... 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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• harak_e

... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• Simulations of Pinhole Imaging for AXAF: Distributed Processing Using the MPI
• CDS GLU, a Tool for Managing Heterogeneous Distributed Web Services
• Distributed Searching of Astronomical Databases with Pizazz

O.R. Hainaut, ESO, H. Boehnhardt, MPS, and S. Protopapa, UMd . MBOSS Home Tables Plots Credits . The absolute R magnitude M11 and colour distributions are represented as histograms and as their cummulative fraction. Grt is the spectral slope. All the plots for which at least one object is present are available in GIF and in Encapsulated PostScript. ... Note that the colours are sorted alphabetically after the M11 (absolute magnitude) and GRT (spectral slope) plots. ... GIF . EPS . ...

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• Redshift Distribution
• ESO - Data Reduction Pipelines Distributed as RPM Packages
• Colours and magnitudes

... Apache HTTP Server Version 2.2 . ... mod_proxy extension for load balancing . ... Thus, in order to get the ability of load balancing, mod_proxy and mod_proxy_balancer have to be present in the server. ... Enabled via lbmethod=byrequests , the idea behind this scheduler is that we distribute the requests among the various workers to ensure that each gets their configured share of the number of requests. ... lbfactor is how much we expect this worker to work , or the workers's work quota . ... worker...

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• Extinction and transformation models
• Some statistical trends and distributions
• HyperLEDA documentation: Resolved Kinematics

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Database of Optical Properties -- Level: subpage

... Posts tagged ?likelihood ratio test? ... I wonder what Fisher, Neyman, and Pearson would say if they see ?Technique? after ?Likelihood Ratio? instead of ?Test.? ... Continue reading ?Likelihood Ratio Technique? Tags: Fisher , likelihood principle , likelihood ratio technique , likelihood ratio test , Neyman , Pearson . Category: Algorithms , arXiv , Astro , Bayesian , Cross-Cultural , Data Processing , Fitting , Frequentist , Jargon , Methods , Objects , Stat , Uncertainty | Comment . ...

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• The AstroStat Slog Blog Archive Likelihood Ratio Test Statistic [Equation of
• A matrix of tweets from #AAS225
• A matrix of tweets from #AAS223

... The colors indicate the relative motions of galaxies with accurately measured distances, with shades of green and blue indicating motions toward us and shades of yellow to red indicating motions away from us. Our nearest neighbors have only small relative motions (represented by yellows and greens), as seen best in the exploded view of the right panel. We, along with all these nearest neighbors, are moving together toward the lower right corner of the figures. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEA1217C7-5BDD-44A2-A705-9BBD496DED2F%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7EF5083A-E00E-4CE2-BF00-8F7C1C6B5C0C%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B229F8C3F-3680-4698-80FC-80501DD2D7BA%7D

... A hundred years later, a handful of Tunguska-sized asteroids have been spotted by telescopes, but most remain unseen. The asteroid designated 2008 TC3 , which made the news on October 6th before colliding with the Earth on October 7th was too small to constitute a part of the "Earth impact hazard". ... 2008 TC3, for example, finally exploded in the atmosphere above Sudan . ... Wednesday, 8 October 2008 01:15 . International Year of Astronomy, Ireland National Node . ...

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• Armagh Observatory
• Atmospheres
• White Dwarf Merger Movie

Astronomy Picture of the Day . A Universe in a Box . ... 21.08.1997 . ... A cube of this universe was cut out and displayed, with each side being about 8 million light years across. ... At the bottom a single slice through this cube is displayed, with helium abundance superposed with a wire mesh. ... August . ... August 1997 . ... 1997 1998 . ... NASA Web Site Statements, Warnings, and Disclaimers . ... U. Based on Astronomy Picture Of the Day . Publications with keywords: universe . ...

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• Journal "Peremennye Zvezdy"
• Астронет > A Universe in a Box
• XWare > APOD

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. August 21, 1997 . A Universe in a Box . ... It is one computerized guess of how gas in the universe was distributed billions of years ago, at redshift 3, when the universe was only a quarter of its present age. ... A cube of this universe was cut out and displayed, with each side being about 8 million light years across. ... About APOD > . ...

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• Building and Installing the Distribution
• Type of Galaxies.
• The Network Time Protocol (NTP) Distribution

documentstyle{preprint} \begin{document} \title{ GLOBULAR CLUSTERS AS DISTANCE INDICATORS } \author{Bradley C.\ Whitmore\\ \\ Space Telescope Science Institute\\ \\ 3700 San Martin Drive\\ \\ Baltimore, MD, 21218\\ \\ whitmore@stsci.edu} \pub{{\em the proceedings of}\\ ~\\ The Extragalactic Distance Scale,\\ ~\\ {\em held May 1996 in Baltimore, MD}} \maketitle \begin{ abstract } The globular cluster luminosity function ( GCLF ) for bright elliptical ...

