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 . ...

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• Stellarium: ScreenImageMgr Class Reference
• Stellarium: StelHTTPTextureLoader Class Reference
• Stellarium: BigStarCatalogExtension::SpecialZoneArray< Star > Class Template

... A number of parameters appear in the parameter area which correspond to the status of the package when the interface is created. These parameters can be changed by typing the new values in the field, or reading them from a previously saved session table. The option in the menu may be used to read a session file. The name of the currently loaded session is indicated in the first text field Session at the top of the parameter area in the Main window. ...

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• VISUAL/PERS
• Loading the Telescope and Instrument Specifications
• FILTER/WAVE

... HST . UDF/ACS Parameters: . Pointing, Filters, Depth, and Status . ... Data . ... Based on a consensus recommendation of a Scientific Advisory Committee to the STScI Director Steven Beckwith, supported by planning documents from a local Working Group , the parameters below have been adopted for the HST/ACS Ultra Deep Field. ... At the center of this picture the light blue diamond shows the ACS/WFC pointing of the Ultra Deep Field (UDF). ... Relative Depth of UDF w.r.t other HST surveys . ...

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• Instrumental Parameters
• ramp_optimal_filter.pro (JWST Pipeline routines in IDL)
• Linear Ramp Filters

... 1.1 Supported Data Formats . 1.1.1 Converting Other Data Formats to Karma Format . 1.1.2 Converting Between Data Formats . ... 1.2 Adding your own Data Formats . ... 2.3 Sequences of Images . ... 2.12 Image Statistics . ... 2.15 Common Image Display Features . ... Image Statistics in the ImageDisplay Widget . ... GUI Command-line Switches . ... 3.2 View Control . ... Data List . ... Advanced Control Panel . Make Data Control Panel . Annotation List . ... Writing other Image Formats . ...

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• User Parameters - Mosaicking Continuum images CentralProcessor 0.11
• SAVE and LOAD
• Index

... region (region-7.5) [xmmsas_20050815_1803-6.5.0] . Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... Reference event file used to define the coordinate system for the source and background regions. ... If operationstyle =`single', the task looks in this parameter for the row number of the source list ( after the list is filtered via expression ) for which to construct source and local-background event-extraction regions. srcidcol . ...

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... 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. ...

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• A Graphical User Interface for a Development Environment (GUIDE)

... Parameters . Filters . ... Direct images . ... The SCORPIO-2 project: . Spectral Camera with Optical Reducer for Photometric and Interferometric Observations - 2 . The broad-band glass filters made in SAO RAS are used for the observation in the Johnson-Cousins (UBVRI) photometric system in the direct images mode. The glass filters transmission curves are shown by solid line. ... The filters transmission curves of the `comets' filters measured with the SCORPIO-2 in the F/4 beam. ...

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• LSVFO: SCORPIO filters
• проект SCORPIO-2: parameters
• Plug-and-Play-HOWTO : Tell the Driver the Configuration

This document contains a summary of the user interface for filtering rows in binary tables. Table filtering allows a program to select rows from an table (e.g., X-ray event list) by checking each row against one or more expressions involving the columns in the table. When a table is filtered, only valid rows satisfying these expressions are passed through for processing. ... select rows whose pha value is exactly 10 . ... 10 pha select rows whose pha value is in the range of 10 to 50 . ...

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• *qplintran* -- Apply linear transformation to a qp file through filter
• Using the PROS software
• Changes for release 1.8

... Class . ... METHOD . ... java.lang.Object ij.plugin.filter.Rotator . ... This method is called by ImageJ to inform the plugin-filter about the passes to its run method. int . ... This method is called after setup(arg, imp) unless the DONE flag has been set. ... The method should return a combination (bitwise OR) of the flags specified in interfaces PlugInFilter and ExtendedPlugInFilter . ... This method is called by ImageJ to inform the plugin-filter about the passes to its run method. ...

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• Convolver (ImageJ API)
• Binary (ImageJ API)
• Translator (ImageJ API)

Next: Loading tables Up: Accessing data files Previous: Accessing data files Contents . ... If file is not open, set default system ID (NPOI). get_datum [, datum ] Read Date from HDS file. ... If file is not open, set default date (the next day). get_geoparms [[, sysid ][, datum ]] Load GeoParms object from HDS file. ... Next: Loading tables Up: Accessing data files Previous: Accessing data files Contents Christian Hummel 2015-04-28 ...

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• Load configuration, tables, and logs

The Agile window provides complete control over the Agile high-speed photometer. ... All other parameters are specified as part of the command that starts an exposure sequence. ... To connect the filter wheel controller, issue this command in the command bar at the bottom of the Log window: agile connDev fw . ... To home the filter wheel controller, issue this command in the command bar at the bottom of the Log window: agile fwhome (there must be a filter wheel mounted in Agile for homing to succeed). ...

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• what to do with the trace data
• Echelle for Beginners
• Astrophysical Research Consortium - Apache Point Observatory

... L-Wide . ... Receiver History . ... Available Filters: . ... Use with e.g. filter 5) NOTE 2 1120-1220 3 1230-1470 4 1550-1820 5 1100-1800 6 1360-1470 7 1320 hipass NOTE 8 1180-1280 9 1280 hipass (ext Output unit. ... Consequently, the calibration for data collected using the hipass 1320 and the hipass 1370 filters only will be mis-calibrated (i.e. by using the opposite polarisation calibration data). ... It is now possible to select any bandpass filter that is not in the 1320 hipass band. ...

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• CIMA Configuration Files
• Arecibo Observatory 430-MHz Gregorian Receiver
• pdev_birdies_25jun07

... Space flight . ... Zero Gravity . ... Characteristics of a Complex Flight: . ... Characteristics of the Reduced Gravity (Lunar Gravitation): . ... Characteristics of the Reduced Gravity (Martian Gravitation): . ... Services / Zero Gravity: General description Technical description Flight parameters Photo gallery Price . ...

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Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Initial binary parameters
• Initial parameters of compact stars
• Other parameters of the evolutionary scenario

... Обзор LPR фильтра. Впечатления от наблюдений с LPR фильтром. ... Характеристики цветных фильтров Baader-Planetarium . Мой перевод pdf- файла о фильтрах с сайта Baader-Planetarium (379 кб) . ...

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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. ...

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• mod_ext_filter - Apache HTTP Server
• Increasing number of open files parameter
• Program parameters

... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

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• White Dwarf Merger Movie
• SCL Sfit Commands

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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... 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 WFPC2 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 # ! ...

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• http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/demo/demo_foc.cl
• SLITLESS (Oct97) --- ST_ECF --- SLITLESS (Oct97)
• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)

MAKING THE PROFILES . First of all you are expected to load a FITS file ("FILE"-"LOAD"). ... By pressing the middle button you copy the profile from the first profile window to the second one. ... An example: first integral can correspond to the profile of active region and second integral can correspond to the profile of quiet chromospheric region. ... The second profile (which is subtracted from the first one) you extract after clicking on "SUBTRACT"-"MARK QUIET PROFILE" and marking the region. ...

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• IMCCE-SAI: Natural Satellites Data Center (NSDC). Parameters