This page holds the archived system performance data (the current data is on the system performance page) . ... Gain,Tsys,Sefd.. Coma,sidelobes, beam efficiency . Pointing errors. Az,za coverage . Hour of day when sources measured. 01sep01 thru 30jul02 (cooled receiver to - room temp amps installed) . ... Hour of day when sources measured (.ps) (.pdf) . ... Hour of day when sources measured. 21aug02 thru 01feb03 (horn focus change to reshimming of elevation rails, pointing model). ...

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• ALFA Performance at 1665 MHz
• alfa C0,1az,3z cor. oct11
• sep11 calibration after installation.

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Facilities . ATNF facilities . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

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• H Emission From Point Sources In The Magellanic Clouds
• casacore: images/Images/ImageTwoPtCorr.h Source File
• casacore: ms/MeasurementSets/MSPointingEnums.h Source File

... The task first computes a background image in order to identify pixels that may be part of a source. The task uses two different algorithms for detecting ``point'' and ``extended'' sources. ... This is necessary because some faint ``point'' sources may have been missed by the point-source detection algorithm, but picked up by the extended-source detection algorithm. ... When the detection process is finished a check is made on extended sources to see if they can be split into two or more sources. ...

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• Point-like Sources
• Comments on Individual Table Columns
• How to extract MOS spectra of a point-like source and associated matrices

STScI . ... You can install this with easy_install or pip. ... If you will be installing on Linux or Macintosh, you also need pip and the compiler packages for your system. ... To install stsci_python, type these commands into a cmd window: c:\python27\Scripts\easy_install stsci.distutils . ... STSCI_PYTHON is now distributed as several separate packages, so that it can more readily fit into the pypi/pip/easy_install ecosystem. ... On Linux or Macintosh, use this command: pip install --download . ...

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• Installing from the Source Code Repository GPI Data Pipeline 1.0 documentation
• Plots for Estimating Point Source SNR
• Appendix B: Point Source SNR Plots

... The essence of the solution is to generate a virtual PC on your desktop PC and install an old Linux distribution, circa 2006, in that. ... There are two major free virtual machines available for Linux, these are VirtualBox and KVM. ... Boot the virtual machine. ... Install a Linux 2.6 kernel if it isn't installed by default (you'll need to reboot the virtual machine after this step): . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIDelayLine/TrolleySoftware) ...

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• OptInt PmWiki : Trolley Software
• OptInt PmWiki : Trolley Software | History
• Computing dispersive atmospheric delay with AATM

Next: Raymond Model Up: *fit* - Fit Data Previous: *fit* - Fit Data . The power law model with galactic absorption will be applied to ROSAT data the extracted earlier The results will be stored in the _prd table in the current directory. input files: rp90_obs.tab, rp90_soh.tab, rp_boh.tab . output file: rp90_prd.tab . ... NOTE: The rp_boh.tab file is not needed for the calculation of the fitted model. ... for help: abs(19:21)*pow(0.5:1.5) # IRAF will not # accept .5 as a valid fraction. ...

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• Spectral Extraction of Point Sources
• The AstroStat Slog VO
• *imcnts* - Find background subtracted counts for a point source

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• ADASS 2003 Conference Proceedings
• AstroWeb -- Internet Resources for Astronomers
• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing

... 1Haynes+ A catalogue at 5 GHz of 915 sources in the Galactic plane is presented. Sources with a peak beam brightness temperature of at least 0.2 K above the surrounding background are included, except in confused regions; a point source of 0.2 K corresconds to 0.26 Jy. ... It was assumed that Hydra A was a point source with a peak flux density of 13 Jy at 5 GHz; this is equivalent to a mean beam brightness temperature of 10.0 K for a beamwidth of 4.1x4.4'. ...

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• Source Positions
• IRAS IDS
• Source Tree Checklist

... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...

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• Parser sources
• Hands On; Lighting Effects1
• Tsearch2 in Japanese

The NICFPS:Dither:Point Source Random script allows you to take a sequence of exposures in a square pattern plus a point in the middle. This pattern is typically used for point sources. ... Any dither point may be omitted by unchecking its checkbox before running the script. ... Dither pattern without randomization . ... Randomization 1. ... Dither pattern with randomization Thanks to Corey Wood for the first implementation of randomization and for the images used in the documentation. ...

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• lsst.tcc: python/tcc/axis/ptCorrFromObs.py Source File
• lsst.tcc: python/tcc/axis/coordConvWithFP.py Source File
• Mirror Controller Actor

... 19 љ*</tt>: landscape textures and data files</li> . ... 73 љIf a file exists in the <em>User Data Directory</em>, it will be used in preference to a file with the same name existing in the <em>Installation Data Directory</em>. ... 79 љ <li>Users who modify files in the <em>Installation Data Directory</em> will likely have their work deleted or overwritten when they upgrade Stellarium. ... In this case , all the files would be in the <em> \<Installation Data Directory>/stars/default</em> directory. ...