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• http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/smov4notes/SMOV4STATUS&PLANNINGMTG20MAY09.pdf
• WFC3 Data Handbook
• Comments

... The upward propagating HF wave is reflected at a particular height. ... The instabilities seen by the radar shortly after the HF is turned on can be divided into two types according to the degree of sophistication required in the model describing the response to the E field of the HF wave. ... The first kind occurs at a particular height determined by k vector and frequency matching conditions on the HF wave, the low and high frequency plasma waves, and the radar EM wave. ... Incoherent Scatter . ...

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• HISA Poster for the 197th Meeting of the AAS, January, 2001

... Trouble Reports . Anonymous FTP . APO35 Mailing Lists . ... These are distributed to people at each member institution, including someone who is reponsible for making the information available to other people. The trouble reports presently exist as paper in a notebook. ... Various files are distributed via anonymous ftp, including the current version of Remark, drawings, and some outdated documentation that has not been transferred to WWW. The address is: ftp.apo.nmsu.edu. ...

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• op020202cloudcam
• field

... Play Information * Game : DOOM II Episode and Level # : MAP01 Single Player : Yes Cooperative 2-4 Player : Yes Deathmatch 2-4 Player : Yes Difficulty Settings : Yes New Sounds : No New Graphics : No New Music : No Demos Replaced : None * Construction * Base : New level from scratch Editor(s) used : DOOMED The Real Thing v4.2 Known Bugs : There seems to be a "hall of mirrors" type effect when looking down the length of the sub-bay. ... It is intermittent, and shouldn't effect play. ...

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• Energy distribution
• Data reduction: histograms and pdf's
• Long description for change bar example

... To get access to the software you must be registered at the ASC RadioAstron Server "ra.asc.rssi.ru" ------------------------------------------------------ IMPORTANT: At present the software "FAKERAT" runs only under 32 bit Linux workstation in X windows with C shell script. ... All procedure runs under C shell. ... Copy all files from the given directory to your computer. ... Then, copy txt-file representing the current version of orbit to the "orbit" subdirectory located in "fakerat_07041020". ...

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• RadioAstron meeting

The radial distribution of metallicity of star-forming galaxies in a galaxy cluster can inform us about the mass assembly and enrichment history of the galaxy cluster. ... Both galaxy clusters are cool-core clusters at redshift z т?? ... The gas-phase metallicity of star- forming galaxies in MACS1115+01 exhibit anti-correlation with projected distance т??0.15 ТБ 0.08 dex/Mpc, whereas the radial metallicity distribution of RXJ1532+30 is statistically flat (т??0.09 ТБ 0.12 dex/Mpc). ...

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• http://www.mso.anu.edu.au/~kcf/ATA/ATA_assign_10.pdf
• Proposed Facility
• Penny Sackett presents John Anderson with a commemorative sculpture

An investigation of the spectral energy distribution (SED) of the compact steep-spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS 2004-447, is presented. ... Analysis of a non-contemporaneous, low-resolution optical spectrum suggests that the narrow-line region (NLR) is much more reddened than the X-ray emitting region suggesting that the gas-to-dust ratio in PKS 2004-447 may be very different than in our own Galaxy. ...

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• casacore: tables/Tables/ExprUDFNode.h Source File
• casacore: tables/Tables/ExprUDFNodeArray.h Source File
• The ATNF Electronics Group : AT Distributed Clock

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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• MONTE-CARLO
• Mid Scales Role
• POWER SPECTRUM OF THE IRREGULARITIES AND IT'S FIXING

... Two high school students from Texas and Louisiana are the winners of the 2012 Priscilla and Bart Bok Awards for their astronomy projects presented at the Intel Science and Engineering Fair in Pittsburgh, Pennsylvania in May. The awards were presented on May 18 by the Astronomical Society of the Pacific (ASP) in partnership with the American Astronomical Society (AAS), supported by funding from the National Science Foundation (NSF). ... The Bok prize is named for Bart and Priscilla Bok. ...

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• ASP: The New and Improved Hubble Space Telescope
• ASP: Astronomical Society of the Pacific to Present 2009 Annual Meeting,

Microsymposium 34, MS059, 2001 A HIPSOMETRICAL FEATURES OF THE LUNAR SURFACE FROM THE CLEMENTINE MISSION. ... The lack of extensive mare basalt fill in the South Pole ­ Aitken Basin, despite the thin crust in this region, suggests hemispheric compositional asymmetry in the deep lunar interior [1]. ... According to new data, the depths of Mare Imbrium, Mare Frigoris, Mare Fecunditatis, Mare Moscoviense are 0.5 km deeper than previous results indicated. ... 1994) The Clementine Mission to the Moon. ...

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• http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf
• http://selena.sai.msu.ru/Rod/Publications/ms38/ms035.pdf
• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf