... Archives . ... The PCA and ICA is used for separating mixed components with some assumptions. ... The need of source separation methods in astronomy has led various adaptations of decomposition methods available. ... I rarely come up with a paper which gathered and summarized component separation methods applicable to astronomical data. In that regards, the following paper seems useful to overview methods of reducing dimensionality for astronomers. [arxiv:0805.0269] . ... Chandra Blog . ...

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• The AstroStat Slog Blog Archive [ArXiv] 1st week, Nov. 2007
• Comments on: [ArXiv] component separation methods By: hlee By: Sam Leach
• The AstroStat Slog Blog Archive [ArXiv] Bimodal Color Distribution in GCS,

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

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• Number of accreting X-ray binaries of selected types
• Initial Distributions of Binary Parameters

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

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• casacore: components/ComponentModels/DiskShape.h File Reference
• casacore: components/ComponentModels/ComponentType.h Source File
• casacore: components/SpectralComponents/SpectralList.h Source File

... To use this file, you must download and install the IDL runtime virtual machine yourself. ... These contain everything you will need to start the GPI pipeline on that OS. .. comment ## DO NOT EDIT THIS LINE ## Marker for automated editing of this file by gpi _release.py **Version 1.0.0** (2014 Feb 14): * ` gpi _ pipeline _1.0_ compiled .zip http :// www.stsci.edu /~ mperrin / gpi / downloads / gpi _ pipeline _1.0_ compiled .zip `_ - GPI pipeline compiled code only * ` gpi _ ...

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• Comments
• Installing Compiled Executables for use with the IDL Runtime GPI Data Pipeline
• Tables available for pysynphot/Synphot

... 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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• External SAS packages
• Comments

... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...

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... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

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. Comment on J0405+3803 . Our image contains a feature of 25 mJy at 14 mas E-NE from the brightest component. It is not visible in the Caltech-Jodrell (CJ) survey image at 5 GHz (Xu et al. 1995) obtained about 6 years earlier. The 1.6 GHz CJ image (Polatidis et al. 1995) does show an extended feature close to the position in question, but somewhat displaced toward west. VLBApls home page . Last modified: 16 Oct 2000

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... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Modules . ... To enable mod_dav , add the following to a container in your httpd.conf file: Dav On . ... In addition, a location for the DAV lock database must be specified in the global section of your httpd.conf file using the DavLockDB directive: DavLockDB /usr/local/apache2/var/DavLock . ... Use the Dav directive to enable the WebDAV HTTP methods for the given container: <Location /foo> Dav On </Location> . ...

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• CHIANTI atomic database

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

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In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

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• Getting Started in Actor Prolog. Component-Oriented Programming.

Radio data are displayed in the following format: . After the title with name of cluster under examination and with line about kind of data under one, e.g. Radio data [ optical data ] [ radio source identifications ] [ radio spectra (1.0 or 1.1) ] . ... The first line contains the number of radio sources associated with the cluster (these are just those sources with entries in sections 'Radio galaxy', 'Radio source' and 'Radio spectrum' below). ... Radio sources in cluster: 2 # . ...

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• DRAO surveys
• A fast-scan extragalactic source survey at 4.755 GHz
• mod_dav - Apache HTTP Server

Next: Building Software from Heterogeneous Environments . ... The core technologies needed to achieve this flexibility are the message bus , distributed objects , and applications frameworks . ... The message bus is a facility used to bind, at runtime, distributed objects (program components) to construct applications. ... Message bus clients (e.g., components or services) can execute on any host computer connected to the message bus, allowing distributed applications to be easily constructed. ...

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• Starlink's Software Distribution System
• CDS GLU, a Tool for Managing Heterogeneous Distributed Web Services
• The Distributed Astronomical Preprint Service

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

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• Chapter 5. Listing of Installed Components
• HI Self-Absorption in the Canadian Galactic Plane Survey: First Results
• HISA Poster for the 32nd Annual Meeting of CASCA, May, 2001

The (extra)Galactic diffuse interstellar medium: dust, molecules & diffuse bands My presentation will be about the cold diffuse to dense interstellar medium. ... Although we have a general understanding of its composition (dust size distribution, atomic and molecular gas) a number of unknown spectroscopic features, such as the "UV bump", "3.4 micron feature", "IR emission bands" and the "diffuse interstellar bands", remain elusive of identification. ...

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• Results scientific researchs 5
• Work Scan Program + Data Viewer (IDL widget)

What follows is a brief list of benchmarks and discoveries that shaped our ideas on atoms and nuclei. ... Discovery of electrons . ... Comparing this to Faraday's results, one could get " Avogadro's number ", the number of (say) hydrogen atoms in one gram of hydrogen--an enormously large number. ... Similarly, energized atoms are only allowed to exist in one of a number of energy levels. ... By the way, Avogadro's number is 602,000,000,000,000,000,000,000 (6.02 10 23 ) molecules in 1 gr hydrogen. ...

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• The F1 format
• The plot of the magnetic conjugation's time distribution
• ASCII files description

. dfos = Data Flow Operations System, the common tool set for DFO make printable . You are now ready to copy the other dfos components from your reference installation to the new site. Make sure you adapt the configuration to your new site. If you need details, there is more detailed documentation available which however is not maintained anymore and partly outdated. Nevertheless it might prove useful: . initial tool set . creating ABs . finish . Send comments to . Last update: November 9, 2011

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• enterCommentsBulk
• list of DFS Department documentation templates
• ESO - Data Reduction Pipelines Distributed as RPM Packages

... arXiv.org . astro-ph . ... We fit the near-infrared to radio spectral energy distributions of 30 luminous and ultra-luminous infrared galaxies with pure starburst models or models that include both starburst and AGN components to determine important physical parameters for this population of objects. In particular we constrain the optical depth towards the luminosity source, the star formation rate, the star formation efficiency and the AGN fraction. ...

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2014 May version . ... Green D. A., 2014 , Bulletin of the Astronomical Society of India, 42 , 47-58. ( .pdf , or arXiv.org:1409.0637 ) If you make use of the detailed version of the catalogue, then plaese also cite: . Green D. A., 2014, `A Catalogue of Galactic Supernova Remnants (2014 May version)' , Cavendish Laboratory, Cambridge, United Kingdom (available at "http://www.mrao.cam.ac.uk/surveys/snrs/" ). ... Copyright D. A. Green 2014. 25872nd access to this version of the catalogue. ...

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• Comments on Dave Green's SNR Catalogue?
• OptInt PmWiki : MROIDelayLine / Delay Line Prototype Software
• Inference of Coefficients for Use in Phase Correction

Next: stecf.cplucy - Enhanced Two-channel Up: The ``stecf" IRAF Layered Previous: The ``stecf" IRAF Layered . For many years the ST-ECF has developed IRAF tasks and packages for HST and related data analysis. ... To allow wider and more efficient distribution and to bring all components to a uniform level of quality and documentation we have decided to combine these components into a standard-format IRAF package to be called ``stecf''. ...

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• AstroAsciiData