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. ...

... 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 . ...

... 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....

... 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. ...

... 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 - ...

... 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. ...

... 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'); ...

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 ) ; . ...

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. ...

... 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: ...

... St Petersburg 23, September 2014 1 Motivation · Origin of Martian moons? ... Considered error sources: ­ Phobos a priori ephemerides; ­ Phobos a priori GM value; ­ measurements noise; ­ different strategies; · Methods: ­ real data analysis; ­ 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! ...

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

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. ...

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 . ...

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 . ...

... 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. ...

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

... 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 # ! ...

... 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 ...

... 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 . ...