The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

function fringevissq,c,k,n,normal=normal . ... Zero if no counts. The first index in the frames must correspond to the phase bins. Use k to select a baseline, if multiple baseline are present. ; . ... if n_elements(k) eq 0 then k=1 . ... nominator=add(abs(fringevis(c-avg(c),k))^2-s,n,r(0)-2)/n . denominator=(add(s,n,r(0)-2)/n)^2 . index=where(denominator eq 0,count) . if count gt 0 then denominator(index)=1 . ... if normal then norm_factor=4.0/sinc(float(k)/n0)^2 $ . ...

... Search . ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Careers overview . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... In the regions of highest optical obscuration and infrared confusion, only 21-cm emission can be used to find galaxies in the Zone of Avoidance. ... The big breakthrough should come in the south, however, with the advent of the Parkes telescope multibeam system. ...

... A comparison of the computed and experimental relations F max ( H), as well as comparison of drift scans of point sources across different horizontal cross-sections of the BP with the corresponding computed cross-sections were made. ... The drift scans of the point source 3С84 (H=87 o ) at the wavelength 7.6 cm across the horizontal cross-sections of the BP (black lines) and the computed horizontal cross-sections of the BP corresponding to them (red lines). ...

... The close proximity of the Magellanic Clouds allows us to probe the nature of these star forming regions at small spatial scales. ... We present the spatial analysis, via aperture/annulus photometry, of 16 Large Magellanic Cloud (LMC) and 16 Small Magellanic Cloud (SMC) H II region complexes using the Spitzer Space Telescope's IRAC (3.6, 4.5, 8 ЮМm) and MIPS (24, 70, 160 ЮМm) bands. ... The IRAC, MIPS, UV, and HЮБ spatial analysis are compared with the spatial analysis of the TIR. ...

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

... The two common precisions single precision (SP) and double precision (DP) on a system based on IEEE 754 can specified with INTEGER , PARAMETER :: SP = SELECTED_ REAL _ KIND (6,37) INTEGER , PARAMETER :: DP = SELECTED_ REAL _ KIND (15,307) REAL ( KIND =SP) :: single_ precision _variables REAL ( KIND =DP) :: double _ precision _variables If we wish to work with at least 14 decimal ...

. back one page . previous slide . next slide

Nowadays at the Department the experimental and theoretical investigations, including astronomical and ionospheric observations, active experiments with space vehicles are taking place. ... Solar Corona physics and erruptive phenomenae. ... Stellar astronomy. ... The Department has organized and put into practice more then 50 expeditions for observation of Solar ecllipces, aurorae polaris, comets, meteor streams, controlled space experiments, and also for investigations of geophysical characteristics. ...

http://www.mso.anu.edu.au/~ralph/freefree.html . Ralph S. Sutherland . New calculations of free-free transition matrix element integrals are performed using modern symbolic computing techniques to evaluate the hypergeometric functions with complex arguments. The results are presented in both graphical and tabular form including accurate extrapolation methods. ... http://msowww.anu.edu.au/~ralph/data/freefree/ . ...

... Posts tagged ?special session? ... We organized a Special Session on Time Series in High Energy Astrophysics: Techniques Applicable to Multi-Dimensional Analysis on Sep 7, 2011, at the AAS-HEAD conference at Newport, RI. ... Tags: 2010 , 215 , AAS , AAS 215 , astroinformatics , astrostatistics , complex data , January , Methods , special session , Washington . ... Tags: 2008 , AAS , April , astrostatistics , HEAD , Los Angeles , March , Methods , Omni , special session , techniques , workshop . ...

... National Astronomy and Ionosphere Center . ... web: www.naic.edu/~gibson . ... Ph.D. in Astronomy . ... University of Wisconsin-Madison . ... Staff Research Associate . ... National Astronomy and Ionospheric Center . Sep 2005 - present . Postdoctoral Research Associate . ... University of Calgary . ... Graduate Research Assistant . ... University of Michigan Space Physics Research Laboratory . ... Mentor to Graduate Students, University of Calgary Radio Astronomy Laboratory . ...

... I've included typical values in some cases: int num_gd_trials; /** Number of trial group delays */ int num_bas ; /** Number of baselines measured by FT (up to 9) */ int num_channels = 5; /** Number of spectral channels used for fringe tracking */ int num_output; /** Total number of combiner outputs in use */ int num_win = 5; /** Number of windows (subframes) per camera : TODO : not needed? */ Monitor Data ===== /** * Pixel data at a modulator position from all cameras. ...

... Despite the wide spread use of the terms MTF, CTF, limiting resolution, minimum resolvable target, and contrast to describe CCD image system quality, the terms are often misused and their relations are little understood. ... The modulation transfer function (MTF) is a Fourier transform of the line spread function i.e. its equivalent as an integral sum of sine waves taken over the whole range of spatial frequencies. MTF by its Fourier nature can only be used to operate on sinusoidal frequencies. ...

Next: Identification and Analysis of Binary Star Systems using Probability Theory . ... We present a computing code for modelling energy flux distributions, photometric indices and spectral line profiles of (non-)radially pulsating Main-Sequence stars. ... In the case of slowly rotating stars one can use the zero-rotation approximation to describe stellar pulsations. Such a model was used already by Cugier, Dziembowski & Pamyatnykh (1994) to study nonadiabatic observables of Cephei stars. ...

... Mean s of visual simulation of the design and verification of macro can improve the efficiency of professionals in the design, development and maintenance of software onboard the spacecraft. The use of these funds will reduce the number of errors in the macro. ... We use graphical notation DRAGON (Friendly Russian Algorithmic Language that provides Visibility) visual representation was proposed to use. « » `' `' programs and processes implemented by onboard equipment [1]. ... DRAGON . ...

Analysis of general features of the chaotic system behavior and investigation of the properties of concrete chaotic sources. ... Analysis of information properties of chaotic systems and chaotic oscillations as concrete objects for information processing and comunications. ... This hypothesis gives a possibility of designing simple mathematical structures accomplishing various processes of information processing using chaos. ... Activities | ... E-mail: chaos@mail.cplire.ru ...

... On discrete arithmetical subgroups of complex Lie groups (in Russian), Math.Sbornik, 1968, vol.77, p.542­545. ... The quotient of Picard group in complex ball B (in Russian), Uspekhi Mat.Nauk, 1973, vol.28:2, p.236­237. ... Discrete reflection groups in the complex ball, I (in Russian), Funct. ... Discrete reflection groups in complex ball,II (in Russian), Group the­ ory and homological algebra. ... Cocycles of complex reflection groups (in Russian), Group theory and homological algebra. ...

... This task constructs the PPS product OM OSW FITS source timeseries from two rate files (source and background) produced by separate runs of EVSELECT on a tracking-shifted, QE-corrected OM fast-mode event-list. ... The counts measured in the source and `background` regions, together with the PSF function evaluated over the corresponding regions, are used to set up equations which are then solved to yield source and background rates evaluated for the nomimal coincidence-loss region (r=12 pixels). ...