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1. Creating reconstruction image and background image from an input source list
... 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. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/ewavelet/node9.html -- 3.8 Кб -- 01.07.2008
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2. CREATE FULLTEXT CONFIGURATION
... 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 | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/sql-fts-createcfg.html -- 10.1 Кб -- 13.04.2008
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3. Create an XSPEC compatible PHA FITS file
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 . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node215.html -- 5.8 Кб -- 01.10.2012
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4. Creation of SPIKE / RPS2 Orbit Models
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. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/spst/lrpg/documentation/procedures/obsolete/lrpg_create_orbit_model.html -- 2.6 Кб -- 26.04.1999
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5. Creation of the Input Emission Spectrum
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 . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node200.html -- 3.2 Кб -- 23.02.1996
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6. Problem creating a new system call
... Just to learn how to generate a system call, I created a simple system call that basically sets and resets the value of a global parameter "PREFETCH". SYSTEM CALL code ********************************** int PREFETCH = 0; /* this is a global variable */ . ... To execute the sys_prefetch system call, I wrote a prefetch.c file with the following code. ************************code to call sys_prefetch***************** #include <linux/unistd.h> _syscall2 (int, prefetch, int, mode, int, nr_hints) . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/linux/khg/HyperNews/get/khg/135.html -- 4.2 Кб -- 23.03.2000
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7. Package: mt
These routines are meant to provide management of a pool of threads which may execute concurrently. ... Register new thread information for the threads in a pool. mt_get_thread_info . ... Multithreading Level: Safe under Solaris 2. ... Multithreading Level: Safe. void mt_new_thread_info (KThreadPool pool, void *info, uaddr size) . ... Multithreading Level: Safe. void mt_PROTO_func (void *pool_info, void *call_info1, void *call_info2, void *call_info3, void *call_info4, void *thread_info) . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/karma/lib/mt.html -- 11.8 Кб -- 24.12.2007
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8. Preparation of parameter file
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 ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node228.html -- 6.1 Кб -- 28.04.2015
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9. The BASIC RULES on CREATION of the RUSSIAN-AUSTRALIAN SCIENTIFIC-RESEARCH
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. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/kollibri/osnpl_e.htm -- 3.0 Кб -- 09.12.2000
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10. http://www.naic.edu/~phil/misc/creatingharmonics.html
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/misc/creatingharmonics.html -- 4.1 Кб -- 15.08.2003
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11. How to create a new tool in CASA Bojan Nikolic web pages (r. 329)
... 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 . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/sweng/casanewtool.html -- 19.7 Кб -- 04.04.2016
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12. SEEING (V1.3) --- Apr00 --- SEEING (V1.3)
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] . ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/imres/seeing.hlp.html -- 4.0 Кб -- 06.06.2006
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13. Samara University scientists have developed a new technology to create solar
... News . ... Pre-university education . ... Samara University scientists have developed a technology of new-designed photoelectric converters for solar batteries of spacecraft. ... The new solar batteries will be as much effective as their contemporary nanoheterostructured counterparts surface-supported by germanium, and the cost will be five times cheaper. ... Scientists of Samara University (joint SSAU and SSU) developed a technology basis of new silicon-based photoelectric converters (FEC). ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/engnews/12278/ -- 27.8 Кб -- 18.02.2016
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14. Колготки для кукол Zapf Creation Baby Annabell 2 пары 792-261 в ассортименте -
... Бренд: Zapf Creation, Тип: Колготки для кукол . Аксессуары для кукол . ... Пособие содержит темы, подготовленные на основе базовой учебной программы по дисциплине "Банковский маркетинг". ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku5800.html -- 18.8 Кб -- 14.02.2016
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15. Examples of creating files
. To create a file with the cat command: cat > memo remember to make appointment at opticians get cost of scheduled flight to Athens Ctrl-d . This creates a file called memo in the current directory containing two lines of text. To create a file with the echo command: echo use an editor for large files > tips . This creates a file called tips in the current directory containing a single line of text.
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/examples/create.html -- 2.2 Кб -- 17.01.1997
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16. A Method for Minimizing Background Offset Errors When Creating Mosaics
... When creating a mosaic from a set of individual frames, the correct background offset for each frame must be determined for proper matching. In this paper we describe a method for constructing a mosaic from a set of individual frames by applying a minimization technique. ... Typically these are frames with some known defect (see ? ... Determining which frames to exclude from the final mosaic is critical, since one bad frame can create background offset errors that propagate throughout the mosaic. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/reganm.html -- 12.3 Кб -- 03.11.2000
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17. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Revs - number of orbits of dust from ejection to 2014 . Ep - ejection epoch (year) . Da0 large particles . rE-rD - distance of the dust trail node from Earth's orbit (Earth radius=0.00004AU) (Impact radius=0.00005AU) (trail widths can easily be a few Earth diameters, depending on ejection velocities) . fM - estimate of the along-trail dispersion. ... Year Mo Da . ... Revs . ... Da0 . ... 0.001 . ... 0.000 . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~dja/209P/encpar2014.html -- 13.1 Кб -- 22.05.2014
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18. Creative WebCam NX Ultra - Hand Made
... Киевский клуб любителей астрономии "Астрополис" > . ... Hand Made (Модераторы: Diskus , Hornet ) > . Creative WebCam NX Ultra . ... 03 Март 2006, 00:57:32 ? Есть возможность за недорого забрать вебкамеру Creative WebCam NX Ultra. ... Записан . Клуб Астрополис, Администратор . ... Ответ #1 : 03 Март 2006, 01:27:07 ? ... Цитата: Vladimir Nebotov от 03 Март 2006, 00:57:32 Есть возможность за недорого забрать вебкамеру Creative WebCam NX Ultra. ... Клуб Астрополис, Модератор . ...
[ Сохраненная копия ]  Ссылки http://www.astroclub.kiev.ua/forum/index.php?topic=940.0 -- 70.5 Кб -- 09.04.2016
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19. Black Hole Creation in Massive Binary Systems
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 . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node64.html -- 8.4 Кб -- 26.02.1997
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20. Space Laser Creates Artificial Star
Astronomy Picture of the Day . ... 25.04.2001 . ... AURA , NSO , NOAO , NSF Explanation: Some astronomers don't like stars. ... So rather than try to eradicate existing stars with a laser, these astronomers create an artificial star of their own right where they need it -- with a laser . ... Above , an artificial star was created with a four-watt laser at Richard B. Dunn Solar Telescope on Sacramento Peak in New Mexico . ... April . ... April 2001 . ... A Telescope Laser Creates an Artificial Star . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1167714 -- 14.3 Кб -- 26.04.2001
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