... Doug's Home Page . ... S-Lang structures are converted to hash references in Perl , as shown below. ... n\n ; print Structure contents:\n ; # you can treat $s as a reference to a hash array in most respects, except: # - the order of the keys in the array matches that of the # original S-Lang structure # while ( my ( $ key , $ value ) = each %{$s} ) { print key $ key \t has a value of $ value \n ; } print \n ; $$s{afield} = 'a changed field value '; print ...

... Bojan Nikolic web pages (r. 329) . ... Atmospheric Modelling for ALMA . This is also a very simple program (sharing some code with dispersive ) to compute the atmospheric absorption due to dry and wet components of the atmosphere. ... Invoking the help option: ./absorption --help Compute absorption by the atmosphere This program is part of AATM version 0.09 GPL license -- you have the right to the source code. ... Computing atmospheric absorption with AATM . ...

Part 1 of the course: . describes various data types available in computer languages (on the base of Pascal ), . introduces basic data structures used in programming and . shows program realization of the structures. ... This part is available in Russian as LaTeX and PostScript files. ... presents a set of typical algorithms of non-numerical programming and . ... The text of this part is in preparation. The authors are thankful to V.Titov and A.Shneewais for useful discussions. ...

Next: Implementation Up: Image Restorations of High Previous: Technique . This method has been tested on many kinds of data both real and simulated. Here we present three examples in which the structure of the background is of increasing interest and photometry of point sources of diminishing importance. ... Fig. 1 shows the results of this and Fig. 2 shows the photometric accuracy and also a histogram of the background image. ... Fig. 4 shows the quality of the resulting photometry. ...

... Classes . ... casa . casa::LatticeTwoPtCorr< T > . ... Method { . ... autoCorrelation ( MaskedLattice < T > &out, const MaskedLattice < T > &in, const IPosition &axes, Method method, Bool showProgress= True ) const . ... template<class T> . ... Helper functions to convert method types to and from strings. template<class T> . ... Helper function to provide output lattice shape give the input shape and the axes to find the structure function over. template<class T> . ... References casa::square() . ...

Underdetermined sets is a new type of data structures (terms) developed in Actor Prolog . ... The point is that an underdetermined set can include some indefinite rest (a tail) like a list in usual Prolog . At the same time, the order of elements of an underdetermined set can be arbitrary one and it does not affect results of unification of underdetermined sets. Moreover, Actor Prolog guarantees that a rest of an underdetermined set never contains elements that are explicitly given in the set. ...

Appendix B: Annotated Bibliography There are a wide variety of texts available for those who are interested in learning more about assembly language or other topics this text covers. ... Microprocessor Programming for Computer Hobbyists Neill Graham TAB books ISBN 0-8306-6952-3 1977 This book provides a gentle introduction to data structures for computer hobbyists. ... IBM Assembler Language and Programming Peter Able Prentice-Hall ISBN 0-13-448143-7 1987 A college text book on assembly language. ...

... A1963CHECKTIMES - EXAMPLE SCRIPT TO CHECK A1963 TIMES. A1963CMPTIMES - A1963 COMPUTE TIMES GIVEN AZ,RA FROM SOURCE FILES . ... Next Routine] [List of Routines] NAME: a1963checktimes - example script to check a1963 times. ... Previous Routine] [Next Routine] [List of Routines] NAME: a1963cmptimes - a1963 compute times given az,ra from source files SYNTAX: a1963cmptimes,yymmdd,srcfile,datI,srctime=srctime ARGS: yymmdd: long date (AST) for source file. ... This used the slew rates for the move time. ...

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

... Retrieve the list of all available HK parameter validity ranges for instrument EPN from the CAL and construct a GTI data set with name hkgti_epn.ds : hkgtigen instrument=epn withgtiset=true gtiset=hkgti_epn.ds . ... As 1. but do not consider any present validity ranges for parameters P1 , and P2 : hkgtigen instrument=epn withparameters=true except=true parameters="P1 P2" \ withgtiset=true gtiset=hkgti_epn.ds . ... IN [10,20]"\ withgtiset=true gtiset=hkgti_epn.ds . ...

This diagram illustrates a frame-like layout with 'position: fixed'. The illustration shows a four-panel frameset. The top panel ("header") covers the entire width of the frameset and takes up 15% of the vertical space. ... To the right of the sidebar and below the header is the "main" area, whose dimensions are computed based on remaining available space. Finally, at the bottom, the "footer" area is 100px high and covers the entire width of the frameset. ...

... This paragraph shows the very simplest possible example of how to do the relative calibration of a CCD--frame. ... Darks . ... AVERage/IMAge DARKAV = DARK01,DARK02,DARK03,DARK04 . ... COMPute/IMAge DENOM = FLATAV-DARKAV . ... The first two commands compute the simple averages of the dark and flat field images. The third command computes the dark subtracted average flat field. ... Note that there has been no correction for bad columns in either the flat field, the dark frames or the data frames. ...

In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

To connect to the anonymous ftp server at the Univerity of Edinburgh and list the files in the login directory: ftp> open ftp.ed.ac.uk Connected to pcserver2.ed.ac.uk. ... If you experience any problems with this service or wish to make a comment then send email to: ftpmaster@edinburgh.ac.uk 220 The date and time is Fri May 16 16:13:03 1995 Name (ftp.ed:erpl08): anonymous 331 Guest login ok, send your email address as password. ...

... Basic time functions . ... Example 2: Set a random number seed . ... Uses of time functions include: . ... time_t time(time_t *tloc) -- returns the time since 00:00:00 GMT, Jan. 1, 1970 , measured in seconds. ... timer.c */ #include <stdio.h> #include <sys/types.h> #include <time.h> main() { int i; time_t t1,t2; (void) time(&t1); for (i=1;i<=300;++i) printf(``%d %d %d n'',i, i*i, i*i*i); (void) time(&t2); printf(`` n Time to do 300 squares and cubes= %d seconds n'', (int) t2-t1); } . ...

... Spectral energy distributions (SED) for starburst galaxies and ULIRGs are made public available using self-consistent radiative transfer computations assuming dust for the diffuse ISM ( Siebenmorgen et al, 2014). ... In the library of SED models we consider three basic model paramters and use: . ... the radiative transfer model: Kr gel and Siebenmorgen, 1994, AA 282, 407 . ... The starburst model and the SED library is described by Siebenmorgen and Kr gel, 2007, AA 462, 445 . ...

Stellarium 0.12.3 . ... Classes . ... Scripting . ... Scripting Engine . ... Script Console . ... Since version 0.10.1, Stellarium includes a scripting feature based on the Qt Scripting Engine . ... Prior to version 0.10.0, Stellarium used a different scripting engine called StratoScript . ... Prior to version 0.10.0, Stellarium had a simple scripting engine, known as StratoScript . ... This script prints "Hello Universe" in the Script Console output window. core.debug( "Hello Universe" ); . ...

This module illustrates many of the aspects of the Apache 1.2 API and, when used, demonstrates the manner in which module callbacks are triggered by the server. ... Source File: mod_example.c . ... The files in the src/modules/example directory under the Apache distribution directory tree are provided as an example to those that wish to write modules that use the Apache API. ... Example . ... Uncomment the "AddModule modules/example/mod_example" line near the bottom of the src/Configuration file. ...

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

... Between them, the following points are touched: ICRF-2 structure, ICRF Core sources selection, and some expected user's requirements. ... Suggested total number of sources is close to the number of sources already observed in the IVS and VCS sessions, and for most of them reliable positions are derived, mostly for declination > -40 deg. ... So, results of source position time series analysis heavily depend on method used for time series computation and should be used with care. ...