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1. IAA GPS Analysis Center
Results of analysis . ... IAA EOP Service . ... EOP series are regularly submitted to the IERS, and also are available at the IAA EOP Service page. EPN coordinate time series . EUREF Permanent GPS Network (EPN) coordinate time series is computed from analysis of available EUREF weekly solutions. ... Second solution is based on independent combination of individual EPN Analysis Centers' solutions . ... USNO GPS Timing Operations . ... GPS Time Series . ... EPN : European Permanent GPS Network . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/GEO/ac_gps/index.htm -- 9.0 Кб -- 09.04.2016
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2. ASC home page
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/ -- 1.2 Кб -- 01.10.2012
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3. National Astronomy and Ionosphere Center (Arecibo Observatory)
. " The Arecibo Observatory is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations . expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation."
[ Сохраненная копия ]  Ссылки http://www.naic.edu/ -- 3.1 Кб -- 27.02.2014
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4. Johnson Space Center redirect
[ Сохраненная копия ]  Ссылки http://www.jsc.nasa.gov/ -- 1.3 Кб -- 15.08.2013
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5. MCCME: Moscow Center for Continuous Mathematical Education
... НЕПРЕРЫВНОГО МАТЕМАТИЧЕСКОГО ОБРАЗОВАНИЯ . ... Кружок ?Олимпиады и математика? ... Московская математическая олимпиада . Заочный математический конкурс . ... Устные математические олимпиады . Олимпиады по программированию . Математический праздник . Математические регаты . ... Математические бои . Олимпиада по геометрии им. И.Ф.Шарыгина . ... Программа ?Math in Moscow? Научные конкурсы . Творческий конкурс . ... График олимпиад . ... XXVII Математический праздник . ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/ -- 18.8 Кб -- 03.03.2016
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6. http://www.gao.spb.ru/english/personal/malkin/publ/zm10c.pdf
Central Astronomical Observatory at Pulkovo of Russian Academy of Sciences PUL Analysis Center Pulkovo IVS Analysis Center (PUL) 2009 Annual Rep ort Zinovy Malkin, Natalia Miller, Elena Popova Abstract This report briefly presents the PUL IVS Analysis Center activities during 2009 and plans for the coming year. The main topics of the investigations of PUL staff in that period were ICRF related studies, computation and analysis of EOP series, and VLBI2010 related issues. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm10c.pdf -- 66.6 Кб -- 08.11.2010
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7. Science Results from Pan-STARRS1
STScI . ... Science Blog . ... Visitors . ... Parking . ... Visitor parking at the Space Telescope Science Institute is extremely limited. ... Visitors parking in these locations risk ticketing and/or towing of their vehicle. ... Visitors to STScI may park at the San Martin Center Garage, located approximately 1/8 mile south of the Space Telescope Science Institute. ... Visitors should obtain a ticket at the garage entrance gate and use any available visitor space located to the right of the entrance. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/panstarrs1/parking -- 15.4 Кб -- 10.04.2016
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8. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... V348 Aql, USNO-B1.0 0904-0422027 . ... Meinunger (1966) classified it as an eclipsing binary with a period very close to 1 day, noting however that the period and derived minima times were uncertain due to the low variability amplitude. As of July 2011, the O C gateway (Paschke Brat 2006; Paschke 2009) lists, in addition to Meinunger's photographic data, 2 visual and 3 CCD times of minima from Paschke (1988, 1996, 2006), Stepan (1995), Br t et al. ... Meinunger (1966) . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1252756 -- 18.0 Кб -- 17.11.2011
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9. The ROSAT RESULTS ARCHIVE: Tools and Methods
... The ROSAT Results Archive (RRA) is a publicly accessible collection of source lists, images, spectra, lightcurves and counting rates derived from pointed-phase observations of the ROSAT X-ray satellite observatory. ... This paper discusses the methods and tools used to screen ROSAT source results, and discusses ways in which the data will eventually be made accessible to the general astronomical community. ... Each field and source gets assigned a set of quality flags by these scripts: . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/corcoranm.html -- 11.6 Кб -- 23.06.1998
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10. ION Results Page
This page is a mirror of the ION SADS page available at http://sads.cnes.fr:8010 . Besides the information already available on this page, there you can browse the ION QuickLook images. ... The ION experiment flown on the Interball-Aurora mission performs simultaneous ion and electron measurements. Two mass spectrometers looking in opposing directions perpendicular to the satellite spin axis, which points toward the sun, measure ions in the mass and energy ranges 1-32 amu and ~ 0 to 14,000 eV. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/auroral/ion.htm -- 5.1 Кб -- 23.04.1998
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/auroral/ion.htm -- 5.1 Кб -- 23.04.1998
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11. THE DEEP X-RAY RADIO BLAZAR SURVEY (DXRBS) I. Methods and First Results
