. Main Page . Adapter . Parameters . Optics . Filters: . Broad . Middle (SED) . Comets bands . Narrow (IFP) . Multislit . Grisms . Fabry-Perot . Gallery . References . Manuals . Last update: . 4 Aug 2013 .

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• http://mavr.sao.ru/hq/lsfvo/devices/scorpio/contents_IFP.html
• SCORPIO-2 project: filters
• LSVFO: SCORPIO filters

. Main Page . Adapter . Parameters . Optics . Filters: . Broad . Middle (SED) . Multislit . Grisms . Gallery . References . Manuals . Last update: . 10 Sep 2013 . Webpage responsible . M.M.Gabdeev (gamak@sao.ru) .

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• http://www.sao.ru/hq/lon/SCORPIO/contents_gal.html
• http://www.sao.ru/hq/lon/SCORPIO/contents.html
• LSVFO: SCORPIO filters

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: StelQGLTextureBackend Class Reference
• StelTexture::StelTextureParams Struct Reference
• Stellarium: SphereParams Struct Reference

... File . ... use frames summary class fields routine details file attributes . ... JWST Data Processing - NIRCam Cryo tests . ramp_OPTIMAL_FILTER , data0 . ... data0 in out required type=fltarr(2048,2048,Ngroup) . ... IDL> ramp_optimal filter, data0 . ... M. Robberto, created 25 Apr. ... Lines: . 32 lines . ... Tue Apr 30 15:07:13 2013 . ...

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• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
• Tabular Reference Data
• corrector.pro (JWST Pipeline routines in IDL)

... HK file type: PeriodicHousekeeping [22 parameters ] ---------------------------------- FILTER_WHEEL string [E1257] FILTER_WHEEL_POSITION Uint16 [E1317] FILTER Uint16 [E1317] This parameter is translated as follows : Translator's name: EMOS1 Filter 0 = Closed 247 = CalThin1 267 = Thin1 514 = CalThin2 534 = Thin2 781 = CalMedium 801 = Medium 1047 ...

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• Parameters

... 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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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• Recognition of Anomalous Events
• CAOS Simulation Package 3.0: an IDL-based Tool for Adaptive Optics Systems

... 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.) ...

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• Chandra Images for G340.6+00.3
• Chandra Images for G332.4+00.1
• Chandra Images for G352.7-00.1

... This section gives a brief description of each of the parameters available to SCHED that are specifically for VLA observations or are especially useful for VLA observations. ... Should be provided for non-VLBI observations. ... This used to be required in order to obtain calibration data for the VLBI observations. ... FREQ: and DOPPLER Warning -- these parameters cannot be used for non-VLBI observations at the VLA since they are only used to adjust the baseband converter frequencies. ...

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• casacore: casa::FunctionTraits< T > Class Template Reference
• casacore: casa::FunctionWrapper< T > Class Template Reference
• casacore: casa::CompoundFunction< T > Class Template Reference

RSAA Home . GSAOI Home . ... Other Links . ... Control Software Links . Optics Links . Micro-Optics Links . ... Optical Materials Databases . ... Rockwell Science Center home page . ... Santa Barbara Research Center home page . ... CCD-World home page . ... SDSU home page . ... EPICS home page . ... Optics Society of America . SPIE - Society for Optical Engineering . ... ZEMAX software (Focus Software page) . OPTICAD software (Focus Software page) . ... RedHat home page . ...

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• Instrumentation Links.
• Gemini South Adaptive Optics Imager Performance Calculator

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• The Galaxy Gallery: Messier Objects

The magnetic mapping is fulfilled by the magnetic field line tracing from the satellite position up to the Ionosphere (stop trace at the altitude 110 km). ... As a rule the Tsyganenko [1987] external magnetic field model and IOPT = 3 (Kp = 2) are used. ... The output file includes the following information: . ... For example the file with name aa9610d1.geo contains the information corresponding to the aposteriory magnetic mapping for INTERBALL Auroral Probe for the first decade of October 1996. ...

