Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 109822 (152 сайтов) ---- Время поиска: 0.26сек.   

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.sao.ru/hq/lon/SCORPIO/filters/filters.html.

1. LSVFO: SCORPIO filters
SCORPIO FILTERS . UBVRcIc-filters . Glass filters for Jounson-Cousins photometric system. ... Broad-band filters parameters (filter+optics+CCD EEV42-40): . name . Tmax(%) . ... ASC-file . Image . ... SED-filters . Middle-band filters for Spectral Energy Distribution. ... SED filters parameters (for beam F/4) . ... SED 830 and SED 930 . ... Middle-band filters for comets molecular bands. ... IFP-filters . ... IFP filters parameters (for beam F/4) . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lsfvo/devices/scorpio/filters/filters.html -- 10.0 Кб -- 04.02.2013
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lsfvo/devices/scorpio/filters/filters.html -- 10.0 Кб -- 04.02.2013
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio/filters/filters.html -- 10.0 Кб -- 02.02.2013
Похожие документы

2. A New Entropy Measure Based on Multiple Resolution and Noise Modeling
... Previous: Background Fluctuation Analysis from the Multiscale Entropy . ... A new measure of information is defined which is based on noise modeling and incorporates resolution scale. Properties of this measure are discussed. ... Additionally it allows for image noise modeling, and subsequent noise removal. ... Hence information- and entropy-based processing technologies will be necessary for the effective design and implementation of large, future generation, image databases. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/murtaghfd/ -- 17.8 Кб -- 16.07.1999
Похожие документы

3. what to do with the trace data
... Here is a sample parameter file that is set to plot the B filter trace data. ... One can generally get by with the default graph parameters. input = B.a list of images or list files to be graphed (wx1 = 3000.) left world x-coord if not autoscaling ... autoscaling (wy2 = 100.) upper world y-coord if not autoscaling (wcs = logical ) Coordinate system for images (axis = 1) axis along which projection is to be taken (transpose = no) transpose the x and y axes of the plot (pointmode = no) ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Instruments/filters/tracehelp.html -- 4.8 Кб -- 22.02.2001
Похожие документы

4. *qplintran* -- Apply linear transformation to a qp file through filter
... Transforms a qpoe file according to the specified parameters. ... Any type of filtering can be applied to the input qpoe file, including region filtering. In addition, the size of the output event record can be different from the size of the input event record. Of course, usually one makes the output record equal to or smaller than the input. If the output record size is made greater than the input record, a warning is issued and the ``extra'' part of the record is undefined.) ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node52.html -- 6.2 Кб -- 01.10.2012
Похожие документы

5. Uses of Class ij.plugin.filter.PlugInFilterRunner (ImageJ API)
... Class . Use . ... GenericDialog. addPreviewCheckbox ( PlugInFilterRunner pfr, java.lang.String label) . ... UnsharpMask. showDialog ( ImagePlus imp, java.lang.String command, PlugInFilterRunner pfr) . ... Translator. showDialog ( ImagePlus imp, java.lang.String command, PlugInFilterRunner pfr) . ... StackLabeler. showDialog ( ImagePlus imp, java.lang.String command, PlugInFilterRunner pfr) . ... Rotator. showDialog ( ImagePlus imp, java.lang.String command, PlugInFilterRunner pfr) . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/filter/class-use/PlugInFilterRunner.html -- 18.1 Кб -- 02.12.2010
Похожие документы

6. Determination of the Detector Parameters
The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/desc/det_per.html -- 5.0 Кб -- 16.02.2000
Похожие документы

7. List of Frequency File Parameters
Next: Setup Files Up: Frequency Catalog Previous: Frequency Catalog Contents . The parameters of the frequency file tell SCHED over what frequency range the group if usable and on which stations. Most of the parameters are the same as parameters in the setup file since they are meant for direct substitution once the correct frequency group has been identified. ... This will be matched against the station name in the setup file. The name VLBA will be a default for all VLBA stations. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/List_Frequency_File_Paramet.html -- 10.9 Кб -- 10.04.2016
Похожие документы

8. Stellarium: TextureParams Struct Reference
Stellarium 0.12.3 . ... FileљStructure . ... TextureParams Struct Reference . Parameters specifying how to construct a texture. More... #include < StelTextureParams.hpp > . ... filtering (const TextureFiltering filtering) . Set texture filtering mode. ... Texture filtering mode. ... Default parameters (no mipmaps, linear filtering, clamp to edge wrap mode). ... TextureParams c = TextureParams ().generateMipmaps() .filtering(TextureFiltering_Nearest).wrap(TextureWrap_Repeat); . ... wrap . ...