Next: Adaptive filtering from Up: Noise reduction from Previous: The Wiener-like filtering . In the above process, we do not use the information between the wavelet coefficients at different scales. ... At each scale, by changing all the wavelet coefficients of the plane by the estimate value , we get a Hierarchical Wiener Filter. ... We get . Estimate the standard deviation of the noise of the first plane from the histogram of . ... Estimate the standard deviation of the noise from . ...

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• Adaptive filtering from the wavelet transform
• The Wiener-like filtering in the wavelet space

... Posts tagged ?spatial statistics? ... As a part of exploring spatial distribution of particles/objects, not to approximate via Poisson process or Gaussian process (parametric), nor to impose hypotheses such as homogenous, isotropic, or uniform, various nonparametric methods somewhat dragged my attention for data exploration and preliminary analysis. ... I decide to discuss Kalman Filter a while ago for the slog after finding out that this popular methodology is rather underrepresented in astronomy. ...

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• Stars with Less Secure Periods
• The AstroStat Slog Pareto distribution
• Comments on: Grating Dispersion [Equation of the Week] By: vlk By: hlee

... The absolute flux calibration of NICMOS will be calculated from observations of standard stars with known flux distributions F( ). ... In order to expand the set of IR standard stars in the appropriate flux range for NICMOS, M. Rieke, R. Thompson, and collaborators at the University of Arizona are making photometric observations of solar-analog stars, which will be used to normalize the solar spectrum to the observed IR magnitudes. ... Relative flux references accurate to 1.5% for standard...

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• http://www.stsci.edu/documents/dhb/webvol2/c21_wfpc1errors.fm6.html
• The Herschel Exploitation of Local Galaxy Andromeda (HELGA). VI. The
• Linear Ramp Filters

... Apache HTTP Server Version 2.2 . ... This document describes the use of filters in Apache. ... The Filter Chain is available in Apache 2.0 and higher, and enables applications to process incoming and outgoing data in a highly flexible and configurable manner, regardless of where the data comes from. ... A wider range of applications are implemented by third-party filter modules available from modules.apache.org and elsewhere. ... There are two ways to use filtering: Simple and Dynamic. ...

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• Digital backends
• Module Index - Apache HTTP Server
• Modul-Index - Apache HTTP Server

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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• Introduction
• Dependence on the Scenario Parameters and Initial Distributions
• #tex2html_wrap_inline12480#-#tex2html_wrap_inline12482# Dependence for the

... Обзор LPR фильтра. Впечатления от наблюдений с LPR фильтром. ... Характеристики цветных фильтров Baader-Planetarium . Мой перевод pdf- файла о фильтрах с сайта Baader-Planetarium (379 кб) . ...

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• Baader NEODYMIUM (Moon & Skyglow) filter

... The radial PSF distribution of the filter FilterId is tabulated in the extension PSF- FilterId . ... radial PSF of U-filter . ... radial PSF of UVW1-filter . ... radial PSF of UV grism 1st order (TBC) . ... The value of the cumulative PSF is normalized to 1.0 at this fixed aperture radius. The aperture radius is listed for each filter elements in the keyword APERTURE. ... Therefore the aperture radius is listed separately for each filter in the keyword APERTURE of the filter extensions. ...

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• How to extract MOS spectra of a point-like source and associated matrices
• Stage Three: ``filter''

Distribution of the analyzed SEPs with different >100 MeV proton fluxes ( J 100 ) at the microwave flux density plane ' S 9 vs. ... 1) General correspondence takes place between intensities of microwave bursts and proton fluxes - J 100 increases when S 9 and S 15 rise. ... 3) Powerful microwave bursts ( S 9 , S 15 >3000-10000 sfu ) with hard radio spectra ( S 9 < S 15 ) correspond to majority of powerful proton fluxes ( J 100 >10 pfu ). ...

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SCORPIO FILTERS . UBVRcIc-filters . Glass filters for Jounson-Cousins photometric system. ... Broad-band filters parameters (filter+optics+CCD EEV42-40): . name . Tmax(%) . ... ASC-file . Image . ... SED-filters . Middle-band filters for Spectral Energy Distribution. ... SED filters parameters (for beam F/4) . ... SED 830 and SED 930 . ... Middle-band filters for comets molecular bands. ... IFP-filters . ... IFP filters parameters (for beam F/4) . ...

