... It may be desirable to apply (in addition to the source selection described above) some definite upper limit to the number of sources to be plotted - say, to plot only the first 50 brightest sources. Such a limit may be difficult or impossible to achieve by use of the expression parameter. ... The parameter ncutsortexpression has been provided to allow the sources to be sorted. ... slconv srclisttab=bert.ds:SRCLIST radiusexpression='RATE' withncut=yes ncutsortexpression='RATE' ncut=10 . ...

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Next: Inspection of results Up: *fit* - Fit Data Previous: Verbose Mode . If the number of net counts for a source is less than it is impractical to fit the data in all 34 energy bits. However, if the flux is required, then a fit must be performed first. ... Fit will then calculate the normalization of the model and xflux can be used to determine the flux and luminosity of the source from the best fit model. xs> fit rebin=yes . ...

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• *qpspec* - Time Resolved Spectral Fitting
• The AstroStat Slog background
• *imcnts* - Radial Profile of an extended source at the field center

... These data were originally part of a PhD-thesis at Leiden Observatory by M.H. Wieringa (1991). 1 name Name of source (char8, example : '76W0771*') 2 freq MHz Frequency of source detection in MHz (int, example : 327 or 608 ) 3 ra_1950 radians B1950 Right Ascension (in radians) ( real , example : 2.328327) 4 ra_1950_deg degrees B1950 Right Ascension (in degrees) ( real , example : 133.403290) 5 ra_err seconds Error in RA ( ... 70W : Umi, 327 MHz only, one field. ... Columns 21 Rows 5850...

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• GPS sources
• IRAS Small Scale Structure Catalog
• The ROSAT All-Sky Survey Faint Source Catalogue

... C N Maximum number of axes in a GDS set INTEGER MAXAXES PARAMETER ( MAXAXES = 10) N Maximum number of subsets INTEGER MAXSUBS PARAMETER (MAXSUBS = 2048) N Size of internal data buffer INTEGER MAXDATA PARAMETER (MAXDATA = 4096) N Names of input and output set CHARACTER*80 SET1 , SET2 N Dimension of subsets INTEGER SUBDIM N Number of subsets INTEGER NSUBS N Array containing axis permutation INTEGER AXPERM1( ... 0) CFOR CALL FINIS STOP END . ...

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• Unified Radio Catalog: results for Version 1.1
• HIPASS Bright Galaxy Catalog
• The HIPASS Bright Galaxy Catalog

NStars 1: photometric surveyse --- | ... There are a number of 2MASS sources which have (faint) counterparts on POSS II F (R) or N (I), but don't have an entry in the GSC 2.2. ... It is possible that some images might have no GSC counterpart due to proper motion taking the source outside the 6 arcsecond search radius between the palte-taking and the 2MASS observation. ... Figure a1.1: The (F-J)/(J-K) two-colour diagram for faint sources with GSC2.2 counterparts. ... Intermediate sample . ...

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• Target Count Rates
• The 24 Micron Source Counts in Deep Spitzer Space Telescope Surveys
• Resources for mapping HST papers to proposals

... The numbers of three types of compact binaries containing accreting NSs and BHs, which are most interesting from the point of view of their observational appearances, have been calculated as a function of time: i) X-ray transient source containing a NS in an eccentric orbit around a main sequence Be-star (the observed prototype: A0535+26), ii) BH The evolution of the selected types of X-ray binaries during the first 10 million years after the starburst onset is presented in Fig. ...

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• Population Synthesis of X-ray Sources at the Galactic Center
• Population synthesis of X-ray sources at the Galactic center
• Evolution of the Double Neutron Star Merging Rate andthe Cosmological Origin of

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• worker - Apache HTTP Server
• research field
• mod_logio - Apache HTTP Server

.

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• Means and Deviations
• Energy and the Environment: Resources for a Networked World

AGN dust model of 3CR sources Frank Heymann (PhD), Martin Haas, Endrik Krgel, Christian Leipski MIR imaging spectroscopy ISM dust model PAH SED of a clumpy AGN torus CenA (ESO) Crete 2010 vectorized Monte Carlo model Ralf Siebenmorgen 1) Ground based MIR imaging Nuclear activity in nearby galaxies Surface brightness AGN viz. starbursts Ralf Siebenmorgen 10m telescopes ... Ralf Siebenmorgen Crete 2010 PAH in a mono-energetic heating bath if | ... Crete 2010 ...

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• The Cross-correlations
• Identifications and Efficiency
• ESO - vo2002

... Canadian Astronomy Data Center, DAO/NRC . SkyCat is a tool that combines image visualization with access to astronomical catalogs and data archives. SkyCat uses a standardized URL syntax to access a large number of data sources on the net. ... More information on SkyCat can be found at the SkyCat Web site. The ESO SkyCat Tool includes the following features: . ... PostScript color printing of the display (image + graphics), . ... overlay catalog sources on an image, . ...

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• Recreating Einstein Level One Processing Exposure Masks and Background Maps in
• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits

SIMPLE = T / file does conform to FITS standard BITPIX = 8 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A .. ... IMAGEW = 4256 / image width IMAGEH = 2832 / image height ANRUN = T / Solve this field! ...

