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21. Supernova 1999aa in NGC 2595
SN 1999aa - A Third Supernova Discovery . Just 9 weeks after the discovery of SN 1998ey a suspect was found 1" east and 28" north from the centre of NGC 2595 on Feb.11.0166 U.T.. ... Further inspection of 6 images of NGC 2595 taken during Feb. and March 1998 showed no object at the position of the suspect. ... Beijing Astronomical Observatory recorded SN 1999aa on Feb. 11.6 and 12.6 UT, the first obervation being only 14 hours after the discovery. ... Back to Supernova 1999aa in NGC 2595 . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/snimages/sn1999/sn99aa1.html -- 4.9 Кб -- 22.12.2007
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn1999/sn99aa1.html -- 4.9 Кб -- 19.04.2014
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22. TUI:Tidbits:Entering Sexagesimal Offsets and Durations
Many entry fields permit sexagesimal entry (h:m:s.s or :':"). ... Sexagesimal entry is flexible in that you can specify one to three fields, as you desire. ... Offset and duration entry widgets assume that a single field is decimal arc-seconds or seconds ('.' or s.s) and two fields are (arc) minutes and seconds (':"." or m:s.s). ... You may specify one to three fields. ... Note: sexagesimal positions are entered in the same fashion, but a single field is decimal hours or degrees (h.h or . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/35m_operations/TUI/Tidbits/RelSexagesimal.html -- 3.4 Кб -- 05.09.2014
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23. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0295-1-0.ps.gz
XMM­Newton CCF Release Note XMM­CCF­REL­295 Modifications to EMOS Bad Pixel Table M.J.S. Smith March 1, 2013 1 CCF Components Name of CCF VALDATE EVALDATE Blocks Changed CAL Version XSCS Flag EMOS1 BADPIX 0036 2013­01­21T06:31:40 -- BADPIX NO 2 Changes Following the suspected MOS1 impact event of revolution 2382, in which CCD3 sustained extensive damage, several hot pixels developed in other MOS1 CCDs. ... This CCF reflects the currently uploaded MOS1 Bad Pixel Table. ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0295-1-0.ps.gz -- 138.3 Кб -- 01.03.2013
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24. CH Cyg
... The hot component shows very spectacular activity: irregular outbursts accompanied by fast, massive outflows and jets. ... Diffraction-limited images for both components of CH Cyg binary system were reconstructed using visible speckle interferometry at BTA 6-m telescope (Fig.1). The orbital period 15.6 years and masses: 2.0 Msun and 0.7 Msun for red giant and white dwarf, respectively were derived from angular distance (0.042") and magnitude difference (2 m ) of the components. ... Fig.1. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2010/CHCyg/ -- 4.2 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2010/CHCyg/ -- 4.2 Кб -- 02.10.2012
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25. Northeast Astronomy Forum & Telescope Show (NEAF) - Events Calendar
STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... For over 30 years, itтАЩs been our passion to create the finest telescopes available for the astronomy enthusiast. ... Events . Meade Events . ... Event Calendar . Northeast Astronomy Forum & Telescope Show (NEAF) . ... Meade is happy to announce that we will be attending the Northeast Astronomy Forum & Telescope Show, a.k.a. NEAF, one of the largest astronomy trade shows in the United States. ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/event/northeast-astronomy-forum-telescope-show-neaf.html -- 73.3 Кб -- 09.04.2016
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26. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Кб -- 15.12.2015
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27. source comment
Comment on J0513-2159 . Our image shows an extension to about 5 mas SE from the brightest feature. The EVN 8 GHz image by Dallacasa et al. (1998), with about five times larger resolution, shows an extension from the brightest feature roughly opposite to our direction. As noted by Dallacasa et al. (1998), the structure detected has a highly inverted spectrum, which, together with the reported variability in the source, could explain the structural disagreement. ...
