The A/D rms values versus mixer input power were measured using a sine wave input to the baseband mixer chassis. We wanted to see how large a sine wave we could push through the mixer chassis before compression set in. ... Before the sine wave was injected, the gain levels in the bbm were adjusted to give a 30 count rms on input noise. ... The plots show t he A/D rms levels vs sine wave input to the mixer (.ps) ( .pdf ). ... We got to an rms of 1400 with close to 1dbm input. ...

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• spectral_jumps_at_powers_of_2
• polATsys sep12
• ALFA Performance at 1665 MHz

... PRIMESRC : The INDEX value (see column description below) of the prime source. E_EXPRn : There are n ( ) occurrences of this keyword, one for each EPIC source list added to the RGS list. ... E_mBNDn : Similar to the E_EXPRn keyword, but this records the value of either ID_BAND (in the input RGS source file, when filemode =`modify') or bandids , which is used to select the EPIC sources and to calculate the RATE value, transmitted into the output RGS source list. ... real32 . ... EPIC_FILE . ...

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• Quick start.
• Start and stop times
• Description

... 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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• User interface
• casacore: tables/Tables/ExprRange.h Source File
• Plotting

... Abstract Return the character value of a kernel variable from the kernel pool. ... Brief_I/O VARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- name I Name of the variable whose value is to be returned. start I Which component to start retrieving for name room I The largest number of values to return. lenout I The length of the output string. n O Number of values returned for name. cvals O Values associated with name. found O True if variable is in pool. ...

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• CSPICE Routines: GDPOOL_C
• CSPICE Routines: GIPOOL_C
• covar2ellipse.pro (JWST Pipeline routines in IDL)

... The default search window is a circle. ... EPOCH value - Equinox of coordinates EQUINOX value -/ value : integer ( default ) 1950 ---------------------------------------------------------------------------- CATALOGs arglist - Types or Names of select catalogs : arguments : (Only the first characters is enough) ( default ) All - All available catalogs Radio - All radio catalogs Infra-red - All catalogs of Infra-Red sources Objects - ...

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• Getting Started
• Starting up
• Starting the whole thing

... 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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... INSERT INTO pg_ts_cfg (ts_name, prs_name, locale) VALUES ('default_english', 'default', 'en_US.UTF-8'); . Insert a row into pg_ts_dict to load the english dictionary files. INSERT INTO pg_ts_dict ( SELECT 'en_ispell', dict_init, 'DictFile="/usr/local/pgsql/share/contrib/english.dict", AffFile="/usr/local/pgsql/share/contrib/english.aff", StopFile="/usr/local/pgsql/share/contrib/english.stop"', dict_lexize FROM pg_ts_dict WHERE dict_name = 'ispell_template'); ...

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• Tsearch2 in Japanese
• Lighting plug-in
• ntptrace - trace a chain of NTP servers back to the primary source

The best way to explain what the logical actors are, is to consider an example. ... An example of logical actors (the Actors.A program). ... The principle of logical actors. -- ------------------------------------------- project : (( 'Main' )) ------------------------------------------- class 'Main' specializing 'Dialog': -- identifier = "input" ; x = 27 ; y = 8 ; -- i; j; -- w1 = ( 'TextPage', value_1=i, value_2=j, text_color='White', background_color='Red', x= 9 , y= 4 ) ; . ...

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• Getting Started in Actor Prolog. Analyzing Web Sites.
• Actor Prolog User Guide. SADT.
• EIT Server Input File Format

Sherpa Aneta Siemiginowska 1 SHERPA CIAO's Modeling and Fitting Application Aneta Siemiginowska CXC Astrostatistics Workshop, HEAD meeting , New Orleans, Septemter 2004 Sherpa Aneta Siemiginowska 2 Modeling and Fitting Software XSPEC - analysis of 1D X-ray data (imaging + grating) ISIS and Pint of Ale- primarily for analysis of highresolution (ie grating) X-ray data ... Jointmode data: spatialspectral, spatialtiming Use scripts based on Sherpa only commands. ...

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• *search_grid* - Customized grid
• Detect
• Model Spectra for Spectral-Fitting Program

... Here is an example of the output header of CATS data. ... SIMPLE=T / BITPIX=8 / character information NAXIS=0 / no image data array present EXTEND=T / may be standard extensions OBJECT= CATS SEARCH / CATS search result ORIGIN=SAO RAS DATE=01/01/1997 / date of file creation END XTENSION=TABLE / F-file table extension BITPIX=8 / 8-bits ... NAXIS1=93 / No. of characters per row NAXIS2=1000 / the number of lines (sources) TFIELDS=10 / there are 16 fields per row EXTNAME= CATS / object name: ...

