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1. http://zebu.uoregon.edu/1998/ph101/l19.html
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1998/ph101/l19.html -- 7.0 Кб -- 02.12.1998
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2. XVIII International Astronomy Olympiad: Important Notes for interested
... Since founding of the Olympiad] The Olympiad participants are not supposed to study at any institutions of higher education (university or school which can be considered technical colleges). ... Note: Exception may be done for the second time participating in IAOs students not older than 14.00 years on January 1st of the year of the Olympiad (i.e. born after January 01, 1999). ... Team of region, city, town: . ... of the XVIII International Astronomy Olympiad (2013), . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/iao/statutes/iao3i13.html -- 10.5 Кб -- 14.05.2014
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3. http://www.sao.ru/cats/~satr/RFSymp/abs/38_Verkhodanov2.ps
PHASE ANALYSIS IN STUDY OF COSMIC MICROWAVE BACKGROUND O.V.Verkhodanov 1 , P.D.Naselsky 2 , L.­Y.Chiang 2 , A.G.Doroshkevich 3 , I.D.Novikov 3,2 1 Special Astrophysical Observatory of RAS, Nizhnij Arkhyz, Russia 2 Niels Bohr Institute, Copenhagen, Denmark 3 AstroSpace Center, Moscow, Russia vo@sao.ru Phase analysis based on the complex values of spherical harmonics of the CMB fluctuation expansion is an extremely important method of observational cosmology. ... 2003, 2004, 2005). ...
[ Текст ]  Ссылки http://www.sao.ru/cats/~satr/RFSymp/abs/38_Verkhodanov2.ps -- 93.7 Кб -- 09.10.2006
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4. Cosmology / Relativity / Gravity Wave Astronomy
One very important space mission has already provided definite answers about cosmology, the quest to understand the origin and fate of the Universe. ... Ground-based gravitational wave telescopes like LIGO and VIRGO now being completed; and space-based telescopes like LISA should open an entire new window on the Universe, by looking at the gravitational radiation being emitted by extremely large or compact sources, like double black holes, or coalescing neutron stars. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~pfreire/space/index04.html -- 4.6 Кб -- 27.01.2008
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5. Background correction
... One important issue for the spectral analysis with X-ray detectors is the treatment of background for extended sources. ... To deal with the particle background (more or less constant outside proton flares), one should assign weights to the reference event list and extract images or spectra using the same spectral or spatial (in detector coordinates) selection as the source. The original spatial selection (on the source) is usually applied to sky coordinates (not detector coordinates). ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/evigweight/node11.html -- 5.9 Кб -- 02.07.2008
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6. TCV [Oulu]
spaceweb@oulu.fi - last update: 20 September 1998, 2020 UT (RR) . Traveling Convection Vortex (TCV) is a name given to a specific type of daytime magnetic impulsive events observed by high-latitude ground-based magnetometer arrays. Since the most likely source for TCVs is the solar wind , they are considered to be important processes in transfering energy from the solar wind into the magnetosphere . ... For example, one AMPTE Lithium release in the solar wind caused a TCV event . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/tcv.html -- 8.7 Кб -- 13.05.2001
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7. Space Telescope Imaging Spectrograph Instrument Handbook
Space Telescope Science Institute . ACS Instrument Handbook Cycle 19 . ... Advanced Camera for Surveys Instrument Handbook for Cycle 19 > Chapter 5: Imaging > 5.2 Important Considerations for ACS Imaging . ... The WFC and HRC shared two filter wheels. ... Unfil tered or two-filter imaging yields significantly degraded PSFs (particularly for the WFC), so these modes are typically used only for polarization observations or HRC coronagraphic acquisitions. ... Filter . ... WFC . ... HRC . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/documents/handbooks/cycle19/c05_imaging3.html -- 144.9 Кб -- 05.02.2013
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8. Zeldovich-100 / International Conference / Moscow, Russia
Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/zeldovich-100/ -- 14.9 Кб -- 09.04.2016
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9. The AstroStat Slog Blog Archive [ArXiv] Correlation Studies, June 12, 2007
... Archives . ... ArXiv] A Lecture Note, June 17, 2007 . ArXiv] Solar Cycle, June 18, 2007 . Jun 18th, 2007| 05:08 pm | ... One of arxiv/astro-ph preprints, arxiv/0706.1703v1 discusses correlation between galactic HI and the cosmic microwave background (CMB) and reports no statistically significant correlation. ... Are these correlation studies truly statistical science? ... Therefore, I have been doubting what is so important about correlation in astronomy. ... Chandra Blog . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2007/arxiv-correlation-studies-june-12-2007/index.html -- 23.3 Кб -- 01.03.2014
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10. Important Notes - Please check these
Next: Links to Manual Sections Up: Contents Previous: Contents Contents . ... All VLBA stations have two RDBE units for a total of 8 channels with the DDC. ... SCHED knows how to set up the details for most observations at most stations. ... Please see the discussion of the input parameter PRECDATE . ... Please note that all setup files intended to be used for spectral line observations using DOPPLER must have all channels distinguished, in the setup file, by frequency and polarization. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Important_Notes_Please_chec.html -- 7.3 Кб -- 10.04.2016
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11. Red dwarfs: The most important stars in the Universe | Astronotes
... Sun . ... Our Galaxy . ... Stars . ... Artist's impression of the red dwarf star CHRX 73 A and its companion object CHRX 73 B. The companion object is around 12 Jupiter masses, and may either be a planet or a brown dwarf. ... In Astronomy-speak, red dwarfs are low-mass stars; our own Sun is 2.5 times as heavy as even the biggest red dwarf. ... In our galaxy, the Milky Way, red dwarfs are the most common type of star . ... Tweets that mention Red dwarfs: The most important stars in the Universe | ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/most-important-stars-in-the-universe.html -- 52.2 Кб -- 09.04.2016