[ Сохраненная копия ]  Ссылки http://www.vsop.isas.ac.jp/VLBApls/J0513-2159.comment.htm -- 1.8 Кб -- 16.10.2000
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28. Science with CXO
Next: Conclusion Up: No Title Previous: The Transmission Gratings . ... The potential of Chandra is illustrated in Figure which shows the official "first-light" image. ... Figure: The official CXO first light image - the supernova remnant CasA. Perhaps the neutron star - black hole connection and the utility of CXO are best illustrated by an early observation of the Crab Nebula and pulsar taken as part of the HETG calibration. ... Figure shows the zeroth-order image of the Crab Nebula. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/images/chandra/crete_astro-ph/node6.html -- 6.0 Кб -- 07.12.1999
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29. IAU Commission #34 (Interstellar Matter)
... Feeding the Monster: Gas Caught in its Death Spiral into a Massive Black Hole . ... Stromlo Professor Mike Dopita have used the Hubble Space Telescope to discover how a massive Black Hole in a nearby galaxy feeds itself. ... Earlier Hubble Telescope data obtained by another team member, Professor Holland Ford of Johns Hopkins University in Baltimore, Maryland, had found a disk of gas rushing around the Black Hole at a speed of 500 kilometers a second. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mad/M87pr.html -- 10.5 Кб -- 09.04.2016
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30. http://selena.sai.msu.ru/Symposium/lipskiy.doc
LIPSKIY-RODIONOVA' LUNAR ANTIPODES AS PRECURSORS OF A REGULAR WAVE PLANETOLOGY G.G.Kochemasov IGEM of the Russian Academy of Sciences, Moscow, Russia kochem@igem.ru / Fax: (009)(095)230 21 79 The first observations of the lunar far side allowed to compare it with the near side and draw very important conclusions in the very beginning of planetary studies based on spacecrafts. ... Celestial bodies are dichotomic. ... The concept of celestial bodies includes Sun (a star) as one of them. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Symposium/lipskiy.doc -- 89.0 Кб -- 06.10.2008
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31. Who is tweeting about #AAS223
... Data Collection and Analysis . AAS 223 . ... The data below shows who has been tweeting about the 223rd meeting of the American Astronomical Society , with a cut-off to avoid being drowned by the " long tail " of the distribution. ... If you mouse over the bar then you the user's actual name (or at least whatever text was given to Twitter) and the number of tweets or retweets they made. ... Total number of tweets , of which were made by the following accounts (the cut off to appear is tweets): . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~dburke/aas223/user-count.html -- 8.5 Кб -- 28.02.2014
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32. Laplase
... Pierr Simone Laplas.) For his bright intellect and an outstanding achievements in several sciences (astronomy, physics, mathematics) Laplas was called "a French Newton". He became a consistent follower of Newton and rut a task before himself of explaining the planets motion, the movement of their satellites, the ocean rising tides in the Earth and a complicated motion of the Moon. Laplas showed that the planets inequalities should be periodical (based on Newton's gravitation principal). ...
[ Сохраненная копия ]  Ссылки http://www.space.vsi.ru/laplase.htm -- 3.2 Кб -- 14.10.2000
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33. http://www.gao.spb.ru/personal/neo/eng/occultat/data/occ-nea.txt
... All angular values are expressed in degrees. ... But those who have the facilities for high-speed photometry could try to observe these phenomena. h m ° ° ° ° 2016 April 1 18 51.0 84.9 57.4 345 20 168378 1997 ET30; 17.8 ; 1.7 km; 7.2; 0.47s 18 58.0 67.3 45.6 325 26 U2 027489793 ; 10.6;14h06m06.171s;-12°01'21.53 19 05.0 49.6 38.1 307 22 2016 April 10 22 10.4 106.6 -31.2 311 75 297274 1996 SK; 20.3; 1.7 km; ...