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• WDM Quick Reference
• harak_e
• Access via e-mail

... St Petersburg 23, September 2014 1 Motivation Ї Origin of Martian moons? ... Considered error sources: ґ Phobos a priori ephemerides; ґ Phobos a priori GM value; ґ measurements noise; ґ different strategies; Ї Methods: ґ real data analysis; ґ simulations. ... St Petersburg 23, September 2014 8 Simulations: sensitivity of the measurements to the a priori GM value Simulations: zero noise+ IMCCE a priori ephemerides +GMPH = 7.16 * 105 m3/sec2. ... St Petersburg 23, September 2014 14 Thank you! ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm09c.pdf

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: include/tcc/telMod.h Source File
• lsst.tcc: python/tcc/axis/oneSlewIter.py Source File
• lsst.tcc: python/tcc/mir/mirrorDevice.py Source File

ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM BYTE MNEM CONTEXT 1 - 2 NR Record length in bytes (usually 416) 3 - 6 STCOD IAGA station code, 3 letters, 4th arbitrary 7 - 9 CMP order of the components in data block, 3 10 letters and space 11 SC scaling factor, multiply all data and base values by X (SC=0 X=1, SC=1.. ... Components code: D,I-in 0.1'; H,F,X,Y,Z in nT; E-magnetic east component perpendicular to H in nT; Usually data recorded as XYZ. ... Digital geomagnetic data base for VIKING period. ...

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• DIGITAL WDC EXCHANGE FORMAT FOR OBSERVATORY 1.0 MINUTE VALUES
• "Exploration" as a Classroom Resource
• The Sun

About the World-Wide Web . World-Wide Web Map . World-Wide Web Servers: Summary . The World-Wide Web Virtual Library : Subject Catalogue . ... Mappa WWW ? ... The WWW of GARR . ... Opera Software - Bringing speed and fun back into Internet browsing . VirtualLibrary: The Italian General Subject Tree . The WDVL (Web Developer?s Virtual Library) . ... Italian WWW Compilation at Milan?s CNR . Internet Resources Compilation at CSR4 . ... Internet Resources Compilation at UNIFI . ...

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• Labir Locally Mantained Hotlist
• Linked HTML Resources
• Determination of the Detector Parameters

OptInt PmWiki . ... Edit Page | ... Attach | ... Documentation Index . ... Markup Master Index . Text formatting rules | ... This page contains the most frequently used wiki markup, briefly. ... See Links . ... page name]] . ... GroupName/PageName]] or [[GroupName/page name]] . ... See Page directives , Comment markup , Page variables . ... See Include other pages , Page text variables . ... See Page variables , Page text variables , Page lists . ... name:description:) sets a page text variable . ...

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• OptInt PmWiki : PmWiki / Forms
• OptInt PmWiki : Forms
• OptInt PmWiki : PmWiki / Markup Master Index

... source code A class to hold all the information from a NIFS-produced data cube. ... Returns the data content of scidata as a numpy array. source code . ... Returns a spectrum from the specified spaxel, over the designated wavelength or velocity range. source code . ... source code Returns the data content of scidata as a numpy array. ... The fitscube instance is updated in-situ. source code Returns a spectrum from the specified spaxel, over the designated wavelength or velocity range. ...

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• Roof closed before the rain starts, and members inspect the 'scope
• University Problem Based Learning Exercises for Teaching Astronomy and Physics

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/renderer/StelTextureLoader.hpp Source File
• Stellarium: core/renderer/StelCircleArcRenderer.hpp Source File

... The package stsdas.graphics needs to be loaded (to run imdisp_pos for getting # the NDC's of the display image) # set imtype="fits" # print " " print " *** Start of impol FOC demo *** " print " [stecf.impol and stsdas.graphics need to be loaded] " print " " # # (First delete any model reflection nebulae left over from previous demos) # print " Deleting any old demo files " imdel reflneb1*.fits verify=yes # # An input (intensity) image is required. ... First delete any previous list files # ! ...

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• http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/demo/demo_special.cl
• http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/demo/demo_wfpc2.cl
• http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/demo/demo_nicmos.cl

... Create table of reflection nebula parameters from ascii file # ! ... Bin the output # data 2x2 input pixels and only output pixel values with polarization # errors less than 7% # print Running hstpolima to calculate polarization images.... hstpolima imalis= @reflintlist.lis errlis= @reflerrlist.lis \ instpolt= foc-pol-filt-001.tab xybin=2 binrej=10.0 errlim=7.0 outroot= reflneb1f # # Overplot the derived polarization vector map on the image already displayed # imdisp_pos ...

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• list of DFS Department documentation templates
• The Cross-correlations
• ESO - Science Announcements

... 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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