... User Guide ] Task: uvgains Purpose: Create baseline-based channel gains from averaged uv-data Categories: uv analysis UVGAINS averages uv-data, and creates channel gains for each baseline for either spectral line or wideband channels. ... To apply the channel gains to another uv-data file, use COPYHD to copy the channel gains items (cgains, ncgains, ncbase) or wideband gains items (wgains, nwgains, nwbase) into the other uv-data file. ... Only un-averaged channel data can be used with options...

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• Index
• userhtml
• Spectral Line Processing and FITS files

... HST . FAQ: How do I know that wavecal processing worked correctly? ... Data . ... HST Peer Review Process . ... HST Overview . Overview . ... Phase I Proposing . ... Retrieving HST Data . ... ID: How do I know that wavecal processing worked correctly? Wavelengths in 1-D extracted spectra and 2-D rectified images will not be correct unless the offset of the Mode Select Mechanism (MSM) in the dispersion direction was successfully determined from the wavecal associated with the observation. ...

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• Errors in Processed TIME-TAG Data from STIS Now Corrected
• Fine Guidance Sensor Instrument Handbook
• On-The-Fly Calibration/Reprocessing Systems

... This article describes the AXAF aspect determination pipeline and its components, and highlights a procedure for determining centroids-a crucial step in deriving the post-facto aspect solution. ... The Ground Aspect Determination System (GADS) pipeline is a collection of tools which process aspect telemetry and generate aspect data products. ... Using a subset of ACA pixel data from the Aspect Interval, we identify poorly-fitting PSFs and find spoiler stars in star and fiducial light images. ...

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• ISO-SWS Data Analysis
• The Basic Calibrated Data Processing Pipeline for SIRTF IRS
• The SRON-HeaD Data Analysis System

Next: IDL Up: Data Processing Previous: Quick Look Tools . The Lynxx software has its own quick analysis tools. ... As previously discussed, the images can be rescaled, but if intensities are to be measured, the images should not be rescaled. ... Before starting any analysis on an image, the calibration frames must be removed from the image. ... Meas intensity is the command that will measure the intensity of the object in a square region around a star. ... It is advised to use the SBIG software. ...

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• Quick Look Tools
• Notes on IPC and PSPC Spectral Fitting
• The AstroStat Slog confidence interval

... 3.2 CTI correction In CCDs part of the charge released by an absorbed photon is lost during transfer to the readout node. This loss depends on several parameters, in particular on the position where the photon was detected, its energy, the temperature of the CCD, and the saturation of traps by charges preceding along the readout direction. ... The model accounts for the e ects of incomplete charge collection close to the detector surface. ...

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• http://xmm.vilspa.esa.es/sas/8.0.0/doc/calpnalgo.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/calpnalgo.ps.gz
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/calpnalgo.ps.gz

... The data was taken over many days with the same source in more than one file. ... You want to convert the data to kelvins (this is galactic work) and then average all the scans for each source. ... input each onscan, average, and then scale to kelvins . place all of the averaged scans in an array, when done with the file, store this array in an idl save file for this day. ... Average together scans of the same source and then baseline them. input all of the daily save files into a single array . ...

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• http://www.naic.edu/~phil/notes/idlspcproc.html
• p2111
• OLD ANALYZ instruction sequences HI in galaxies

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• Processing the "Face on Mars" Images
• Dr. Victoria I. Prokhorenko
• Phobos Mission

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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• East Siberian Center for the Earth's Ionosphere Research. Capabilities and

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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Next: Illumination Corrected Flat Up: Special Processing Options Previous: Sky Illumination Frame . After the illumination frame has been created, one can multiply the original flat field by the illumination frame, resulting in an adjusted flat field. ... The output frame is called sky flat. ... How good this new flat field is can be checked by correcting the blank sky once more, using this sky flat. ... To create the sky flat fields the command SKYFLAT/CCD is available. ...

