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1. A matrix of tweets from #AAS221
... Circle area is proportional to the number of tweets + retweets tweets retweets . Order accounts: by user number (effectively random) by number of tweets (includes retweets) by number of followers by number of followers that also tweeted about AAS221 by number of friends that also tweeted about AAS221 . ... The top/left position is for the user with the largest number of followers, and the bottom/right is for the smallest number of followers. by number of followers that also tweeted about AAS221 . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~dburke/aas221/user-matrix.html -- 9.2 Кб -- 25.02.2013
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2. How Do You Feel About Numbers? - an Astronomy Net Exploration Forum Message
Astronomy Discussion Forums . Forums: . ... How Do You Feel About Numbers? ... Post Message | ... Posted by Richard D. Stafford, Ph.D. on September 15, 2002 16:22:25 UTC . ... Wait - harvey1 - September 15, 2002 - 22:20 UTC . I don't follow you! - doctordick - September 16, 2002 - 14:59 UTC . ... www.astronomy.net . About 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/14.shtml -- 18.0 Кб -- 09.04.2016
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3. Number of accreting X-ray binaries of selected types
... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node8.html -- 5.9 Кб -- 21.06.1996
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4. SAI Supernova catalog
... Initially SAI Supernova Catalogue was presented in the form of filebased system. ... The current version of SAI Supernova Catalogue presents data on supernovae together with data on their parent galaxies. ... The main source of data for the galaxies was LEDA database. ... In some cases our data were compared with the ones from the Asiago Supernova Catalogue and from List of Supernovae at Harvard-Smithsonian Center for Astrophysics, but the compilation of our Catalogue is carried out independently. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/sn/sncat/ -- 5.9 Кб -- 04.02.2013
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5. The field of p-adic numbers and its finite extensions (Spring 2010)
... The absolute Galois group of Q, denoted Gal(\bar{Q}/Q) in the sequel, is a fundamental object in arithmetics since it carries a lot of informations about number fields. ... A classical way to study this group is to use p-adic numbers. ... firstly, we will explain the classical d vissage of Gal(\bar{Q_p}/Q_p) based on ramification theory; as a corollary, we will deduce that any finite extension of Q_p is resoluble; . ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/ium/s10/p-adic.html -- 2.8 Кб -- 01.02.2010
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6. casacore: casa::RefRows Class Reference
... Classes . ... casa::RefRows . ... Class holding the row numbers in a RefTable . ... RefRows (const Vector < uInt > &rowNumbers, Bool isSliced= False , Bool collapse= False ) . Create the object from a Vector containing the row numbers. ... Convert this object to a Vector<uInt> by applying the given row numbers. ... Get the row vector as is (thus sliced if the object contains slices). uInt . ... Vector < uInt > casa::RefRows::convert . ... const Vector < uInt >& casa::RefRows::rowVector . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/classcasa_1_1RefRows.html -- 34.6 Кб -- 14.02.2011
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7. Discussion
Next: Summary Up: The Second EGRET Catalog Previous: Upper Limits for . In regions of the sky where two or more sources have overlapping point spread functions, it is often difficult to resolve the number of sources and their locations. ... As an example, Nolan et al.(1995) list a source 0445+62 at l = 146.89 , b = 10.65 , with a = 4.0 and a source 0500+59 at l = 150.52 , b = 10.25 , with a = 4.2. ... Both of these sources lie close to the threshold adopted for this catalog. ... 1995). ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/EGRET2/node12.html -- 6.3 Кб -- 08.05.1998
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