... Miriad has a couple of tasks available for finding positions of sources (see also cgcurs in Chapter 17 ). ... It fits a 2-D parabola to the image intensities in a 3 by 3 pixel box centred on the brightest pixel in a specified region and reports the fitted location and intensity. ... Input image . ... The quality of your fit can improve significantly by selecting a snug region, and/or using the clip keyword to keep pixel values with little signal (e.g. sidelobes and noise) out of the fitting process....

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• Selavy and the ASKAP Source-finding Service
• Unified Radio Catalog: results for Version 1.1
• uvsfit

... The quickest way to learn how each observation was performed is to use the iminfo task in the STSDAS toolbox.headers package to look at the headers of the science data. ... Number of extensions . ... Given that NICMOS data files contain multiple extensions, the number of the desired extension must always be specified. ... In order to simplify access to NICMOS FITS image extensions, each extension header contains the two keywords: EXTNAME (extension name) and EXTVER (extension version number). ...

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• COS Instrument Handbook
• STIS Instrument Handbook
• Appendix B: Point Source SNR Plots

... The generation of simulated sources whose physical properties are well understood is useful in assessing the functionality of point source analysis software. Qpsim is an IRAF/PROS task which will generate events from sources of given intensity, shape, and position and either overlay them on a flat background in a new QPOE file or inject them into an existing QPOE file. ... The simulated data can be a useful tool in calibrating point source analysis software. ...

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

... CI Cam is known to be a B[e] star and X-ray transient source. ... Figure 1. The light curve of CI Cam in residuals relative to the mean level of the slow variability (top) . The radial velocity curve of the HeII emission (middle) . ... The V light curve is shown in Figure 1 (top). ... Comparison of two CI Cam spectra in the region of HeII line. ... The radial velocity curve of HeII in CI Cam has a saw-tooth shape that may be an evidence of an elliptical orbit. ...

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• Radio sources identfification
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• harak_e

... A2584 used the cband receiver and the mock spectrometers to cover a 1 ghz band at cband. ... Of the 14 bands, some were 11 Mhz and others were 86 Mhz. the digital filtering and offsetting was used. 01-17nov10 : gortex cover comes loose from cband horn mouth. moisture get ins horn, causes tsys to go up . 22feb11: the wideband H2CO line did not line up with the narrow band H2CO line. ... The plots for 22feb11 below have jumps across the band in Tsys. ... Plots were made of: . ... cntsToK and Tsys . ...

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• ALFA performance at 1.665 GHz AO Technical Memo 2004-01
• ALFA Performance at 1665 MHz
• pdev_birdies_25jun07

DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM
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... 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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• The ROSAT All-Sky Survey Faint Source Catalogue
• Noise distributions
• COMPACT RADIO

... The x-ray spectral analysis consists of a comparison between the observed pulse height spectrum and a pulse height spectrum calculated using a given spectral model. ... To obtain the spectral parameters for an x-ray source, several steps need to be followed. For each source: . ... obtain the best fit parameters for a spectral model - repeated for each model of interest . obtain a 1-D or 2-D grid of values around the best fit values - this can be done for as many models as desired . ...

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• Model Spectra for Spectral-Fitting Program
• Chandra Images for SNRJ 0540.1-6919
• Chandra Images for SNR J0526.0-6604

... SELECT file, title, rank(ts_vec, to_tsquery('create schema')) FROM postgresql_manual WHERE ts_vec @@ to_tsquery('create schema') ORDER BY rank(ts_vec, to_tsquery('create schema')) DESC LIMIT 5; file | title | ... CREATE SCHEMA | ... SELECT file, title, rank('{0, 0, 0.01, 0.99}',ts_vec_tb, to_tsquery('create aggregate')) FROM postgresql_manual WHERE ts_vec_tb @@ to_tsquery('create aggregate') ORDER BY rank('{0, 0, 0.01, 0.99}', ts_vec_tb, to_tsquery('create aggregate')) DESC LIMIT 5; file | ...

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• Lighting plug-in
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• Intro

... Science . ... Science Users Information > Science Publications > Science Announcements . ... Observing Facilities . ... Observing with ESO Telescopes . ... Instrument Pipelines . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... Science Announcements . ... Published: 05 Oct 2015 . ... New data products resulting from the VST Public Survey ATLAS are now available via the dedicated Phase3 query interface at the Science Archive Facility . ... Published: 31 Aug 2015 ....

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• list of DFS Department documentation templates
• ESO - How do I interpret the SEQ TIME keyword values?
• ESO - Negative pixel values in the 2D spectrum image are not being ignored by

J/MNRAS/429/2080 Lockman Hole 10C sources radio spectral indices (Whittam+ 2013) ================================================================================ The faint source population at 15.7 GHz. ... 2011, Cat. ... 2008, Cat. ... For 10C sources without a counterpart in the GMRT image, three times the local noise is included as an upper limit on the flux density at 610MHz. ... 1.4-GHz flux density value from NVSS catalogue, including upper limits for undetected sources 76 I1 --- f_SNVSS [0/1]? ...