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• Magnetic mapping file description

... dust_AbsXSec . Absorption Cross section. typedef void . ... Calculates the equilibrium temperature given the absorption cross section and a radiation field. double . ... Calculates the absortion cross section of a species/size of dust grain . ... The grain absorption cross section . ... The absorption cross section of the grain . ... Calculates the equilibrium emission at wavelength lambda from a (large) grain at temperature T and with absorption cross section xsection. double dust_EquiT . ...

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• write_fits.c File Reference
• read_fits.c File Reference
• DUST: dust_sdpars Struct Reference

... Files . ... tcc.msg.formatObjFields Namespace Reference . ... Definition at line 36 of file formatObjFields.py . ... Definition at line 107 of file formatObjFields.py . ... Definition at line 115 of file formatObjFields.py . ... Definition at line 129 of file formatObjFields.py . ... Definition at line 122 of file formatObjFields.py . ... Definition at line 213 of file formatObjFields.py . ... Definition at line 139 of file formatObjFields.py . ... Definition at line 247 of file formatObjFields.py ....

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• lsst.tcc: tcc.parse.getCoordSys Namespace Reference
• lsst.tcc: tcc.parse.getPVTList Namespace Reference
• APO - MSSSO filters

... The timecode of these receivers is sampled via a STREAMS module in the kernel (The STREAMS module has been designed for use with SUN Systems under SunOS 4.1.x. It can be linked directly into the kernel or loaded via the loadable driver mechanism). ... The reference clock support in xntp contains the necessary configuration tables for those receivers. In addition to supporting up to 32 different clock types and 4 devices, the generation a a PPS signal is also provided as an configuration option. ...

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• Debugging Hints for Reference Clock Drivers
• NIST Modem Time Service
• Zen: sncat design

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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• Tunable Kernel Parameters?
• Mail Filters
• Digital backends

... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Travel to E-ELT Armazones . ... ESO . ... Survey Telescopes . ... Images . ... Star Clusters . ... Usage of ESO Images and Videos . ... Usage of ESO Videos and Images . ... Catch a Star 2013 . ... The image shows the near-diffraction-limited image of a 17-mag reference star, as recorded with NAOS-CONICA during a 200-second exposure in the K-band under 0.60 arcsec seeing. ...

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• Image of a 17-mag Reference Star | ESO Ireland
• Image of a 17-mag Reference Star | ESO Australia
• Image of a 17-mag Reference Star | ESO United States

... Detailed information about each program can be found in the separate manual pages. blockmean L2 (x,y,z) data filter/decimator blockmedian L1 (x,y,z) data filter/decimator blockmode Mode (x,y,z) data filter/decimator filter1d Filter 1-D data sets (time series) fitcircle Finds the best-fitting great circle for a set of points gmtconvert Convert between ASCII and binary 1-D ... Wessel, P., and W. H. F. Smith, 1991, Free Software Helps Map and Display Data, EOS Trans., ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/triangulate.html
• ADS Abstract Service

... Class . ... METHOD . ... java.lang.Object ij.plugin.filter.UnsharpMask . ... public class UnsharpMask . ... Unsharp masking subtracts a blurred copy of the image and rescales the image to obtain the same contrast of large (low-frequency) structures as in the input image. ... This method is invoked by a Generic Dialog if any of the inputs have changed (CANCEL does not trigger it; OK and running the dialog from a macro only trigger the first DialogListener added to a GenericDialog). void . ...

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• MaximumFinder (ImageJ API)
• Uses of Class ij.plugin.filter.PlugInFilterRunner (ImageJ API)
• Translator (ImageJ API)

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 . ...

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• WCS2DR (V1.0) --- Jan00 --- WCS2DR (V1.0)
• SEEING (V1.3) --- Apr00 --- SEEING (V1.3)
• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)

... 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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• Arecibo Observatory 610/700-MHz Band Receiver
• Arecibo Observatory Narrow S-Band Receiver (2.24-2.42 GHz)
• Arecibo Observatory: S-Low Band Receiver