... Posts tagged ?posterior distribution? ... stat.AP:0811.1663] . Open Statistical Issues in Particle Physics by Louis Lyons . ... Category: arXiv , Bayesian , Cross-Cultural , Data Processing , Frequentist , High-Energy , Methods , Physics , Stat | ... Accounting for Spatial Correlation in the Scan Statistic by Loh &Zhu [stat.AP:0712.1458] provides a picture that helps us to understand excessive false alarms in source detection when the image data set is based on the Poisson point process. ...

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• The AstroStat Slog Pareto distribution
• The AstroStat Slog distribution
• The AstroStat Slog Blog Archive chi-square distribution [Eqn]

Aims: We present an analysis of a galaxy (SAGE1CJ053634.78-722658.5) at a redshift of 0.14 of which the infrared (IR) emission is entirely dominated by emission associated with the active galactic nucleus. Methods: We present the 5-37 ЮМm Spitzer/IRS spectrum and broad wavelength spectral energy distribution (SED) of SAGE1CJ053634.78-722658.5, an IR point-source detected by Spitzer/SAGE. ... We compare the source with models of emission from dusty tori around AGNs. ...

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• ``Robots Are Us'': Automated Information Discovery
• Techniques and Review of Absolute Flux Calibration from the Ultraviolet to the
• Infrared Spectral Energy Distributions of Nearby Galaxies

Radio pulsars strictly periodic signals 14.03.2016 B 10 G;E 10 V / cm 12 10 2 Individual pulses and average profile of pulsar 14.03.2016 3 Average profiles of pulsars 14.03.2016 average energy distribution of pulses by phase of period. ... 14.03.2016 5 2695 Giant pulses (GPs) of pulsar Intensity, a.u. Time, ms Pulses that exceed the average profile over 30 times were called giant pulses. ... 2005) 14.03.2016 8 Individual pulses energy distribution 1937+21. ...

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• Fractal Matter Distribution

Results on nonequilibrium distributions of charged particles and radioisotope sources of current are as the following: . the new power-law distribution of charged particles in nonequilibrium media, for example, in the thin metalic films, under powerful energy source pumping were obtained ( together with V.I.Karas, V.M.Kontoriovich, V.E.Novikov); . ...

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• The Discovery of Atoms and Nuclei
• The summary plot of time distribution of the multisatellites magnetic
• The plot of the magnetic conjugation's time distribution

... Latest SNe . ... Statistics on Supernovae Discoveries . Discoveries by amateurs have been rising in recent years. ... And the next page shows the amateurs who have discovered a supernova: . ... All SNe since 1885. (external link) . The next pages relate to all supernovae discovered so far, their properties and their parent galaxies: . SNe distribution according to galaxies' morphological type. ... SNe distribution according to their magnitudes. All SNe distribution since 1885. ...

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• Building and Installing the Distribution
• The Network Time Protocol (NTP) Distribution
• Supernovae distribution according to their magnitudes.

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• Velocity Distribution of the XLSS-03 Cluster | ESO
• Distribution of Exoplanet Distances | ESO
• ESO - ESO-MIDAS Releases and Distribution

... Edgeworth Kuiper Belt Objects (EKOs) orbit beyond Neptune and offer important clues about the formation of our solar system. ... Ascertaining the true extent of the transneptunian objects (TNO) inclination distribution is important for planning TNO surveys. ... Past surveys of TNOs are probably a poor representation of the true distribution of EKO inclinations because most were found in surveys centred on the ecliptic. ...

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• New Approaches to Risk Assessment from Near-Earth Objects
• Galactic distribution and absolute magnitudes
• Refereed Journal Publications 2004

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During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the 'asteroid' was found on March 30 to have a short tail! ... it was renamed periodic comet P/2004 CB (LINEAR). ... Back to Previous News . Siding Spring Survey Main Page . ... Follow-up Astrometry with the 1.0-m at SSO . Previous News Items . Anglo-Australian Near Earth Asteroid Survey 1990-96 . ...

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• The SMS Survey
• The High-Z SN Search Description
• Lecture 19: Probability Distribution Functions

Discovery of four binary millisecond pulsars . D. R. Lorimer (The University of Manchester, NRAL, Jodrell Bank, UK), . A. G. Lyne (The University of Manchester, NRAL, Jodrell Bank, UK), . M. Bailes (ATNF, CSIRO, Australia), . R. N. Manchester (ATNF, CSIRO, Australia), . ... B. Stappers (MSSSO, ANU, Australia), . S. Johnston (RCfTA, University of Sydney, Australia), . F. Camilo (The University of Manchester, NRAL, Jodrell Bank, UK) . ...