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• Description of algorithm
• Spectral energy distribution
• SCORPIO-2 project: filters

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• Titan Observed Through Nine Different Filters on November 26, 2002 | ESO
• Spectral Energy Distribution of GRB 050904 | ESO
• Distribution of Galaxies | ESO

... Up: Science Data Pipelines . ... We designed and developed a package which simulates extragalactic point source data within a given field of view and SIRTF band. ... The simulator is modular and extensible to enable multi-wavelength simulations, has been optimized by utilizing parallel processing capabilities, and will be used to test pipeline software. ... The extragalactic simulator is capable of generating large numbers of galaxies within a given patch of sky for SIRTF pipeline testing. ...

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• The HST Science Data Archive as a Discovery Tool: First Experiment
• The ISOPHOT Interactive Analysis PIA, a Calibration and Scientific Analysis...
• ADASS 2003 Conference Proceedings

... 1) Studying distributions of stars of different ages in irregular and spiral galaxies we found for each galaxy a clear correlation between the age of stars and the spatial size of the subsystems of stars of this age. ... We made a stellar photometry of eight NGC 1313 fields and of its dwarf companion AM 0319-662 and studied the visible distribution of stars of different ages and of metallicity in the galaxy. ... This disappeared galaxy was the cause of the gravitational deformation of NGC 1313. ...

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• Measurement of the dark halo shape in polar ring galaxies

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Telescopes and Observatories . ... The majestic star-forming region in the Lagoon Nebula. The pale ring to the right is an internal reflection in the telescope.€а (Image credit: ESO/ VPHAS+/ V. Kalari and J. Vink (Armagh Observatory) . ... The 18 component images were further processed twice. ... Venu and his colleagues use images like this to identify individual young forming stars in the Lagoon Nebula and determine their ages. ...

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Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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• Vladimir Marsakov Abstracts
• MONTE-CARLO
• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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• Description of SED models

Searching for GRB -GWB coincidence during LIGO science runs Isabel Leonor University of Oregon LIGO-G050216-00-Z Motivation almost 40 years since GRBs were discovered past 15 years has been time of important clues isotropic and inhomogeneous distribution (BATSE); first optical, x-ray, radio counterparts; redshift measurements; association with core-collapse supernovae yet important ...

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• http://zebu.uoregon.edu/2004/es399/iw3.html
• http://zebu.uoregon.edu/~uochep/talks/talks06/G060447-00.pdf
• Physics 410/510 Observational Cosmology

The computed band passes. ... The interim correlator input is filtered by 8 analog filters (50 Mhz wide at the 260 Mhz IF... one for each sub correlator). ... For bandwidths of 25 Mhz and below the real data stream is digitally down converted to complex samples I, Q streams. ... The Top figure is the halfband filter bandpass computed from the filter coefficients. ... The computed filter has aliased power, extra IQ filtering, and two applications of the filter on the resulting real bandpass. ...

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• http://www.naic.edu/alfa/galfa/docs/galspect/spectrometer/galfa-fir.pdf
• lowpass digital fitlers
• compare dlpf shapes

... AMGPS detected a total of 86 methanol masers, 48 of which are new detections. ... It is to be noted that a significant number of methanol masers detected prior to AMGPS were from surveys targeted towards OH masers and HII regions selected from their IRAS colors. ... The total number of methanol masers ! ... For a survey with a flux density limit of 0.27 Jy, the completeness is between 89% and 94%, which from the statistics of AMGPS gives the total number of methanol masers between 1197 and 1264. ...

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• http://www.atnf.csiro.au/research/conferences/student_symposia/ASS2002/programme.ps
• Pre- and Post-Correlation filters
• casacore: casa/Logging/LogSink.h Source File

... The distribution of galactic RCB stars is controversial. Several authors have argued that they belong to a thick galactic disk, and are thus old Population I stars. However, they may alternatively belong to the even older galactic bulge (Population II). ... In either case, the populations are sufficiently old that RCB stars must have relatively low masses ( ). ... These are the only RCB stars for which a distance is known and hence for which an absolute magnitude can be deduced. ...

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• Showing and setting time
• Low-Mass Star Formation
• Armagh Observatory

... The filter "Lighting Effects" is a freebie that came with this program, and in my opinion is practically worth the whole purchase price all by itself. ... You can select different light sources, and combine them with texture channels to warp your image. ... Depending on how you use it, pure white is the highest point on the image, and black the lowest. ... You can adjust the brightness and spread here, or choose other types of lighting. ... Use these if your image is turning out too dark or light. ...

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• Building and Installing the Distribution
• APOD: 2001 June 17 - Colorful Clouds Of Carina
• The Network Time Protocol (NTP) Distribution