... Here we discuss our survey methods, identification procedure and first results. Our survey is found to be efficient at finding flat-spectrum radio-loud quasars (FSRQs, 59 of our first 85 IDs) and BL Lacertae objects (22 of our first 85 IDs), a figure which is comparable to or greater than that achieved by other radio and X-ray survey techniques. ... Particularly important is the identification of a large population of FSRQs ( of DXRBS FSRQs) with ratios of X-ray to radio luminosity . ... FSRQs . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/dxrbs_paper.html -- 8.4 Кб -- 03.12.2003
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12. APOD: October 17, 1999 - Black Holes in Galactic Centers
... October 17, 1999 . Black Holes in Galactic Centers . ... HST , NASA . Explanation: Do all galaxies have black holes at their centers? Although not even a single galaxy has yet been proven to have a central black hole , the list of candidates continues to increase. ... In all the galaxies studied, star speeds continue to increase closer the very center . This in itself indicates a center millions of times more massive than our Sun is needed to contain the stars. ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap991017.html -- 4.5 Кб -- 02.10.2012
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13. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/mk_frametimes.pdf
EPIC ESAC A time jump analysis on EPIC-pn with some side results Marcus G. F. Kirsch M.J. Freyberg, E. Kendziorra Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 menu EPIC ESAC · Do we still have time jumps? ... Can a time jump detection be implemented in a sort of routine check (Qcheck)? Are there time issues that we still do not understand ? ... Are the frame times correctly used? ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200502/mk_frametimes.pdf -- 539.0 Кб -- 16.05.2014
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14. Баллистический центр Института прикладной математики им. М.В.Келдыша РАН
... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...
[ Сохраненная копия ]  Ссылки http://www.kiam1.rssi.ru/ -- 4.2 Кб -- 02.02.2013
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15. U of O High Energy Physics Seminars
September 24, 2010 (Friday) Bob Hirosky, University of Virginia . ... This talk summarizes some of our latest results from the summer 2010 conferences and discusses future prospects with a substantial increase of available data. 2:00pm, 472 Willamette Hall . ... CMS has found a ridge in the two-prticle correlation of hadrons produced in pp collisions at 7 TeV at LHC. ... Interpretation of the phenomenon will be given. 4:00pm, 472 Willamette Hall . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/~uochep/seminars/seminars-fall10.html -- 3.3 Кб -- 06.05.2011
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16. ChaMPlane data_archive_.html
... Fields Observed . ... Data Archive . ... Complete Optical and X-ray data for all ChaMPlane fields are available through the DS9 VO interface . ... functionality of DS9 is available to manipulate the results in addition to those provided by the "Champlane tools" You can select images, compare . ... our region of interest has been selected by drawing a red square region on the image. at bottom left the high res optical image of that selected region, and on the right is the X-ray image. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChaMPlane/virtual_obs.html -- 10.9 Кб -- 01.10.2012
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17. http://www.atnf.csiro.au/computing/software/gipsy/tsk/trace.dc1
Program: TRACE Purpose: TRACE plots image values at user given positions as function of distance to a plot centre (in 2-d (sub)sets). Category: ANALYSIS, PLOTTING File: trace.c Author: M.G.R. Vogelaar Keywords: INSET= Give set (, subset): Only one subset is allowed. ... XYBOX= Give size of box around one pixel: [3,3] The resulting value at a selected position is an average of the pixels in the defined box around that position. ... POSITION= Give position x, y: Physical values are allowed. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/tsk/trace.dc1 -- 7.2 Кб -- 22.07.1996
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18. Results and Discussion
... In Figures 2 and 3 we show the 6m telescope spectra of blue compact galaxies HS 1013+3809 and HS 1442+4250, in which typical high excitation HII-region narrow emission lines are seen. ... for red part of HS 1442+4250. ... This correction = 354 km s -1 was calculated for HS 1013+3809 and = 202 km s -1 for HS 1442+4250. ... While HS 1013+3809 looks very symmetric and very compact, with intense star formation burst taking place in its very center, HS 1442+4250 is well elongated, resembling edge-on disk...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/1998/Poor_for_SAO/node3.html -- 8.1 Кб -- 05.03.1999
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19. Population Synthesis of X-ray Sources at the Galactic Center
Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node72.html -- 6.7 Кб -- 01.03.1997
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20. Cosmic Phys Rus
... Abstract . ... Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . ... Mingaliev M.G. Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . ... Moiseev A.V. Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . Scanning FPI for Galactic and Extragalactic Observations in SAO RAS . ... Semenova T.A. Special Astrophysical Observatory of the Russian Academy of Sciences (SAO RAS), Russia . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/katya/CosmosPh/en/prel-prog_partic.html -- 13.5 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/katya/CosmosPh/en/prel-prog_partic.html -- 13.5 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/katya/CosmosPh/en/prel-prog_partic.html -- 13.5 Кб -- 02.10.2012
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