Найдено документов: 197475 (147 сайтов) ---- Время поиска: 0.34сек. |
Показаны документы, содержащие фрагменты текста из документа
http://xmm.vilspa.esa.es/sas/6.5.0/doc/asmooth/node17.html.
http://xmm.vilspa.esa.es/sas/6.5.0/doc/asmooth/node17.html.
1. Parameters
... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... The image dataset to be smoothed. outset . ... This parameter is read if smoothstyle =`simple' is chosen and prescribes the shape or type of convolver to use to smooth the image. width . ... See section 3.3 for further details. normalize . ... If set, the task reads from parameter invarianceset an image of the variances (squares of the standard deviations) of the input image values. invarianceset . ...
[
Сохраненная копия
]
Ссылки http://xmm.vilspa.esa.es/sas/6.1.0/doc/asmooth/node17.html -- 22.1 Кб -- 22.11.2004
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>15234) - xmm.vilspa.esa.es/ )
2. Edition of the Table Containing the Atomic Parameters
. Next: Edition of the Up: Typical Run Previous: Creation of the . All of the atomic data listed in 13.2.1. are needed by the program and are to be entered via this table. A template can be found in MID_CLOUD: ABSP.TBL . The quoted parameters are from Morton and Smith (1973) and according to the author the wavelengths are: . vaccum for 2000 ?, air for 2000 ? . Command: . The actual format of this table is described in section Auxiliary Data. Rein Warmels . Mon Jan 22 15:08:15 MET 1996
[
Сохраненная копия
]
Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node190.html -- 2.9 Кб -- 23.02.1996
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1940) - www.sao.ru/ )
3. Task parameter manipulation
The current set of keyword-value pairs of a task can be monitored by typing ESC K while the name of the task is present in the User Command Area. This causes (part of) the Common Output Area to be overlaid with a display containing the current user input parameters of the task. ... If there is currently a set of parameters displayed on the screen (as the result of typing ESC K ), these parameters will be edited; otherwise the name of the task is derived from the User Command Area contents. ...
[
Сохраненная копия
]
Ссылки http://www.atnf.csiro.au/computing/software/gipsy/hermes/keytable.html -- 3.6 Кб -- 16.01.2009
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>9049) - www.atnf.csiro.au/ )
4. 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
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>49075) - www.eso.org/ )
5. Index
... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... ACCUM . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... PCS MODE Fine Special Requirement . ...
[
Сохраненная копия
]
Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelp22/ix.html -- 51.8 Кб -- 02.06.2014
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>9988) - www.stsci.edu/ )
6. Regions and Source Parameters
... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...
[
Сохраненная копия
]
Ссылки http://hea-www.harvard.edu/PROS/PUG/node89.html -- 5.8 Кб -- 01.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>2291) - hea-www.harvard.edu/ )
7. Program parameters
Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...
[
Сохраненная копия
]
Ссылки http://www.arcetri.astro.it/science/Radio/red/searchdup/node2.html -- 8.0 Кб -- 30.06.2000
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>7412) - www.arcetri.astro.it/ )
8. http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/nwclient/NET.CFG
LINK DRIVER 3C5X9 ; ; The following two parameters are required when using two or more EtherLink ; III adapters in a single machine. These parameters specify which specific ; EtherLink III adapter the driver is to attach itself to. PORT NNN, where NNN is the hex base address of the 3C509 ISA adapter ; ; SLOT NN, where NN is the slot number containing the 3C529, 3C579, or ; 3C509 configured as an EISA adapter. PORT 200 ; SLOT 3 ; ; The next line specifies the frame type. ...
[
Сохраненная копия
]
Ссылки http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/nwclient/NET.CFG -- 1.7 Кб -- 06.03.2001
Похожие документы
Похожие документы
9. (Untitled)
The data in the Table on p. 5788 – 5789 embrace estimated parameters for 128 binary systems in near Earth, Mars crossing, main belt and Trojan orbits (more than 90% of corresponding objects are marked in the Table "Minor planet lightcurve parameters" as undoubtedly binary and in other cases as suspected binary). ... The data were presented by P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic) (see Pravec, P., Harris, A. W., 2007. Binary Asteroid Population. ...
[
Сохраненная копия
]
Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user9gs2.htm -- 2.3 Кб -- 10.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>423) - www.ipa.nw.ru/ )
10. cat5
. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.
[
Сохраненная копия
]
Ссылки http://www.wdcb.ru/stp/cat5MOD.html -- 2.2 Кб -- 18.01.2010
Похожие документы
Похожие документы
11. Passing arguments to the shell
Shell scripts can act like standard UNIX commands and take arguments from the command line. Arguments are passed from the command line into a shell program using the positional parameters $1 through to $9 . Each parameter corresponds to the position of the argument on the command line. ... For example: cat printps # This script converts ASCII files to PostScript # and sends them to the PostScript printer ps1 # It uses a local utility "a2ps" a2ps $* | lpr -Pps1 printps elm.txt vi.ref msg . ...
