... If the parameter withinputlist is set to ``true'', the reconstruction and/or background image will be created using source parameters from an input source list. ... Use parameters makerecon and savebkgrnd to specify which of the output images you want to create. Only sources originally detected at scales up to maxscale will be used for to calculate the images. The value of maxscale will also control the scale of the kernel used to filter the background image. ...

... CREATE FULLTEXT CONFIGURATION -- create full-text configuration . CREATE FULLTEXT CONFIGURATION cfgname PARSER prsname [ LOCALE localename ] [ AS DEFAULT ]; CREATE FULLTEXT CONFIGURATION cfgname [ { PARSER prsname | ... PARSER . ... LOCALE . ... Create new configuration test with default parser and ru_RU.UTF-8 locale. CREATE FULLTEXT CONFIGURATION test PARSER default LOCALE 'ru_RU.UTF-8'; =# \dF+ test Configuration "public.test" Parser name: "pg_catalog.default" Locale: 'ru_RU.UTF-8' Token | ...

... These routines allow simple creation of standard and shared-memory XImage data structures, as well as the transmission of these to the X server. ... xi_check_shared_images_available . ... Write an XImage structure to a drawable. flag xi_check_shared_images_available (Display *display) . ... void xi_put_image (Display *display, Drawable drawable, GC gc, XImage *ximage, int src_x, int src_y, int dest_x, int dest_y, unsigned int width, unsigned int height, flag shared_memory, flag wait) . ...

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

Next: Rebin the XSPEC PHA Up: PHA Distributions Previous: Produce a spectral data . Write the contents of "*_obs.tab" to an ascii file using these parameter settings for the task 'tdump'. cl > epar tdump table = "*_obs.tab" name of table to dump . cdfile = "STDOUT") output file for column definitions . ... pwidth = 80) output page width . ... chanpres = no Channel data present? . ... Next: Rebin the XSPEC PHA Up: PHA Distributions Previous: Produce a spectral data rsdc@cfa.harvard.edu . ...

SPIKE currently uses constants for all orbit parameters except longitude of the ascending node (large omega). ... Log into planinst or planning. run the following report: $report spss_data_dk:[planinst.kinzel.c1]lrpfit/par=(fit:sx_940890,cycend:1998.200)/out=lrpfit.rpt . ... set default [lrp.orbits] . ... To create the plots, run the MONGO file . ... When ready, (link to creating batch cv-desc files), update the cv-desc files and make this constraint set the operational set when RPS2 will be released. ...

Next: Edition of the Up: Typical Run Previous: Creation of the . The coefficients of the continuum are to be entered in keyword CLDCT. Edition of the table containing the emission line parameters. ... Command: . ... Computation of the spectrum. The command COMPUTE/EMI creates a 1D image, containing emission lines and continuum. ... EMI : input table containing the emission line parameter. if no table name is given, the output spectra will contain only . ...

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

RUSSIAN-AUSTRALIAN RESEARCH SCHOOL MICRO-SATELLITE "KOLIBRI-2000": BASIC RULES of DEVELOPMENT . A characteristic feature of the project "Kolibri-2000" is the solution of the task of using micro-satellites in the interests of improving school education and involving schoolchildren in space technologies. ... A radioline in the radio amateur frequency range is employed on Kolibri-2000 to dump scientific payload data to the participants in the Project. ...

TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...

... Home All Namespaces All Classes Functions Coding Style Scripting Plugins File Structure . ... Manage textures loading. ... createTexture (const QString &filename, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams ()) . Load an image from a file and create a new texture from it. ... createTextureThread (const QString &url, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams (), const QString &fileExtension=QString(), bool lazyLoading=true) . ...

... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

... Suppose we have 2 tones Acos(at) and Bcos(bt). ... The individual freq terms are then: . ... square :[Acos(at) + Bcos(bt)]^2: [Acos(at)]^2 +[Bcos(bt)]^2 + 2ABcos(at)cos(bt) . ... A^2(cos(2at) -1)/2 . ... A^3cos(at)*[cos2at - 1)/2=A^3([cos(3at) + cos(at)]/2 - cos(at)]/2=A^3(cos(3at) -cos(at))/4 . B^3cos(bt)*[cos2bt - 1)/2=B^3([cos(3bt) + cos(bt)]/2 - cos(bt)]/2=B^3(cos(3bt) -cos(bt))/4 . let C2= 3AB^2 and C3=3BA^2 . ... C 3cos(bt)[cos(2at)-1]/2=C3[{cos((2a-b)t)+cos((2a+b)t)}/2+cos(bt)]/2 . ...

phpBB2 - attach_mod schema - Postgresql $Id: attach_postgres_schema.sql,v 1.3 2003/03/09 02:21:03 acydburn Exp $ */ /* Create auto_increment values */ CREATE SEQUENCE phpbb_extensions_id_seq start 1 increment 1 maxvalue 2147483647 minvalue 1 cache 1; CREATE SEQUENCE phpbb_forbidden_extensions_id_seq start 1 increment 1 maxvalue 2147483647 minvalue 1 cache 1; CREATE SEQUENCE phpbb_extension_groups_id_seq start 1 increment 1 maxvalue 2147483647 minvalue 1 cache 1; ...

seeing -- Create a simulated ground-based star image based on a model of atmospheric turbulence seeing output xdim ydim gamma fwhmx fwhmy . output = "" [image] . The name for the output image to be created. xdim = 512 [integer] . The X dimension for the output image. ydim = 512 [integer] . The Y dimension dor the output image. gamma = 1.6666 [real] . ... For a discussion of the significance of this please see the discussion below and the references given. fwhmx = 5.0 [real] . ...

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

To create a tarfile containing several files: tar cvf data.tar *.dat . This creates a tarfile data.tar containing all the files in the current directory which have the filename extension .dat . ... To create a tarfile of a directory: tar cvf project.tar Project Project/README Project/Makefile Project/Makefile Project/main.c Project/screen.c Project/menus.c Project/calculator.c Project/setup/configuration . ... This creates a tarfile book.tar containing the directories text and illustrations . ...

... Hubble 25th Anniversary: Pillars of Creation . ... The result is this sharper, wider view of the region dubbed the Pillars of Creation , first imaged by Hubble in 1995 . ... The light-years long columns of cold gas and dust are some 6,500 light-years distant in M16 , the Eagle Nebula, toward the constellation Serpens. ... APOD Talk: Friday, January 9 in New York City . January . ... Publications with keywords: M 16 - Eagle Nebula . ... Inside the Eagle Nebula . ... M16: Pillars of Creation . ...

Next: Binary Radiopulsars with Black Up: Black Holes in Binaries Previous: Black Holes in Binaries . Two different types of stellar BH formation exist: (1) direct core collapse   of a massive star and (2) AIC of a NS. A BH of the first type presumably will have a mass comparable to that of the collapsing star and can be born both from a single star and in a binary system. ... Next: Binary Radiopulsars with Black Up: Black Holes in Binaries Previous: Black Holes in Binaries Mike E. Prokhorov . ...