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/personal/neo/eng/occultat/data/occ-nea.txt -- 5.5 Кб -- 28.03.2016
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34. http://www.iki.rssi.ru/vprokhor/camp2/fspdescr.htm
... Each plot shows the information about 4 S/C, by the different color. for the INTERBALL TAIL PROBE - the red color is used, . ... The polar diagram, which shows the corrected geomagntetic co-latitude and corrected geomagnetic local time of the 4 spacecraft during the time intervals selected in accordance with the FSP1 criteria. ... In the last 4 plots the days are shown along X axis, in the last two plots the Universal time is shown along the Y axis . ... for the POLAR - the third line, . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/camp2/fspdescr.htm -- 3.0 Кб -- 19.11.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/camp2/fspdescr.htm -- 3.0 Кб -- 19.11.1999
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35. Phil Plait's Bad Astronomy: Bad TV
... Bad Astronomy . ... On Thursday, February 15th 2001 (and replayed on March 19), the Fox TV network aired a program called ``Conspiracy Theory: Did We Land on the Moon?'', hosted by X-Files actor Mitch Pileggi. ... Dust around the lander . ... However, it appeals to our common sense: when the sky is black here on Earth, we see stars. ... Bad: The program claims that when the top half of the lander took off from the Moon to bring the astronauts back into orbit, there was no flame from the rocket. ...
[ Сохраненная копия ]  Ссылки http://www.badastronomy.com/bad/tv/foxapollo.html -- 63.7 Кб -- 09.04.2016
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36. Астрономия для школьников
... NASA, Maas Digital This animation shows a conceptualized view of Deep Impact's encounter with comet Tempel 1. Approximately 24 hours before impact, the flyby spacecraft releases the impactor into the comet's path. The impactor uses control software and thrusters to guide itself towards the nucleus of the comet. ... The resulting collision between comet and impactor will likely punch a crater, anywhere from the size of a Sport Utility Vehicle to a football stadium, into the comet's nucleus. ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/films/deepimpact.html -- 13.4 Кб -- 09.04.2016
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37. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AHall-P.pdf
Neptunes in the Noise: Improved Precision in Exoplanet Transit Detection AimИe Hall , Simon Hodgkin , Gabor Kovacs and Don Pollacco 1 1 1 1 2 Institute of Astronomy, University of Cambridge 2 Department of Physics, University of Warwick Figure 2 (right): Distribution of radii of all known exoplanets (grey), with those from Kepler (green) and SuperWASP (blue) also shown. We present early results from a new analysis of raw data taken with the SuperWASP telescope[1]. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AHall-P.pdf -- 2664.7 Кб -- 16.04.2014
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38. http://www.jsc.nasa.gov/roundup/online/2005/0905_p8_11.pdf
... NASA S114E5070 View of the Space Shuttle Discovery's crew cabin and the Orbiter Docking System, photographed as part of the survey sequence performed by the Expedition 11 crew during the STS-114 R-Bar Pitch Maneuver on Flight Day 3. ... STS-114 Commander Eileen Collins Backdropped against a colorful part of Earth, this full view of the International Space Station was photographed by a crewmember onboard the Space Shuttle Discovery following the undocking of the two spacecraft. ...
[ Текст ]  Ссылки http://www.jsc.nasa.gov/roundup/online/2005/0905_p8_11.pdf -- 643.9 Кб -- 14.09.2005
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39. A New Entropy Measure Based on Multiple Resolution and Noise Modeling
... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/murtaghfd/ -- 17.8 Кб -- 16.07.1999
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40. GRB follow-up team
... Team . ... All the results we present were obtained with the SCORPIO instrument mounted at the 6-m telescope of SAO RAS. TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1090 SUBJECT: GRB001109, Host Galaxy Spectroscopic Observations DATE: 01/09/08 07:28:47 GMT FROM: Vladimir Sokolov at SAO RAS <sokolov@sao.ru> . ... TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1092 SUBJECT: GRB001109, Host Galaxy Astrometry DATE: 01/09/11 08:19:24 GMT FROM: Vladimir Sokolov at SAO RAS <sokolov@sao.ru> . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/grb/hosts/GRB001109/GRB001109.html -- 9.8 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/grb/hosts/GRB001109/GRB001109.html -- 9.8 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/grb/hosts/GRB001109/GRB001109.html -- 9.8 Кб -- 10.04.2016
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