Point Source SNR Plots . In this section we present plots which may be used to rapidly estimate signal-to-noise ratio (SNR) for point sources with stellar spectra observed through popular WFPC2 filters. ... There are separate lines for PC1 (light lines) and the WFC (heavy lines), as well as for ATD-GAIN=7 (default, solid lines), and ATD-GAIN=15 (dashed lines). Dotted lines across the top of each plot indicate the onset of saturation. ... We now give a sample SNR calculation using these plots. ...

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• Appendix B: Point Source SNR Plots
• Herschel Key Program Heritage: a Far-Infrared Source Catalog for the Magellanic
• WFPC2 ETC for Point Sources - v4.0

... Proposing for VLBI Time at Arecibo . ... Documentation (Field System, VLBA4 terminal, Mark 5 system) . ... In 2001, the Arecibo Observatory received its hybrid VLBA-MARK IV (VLBA4) data acquisition system, and currently NAIC commits Arecibo to support VLBI observing up to a maximum of 4% of the 305-m's observing time. ... Tracking Time (h:mm) . ... The inclusion of the 305-m Arecibo radio telescope can dramatically boost the sensitivity of VLBI observations, even with its limited source tracking...

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• ALFA Performance at 1665 MHz
• ALFA performance at 1.665 GHz AO Technical Memo 2004-01
• system Performance

... NB The next 2 columns will only be present if the parameter usecat has been set to true . ... Source parameters such as count-rates, magnitudes and semi-major axes, are given in sub-tables-eg the column CORR_RATE is actually a vector column containing the values for each filter. ... QUALITY FLAGS Each source has an associated ``quality flag''. ... 0 1 Source lies above one or more bad pixels . ... QFLAG The quality flag for each source in each filter obtained from the input source-lists. ...

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• Point-like Sources
• Example 1: Point source

... 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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• Upper Limits for Sources not Detected
• Up-date RC-sources Spectra
• Source Positions

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Online Resources . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... H Emission From Point Sources In The Magellanic Clouds . ... Large numbers of the many types of emission-line object that are found in the Magellanic Clouds were first identified through H surveys of one kind or another...

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• casacore: casa/Utilities/Compare.h Source File
• Australia Telescope National Facility
• USNO/ATNF_VLBI

... 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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• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• ADASS 2003 Conference Proceedings
• ADASS 2002 Conference Proceedings

... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

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• Radiopulsars as Sources of Cosmic Rays

Next: *imcnts* - Radial Profile Up: Radial Profiles and Projections Previous: *tabplot* - Displaying a . ... Input a spatially blocked and energy filtered image from above and use with the background determined from the broad-band background map. cl xray xr xspatial xs imcnts addbkg=no # Do not add the background error Source image file : xdata$snr.qp Source region descripter: c 503 513 50 p 503 513 0 360 n=10 # circular region centered on point ...

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• Quantum Efficiency Correction (a.k.a. `flat-fielding')
• SAO RSDC Home Page - RRA - PSPC
• Chandra Images for SNR J0526.0-6604

ACE Real Time Solar Wind (RTSW) data, Kp index, solar and geophysical forecasts are contributed by the U.S. Department of Commerce, NOAA, Space Environment Center and are available to broad community at http://www.sec.noaa.gov/index.html . ... The Kp planetary index is prepared by the U.S. Dept. of Commerce, NOAA, Space Environment Laboratory. from preliminary data provided by the contributing stations and the U.S. Geological Survey. ... Instrument Web site is at URL: http://swepam.lanl.gov ...

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• "Exploration" as a Classroom Resource

... Apache HTTP Server Version 2.2 . ... Filter Types . ... It is important to make the distinction between a protocol and a resource filter. ... If you are writing a filter and you want to know if it is resource or protocol, the correct question to ask is: "Can this filter be removed if the request is redirected to a different resource?" ... So, instead of starting from scratch, we simply point the front of the resource filters for the sub-request to the front of the protocol filters for the old...

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• LASG - Administravia
• Arcetri designs innovative superconductor microwave filters for the Sardinia
• Algorithm

... Visited 5572 times - Selected 51 months ago . ... Visited 6948 times - Selected 51 months ago . ... Visited 4688 times - Selected 51 months ago . ... Visited 7791 times - Selected 51 months ago . ... Visited 9271 times - Selected 51 months ago . ... Visited 7887 times - Selected 51 months ago . ... Visited 4431 times - Selected 51 months ago . ... An online resource for building customized observing lists based on a database with over 10,000 deep sky objects. http://www.virtualcolony.com/sac/ . ...

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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/base/wrapperTestCase.py Source File
• TUI:Scripts:Built In Scripts:NICFPS:Dither:Extended Source
• lsst.tcc: python/tcc/axis/ptCorrFromObs.py Source File

... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

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• di_eks
• Instrumentation
• NEdit.org

Simulations for ALMA: Discussion points Robert Laing European Instrument Scientist Simulations for ALMA IRAM, Sept 8 -11 2008 Issues for the user What simulations are needed to help (inexperienced) users? ... What can we do to promote collaboration ALMA 3 Robert Laing European Instrument Scientist Simulations for ALMA Technical Issues Voltage patterns Critical for I and polarization Start with EM simulations; then use measurements Can we do better than MEM / multiscale clean? ...

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• Monitoring of variable sources at 15 GHz
• G332.4-0.4
• The quasar fraction in a sample of giant radio sources

These pages collect together references to many pictures of the solar system that can be found on the Net. ... Since I originally compiled this list the number of relevant images has grown tremendously. ... http://www.jpl.nasa.gov/pictures/ . ... ftp://dftnic.gsfc.nasa.gov/images/gifs/ . ... http://www.jpl.nasa.gov/galileo/images.html . http://www.jpl.nasa.gov/magellan/images.html . ... http://nssdc.gsfc.nasa.gov/image/planetary/ . ... NASA Image Access Homepage (Planetary Photojournal) . ...

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• "Exploration" as a Classroom Resource
• Jupiter Picture List
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

. Previous . OpenFTS: Open Source Full Text Search Engine . http://openfts.sourceforge.net/ . OpenFTS Mailing List Archives . http://sourceforge.net/mailarchive/forum.php?forum=openfts-general . OpenFTS Contributions . http://openfts.sourceforge.net/contributions.shtml . Includes Link to Search::OpenFTS::Crawler, a Perl-based search engine web spider that uses Tsearch2. PostgreSQL Documentation and Mailing List Search Engine which uses Tsearch2 . http://pgsql.ru

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• Hands On; Lighting Effects1
• Spectracom 8170 and Netclock/2 WWVB Receivers
• Parser sources

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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... Resources . ... Women in Astronomy . ... Moon Resource Guide . ... Astronomy of Many Cultures Resource Guide . ... Black Holes: An Introductory Resource List . ... To be included among the representative women for whom we list individual resources, an astronomer must have had something non-technical about her life and work published in a popular-level journal or book. ... Maintained by two women astronomers, this site includes brief information on women from many fields of science, not just...

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• ASP: Astronomical Pseudo-Science: A Skeptic's Resource List
• ASP: Black Holes: An Introductory Resource List
• ASP: Astronomy and the Environment

. The Source Code Control System is an essential tool for any project with multiple source files or which has several people working with multiple source files. It provides a way to keep track of a source file's development and to prevent it from being altered by more than one person at a time. Putting files under SCCS control . Checking out files . Checking in files . Getting information about files . Creating new releases . Comparing files under SCCS control .

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