... use frames summary class fields routine details file attributes . GLS routines to calculate linear fit . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = linearize_mr( time , ramp ) . ... result = cephes_ndtri( y0 ) . ... Lines: . ... McCabe complexity: . ...

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alignasn -- Change the relative shifts in association file alignasn association . ... calnicb style association file with list of images to be aligned. ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...

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• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• MAKEPRFCORR (Nov98) --- nictools --- MAKEPRFCORR (Nov98)
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)

The starting page - The catalogues page - The list of the PUL2 fields - The list of the Pul-3(Pul-3SE) fields - The list of the PUL_ERS fields . please read short description of the access form controls . ... Relative proper motion in RA *cos(DE), arcsec/yr . ... s. e. relative proper motion in RA *cos(DE), arcsec/yr . ... Number of Pul2 area . ... Check the apropriate checkbox to output these data and radiobutton to select stars within interval. back to the list of the Pul2 fields . ...

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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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• Program parameters
• mod_macro - Apache HTTP Server
• Description of program searchdup

... CentralProcessor 0.11 documentation . ... These parameters govern the pre-processing needed for the science field, to split by beam, flag, apply the bandpass (although none of the parameters listed here relate to that), and average to continuum resolution. ... FIELD_SELECTION_SCIENCE . ... Range of channels in science observation (used in splitting and averaging). ... Dynamic threshold applied to amplitudes when flagging science field data [sigma] . ... User Parameters - Bandpass Calibration . ...

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• WCSLIB: prjprm Struct Reference
• Parameters Specific to the VLA
• WCSLIB: disprm Struct Reference

... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...

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• Initial parameters of compact stars
• Parameters of binary compact star evolution
• The Model

... A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. The text of the "outer" box (at the end of line 1, halfway into line 2, and halfway into line 3) is shifted upward 12px. The text of the "inner" box, thought shifted upward as well, has been relatively positioned so that it lies in its normal flow position at the end of line 2. ... The lines, as they appear in the image, contain: Start 1 Beginning of body contents. 2 of outer contents. Inner contents. ...

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• Long description for example illustrating positioning with respect to a
• Long description illustrating absolute positioning with respect to the initial

XMM-Newton Science Analysis System . ... This task returns the following statistical information for each column in the list specified by the parameter column , present in the table specified by the parameter table : . The minimum value . The maximum value . The mean average . The root mean squared . ... The results are written to the standard output as well as the text file specified by the parameter resultfile . XMM-Newton SOC/SSC -- 2008-07-02 ...

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• EPIC Related CAL Routines

... Wind, Air Temperature, Dew Point and Relative Humidity Statistics, yearly, 2000 to 2005 (pdf) and seasonal, 1999 to 2007 (pdf) . Wind and Wind gust . Temperature . Relative Humidity . Dew-point Temperature . ... Real Time Astroclimate . ... Astroclimatology of ESO Sites , ESO Wide Review, April 2000 . Paranal Long Term Astroclimate Analysis . ... Send comments to <Marc.Sarazin@eso.org> . Last update: September 8, 1999 . ...

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• web4 Astroclimatology
• extractStat
• ESO - Science Announcements

... Posts tagged ?nuisance parameter? ... Ah ha~ Once I questioned, ?what is systematic error?? (see [Q] systematic error. Thanks to L. Lyons? work discussed in [ArXiv] Particle Physics , I found this paper, titled Systematic Errors describing the concept and statistical inference related to systematic errors in the field of particle physics. ... Continue reading ?systematic errors? ... Comment . ... ArXiv]4th week, Mar. ... Entries RSS . Comments RSS . ... Entries (RSS) and Comments (RSS) . ...

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• Model Spectra for Spectral-Fitting Program
• The AstroStat Slog Blog Archive different views
• The AstroStat Slog Blog Archive [ArXiv] Identifiability and mixtures of

This page gives the name and meaning of the various parameters which can be queried in HyperLeda through SQL requests . ... real . ... actual error on t . ... log 10 of apparent major axis diameter d25 at 25 mag.arcsec -2 (d25 in 0.1') . ... actual error on logd25 . ... Apparent maximum rotation velocity of gas . ... log 10 of apparent corrected diameter (dc in 0.1') . ... total apparent corrected B-magnitude . ... total apparent corrected U-B color . ... Questions: leda@univ-lyon1.fr ...

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• Order Definition
• Implementation
• Documentation: LEDA: parameter: vvir

... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...

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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• ADASS 2003 Conference Proceedings
• Application of the Minimum Determination Algorithm to the Study of the Fine

... 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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• DUST: dust_silsdpars Struct Reference
• DUST: rastsizedist.hxx File Reference
• DUST: dust_sdpars Struct Reference

... They are concerned with Attitude Control System of the spacecraft, satellite visibility from tracking stations, limits on the satellite autonomous operations during the orbit, and needs for auxiliary operations with the spacecraft. ... Among the operational constraints the most important one is the number of programmed slews per orbit, which determines the maximum number of radio sources to be observed during one orbit. ... System temperature (K) . ... Progress of the RadioAstron Project in Pictures...

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... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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... ClassљIndex . ... StelRendererStatistics Class Reference . Stores and provides access to statistics about a StelRenderer backend. ... getNext (const char *&name, double &value) . Get next statistic name and value. ... Access statistic with specified index to modify it. ... while (statistics.getNext(name, value)) . ... Name of the statistic will be stored here (only a pointer to it). value . ... A clean way to do this is to use an enum with name corresponding to the name of the statistic. ...

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• Stellarium: ScreenImage Class Reference
• Stellarium: SphereParams Struct Reference
• Stellarium: RendererStatistics Class Reference

... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Celestial Mechanics

The MOD and IOPT parameters value depend of the external magnetic field model (MOD), used during magnetic mapping and IOPT version (IOPT = Kp + 1), see the table: . MOD . External model . IOPT range . ... N.A.Tsyganenko, Planet. Space Sci., ... N.A. Tsyganenko, A magnetospheric magnetic fields model with a warped Tail current sheet: Planet. Space SCI., ...

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• ASCII files description
• IKI SSC, INTMINS APRIL99
• IKI SSC INTMINS APRIL98

... CREATE FULLTEXT DICTIONARY -- create a dictionary for full-text search . CREATE FULLTEXT DICTIONARY dictname LEXIZE lexize_function [ INIT init_function ] [ OPTION opt_text ] ; CREATE FULLTEXT DICTIONARY dictname [ { INIT init_function | ... CREATE FULLTEXT DICTIONARY will create a new dictionary used to transform input word to a lexeme. If a schema name is given (for example, CREATE FULLTEXT DICTIONARY myschema.dictname ... ) then the dictionary is created in the specified schema. ... INIT . ...

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• CREATE FULLTEXT CONFIGURATION
• ALTER FULLTEXT CONFIGURATION
• CREATE FULLTEXT PARSER

... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fb Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/M3000