[
Сохраненная копия
]
Ссылки http://comet.sai.msu.ru/UNIXhelp/scrpt/scrpt2.1.html -- 2.8 Кб -- 17.01.1997
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>162) - comet.sai.msu.ru/ )
12. FFIT - Command Syntax
... spectrum . ffit . ... grids . ... These commands read in a grid of model spectra. ... Values for the parameters are taken from the input models themselves, to avoid mixups. The syntax of the command arguments is precise. model{ . ... If there is only one spectrum to fit, one should set default parameters for the secondary which lie within the model grid, with <L_2/L> being a very small value. ... The output is saved in a file <file.fit> , where <file> was the name of the spectrum being fitted. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/~csj/software_store/guide/ffit_commands.html -- 9.1 Кб -- 30.08.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1268) - star.arm.ac.uk/ )
13. Gemini South Adaptive Optics Imager Performance Calculator
... Dark current e - /s/pix . ... OH continuum photon/s/m 2 /arcsec 2 / m . ... Imager: . ... Adaptive Optics: . ... Object signal e - /pix . Sky thermal signal e - /pix . Sky OH continuum signal e - /pix . Sky OH line signal e - /pix . Telescope thermal signal e - /pix . AOS thermal signal e - /pix . Cryostat signal e - /pix . Dark signal e - /pix . Total signal e - /pix . ... This tool models the performance of the Gemini South Adaptive Optics Imager (GSAOI) . ...
[
Сохраненная копия
]
Ссылки http://www.mso.anu.edu.au/gsaoi/performance/gsaoi_calc.shtml -- 34.4 Кб -- 10.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>429) - www.mso.anu.edu.au/ )
14. The Effect of Relativistic Wind on Accretion Flow Parameters
... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...
[
Сохраненная копия
]
Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node56.html -- 10.8 Кб -- 26.02.1997
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>370) - xray.sai.msu.ru/ )
15. Stellarium: SphericalRegion::DrawParams Struct Reference
Stellarium 0.12.3 . ... FileљStructure . ... SphericalRegion . DrawParams . ... SphericalRegion::DrawParams Struct Reference . Parameters specifying how to draw a SphericalRegion . More... #include < StelSphereGeometry.hpp > . DrawParams (class StelProjector *projector) . Construct DrawParams with default parameters and specified projector. ... Do not subdivide the region to follow projection distortions. ... class StelProjector * SphericalRegion::DrawParams::projector_ . ...
[
Сохраненная копия
]
Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/structSphericalRegion_1_1DrawParams.html -- 22.0 Кб -- 28.02.2014
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>484) - astro.uni-altai.ru/ )
16. The Tenth Cambridge (10C) Survey
Welcome to the 10C Survey website! ... The first 10C Survey results from an area of 27 sq. degrees complete to 1 mJy and 12 sq. degrees complete to 0.5 mJy have now been released. ... The first results from the survey, which is the deepest extragalactic radio source survey of any significant extent (> 0.2 sq. degrees) above 1.4 GHz, including the deep 15.7-GHz source count are contained in AMI Consortium: Davies et al. ... For each field, deep and shallow areas have been defined. ...
[
Сохраненная копия
]
Ссылки http://www.mrao.cam.ac.uk/projects/surveys/10C/index.html -- 5.4 Кб -- 17.12.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1272) - www.mrao.cam.ac.uk/ )
17. Database of Optical Properties -- Level: subpage
... This page will contain a form to pass parameter values for a on-line working code producing figures illustrating the dependence of optical properties of different scatterers on their parameters. Specify the parameters and press start calculation button to produce a figure. ... Independent variable: x v a/b alpha Re(m)? another? ... Number of curves: 1 2 3 . ... Curve #1: . Particle shape: sphere spheroid another? TE/TM mode: TE TM . Other parameters: x= Re(m)= Im(m)= a/b= alpha= . ...
[
Сохраненная копия
]
Ссылки http://www.astro.spbu.ru/DOP/9-TOOL/index.html -- 5.4 Кб -- 19.11.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>243) - www.astro.spbu.ru/ )
18. A Python-based IRAF Task Parameter Editor
... As part of the development of a new Python-based CL for IRAF tasks by the Science Software Group at STScI, we have developed a GUI-based parameter editor for IRAF tasks using Tkinter. This new parameter editor is intended to provide the equivalent functionality of the IRAF EPAR task, but to make parameter editing easier by using appropriate user interface elements, such as menu choice lists, action buttons, and file browsers. ... Figure 1: The GUI-based Python/Tkinter IRAF task parameter editor. ...
[
Сохраненная копия
]
Ссылки http://www.adass.org/adass/proceedings/adass99/P1-54/ -- 11.1 Кб -- 06.10.2000
Похожие документы
Похожие документы
19. SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...
[
Сохраненная копия
]
Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/slitless/slitless.hlp.html -- 7.3 Кб -- 06.06.2006
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>224) - www.stecf.org/ )
20. Uses of Class ij.io.FileInfo (ImageJ API)
... Class . Use . ... Packages that use FileInfo . ... ij.io . ... Methods in ij that return FileInfo . ... Returns a FileInfo object containing information, including the pixel array, needed to save this image. ... Returns the FileInfo object that was used to open this image. ... Displays the dialog and returns a FileInfo object that can be used to open the image. static FileInfo . ... Returns the FileInfo object used to import the last raw image, or null if a raw image has not been imported. ...
[
Сохраненная копия
]
Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/io/class-use/FileInfo.html -- 16.9 Кб -- 02.12.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>406) - www.astro.louisville.edu/ )
Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
Комментарии, вопросы? Пишите: info@astronet.ru или сюда