... The table that contains the event data - need to at least contain the columns named with the xcolumn , ycolumn , ecolumn parameters. colortablechoice . ... Choice parameter determining source of the color table that is to be used for the color coding. ... The name of the column that specifies the position of the event; passed to evselect as parameter xcolumn . ... The name of the column that specifies the scalar event attribute that is to be color-coded; passed to evselect as parameter zcolumn . ...

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

Fundamental parameters and time evolution of mass loss are investigated for post-main-sequence stars in the Galactic globular cluster 47 Tucanae (NGC 104). ... We confirm the cluster's distance as d = 4611+213 -200 pc and age as 12 ТБ 1 Gyr. Horizontal branch models appear to confirm that no more red giant branch mass loss occurs in 47 Tuc than in the more metal-poor Я? Centauri, though difficulties arise due to inconsistencies between the models. ...

... Possible values: @ echo mod1i1 - mod1i6; mod2i1 - mod2i6; mod3i1 - mod3i7 @ echo 5) the 2 letter name of the file for the time interval @ echo 6) step (sec, integer) @ echo 7) name of the file , which contains the resulting files extension set @ echo ---------------------------------------------------------------------- @cd ..\ikiodb @if %7.==. goto noparm @if exist indata \p% 2.hed copy indata \p% 2.hed orb.hed @if ...

... Parameters can be used as fixed or free parameters depending on the setting in MASK= To fix a parameter use 0. ... Use box -4 -10 9 5 and let all parameters be free in the fit : USER qfit USER QFIT FILENAME= data USER QFIT APPEND= USER QFIT AUTOVIEW=y USER QFIT INSET=n4736ave 1 Set n4736ave has 3 axes RA from -20 to 20 DEC from -31 to 20 LAMBDA from 0 to 1 BOX range for set n4736ave : RA from -20 to 20 DEC from -31 to 20 USER QFIT CLIPLOHI= ...

Full-Text Search in PostgreSQL: A Gentle Introduction . ... Fast Backward . ... DROP FULLTEXT PARSER -- remove a full-text parser . DROP FULLTEXT PARSER [ IF EXISTS ] prsname [ CASCADE | ... DROP FULLTEXT PARSER removes full-text parser from the database. ... To drop a parser and all FTS objects, which depends on it, CASCADE must be specified. ... Automatically drop FTS objects that depend on the parser. ... Refuse to drop the parser if any objects depend on it. ... CREATE FULLTEXT PARSER . ...

Next: External Functions Up: Fitting of Data Previous: The Corrected Gauss--Newton . ... Basic functions are either defined in the system or defined by the user as external FORTRAN routines. ... Basic functions are specified by the name, the independent variable(s) and parameter(s), with optional guesses for the parameters, following the syntax: name(var1[, ];par1[, ]) [par1=value] . ... Parameters are defined by unique names after the semicolon in the function specification. ...

Next: Data Analysis Applications . ... The past decade has witnessed a movement within the astronomical software community towards Open Systems . ... We present examples of user-customizable systems that can be built from existing tools, based on commonly-used infrastructure: a parameter interface library, FITS file format, Unix, and the X Windows environment. ... However, the currently available parameter file systems have serious limitations when inserted into a heterogeneous environment. ...

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. ...

Some Documentation for the IDL ICRED . ... This is the system which recieves all command inputs. it decodes inputs and selects tasks, parses parameter inputs and also runs the 'go', 'list' and 'help' commands. It does no error checking, for example to see if the parameter inputs are sensible (e.g. it does not check if an x-range has been entered as 'chicken', rather than a more understandable range of say 10,20). 2) the task decoders: icred_<taskname>.pro . ... Other tasks or important commands: . ...

main parameters . ... Small Detector   (SD) with thin polyethylene moderator and cadmium shield ; . Medium Detector (MD) with medium polyethylene moderator and cadmium shield ;   . Large Detector (LD) with thick polyethylene moderator and cadmium shield ; . ... Duty regime ; . ... Duty” frame with keeping data (92 bytes) in Duty r egime . Standard” frame with 6 spectra (212 bytes) in Mapping r egime . Profile” frame with 6 spectra and 2 profiles (512 bytes) in Burst r egime ...

... In this poster we propose a hypothesis that within fixed assumptions about internal physics (opacity, thermodynamics, nuclear reactions) a strict relation between the surface helium abundance and the entropy of the adiabatic part of the convective zone exists for all solar models. This hypothesis is verified with models under simplified physics (Christensen­Dalsgaard 1988) and with six evolutionary models computed by Christensen­Dalsgaard (1992). ... 1990, Christensen­Dalsgaard 1991). ...

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

... Scoring Necessary step towards more automated certification Idea: · define key QC1 parameters , check new values against trending for those · evaluate compliance: o if new within defined range, ok o if outside: nok · user may focus on nok ones, while ok is certified automatically in `confidence mode ' Required: · configure set of key parameters per product · configure comparison mode o fixed: ...

Astronomical Data Analysis Software and Systems VII ASP Conference Series, Vol. ... This trend has allowed projects and users to build customized processing systems from existing components. We present examples of user­customizable systems that can be built from existing tools, based on commonly­used infras­ tructure: a parameter interface library, FITS file format, Unix, and the X Windows environment. ... User Applications Users often need to sequence several tools. ...

... Here is a sample parameter file that is set to plot the B filter trace data. ... One can generally get by with the default graph parameters. input = B.a list of images or list files to be graphed (wx1 = 3000.) left world x-coord if not autoscaling ... autoscaling (wy2 = 100.) upper world y-coord if not autoscaling (wcs = logical ) Coordinate system for images (axis = 1) axis along which projection is to be taken (transpose = no) transpose the x and y axes of the plot (pointmode = no) ...

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

... comet nucleus. ... Very Long Baseline Interferometry (VLBI), Near Earth Objects (NEOs), cometary families , terrestrial type planets, collidings, transition of a comet nucleus , initial heliocentric parabolic orbit, heliocentric elliptical trajectory, a pairwise three dimensional two-body problem, the Sun - comet nucleus , terrestrial planet - comet nucleus , orbital parameters of a nucleus , sphere of influence of a ...

Nikolay Gusev: Summary In many cases mathematical treatment of liquids is done in the framework of incompressible fluid. ... Therefore it is reasonable to study the equations of low compressible fluid motion, in particular, convergence of their solutions to the corresponding incompressible limit. To emphasize the fact that the fluid is low compressible one should introduce a parameter which represents a measure of compressibility. ... Regularity and uniqueness of the solutions in dimension 2. ...