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• correlator:distribution [ATNF VLBI Wiki]
• A Tutorial on Radio Pulsars
• The spectral energy distribution of PKS 2004-447: a compact steep-spectrum

Next: Power of test Up: Basic principles of Previous: Test statistics . In principle, it is possible to compute a value of the statistic for a single frequency and to test its consistency with a random signal ( ). ... The factor N means that there is an increased probability of accepting a given value of the statistic as consistent with a random signal. ... In the command individual descriptions, we often refer to probability distributions of specific statistics. ...

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• Some statistical trends and distributions
• Sky and redshift distribution
• Distribution Policy

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Test of the Initial Mass-Ratio Distribution
• Frequency distribution of galactic binaries
• Old neutron star distribution in the Galaxy

... Up: Software Systems and Tools . ... The Starlink Software is a collection of astronomical packages and utilities comprising over 120 separate components. When built, the system needs between 500 and 650 MB disk space (without source) making it ideal for distribution on CD-ROM. Each component has been individually packaged into an easy-to-install bundle for users to obtain over the Internet via a ``point and click'' WWW interface from the Starlink Software Store. ...

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• The HST Science Data Archive as a Discovery Tool: First Experiment
• ADASS 2002 Conference Proceedings
• Distributed Data Systems, Data Mining

... Class . ... FRAMES NO FRAMES All Classes . ... FIELD | CONSTR | METHOD . DETAIL: FIELD | ... java.lang.Object ij.plugin.Distribution . ... public class Distribution . ... This plugin implements the Analyze/Distribution command. ... This method is called when the plugin is loaded. void . ... Constructor Detail public Distribution () . ... This method is called when the plugin is loaded. 'arg', which may be blank, is the argument specified for this plugin in IJ_Props.txt. ...

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• Uses of Class ij.plugin.Distribution (ImageJ API)

... Right: cold gas traced by [CII] emission (red) accreting onto a primeval galaxy (green) at z=7.1 ( Maiolino et al. 2015 ) (image credit: ALMA Press Release ) . ... 2010 , Cicone, Maiolino et al. ... 2012 , Cicone, Maiolino et al. ... Right: observed distribution of the average stellar metallicities of passive and star forming galaxies in the local universe, supporting starvation/strangulation as primary quenching mechanism in low/intermediate mass galaxies ( Peng, Maiolino, Cochrane 2015 ). ...

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• James Gordon - Latex
• OptInt PmWiki : PmWiki / Page File Format
• OptInt PmWiki : Page File Format

... Binary orbits in the acceleration/period plane . Circular Orbits . ... We first present the equations for the period and acceleration of a pulsar in an eccentric binary system as a function of its position in the orbit. ... In Freire, Kramer & Lyne (2001) (from where most of this text and following equations are taken), we describe in more detail how circular binary orbits can be determined from the observed periods and accelerations of the pulsar. ... where is the orbital period of the binary. ...

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• weight on turret floor
• The SMUDGES Survey
• Pulsar Highlights - First ALFA MSP

... 13-Aug-2014 12:13 106K lk_20140815_0905.tar.. 15-Aug-2014 09:06 106K lk_20140901_0823.tar.. 01-Sep-2014 08:23 103K lk_20141016_1324.tar.. 16-Oct-2014 13:25 103K lk_20141211_1708.tar.. 11-Dec-2014 17:08 103K lk_20150430_0315.tar.. 30-Apr-2015 03:15 103K lk_20150430_0420.tar.. 30-Apr-2015 04:20 103K lk_20150818_1511.tar.. 18-Aug-2015 15:11 104K lk_20151113_1903.tar.. 13-Nov-2015 19:04 105K lk_20160314_0610.tar.. 14-Mar-2016 06:11 105K . ...

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• The NMW survey homepage

XMM-Newton CCF Release Note XMM- CCF -REL-169 EPIC MOS low energy response and Quantum Eфciency R. D. Saxton, Steve Sembay 5 August 2004 1 CCF components Name of CCF VALDATE EVALDATE Blocks changed XSCS ag EMOS1 QUANTUMEF 0016. CCF 2000-01-01 QE TOTAL NO EMOS2 QUANTUMEF 0016. CCF 2000-01-01 QE TOTAL NO EMOS1 REDIST 0035. CCF 1999-12-10 2000-07-15 CCD REDISTRIBUTION-n NO EMOS1 ... This excess was responsible for small underestimates of the Galactic absorption column. ...

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• Null-hypothesis probability distribution for a weighted sum of Poissonian
• Routines to return random numbers in various distributions
• EMOS redistribution

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• http://observ.pereplet.ru/images/SN101026/sn.html
• http://observ.pereplet.ru/images/SN101219/sn.html
• MASTER OT 054547.15+091200.3 discovery

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Search for distant radio galaxies in SAO
• Vitaly Goranskij, SAI/Moscow Univ.
• The peculiar post-AGB supergiant IRAS04296+3429: optical spectroscopy and its