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• NVSS Source Search ($Revision: 1.6 $ - running v2.17)
• exchange.h Source File
• NVSS Source Search (10-July-1998) Help for NVSS Source Catalog Search

Stellarium 0.12.3 . ... File Structure . File List . File Members . core . planetsephems . calc_interpolated_elements.h . ... 6   copy of this software and associated documentation files (the "Software"), . ... 26   void CalcInterpolatedElements( const double t, double elem[], . ... 36   The cache consists of 3 sets of values: . 37   e0[0..dim-1] are the cached values at time *t0, . ... 41   (*calc_func)(t,elem) calculates the values elem[0..dim-1] at time t, . ...

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• Stellarium: core/renderer/StelGLSLShader.hpp Source File
• Stellarium: core/modules/Landscape.hpp Source File
• Stellarium: core/renderer/StelQGLGLSLShader.hpp Source File

lsst.tcc   1.2.2-3-g89ecb63 . ... Files . ... python . tcc . parse . getRestart.py . ... 11   for key, val in _TranslateDict.items(): . ... 16   """!Get a list of axes from the /Restart qualifier . ... 18   @todo: tweak this once we figure out how the parser handles /Restart vs /Restart=(); . ... 64   # "all" axes requested, so restart all axes except those explicitly negated . ... 67   # only recieved negated axes, all other axes should be restarted . ... tcc.parse.getRestart.getRestart . ...

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• lsst.tcc: python/tcc/base/wrapperTestCase.py Source File
• lsst.tcc: python/tcc/parse/getPVTList.py Source File
• lsst.tcc: python/tcc/util/runningStats.py Source File

... The results of long-term monitoring of Gigahertz-Peaked Spectrum sources were found the statistically significant differences (0.05 significance level) in the high-frequency spectral index distribution between subgroups of galaxies and quasars. ... This can mean that the electron energy distribution for GPS galaxies is steeper than for GPS quasars. ... The first area corresponds to GPS-quasars that have statistically larger value of redfhift, second area corresponds to GPS-galaxies. ...

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• Detection of polarized radiation sources with unusual spectral characteristics
• Metagalaxy sector, archive 1993
• IRAS01005+7910

... Clean . ... Flux Sign Expo . ... The map above is movable . The image is shown in significance with a squared root color map ranging from 0 to 25. ... Original shows mosaics with all data available. Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. ... Exposure maps are in ksec. INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ... Exposure . ...

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... SPARCompiler(TM) Fortran 90 1.0 . FORTRAN 77 3.0.1 . ... important of these. -ansi: Report non-ANSI extensions. -c: Suppress linking, produce .o files -e: Recognize extended (132 character) source lines -fast: Specify common set of performance options - fixed : Interpret all Fortran source files according to fixed form rules -flags: Print summary of compiler options -fnonstd: Non-standard initialization of floating-point hardware -fnonstop: Execute without trapping on invalid, overflow ...

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• Tutorial on Fortran 90, Digital UNIX
• HTML Design Notebook

Each Apache module is described using a common format that looks like this: . Status: status . ... This indicates how tightly bound into the Apache Web server the module is; in other words, you may need to recompile the server in order to gain access to the module and its functionality. ... A module with "Extension" status is not normally compiled and loaded into the server. ... Modules which are not included with the base Apache distribution ("third-party modules") may use the "External" status. ...

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• Server-Wide Configuration
• Apache module mod_headers
• Apache module mod_setenvif

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Quasi-stationary electron distributions for the different values of the particle escape time. ... The electron-cyclotron maser instability is widespread in the Universe, producing, e.g., radio emission of the magnetized planets and cool substellar objects. ... The model used takes into account the radiation escape from the source region and the particle flow through this region. ...

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• Spectrum - control
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... Forum: Character Device Drivers . Keywords: return values . Date: Fri, 25 Apr 1997 21:42:46 GMT . ... In this section I noticed the example foo_write function returns 0 all the time. ... the foo_write () function gets called indefinately. Furthermore, I have noticed that from the source of serial.c (from /usr/src/linux-2.0.0/drivers/char) always returns the number of characters transmitted. ... Also, why isn't there a DEFINITIVE list of return values for all functions? ...

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• mod_setenvif - Apache HTTP Server
• The Arcetri Spectral Code - E.Landi and M.Landini (2002)
• Password Formats - Apache HTTP Server

... In this case the F5-F9 dwarfs turn out to be more metal-rich (by 0.1 in [Fe/H] ) thab G and K dwarfs, and the metallicity of the Hyades cluster turns out to be larger than the solar one [Fe/H] Hyades =+0.1 . ... При этом карлики F5-F9 оказываются богаче металлами, чем более поздние звезды, примерно на 0.1 по [Fe/H] , и металличность звезд Гиад относительно Солнца равна [Fe/H] Hyades =+0.1 . ...

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• MONTE-CARLO