Next: Search Algorithms Up: Computational Methods Previous: Image Restoration . The previous sections have described the most frequently used computational techniques for image handling in optical astronomy. After the images have been calibrated and manipulated to give the best representation of the data the astronomical information has to be extracted. For frames which contain a large number of objects automatic methods are required to locate them. ... Search Algorithms . ...

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... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...

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• Indexing and Searching Distributed Astronomical Data Archives
• Automatic Detection of Linear Features in Astronomical Images
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared

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) . ...

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• SAI SN RESEARCH GROUP

Next: Calling Parameters Up: CAL_getRedistribution Previous: CAL_getRedistribution Contents . The redistribution function of the CCD's is parameterized per CCD and per node. ... It combines the X-ray absorption probability in silicon with an empirical parameterization of the generated charge signal, which is then folded by a Gaussian for noise representation. ... For a given photon of energy (in eV), and absorption at , the collected charge (in eV) is parameterized with the empirical model . ...

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• Description
• Parameters

... After the data from an observation have been received and processed through the STScI pipeline, hardcopy products ( paper products ) are generated which summarize the data obtained. ... Paper products typically summarize the set of exposures that constitute a visit in the Phase II proposal. ... The content of the pages is as follows: . ... Observation Summary: a table summarizing the proposal information for each exposure in the present set, including processing and data quality flags ( Figure 15.4 ...

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• Optional Parameters [Optional_Parameters]
• Model Fitting
• Frequently Asked Questions GPI Data Pipeline 1.0 documentation

... We now describe the input parameters to the self-calibration tasks. ... For selfcal , you need not perform source , dra , or ddec selection if you use the selradec option (see below). minants : The minimum number of antenna that must be present before the tasks will attempt to find a solution. ... and phase : This determines whether the self-calibration tasks solve for just phase ( options=phase , which is the default) or amplitude and phase solution ( options=amplitude ). mfs : . ...

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• ccontsubtract CentralProcessor 0.11 documentation
• Computation
• User Parameters - Bandpass Calibration CentralProcessor 0.11 documentation

... Donate to Support Science Literacy . ... 2016 Annual Awards . The ASP is accepting nominations for the organizationòÀÙs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach. ... Shop the AstroShop . ... The Astronomical Society of the Pacific (ASP) is accepting nominations for the organizationòÀÙs national annual awards which recognize special achievements in astronomy research, technology, education, and public outreach.. ...

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• ASP: Family ASTRO for Families and Friends: Getting Involved and Frequently

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

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• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
• Svetlana G. Pugacheva

... In the past month, I?ve noticed relatively frequent paper appearance in arxiv/astro-ph whose title includes Bayesian or Markov Chain Monte Carlo (MCMC) . ... astro-ph:0708.2340v1] Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm by L. Miller et. al. [astro-ph:0708.1871v1] Dark energy and cosmic curvature: Monte-Carlo Markov Chain approach by Y. Gong et. al. in addition to the previous posting in this slog, [ArXiv] Bayesian Star Formation Study. ...

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• The AstroStat Slog nuisance parameter
• Model Spectra for Spectral-Fitting Program
• *plcreate* -- Defining a Region

... Learning set is formed on basis of the Taken' algorithm. ... For 10, 100, 200, 300 day forecast the time lag was correspondingly = 10, = 100, = 200, = 300. ... For every forecast (10, 100, 200, 300 days) ANN started k = 10 times. ... On figure, 1 it is shown the MAE and RMS statistics for 10-, 200- and 300-day forecast for Xp : M AE = 1 n i=n |f orecastav erag ei - realv aluei |, ... i=1 139 RMS 300 MAE 300 RMS 200 RMS 10 MAE 10 MAE 200 Figure 1: 10, 200, 300 day statistics for Xp forecast. ...

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• Pulkovo Observatory
• Pulkovo VLBI Analysis Center

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• DFOS: Frequently Asked Questions
• Stellar parameters from calibrations of spectral types
• The Brightness of the Night Sky

... Àñòðîíîìè÷åñêàÿ íåäåëÿ ñ 11 ïî 17 àïðåëÿ 2016 ãîäà . ... Àëåêñàíäð Êîçëîâñêèé . ... Äåíü îòêðûòûõ äâåðåé íà Ïóùèíñêîé ÐàäèîÀñòðîíîìè÷åñêîé Îáñåðâàòîðèè 09 àïðåëÿ 2016 ãîäà . ... Ïîëíîå ñîëíå÷íîå çàòìåíèå 9 ìàðòà 2016 ãîäà . ... Ïîëíîå ëóííîå çàòìåíèå 28 ñåíòÿáðÿ 2015 ãîäà . ... Çàòìåíèå, êîòîðîå ïðîèçîéäåò 28 ñåíòÿáðÿ 2015 ãîäà, ÿâëÿåòñÿ ïîâòîðåíèåì ÷åðåç ñàðîñ (öèêë ïîâòîðåíèé çàòìåíèé ðàâíûé 6585 äíåé èëè 18 ëåò 11 äíåé) ïîëíîãî ëóííîãî çàòìåíèÿ îò 16 ñåíòÿáðÿ 1997 ãîäà ñ ìàêñèìàëüíîé ôàçîé 1,20.....

