... yes . string . ... valid data set name . Name of the FITS file containing the list of observed sources . ... Name of the temporary file used by region during filtering of source list . ... Name of the temporary file containing the background regions for the sources. tmpflatset . ... Name of the file containing the temporary flatfielded image. tmpposmaskset . ... Name of the file containing the temporary positive image mask . ... Name of the file containing the temporary negative image mask . ...

Next: Commands Grouped by Up: Command Summary Previous: tsa . BRANCH var comparisons labels . ... define cross reference labels for the 8 parameters . DEFINE/LOCAL key_def data A lower_levels_flag . define the maximum no. of parameters for a procedure . DEFINE/PARAMETER Pi default type/option prompt_str low_lim,hi_lim . define default, type and valid interval for parameter i . ... GOTO label . branch to command line containing label: . IF par1 op par2 command_string . ...

... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

WCSLIB љ 5.15 . ... cel.h File Reference . ... Go to the source code of this file. struct љ . ... CELLEN љљљ(sizeof(struct celprm )/sizeof(int)) . ... celx2s (struct celprm *cel, int nx, int ny, int sxy, int sll, const double x[], const double y[], double phi[], double theta[], double lng[], double lat[], int stat[]) . ... cels2x (struct celprm *cel, int nlng, int nlat, int sll, int sxy, const double lng[], const double lat[], double phi[], double theta[], double x[], double y[], int stat[]) . ...

... tested on SUN and VAX; updated prolog ; ;- ;************************************************************************* pro pcheck, variable , position , dimension , type ; npar = n_params(0) if npar eq 0 then begin print,'PCHECK, VARIABLE , POSITION , DIMENSION , TYPE ' retall endif ; npar ; ; decode valid dimensions ; vdim = bytarr(3) idim = ...

OLAS . vcsolac : automatic environment . ... Random test (FITS file >35 MB, >64 MB, >128 MB, ) . ... Error Handling (corrupted image but valid FITS header, corrupted FITS header, no FITS format, r/w protection on FITS files, rcp failed during transmission of bulk-msg, SIGTERM handling, . ... dhs <--> frameIngest ( A fits file is sent to vcsolac, which does not contain any ESO parameters; tc files are sent to vcsolac; Testing watchdog frameIngest; dhs and frameIngest using same environment; ...) . ...

APIRET rc = Dos32Profile ( ULONG func, PID pid , PRFCMD *profcmd, PRFRET *profret); 0 NO ERROR ok 8 NOT_ENOUGH_MEMORY couldn't allocate profile structures 87 INVALID_PARAMETER some parameter not ok 111 BUFFER _OVERFLOW not enough size in return buffer 115 PROTECTION_VIOLATION invalid return buffer data 126 MOD_NOT_FOUND requested module data not available 303 INVALID_PROCID parameter 2 is not a valid PID 328 SYS_INTERNAL ... pid of process to be profiled 0 if kernel profiling . ...

Cross-sections, albedo, asymmetry factor for homogeneous spheres . ... The dependence on the size parameter x for different refractive indices m=n+k i . ... Q abs (x) . albedo (x) . ... Parameters: n = 1.3; k = 0, 0.01, 0.03, 0.1, 0.3; x = 0--20. ... Notes: Q abs =0, albedo=1, when k=0. ... The dependence on the size parameter rho for different refractive indices m=n+k i . Q ext (rho) . ... Q abs (rho) . albedo (rho) . g (rho) . ... Parameters: n = 1.3, 1.5, 1.7; k = 0; rho = 0--12. ...

Table 4.1: Solar System Standard Targets . Table 4.2: Target Description Keywords . Table 4.3: Positional Parameters for TYPE = COMET . ... Observers for solar system Targets of Opportunity (e.g. a "new" comet or asteroid, a solar-wind disturbance reaching the Jovian magnetosphere, etc.), should complete the Generic Target List ( See 3.12 Generic Targets List [Generic_Targets] ) and the Visit and Exposure Specifications (to the extent possible) in time for the Phase II deadline. ...

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

... Space flight . ... Zero Gravity . ... Characteristics of a Complex Flight: . ... Characteristics of the Reduced Gravity (Lunar Gravitation): . ... Characteristics of the Reduced Gravity (Martian Gravitation): . ... Services / Zero Gravity: General description Technical description Flight parameters Photo gallery Price . ...

... Prev . Next . comedi_command_test -- test streaming input/output configuration . ... int comedi_command_test (comedi_t * device, comedi_cmd * command); . The function comedi_command_test() tests the command structure pointed to by the parameter command and returns an integer describing the testing stages that were sucessfully passed. In addition, if elements of the command structure are invalid, they may be modified. Source elements are modified to remove invalid source triggers. ...

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

Hide Zen home . ... Parameters: table and index descriptors . ... Parameters: index descriptor, value, pointer to table record . ... Also rebuilds internal keys if needed (index is locked when rebuilding). ... These are base methods for search in index - create scan, finish scan, repeat scan. ... Restore one WAL record. Parameters: LSN (LogSequenceNumber), WAL record . ... GiST has no direct access to tables, only via pointers ( the number of page and the number of record on the page) to records. ...

Stellarium 0.12.3 . ... StelGeometryBuilder Class Reference . ... buildCircle ( StelVertexBuffer < VertexP2 > *vertexBuffer, const float x, const float y, const float radius, const int segments=128) . ... buildCylinder ( StelVertexBuffer < VertexP3T2 > *const vertexBuffer, const float radius, const float height, const int slices, const bool orientInside=false) . ... Build a fisheye-textured sphere. ... Build a flat texture mapped ring with 3D coordinates (for example for planet's rings) More.. ...

... Directives | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Programs . ... httpd is the Apache HyperText Transfer Protocol (HTTP) server program. ... Process the configuration directive before reading config files. -c directive . Process the configuration directive after reading config files. ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

... Matrix of Transformation | ... Every set of attitude coefficients (corresponding to a line in attitude data file) is valid for its own time interval and gives the possibility to get a matrix N of tranformation from the GSE coordinate system to the S/C coordinate system as well as a matrix M of tranformation from the S/C coordinate system to the GSE coordinate system. ... and the matrix M of transformation from the S/C to the GSE systems (the direction cosines matrix) is: . ... V GSE = M * V S/C . ...

... 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 . ...

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...