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1. ArtistтАЩs impression of the expected dark matter distribution around the Milky
.
[ Сохраненная копия ]  Ссылки http://www.eso.org/public/images/eso1217b/zoomable/ -- 1.9 Кб -- 12.04.2016
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2. Unexpected Galaxy String in the Early Universe
... Unexpected Galaxy String in the Early Universe . ... 20.01.2004 . ... NSF , NASA Explanation: How could such a long string of galaxies form so early in the universe? Several new measurements of galaxies and clusters in the early universe are reporting structures involving galaxies and clusters that are larger than expected with the new standard "dark-energy" cosmology . ... Publications with keywords: galaxies - early universe . Publications with words: galaxies - early universe . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1196200 -- 14.7 Кб -- 20.01.2004
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3. Leonids 2006
Trail encounter . ... Expected meteor rates . ... The Leonids are the debris of Comet 55P/Tempel-Tuttle. ... The Earth's passage right through the centre of trails is associated with the most spectacular meteor displays (studies show that, as well as how close to the centre of the trail you are, the strength of the display also depends on how far along a trail's length you are). ... The encounter with the 1932 trail will lead to enhanced meteor activity: a nice outburst, but below storm level. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/leonid/2006/info2006.html -- 8.6 Кб -- 21.11.2006
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4. aeronomy software
... The 430 carriage house transmitter was used on two dates to measure the temperatures while the swarm a,b satellite flew through the beam: . tle computation used: . ... 2014.03.22 20:21:50 (utc) . ... compute power for each height sample dynamic spectra of overpass (.gif) . ... vertical scale (time hours utc) 1 second resolution (i averaged 100 ipps together after computing power) . ... I used the predict program (and some idl software) to plot the satellite pass around 8:00 utc on 26mar14 . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/aeron/swarmsat/swarmsat.html -- 7.9 Кб -- 28.03.2014
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5. SMOV Status Planning Meeting Minutes 02/27/97
STATUS REPORTS 1. Observatory Status MOSES status reports: -PCS - nominal -OTA - nominal -EPS - nominal -DMS - nominal - SSR testing, including SAA behavior, continues in data gathering mode with recurrence of now typical re-tries. ... STIS Status - CCD temperature is nominal -83 degC. ... SMS065 - finals are out for review - SMS069 - built and initials out for review - SMS072 - built and initials out for review - SMS076 - built - SMS079 - being worked 2. ... Go back to the Meeting Minutes Page ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/smov/notes/0227smov.html -- 3.7 Кб -- 11.03.1997
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6. APOD: 2004 January 20 - Unexpected Galaxy String in the Early Universe
... 2004 January 20 . Unexpected Galaxy String in the Early Universe . ... Explanation: How could such a long string of galaxies form so early in the universe? Several new measurements of galaxies and clusters in the early universe are reporting structures involving galaxies and clusters that are larger than expected with the new standard "dark-energy" cosmology . The controversy centers on the inability of a dark-energy dominated universe to create such large structures. ... About APOD | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap040120.html -- 5.5 Кб -- 02.10.2012
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7. I Expected More Sense Than That. - an Astronomy Net Exploration Forum Message
Astronomy Discussion Forums . ... I Expected More Sense Than That. ... Post Message | ... Posted by Richard D. Stafford, Ph.D. on November 8, 2002 04:14:05 UTC . ... You are missing the point - harvey1 - November 8, 2002 - 13:10 UTC . I hope Stafford doesn't mind my intruding his forum - mrsouza - November 8, 2002 - 14:55 UTC . ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/exploration/messages/155.shtml -- 15.4 Кб -- 09.04.2016
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8. Harvard College Observatory History in Images
... This is a personal project collecting and documenting early images of Harvard College Observatory, focusing on the site at Observatory Hill (previously Summer House Hill). ... This page shows a list of all images tagged with "donors". [link] 1660-ish Portrait of John Winthrop the Younger (1608-1676) . ... That image is a painting of John Winthrop the Elder's great-great grandson, or the great grandson of this John Winthrop. ... Earliest source: "Thomas Hollis (1659тАУ1731)." ... link] 1891 . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~fine/Observatory/donors.html -- 10.7 Кб -- 10.04.2016
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9. Kepler-10c: the First Mega-Earth | Astronotes
... Planets . ... Earth Satellites . ... The newly discovered ?mega-Earth? ... Its sibling, the lava world Kepler-10b, is in the background (the two planets? proximity is grossly exaggerated) .€а Kepler-10c has a diameter of about 29 000 km, 2.3 times as large as Earth, and weighs 17 times as much. ... The first mega-earth to be discovered is Kepler-10c which orbits a star lying about 560 light years from the Sun in the constellation Draco. ... Astronomers Find a New Type of Planet: The ?Mega-Earth? ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/kepler-10c-the-first-mega-earth.html -- 44.9 Кб -- 09.04.2016
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10. G Quirks and Unexpected Behaviour
... These are ``quirks'' rather than ``bugs''. Below is a list of quirks. When loading a file and ``Reset Intensity Upon File Load'' is disabled, the intensity range of the previous image will be used. ... When moving between two images (such as when blinking, or when loading a new image), the display system attempts to retain the old image parameters (i.e. zoom box). What is retained are the corners of the zoom box measured in image pixel co-ordinates, not world co-ordinates. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/karma/user-manual/node20.html -- 3.5 Кб -- 13.02.2011
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11. Performances of NICS
The overall efficiency (including atmospheric transmission, reflectivity of the telescope mirrors and overall efficiency of the optics and of the detector) for broad-band imaging should be about 25% in H and K, and about 15% in J. The main noise source for both broad- and narrow-band imaging should be the photon noise associated to the background+source flux. ... Flat fielding (and possibly background subtraction) might increase the noise by a factor 2 ? ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/nics/generale/prest.html -- 3.8 Кб -- 28.07.2005
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