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... Calculations of at least two runs with different values of a parameter are required in order to discover to what extent the results depend on the , if at all. ... In order to study how the final statistical distributions depend on the initial functions, the method of Green functions is used. ... Then we can restore any distribution on this parameter (with a certain accuracy) by summing the results for each interval with the appropriate weight. ...

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• Initial parameters of compact stars
• Initial binary parameters
• Initial Distributions of Binary Parameters

Astronomical Data Analysis Software and Systems VII ASP Conference Series, Vol. ... News on the ISOPHOT Interactive Analysis PIA C. Gabriel ISO Science Operations Centre, Astrophysics Division, Space Science Department of ESA, Villafranca, P.O. Box 50727, 28080 Madrid, Spain, Email: cgabriel@iso.vilspa.esa.es J. Acosta­Pulido 1 Max­Planck­Institut f˜ur Astronomie, Heidelberg, Germany I. Heinrichsen 1 Max­Planck­Institut f˜ur Kernphysik, Heidelberg, Germany Abstract. ... 1996). ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/dolenskym1.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/teubenp.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/decuyperjp.ps.gz

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Determination of the Detector Parameters
• Tunable Kernel Parameters?
• Kernel tunable parameters

... Stellar Evolution . Nucleosynthesis in Stars . The Evolution of Star Clusters . JAVA Physics Lab . Alternative Energies Class . Steve Kevan's Physics 251 Class . ... Talk on Solid State Physics of CCD detectors . Talk on Cosmological Issues . ... Digital Spectra of Stars . NETexperts E-mail List . The Electronic Universe Project e-mail: nuts@moo.uoregon.edu ...

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• Cosmological Issues for Theorists

In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...

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ALMA | ... Phase Correction Algorithms | ... On this page, we describe what the phase correction algorithms set out to do and the framework we have developed to optimally use all of the available information. ... We are developing a Bayesian framework to combine all the information we have about the current and future meterological conditions (which are naturally accommodated as priors in a Bayesian scheme) with detailed physical models of the atmosphere. ...

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• Dave Green's `cubehelix' colour schemes
• Data | ALLSMOG
• Paper I: Method Bojan Nikolic web pages (r. 329)

... Chapter 1. ... Problems of observational radio cosmology (6) . ... Analysis of radio astronomical data (32) . ... Data analysis system (33) . ... Actuality, goals and results to depend (45) . ... Interactive processing of continuum radio spectra of radio sources (72) . ... Creation of the astrophysical catalogs data base CATS and its application for selection and analysis of radio galaxy samples (112) . ... Data and methods (176) . ... Results of analysis of known radio galaxies data (179) . ...

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• Lectures
• Radio Sources Parameters

...  ÷åòâåðã, 14 àïðåëÿ 2016 ã., ñîñòîèòñÿ ñåìèíàð êàôåäðû àñòðîôèçèêè. Ïîâåñòêà äíÿ . ... Íà÷àëî â 11 ÷àñ.15 ìèí. Àóä. ...  ÷åòâåðã, 31 ìàðòà 2016 ã., ñîñòîèòñÿ ñåìèíàð êàôåäðû àñòðîôèçèêè . ...  ÷åòâåðã, 24 ìàðòà 2016 ã. , ñîñòîèòñÿ ñåìèíàð êàôåäðû. ...  ÷åòâåðã, 17 ìàðòà 2016 ã. , ñîñòîèòñÿ çàñåäàíèå êàôåäðû. ... ÎÑÏ ÍÈÈ ÏÌÌ Íàöèîíàëüíîãî èññëåäîâàòåëüñêîãî Òîìñêîãî ãîñóäàðñòâåííîãî óíèâåðñèòåòà) . ... Copyright 2016 Àñòðîíîìèÿ â Ñàíêò-Ïåòåðáóðãñêîì óíèâåðñèòåòå . ...

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• Database of Optical Properties -- Level: subpage
• AI SPbU library of scattering codes
• Polarization properties (transmitted radiation)