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... For a tsvector column in a table, returns the distinct words along with their frequency. This includes the number of documents (table rows) containing a word and the number of entries for a word which includes multiple occurrences within a row. stat(txt TEXT) RETURNS SETOF STATINFO . txt' is a select statement that selects a tsvector column from a table. SELECT * FROM stat('SELECT ts_vec FROM ts_readme') ORDER BY ndoc desc, word LIMIT 5; word | ndoc | ...

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• Planetary Picture List
• APOD: 2006 July 29 - The Swarm
• APOD: 2005 January 28 - The Swarm

CONTENTS Volume 25 Number 1 (January 1998) . ... A. A. Ubachukwu . SPECTRAL INDEX ASYMMETRIES IN POWERFUL RADIO SOURCES: COSMOLOGICAL EVOLUTION VERSUS LUMINOSITY SELECTION EFFECTS . ... A. G. Gunn . ... A MEDIEVAL IRISH TREATISE ON ASTRONOMY RECALLED, WITH A MEMOIR OF ITS TRANSLATOR AND EDITOR, MAURA POWER (1887-1916) . ... 1995-1999 Irish Astronomical Journal, Downshay, 12 Heather Lea Avenue, Dore, Sheffield S17 3DJ, S. Yorkshire, United Kingdom WWW Contact: Alastair G Gunn Back to IAJ Home Page ...

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• IAJ: Contents - Volume 22 Number 2
• Atomic data for Stellar Atmospheres: lte_lines
• Performance

... The tension in members of the telescope changes as we move the dome, ch, azimuth, and tiedown tensions. The lifetime of a beam is counted in the number of times the change in tension goes through a cycle. ... Examples of telescope motion with corresponding unbalanced moment. ... The number of cycles were computed for : 5000, 10000, 15000, 20000 kipFeet momemnt change. ... The number of cycles on the telescope was computed using the change in the unbalanced moment (at a corner). ... cycles . ...

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• AO Fax numbers
• Spectral-Line Observing
• Calibration Scans on Continuum Sources

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/kwDict/axis.py Source File
• lsst.tcc: python/tcc/util/runningStats.py Source File
• lsst.coordConv: python/coordConv/testUtils.py Source File

Family ASTRO Event Leaders can follow the links below to find a number of resources and more background reading to help them with their Astronomy Events and expand their knowledge on the topics covered in our series of Leader Kits for educators. ... Print and Web Resources on the Night Sky . ... If you have questions about Family ASTRO, see our Frequently Asked Questions for Educators and Astronomers page , or our Frequently Asked Questions for Families and Friends page. ...

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• ASP: The Astronomy of Many Cultures: A Resource Guide
• ASP: Cosmology: The Origin, Evolution & Ultimate Fate of the Universe
• ASP: Astronomical Pseudo-Science: A Skeptic's Resource List

FIFTEENTH CREW REQUIRED RESOURCES TWELFTH RUSSIAN VISITING CREW IMAGE . ... EXPEDITION FIFTEEN (ISS-15) . ... During ISS-15, it is planned to implement 272 sessions of 47 experiments. ... Breakdown of Experiments and Number of Sessions by Research Areas. Research Area . Experiment Name . Totally . ... Research of space rays . ... Ascent to ISS RS: by Soyuz TMA-10 . ... ISS-15 Crew Commander F. Urchikhin (Russia) . ... RECORDING AND TRANSFER OF SCIENTIFIC DATA TO PRINCIPAL INVESTIGATORS . ...

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USING THE CORRELATION BETWEEN ISGRI SURVEY RESULTS AND OTHER CATALOGUES TO AID SOURCE IDENTIFICATION John B. Stephen, A. Malizia and L. Bassani IASF-INAF, Via P. Gobetti 101, 40129 Bologna, ITALY, E-mail: stephen@iasfbo.inaf.it ABSTRACT In order to help in the identification of INTEGRAL/ISGRI sources, we have developed a software package which allows a rapid and detailed cross-correlation to be performed between various source catalogues. ... We show below some preliminary results from this analysis. ...

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• Титарчук Лев Григорьевич (NRL)
• Spectrum-Roentgen-Gamma - The astrophysical Project at IKI RAN

... A classic test of the standard orientation-dependent unified schemes has been the assessment of the quasar fraction in complete radio samples. Using a sample of giant radiosources (projected size ) out to redshifts of , I demonstrate that the fraction of broad line objects is smaller than that obtained by comparison of quasars and galaxies in the 3CR sample. ... The sample . ... Giant radio sources ( ) have traditionally been of great interest for several reasons. ...

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• Astrophysics Group Variability studies
• NVSS Source Search (10-July-1998) Help for NVSS Source Catalog Search
• Astrophysics Group 10C

... Telescope concept . ... The Submillimetron Project is dedicated to astronomical studies at the submillimeter and far infrared wavelengths using a cryogenic telescope located on the Russian segment of the International Space Station (ISS). The Astro Space Center of the Lebedev Institute of the Russian Academy of Sciences is responsible for developing the Submillimetron Project. ... Currently, the Astro Space Center is carrying out a pre-Project study under contract with the Russian Space Agency. ...

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• Texas Survey of radio sources at 365MHz
• Description of the RadioAstron project, english version