... HST . How precise are the parameters of my double star as measured in Transfer Mode? ... Data . ... HST Peer Review Process . ... HST Overview . Overview . ... Retrieving HST Data . ... Data Analysis . ... HST Science Year in Review . ... FGS Data Handbook . ... A: Analysis of calibration and other data has shown that the separations obtained in the analysis the Transfer Functions of double stars have a precision of around 1 milli arc-second. ...

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• Index
• COS Instrument Handbook
• CDBS FOS Page

... Output parameter that contains the X coordinate centroid. This will be in the units of the input image, e.g. sky pixels, detector pixels or degrees. ycentroid . ... Output parameter that contains the optimum extraction radius in the units of the input image (sky pixels, detector pixels or degrees). optellipxrad . ... Output parameter that contains the optimum X radius in the units of the input image (sky pixels, detector pixels or degrees) for an elliptical extraction region. optellipyrad . ...

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Next: Results of follow-up spectroscopy Up: Data reduction Previous: Reduction of the Calar . In the final spectra, redshifts and line fluxes are measured within MIDAS, applying Gaussian fitting to the emission lines. To determine redshifts for individual galaxies, averages are taken over the prominent individual emission lines (mostly H , H , [O III ] 4959,5007 ?) The line [O II ] 3727 ? ... For all spectra, the individual emission line fluxes of the H , [N II ] 6548,6583 ? ...

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• HyperLEDA documentation: parameter: Mg2
• Estimating the Sky Background
• Documentation: LEDA: parameter: m21c

... The visibility datasets possibly contain correlations for different polarizations and Stokes parameters. There are two basic ways that polarization characteristics can be measured: firstly, two orthogonal feeds can be present on the antennas, and the four different polarization correlations from a baseline can be taken and recorded. ... There are two ways the user can determine which polarizations he or she wants to process, either with the select parameter, or with the stokes parameter. ...

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• User Parameters - Data Location & Beam Selection CentralProcessor 0.11
• User Parameters - Preparation of the Science field data CentralProcessor 0.11
• SCINTILLATION PARAMETERS FOR 49 PULSARS

AUTOMATIC STATION OF ECOLOGICAL CONTROL . ... BASIC PERFORMANCE SPECIFICATION . STATE OF ASEC DEVELOPMENT . AIR POLLUTION MONITORING . ... OF MEASURING CHANNELS . ... unit of measurement . ... Nitric oxide (NO) concentration, . ... power measured by ASEC . ... In particular, RSC Energia finalizes its work on measurement systems designed to measure dust, volumetric activity of radioactive gases and aerosols and other environmental parameters. ... Official WEB-site of S.P.Korolev RSC Energia . ...

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... Guider functions . ... Guide Sensor Performance . ... Guide Sensor Sky Coverage/ Star Availability . Guide Star Selection Criteria . ... Guide fiber organization and reach at plug plate . ... Plug plate holes for guide stars are identical to those for science FO . ... FOV for each of 9 guide stars is 7.4 arcsec dia. (0.45 mm FO, Sumitomo IGN-05/10) . ... Selected guide stars must have no neighbor stars within TBD (5 arcsec) radius that have a brightness within TBD (5 mag.) of guide stars . ...

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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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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• TwoFitlines: An Spectrum and Line Analysis Tool
• A Spectroscopy Exposure Time Calculator for IRAF

... Recent Band Averaged Measurements . Gain, SEFD, Tsys, and Beam width . ... This is the band averaged Gain, SEFD, Tsys, and Beam width for ALFA taken at regular intervals. ... For performance figures as a function of frequency, see the ALFA spectral scans . ALFA spectral parameters & calibration . ... The fit parameters for the spectral scans can be downloaded. ... Details are given in the memo by Desh: ALFA spectral parameters & calibration . ... Spectral scans across the full ALFA band. ...

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• AGES Database Search
• Arecibo Observatory L-Wide Band Receiver
• Arecibo Observatory: S-Low Band Receiver

... WMAP7 -- 7 year WMAP data ( Larson at al., ... SPT -- CMB power spectrum from SPT ( Keisler et al., ... CDM -- flat Universe with cosmological constant . ... N eff 3.046 . ... WCDM -- flat Universe with dark energy . ... CDM, WMAP7+BAO+H0 +CL . CDM, WMAP7+BAO+H0+SPT +CL . ... CDM+f (1), WMAP7+SPT+BAO+H0 +CL . CDM+f (1)+N eff , WMAP7+SPT+BAO+H0 +CL . ... CDM+N eff , WMAP7+BAO+H0 +CL . ... CDM+dn/dlnk, WMAP7+BAO+H0 +CL . ... WCDM, WMAP7+SPT+BAO+H0 +CL . ... WCDM, WMAP7+SPT+BAO+H0+SNSYS +CL . ...

