Chile: La Silla, Paranal and Chajnantor. ... ESO operates three major telescopes (3.6m telescope, New Technology Telescope (NTT), 2.2m Max-Planck-ESO telescope) at La Silla. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/facilities.html -- 30.0 Кб -- 09.04.2016
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7. Galaxy sector, archive 2012
... Contacts . 2012: . ... We refined the fundamental parameters of the components, the orbital periods, and the conditions of photospheric heating of the secondary component by the ultraviolet radiation of the hot component. ... The observations of the star clusters associated with ultra-luminous x-ray sources (ULXs) in four galaxies on the 6-meter and VLT telescopes have shown that all the ULXs are located within 200pc of very young star clusters (younger than 5 million years). ... Archive . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/Science/results/ar_galaxy/res2012.html -- 11.1 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/Science/results/ar_galaxy/res2012.html -- 11.1 Кб -- 10.04.2016
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8. http://www.astro.louisville.edu/information/asa2007.pdf
Brad Carter, Carolyn Brown, Rhodes Hart Drew Foster, John Kielkopf, Ron Moore University of Southern Queensland, Australia University of Louisville, Kentucky, USA OVERVIEW Mt Kent Observatory is now providing live remote observations of southern skies as part of a collaborative project between USQ, the University of Louisville, and Northern Kentucky University. ... This enables observers to make daytime use of a remote telescope during its local night-time, and image otherwise inaccessible skies. ...
[ Текст ]  Ссылки http://www.astro.louisville.edu/information/asa2007.pdf -- 182.5 Кб -- 27.06.2007
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9. http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/mn/mn_18.html
filename: mn_18.elvl % observed energy levels: Edlen, B., 1983, Phys. Scr., 28, 51 % theoretical energy levels: Bhatia, A.K., 1982, J.Appl.Phys., 53, 59 %produced as part of the Arcetri/Cambridge/NRL atomic data base collaboration CHIANTI and the Arcetri Spectral Code % Enrico Landi 1997 . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/chianti/chianti_3.03/elements/mn/mn_18.html -- 2.1 Кб -- 20.07.2000
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10. Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/bykovo/ -- 12.3 Кб -- 16.07.1999
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11. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD2D39734-5129-4DEB-B6F9-0477984E70B9%7D
. The Planck all-sky map at submillimeter wavelengths (545 GHz). The band running through the middle corresponds to dust in our Milky Way Galaxy. The black dots indicate the location of the proto-cluster candidates identified by Planck and subsequently observed by Herschel. The inset images showcase some of the observations made by Herschel s SPIRE instrument; the contours represent the density of galaxies. ESA and the Planck Collaboration/ H. Dole, D. Guц©ry G. Hurier, IAS/University Paris-Sud/CNRS/CNES
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD2D39734-5129-4DEB-B6F9-0477984E70B9%7D -- 3.9 Кб -- 10.04.2016
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