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12. ASP: Robert J. Trumpler Award
Past Robert J. Trumpler Award recipients . ... The Robert J. Trumpler Award of the ASP is given each year to a recent recipient of the PhD degree in North America whose research is considered unusually important to astronomy. ... To be considered for the Trumpler Award, a nominee's Ph.D. must have been awarded within two years of the time of the nomination and most or all of the thesis must have been published in a recognized journal with an issue date prior to 1 January 2013. ... Nominations . ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/membership/awards/trumpler.html -- 8.6 Кб -- 11.10.2012
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13. ESO - Why is Technology Transfer important for ESO
European . ... Public . ... ESO for the Public > Doing Business with ESO > Technology Transfer > Importance for ESO . ... Survey Telescopes . ... People and Events . ... Events . ... ESO Press Conferences and Events . ... SO's public relations and educational activities not only increase the awareness of ESO's scientific results among the general public, they are also an important way of stimulating interest in astronomy amongst school children who will be the next generation of European astronomers. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/public/industry/techtrans/Importance.html -- 33.4 Кб -- 10.04.2016
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14. Extragalactic Gravitational Wave Background
Next: Gravitational Wave Background from Previous: Galactic Gravitational Wave Background . ... It is intuitively clear that at frequencies above the critical ones for our Galaxy, one will detect rare bright jerks produced by coalescing white dwarfs   (at a rate of 1 per 100 year) and NS (at a rate of 1 per - year) in our Galaxy, against a background of the extragalactic stochastic GW. ... Firstly we consider GWB from close individual galaxies, and then will discuss overall extragalactic GWB. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node83.html -- 4.5 Кб -- 04.03.1997
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15. APOD: 2013 March 25 - Planck Maps the Microwave Background
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2013 March 25 . Planck Maps the Microwave Background . ... Visible in all directions, this cosmic microwave background is a complex tapestry that could only show the hot and cold patterns observed were the universe to be composed of specific types of energy that evolved in specific ways. ... About APOD | ... A service of: ASD at NASA / GSFC . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap130325.html -- 5.9 Кб -- 28.02.2014
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16. COALA - Computational Astrophysics Laboratory
... Using the self-consistent 3D hydrodynamical code in Kobayashi et al. (2007) , we simulate the star formation and chemical enrichment history of the Universe. ... We also predict the rates of supernovae and gamma-ray bursts, and the properties of the host galaxies, which will be observed with the ANU's new SkyMapper telescope. ... Supernova feedback on galaxy formation. ... Feedback from active-galactic nuclei (AGN). ... COALA : Universe Galaxy AGN Star Planet ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/universe.html -- 4.8 Кб -- 01.10.2012
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17. Amateur Telescope Makers of Boston
... IC443 is thought to have been formed between 30,000 and 35,000 years ago, and most likely is the remains of the pulsar, G189.6+3.3. Located about 5,000 light years away, the pulsar’s X-ray emissions excite the material of the nebula, causing the chemical components to emit light in their characteristic wavelengths. ... TAK FSQ . ... FSQ: 12x30 minute subs plus 14x5 minute subs, totaling 7 hours, 20 minutes . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
[ Сохраненная копия ]  Ссылки http://www.atmob.org/gallery/showimage.php?id=638 -- 5.7 Кб -- 09.04.2016
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18. Space Research Institute (IKI) Seminar
... Future seminars . P a s t seminars . ... On prediction of critical events in complex systems " . A.A. Soloviev ( International Institute of Earthquake Prediction Theory and Mathematical Geophysics, Russian Academy of Sciences ) . ... The data used by the prediction algorithms are background seismicity (in the case of the lithosphere), macroeconomic indicators (in the case of economic systems), and statistics of several types of less severe crime (in the case of megacities). ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/galeev/abs_eng/e070130.htm -- 5.8 Кб -- 24.01.2007
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/galeev/abs_eng/e070130.htm -- 5.8 Кб -- 24.01.2007
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19. The Cosmic Infrared Background
... 6.02.2002 . ... Credit: A. Kashlinsky ( SSAI ) S. Odenwald ( Raytheon ), 2MASS , NSF , NASA Explanation: What cosmic wallpaper is on the sky? ... Recently, however, the background in near infrared light was imaged at high resolution by the 2MASS telescope , and confirmed earlier estimates that it is over twice as bright as originally expected. ... Visible is light emitted from the very first stars and galaxies in the universe , emitted when the universe was less than half its current age. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1174648 -- 14.9 Кб -- 06.02.2002
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20. Future of the Galaxy
... Line radiative transfer in C 18 O, HCO + , and CS lines is considered in a spherically symmetric chemo-dynamical model of a starless core, evolution of which is driven by the ambipolar diffusion. Theoretical line profiles are compared to observational data on the well-known L1544 core, which is one of possible candidates for collapsing protostellar clouds. ... Comparison between modelled and observed spectra suggests that L1544 has flattened structure and is observed at some inclination. ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/lines.html -- 2.2 Кб -- 27.09.2012
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