... 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 . ...

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• A matrix of tweets from #AAS223
• A matrix of tweets from #AAS225
• A quick look at tweets from the #AAS225

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" . ...

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• A Number Is A Very Specific Thing - an Astronomy Net Exploration Forum Message
• Quicksand As Black Hole Model? - an Astronomy Net Blackholes Forum Message
• The Telescope's F/number - an Astronomy Net General Forum Message

... 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. ...

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• The COOC Criterion (Criterion of Observations versus Calculations)
• The Number of Ejectors in Binaries
• Binary Pulsar Diversity and High Neutron Star Birth Velocity

... 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. ...

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• Number of Supernovae discovered by amateurs since 1957.
• FTS Dictionary Example
• SAI phone numbers

... 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; . ...

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• Algebraic Number Theory
• Number Theory Semester - Poncelet Laboratory
• Conference "Algebraic Geometry and Number Theory"

... 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 . ...

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• casacore: casa::Primes Class Reference
• WCSLIB: WCSLIB version numbers
• Number input

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). ...

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• Version, UI, and Status Information
• Power of test statistics
• HyperLEDA documentation: HyperLEDA: catalogue of designations (a101)

... Cycle 20 Phase II Proposal Instructions . HST Phase II Proposal Instructions for Cycle 20 > Chapter 4: Solar System Targets > 4.1 Target Number [Target_Number] . ... You should define a different target whenever a different target position or timing description is required. For example, separate targets should be defined if you plan to take spectra of several different surface features on a planet, or if you plan to observe the same feature with different timing constraints. ...

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• CSPICE Routines: ERRDP_C
• Mathematical Analysis of the Iterative/Recursive Algorithm
• CSPICE Routines: SCTIKS_C

... Three is a magic number. ... You get three as a magic number. ... Give you three. That's a magic number. It takes three legs to make a tri-pod or to make a table stand. ... When it's three you can see it's a magic number. ... Multiply backwards from three times ten.> Three time ten is.. ... Three times nine is.. ... Three times six is 18, three times five is 15 . Three times four is twelve . And three times three is nine and three times two is six. ... Yeah> That's a magic number. ...

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• Naughty Number Nine
• Control statements
• Tutorial on Fortran 90, Digital UNIX

... Formulas are very similar to equations. Consider for now only equations with one unknown variable , denoted by some letter, which can be x but can also be different. An equation is an equality between two mathematical expressions containing the unknown number (maybe in several places), as well as other numbers which are known. ... For instance--if you multiply two sides of a formula by the same number, the result is still a valid formula, even if what you multiply contains unknown numbers. ...

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• Identities
• Elements of Algebra
• ASCII files description

Unknown numbers are usually represented by letters of the alphabet . ... However, different letters are also used, often hinting at the quantity they represent-- v for an unknown velocity, T for an unknown time, m or M for unknown masses and F for an unknown force. ... An example of case (#1) is the ratio between the length of a circle and its diameter, a universal constant appearing in many equations (for example, Kepler's equation in section (12a)), whose value to 11 decimals is 3.14159265359.. ...

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• Identities
• Vectors
• Kp Index: Classification of Days

... Insert date: . Day: . Month: . ... This CGI -script calculates a day of week of the given date, Julian date of Greenwich noon JD and extracts from the database indices of solar activity: Wolf number for the day W , monthly W m and yealy means W y of Wolf number for month and year of the date. The prediction of Wolf number (which was made in 1998 and, hence, lost actuality) is also presented. The database uses solar activity data got from server of National Geophysical Data Center . ...

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• Extended time series of Solar Activity Indices
• Datafile structure

... Such a limit may be difficult or impossible to achieve by use of the expression parameter. ... radiusup: sources are ordered in order of increasing radius (see subsection 3.5 ). radiusdown: sources are ordered in order of decreasing radius (see subsection 3.5 ). rownumber: sources are ordered in order of increasing row number in the source table. expr: for this value, the task looks in parameter ncutsortexpression for an expression involving column names. ...

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• The SRCLIST table
• Exposure number.
• READ-OUT STREAKS (bit 1) (Algorithm 2- only used by omdetect)

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The number distribution is shown in the middle panel. The right panel illustrates the distribution of chirp mass due to different DWD types, normalized by the total number (2.76†Ч108) of DWDs in the Galaxy (bin size M = 0.001M ? ... The frequency spectra of DWD strain amplitude and number distribution are presented as a function of galactic component, DWD type, formation channel, and metallicity. тИТ4.5. ...

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• Numbers and distances
• Performance
• Hot subdwarfs

... Arithmetic Functions . Random Numbers . String Conversion . Searching and Sorting . ... There are 4 basic integer functions: . int abs(int number); long int labs(long int number); div_t div(int numerator,int denominator); ldiv_t ldiv(long int numerator, long int denominator); . ... In practice no functions produce truly random data -- they produce pseudo-random numbers. ... The stdlib.h provides 2 useful functions to perform general searching and sorting of data on any type. ...

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• Writing programs that use comedi and comedilib
• Time Functions
• Optimization of spectroscopic observations

.

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• Number of papers published using different observatories
• ESO - A number of OmegaCAM filters show vignetting in their central regions.
• PAM Bulletin

Next: Participants Up: Contents Previous: Cover This volume contains the papers presented at the fourth annual conference on Astronomical Data Analysis Software and Systems (ADASS IV) which was held at the Omni Inner Harbor Hotel in Baltimore, Maryland, from the 26th through the 28th of October 1994. ... To help keep up with new trends in software as they relate to advances in astronomy, the ADASS conferences are organized around certain topics of current interest. ...

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• Classification of Objects in the Guide Star Catalog
• The Sociology of Astronomical Publication Using ADS and ADAMS
• Simulations of Pinhole Imaging for AXAF: Distributed Processing Using the MPI

Preface The necessity of the preparation and edition of such intricate publication, that is the printed version offered to the reader, of geoinformation system including the chronological catalogue and evolutionary database of the global tropical cyclogenesis is dictated, in opinion of the authors, whole number of objective circumstances. ... It derivates the serious dissensions in the initial ('raw') information as well as in databases and archives of regional cyclogenesises. ...

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• Myasnyankin Andrey , Moscow Institute of Physics and Technology (MIPT),Space
• Matyushkin Evgeny, Space Research Institute (SRI)
• Proshin Andrej, Space Research Institute (SRI)

... We will consider the rms, (K), for observations with a receiver of system temperature, T , frequency resolution, per polarization, and total integration time per observing cycle, . ... For ``in-band'' frequency switching, the line under investigation is always in the observing band. ... Position Switching or ``Out-of-Band'' Frequency Switching: Here the line is only observed for one half of the time, with noise being present all of the time. ...

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• Getting the Best Performance from the API
• ATOMS by Number
• Converting Arecibo Interim Correlator data into a FITS image

There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...

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• Head Litter of Minor Planet Names
• Information for Authors of Articles
• Keywords_89