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• Stellarium: core/renderer/StelCircleArcRenderer.hpp Source File
• Stellarium: core/modules/LandscapeMgr.hpp Source File
• Stellarium: core/renderer/StelQGL1Renderer.hpp Source File

Beginning from the May of the 1997 we started to publish our daily solar radio observations at RATAN-600 radiotelescope. ... Periscope System: South Sector+Flat Mirror . ... It is possible to track a source by moving the secondary mirror along the arc-shaped railway tracks or to perform azimuthal 2D map synthesis . ... 1) It is possible to simultaneously carry out independent observing programs using individual sectors at various discrete azimuths and secondary mirrors on corresponding railway tracks. ...

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• di_eks
• Radio sources identfification
• harak_e

... a) As source material for the high-school or college curriculum, especially in physics. astronomy and their history. (b) As a source of supplemental projects by high school students or by undergraduates. (c) As material for independent studies, In particular by motivated students who seek to know more about space . ... Those wishing to look up specific topics are advised to use the index file, accessible from the end of any "Exploration" file. ... files not listed and at other resource material. ...

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• Plasma source [Oulu]
• Planetary Picture List
• ULF waves [Oulu]

... a) As source material for the high-school or college curriculum, especially in physics. astronomy and their history. (b) As a source of supplemental projects by high school students or by undergraduates. (c) As material for independent studies, In particular by motivated students who seek to know more about space . ... Those wishing to look up specific topics are advised to use the index file, accessible from the end of any "Exploration" file. ... files not listed and at other resource material. ...

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• The Exploration of the Earth's Magnetosphere"
• Martian mini station (MMS)
• Data sources

Next: Population Synthesis of X-ray Up: Cosmic Rays and Evolution Previous: Supernova Explosions . Immediately after the discovery of pulsars, especially of the Crab pulsar,   it became clear that rapidly rotating NS are copious sources of relativistic particles. ... Figure 37: Evolution of magnetorotational energy of NS in elliptical and spiral galaxies. ...

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• Effect of sources evolution on
• Evolution of the double neutron star merging rate and the cosmological origin
• X-ray Galactic Sources and Binary Radiopulsars as Probes of the Initial Mass

... Light sources: POV-Ray works with point sources of light. ... A real star consists of a spherical light source (the photosphere where the continuum is formed) superimposed by a scattering layer (an atmosphere) responsible for phenomena such as limb darkening and absorption lines. ... For example, in order for the central light source to illuminate the surface, the star must be transparent. ... The POVRay source for creating the white dwarf binary merger movie is given for demonstration purposes. ...

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• Armagh Observatory: Chris Winter [ lte-codes ]
• IAJ: Resources: Observatories
• Simon's links to Grid resources on the WWW

home resources . SEARCH ASP SITE: Match ALL words Match ANY word . ... Books . Favorite Links . ASP Educational Resources . Your resource for unique education materials, ASP favorites, technical publications, and more.. ... Your purchases help support the education programs of the ASP. We feature our favorite new Astronomy books with short descriptions. Looking for archived Books of Note? ... Feature Book . ... Feature Link . ... Publications | ... education | resources | ...

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• Astronomical Society
• ASP: Astronomical Pseudo-Science: A Skeptic's Resource List
• ASP: Educational Resources

Radio Interferometry Principles . Radio Interferometry Signal Processing . ... A radio interferometer consists of a pair of directional antennas that are tuned to receive radio emissions from a source in a desired RF band. ... The antennas are pointed at the radio source of interest and are set up to receive the signal and process it into a form suitable for transmission to the correlator. ... In connected element interferometry, the digital signal goes directly to the correlator. ...

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RTT150 . ... This search system is designed for generating the necessary information on series of pointings (observations of each source consist of sets of exposures with different filters and sometimes with different exposure times) for observed sources. Search results appear at the separate page as a table with the following data: . DATE - real (not evening!) observations date (in YYYY-MM-DD format); . ... Bin - minimal CCD binning mode (may vary during the observations); . ...

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... Global WWW Starting Point and Compilations . ... HTML Manuals and Tutorials . ... ESA/Estec/SAI Home Page . ... Centre de Donn es astronomique de Strasbourg (CDS) Home Page. ... Bibliographical Engine ( xxx forms) - Italian mirror . ... The NASA Home page. An Web Resource Collection by Masters Degree Online . ... The local TCSH . ... The Web Anti-Spam page. ... Apple Italian Home Page . ... Walnut Creek CDRom Home Page and the Italian Mirror . ... A good hotlist of HTML resources around the Web. ...

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• Radioastronomy reduction procedures
• mod_dir - Apache HTTP Server
• HwB: Adapter Tutorial (Offline)