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• Regions and Source Parameters
• Filtering ROSAT HRI data on the basis of background level
• Determine a background subtracted radial profile

Applying Bayesian analysis to polarisation data J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR MKSP Workshop 1 / 15 Outline 1 2 3 4 Polarisation simulations @ radio wavebands Bayesian analysis Analysis of polarisation data Conclusions J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR ...

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• http://www.mrao.cam.ac.uk/~graca/talks/PhiSky_Rocha.pdf
• PPEUC Programme - Cosmic Microwave Background Workshop
• ALMA Phase Calibration Techniques at the Cavendish Astrophysics Group

... 18-1 74 40.5 0.52 Cas A . 18-1 75 38.5 0.49 Cyg A . ...

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• Parameters of the Moon-perturbed orbit
• MILLIMETRON

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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• Program parameters
• Where are the tunable parameters of the kernel?
• Kernel tunable parameters

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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• Other parameters of the evolutionary scenario
• Initial binary parameters
• Restrictions on the Scenario Parameters

... Class . Use . ... Packages that use Roi . ... ImagePlus. roi . Methods in ij that return Roi . Roi . ... Methods in ij with parameters of type Roi . void . ... A subclass of ij.gui.Roi (2D Regions Of Interest) implemented in terms of java.awt.Shape. class . ... Methods in ij.gui with parameters of type Roi . ... Methods in ij.measure with parameters of type Roi . ... Methods in ij.plugin with parameters of type Roi . ... Methods in ij.plugin.filter with parameters of type Roi . ...

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• CurveFitter (ImageJ API)
• Uses of Class ij.measure.Calibration (ImageJ API)
• MaximumFinder (ImageJ API)

instr> Quality Control: . Image flats . ... noise parameters | ... linearity, gain . ... While the ordinary, daily fibre flats mainly measure fibre characteristics, the image flats are exposures of the CCD by the flat field lamp without the fibre system. ... Two kinds of small-scale fluctuations exist in any raw frame: photon noise, and fixed-pattern (gain) noise (the third source, read noise, is negligible here). ... The penalty to pay is added photon noise, inherent in the image flats. ...

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• Parameters
• CONSTRICTOR parameters for astrometric reductions
• Preparation of parameter file

... The Irkutsk IS radar has the opportinuty to measure several ionospheric plasma parameters such as electron density N e , electron and ion temperatures T e , T i , and drift plasma velocity along the sounding direction. ... To the 1999-2001 data we have added the E-layer ionosphere model to electron concentration profile, which has been constructed by integral concentration from the ionosphere beginning from 160 km obtained from experiment. ... Capabilities and samples | ...

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• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
• East Siberian Center for the Earth's Ionosphere Research. Specific character
• East Siberian Center for the Earth's Ionosphere Research. Ionospheric parameter

... 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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Flavor Tagging with a CCD Vertex Detector: Higgs BRs as a Benchmark Chris Potter and Jim Brau University of Oregon Chicago Linear Collider Workshop January 8, 2002 J.Brau , Chicago , Jan 8, 2002 1 Outline Review of Snowmass Study of Higgs Branching Ratio Measurement Investigation of Improved Jet - level NN tag Improved Event- level tags and new estimate of H cc precision J.Brau , Chicago , Jan 8, ... In this analysis, we are essentially tagging on one of the two possible jets. ...

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• http://zebu.uoregon.edu/~uochep/talks/talks00/brau_D3.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks00/brau_P1.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks05/trackrecon.pdf

... Romanyuk , V . ... Instrumental circular and linear polarization is shown to be insignificant. ... It is planned to be used for determination of a magnetic field structure of peculiar stars, and dipole orientation, for study of circular and linear polarization wide depressions within 4200 - 5200 A being characteristic for magnetic star spectra and also for other spectropolarimetric investigations of various objects in narrow (dozens of A) and wide (hundreds of A) spectral regions. ...

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• проект SCORPIO-2: parameters
• SCORPIO parameters
• Parameters of the 41 Dra system components

ENERGOSPECTROMETER OF IONOSPHERIC PLASMA P3-3 . ... The major objective of the P3-3 experiment is complex investigation the main parameters of ionospheric plasma with high time and spatial resolution. ... Measured parameters: . ... The experiment produce regular data - measured with fixed time interval and «packet» data - measured once per specific time interval and producing blocks of TM-information. ... If all parameters will be measured once per second, the experiment will produce 10 MB per orbit. ...

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• Optical static Fourier spectrometer
• Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).
• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).