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• Processing the Data
• Creation of Sky Correction Frames
• Special Processing Options

Next: The STScI NICMOS Calibration Up: No Title Previous: CONICA: The high resolution . The STScI NICMOS Calibration Pipeline . Introduction . ... Dark Current Subtraction . ... Input Data . ... Scalar Background Subtraction . 2-D Background Subtraction . ... Status and Goals of the NICMOS Calibration Plan . ... Photometry . ... Photometric Performance of NICMOS . ... NICMOS Photometry. ... ST-ECF Grism Spectrum Software for NICMOS Grism Data . ... Analysis . ... STScI NICMOS Software . ...

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• STScI NICMOS Software

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . IPAC exists to carry out large, data-intensive processing tasks of critical importance to NASA's infrared astronomy program, and to provide scientific expertise on those projects to the astronomical community. ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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The visibility amplitude bias (there is also a closure phase bias, but this one is nominally corrected by the raw data averaging pipeline) is related to non-Poisson detector statistics due to after-pulsing, and to fixed pattern noise due to non-linearities in the modulation stroke. We determine the bias using so-called incoherent scans, which record data even though the delay lines are deliberately set away from the white light fringe. ... Averaging triple products.. ... Background data loaded. ...

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• ESO - Request Handler FAQ
• ESO - Processing of my NIR daytime calibration data fails - why?
• Astrometry

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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Irregular phenomena in the Earth Pole oscillation process and temporal variations of geopotential Valery Bondarenko, Vadim Perepelkin s The observed irregular phenomena in the Earth Pole oscillation process are very variety. ... These phenomena indicated in the IERS data are the "abnormal" fluctuation of the Earth Pole coordinates which owing to changing of the geodynamical parameters gives negative result in interpolation and forecast of the first approximation mathematical model. ... Fig. ...

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• Pulkovo EOP and Reference Systems Analysis Center (PERSAC)
• The Canadian S2 Correlator - Principles of Radio Interferometry

Modules | ... Apache HTTP Server Version 2.4 . ... Several changes in 2.0 and above affect the internal request processing mechanics. ... There were a number of different code paths in the Apache HTTP Server 1.3 to attempt to optimize subrequest or redirect behavior. ... The Request Processing Cycle . The Request Parsing Phase . ... If a module doesn't pass generated requests through this code, the author is cautioned that the module may be broken by future changes to request processing. ...

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• Processing the "Face on Mars" Images
• worker - Apache HTTP Server
• Multi-Processing Modules (MPMs) - Apache HTTP Server

... Class . Use . ... Packages that use ij.process . ... Classes in ij.process used by ij . ... This abstract class is the superclass for classes that process the four data types (byte, short, float and RGB) supported by ImageJ. ... Classes in ij.process used by ij.gui . ... Used by the Roi classes to return float coordinate arrays and to determine if a point is inside or outside of spline fitted selections. ... Classes in ij.process used by ij.plugin . ... Classes in ij.process used by ij.process . ...

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• Uses of Class ij.process.FloatProcessor (ImageJ API)
• ij.process (ImageJ API)
• FloatPolygon (ImageJ API)

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

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• Meteo :: Kislovodsk Database ::

The investigation of features of electromagnetic waves propagation, their generation and absorption in weakly inhomogeneous chiral media were started and the following results were obtained : . the governing equations to describe the electromagnetic waves interaction with inhomogeneous chiral plasmas were derived (together with N.S.Erokhin); . ... it was proven the 100 % hybrid mode conversion in the case of normal waves incidence upon inhomogeneous plasma (together with N.S.Erokhin); . ...

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• The INTERBALL Auroral PROBE orbital elements collections
• The Dynamo Process
• WAVE EXPERIMENTS ON TAIL PROBE

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

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• Laboratory for processing of very large data amounts on the basis of Big Data
• Nikonorov Artem Vladimirovich
• Bibikov Sergey Alekseevich