Next: Auxiliary utilities Up: MIDAS utilities for Previous: Time series analysis . The commands COVAR/TSA serves for the calculation of the covariance and autocovariance functions. ... COVAR/TSA -- . ... Edelson and Krolik's (1988) method is used for the estimation of the cross correlation function (CCF) of unevenly sampled series. ... DELAY/TSA -- . delay analysis with interpolation: The command computes the time lag function for two time series by the Press et al. (1992) method. ...

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• Auxiliary utilities
• Time series analysis in the frequency domain

... Archives . ... Such eminent astronomer said already least absolute deviation over chi-square , if I match simple mean residual and mean square residual to relevant methodologies, in order. ... Anyway, if one is sure that the data/parameters of interest are sampled from normal distribution, Eddington?s statement is better to be reverted because of sufficiency . ... Instead of sample standard deviation, use absolute mean deviation (simple mean residual, Eddington?s words) to quantify uncertainty. ...

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• The AstroStat Slog probability
• The AstroStat Slog Blog Archive my first AAS. VI. Normalization
• The AstroStat Slog normalization

The LCDM paradigm: successes and challenges on scales of galaxies Anatoly Klypin (NMSU) LCDM · · · · DM profiles, concentrations, .. Clustering of galaxies: P(k) and correlation functions Satellites: abundance, number-density profiles Galaxies and Dark Matter: abundances Dwarfs. ... Springel et al 2008. ... Klypin et al 2010. ... Observations - LCDM: just enough Magellanic Clouds Observations LCDM Vmax > 50 km/s Busha et al 2010 Dark matter profiles: standard LCDM Aquarius simulation. ...

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• http://mavr.sao.ru/hq/lizm/conferences/pdf/2003/2003_p210.pdf
• Description of algorithm

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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• XV-IMAGE

SLR Observations at the Quasar Network Stations I.Gayazov, V.Mitryaev, S.Smolentsev, I.Rahimov, A.Diyakov, V.Shpilevski, V.Pshenkin, Ya.Rets Institute of Applied Astronomy, Saint Petersburg, Russia WPLTN-2012 September 24 - 28, 2012 Saint Petersburg SLR systems installation at the Quasar observatories Observatory Zelenchukskaya Badary Stage Dome building System installation Testing Dome building System installation Testing Dome building ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/ALESH.PS
• Keywords_107
• IAA VLBI Analysis Center

... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...

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Determination of short-term proper motions of fast stars with Pulkovo Normal Astrograph. ... Khovritchev Laboratory of Astrometry and Stellar Astronomy of the Pulkovo Observatory, RAS, Saint-Petersburg Observations Normal Astrograph (D/F=33 cm/3.5m), CCD camera: S2C, FOV = 18x16 arcmin, Pixel size 900x900 mas Determination of the new proper motions of 413 LSPM stars 1 epoch : CCD-surveys and catalogs -- M2000, CMC14, 2MASS, SDSS DR7 2 epoch : CCD-observations with the ...

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• http://www.puldb.ru/nikolaev_2011/PUB_NIKOLAEV_2011/plates2.pdf
• Pulkovo Databases
• Pulkovo databases: photometric observation

This is how a typical dispersion modeling result looks when shown as a map. ... Their numerical values are shown at the top. White normally means no data, but high values may be also shown as white if above the fixed high limit (that is, if no automatic normalization is used for colors). Note that calculations were done both for cell positions and for station positions, so both are colored. PO territories are filled by color corresponding to the average value of cells overlaying them. ...

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• Dr. Victoria I. Prokhorenko

... 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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• Recognition of Anomalous Events
• ADASS 2002 Conference Proceedings
• What Happened to the Results?

... User Guide ] Task: uvfstats Purpose: Print flagging statistics. ... Key: line Normal line parameter. ... This is the default. overall Give a single overall statistic. baseline Determine statistics by baseline number. antenna Determine statistics by antenna number. channel Determine statistics by channel number. ... Possible values are absolute Give flagged correlations as an absolute number rather than a percentage. unflagged Give statistics about the unflagged (rather than flagged) correlations. ...

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• Pulsar Group Observing/Dfb-fold
• casacore: casa::Normal Class Reference
• uvstat

Statistics for Astronomy III: Non-parametric statistics , Error Analysis and Confidence Inter vals B. Nikolic b.nikolic@mrao.cam.ac.uk Astrophysics Group, Cavendish Laboratory, University of Cambridge http://www.mrao.cam.ac.uk/~bn204/lecture/astrostats.html October 2008 Goals for this Lecture Non-parameteric statistics Kolmogorov-Smirnov test U-test (MannWhitney Wilcoxon) Likelihood versus posterior probability Basic ... Probability theory and the model give: P ({xi }| ...

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• http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l2.pdf
• http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l1.pdf
• http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l8.pdf