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1. 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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2. 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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3. DFS commissioning: integration acceptance meeting
... NEWS . WHEN : typically 3 weeks before the official deadline , i.e. date by which the new DFS release has to be operational on the mountain. ... complete list of performed tests. ... description of the new bugs raised during this Integration phase. ... HOW: Integration Acceptance meeting at DFS level with: . ... If needed, specific Integration acceptance meetings at DFS project level and SCCB meetings may be organized to prepare this Integration acceptance meeting. Before this meeting, . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/projects/dfs/team/integration-acceptance.html -- 8.9 Кб -- 13.04.2005
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4. http://zebu.uoregon.edu/2004/es399/lec12.html
For today's in class we will be working with spatial and temporal data sets which are quite noisy. Particularly, you have monthly rainfall totals for the following six locations in Oregon from the period 1950 - 1999. Eugene . Salem . Portland . Astoria . North Bend . Newport . There are many facets of what you can do with this data. Please explore the following questions with some degree of sound statistical reasoning and data presentation: .
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/2004/es399/lec12.html -- 3.3 Кб -- 01.03.2004
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5. early
... User Guide ] Task: early Purpose: Flag data which has early/normal problems. Categories: calibration, uv analysis EARLY is a Miriad task which flags visibility data that it suspects contains early/normal problems. ... If the scatter exceeds some number of sigmas, then the data are assumed to be affected by the early/normal problem, and the entire record is flagged. ... If the signal is noise dominated, no early/normal problems can be detected, and the data will not be flagged. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/doc/early.html -- 3.7 Кб -- 10.04.2016
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6. ASP: Education Newswire
... We considered our current level of technology compared to that of an average alien civilization. Regardless of any modest value of L chosen?500 years, 5000 years, or longer?their level of technology is vastly advanced compared to ours. Thus, most science fiction gets it right by having advanced alien technology, but gets it wrong by not making them sufficiently advanced. ... What would alien civilizations at a distance of 100 or 1000 lightyears know of us (hypothetically)? ... Education . ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/pubs/mercury/0001/j_f00.html -- 12.7 Кб -- 02.10.2012
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7. Selection of observations of empty RGS files
Next: SAS processing Up: Maintenance procedures Previous: Maintenance procedures Contents . Suitable observations should be longer than about 20 ksec, cover all the considered time period, and have different background levels, in particular the highest ones, so the sample should include observations taken at the beginning and end of the science window. It is helpful to consider objects for which no RGS spectrum is expected or to look at the RGS monitor pages. ... Michael Smith 2011-09-20 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node903.html -- 3.7 Кб -- 20.09.2011
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8. 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 Novem