... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... filename list . ... float . ... emldetect: detection likelihood threshold . ... boolean . ... Name of eboxdetect local mode source list . ... Name of eboxdetect map mode source list . ... eboxdetect: detection mask flag . ... false . esplinemap: flag for output of cheesed image . ... emldetect: source list . ... emldetect: source cut-out radius for multiple source fits . ...

... Category: MATH File: lsqfitd.c Author: K.G. Begeman Use: INTEGER LSQFITD( XDAT , Input DOUBLE PRECISION ARRAY XDIM , Input INTEGER YDAT , Input DOUBLE PRECISION ARRAY WDAT , Input DOUBLE PRECISION ARRAY NDAT , Input INTEGER FPAR , In/Output DOUBLE PRECISION ARRAY EPAR , Output DOUBLE PRECISION ARRAY MPAR , Input INTEGER ... NPAR Number of parameters. ... FUNCD = FPAR(1) + FPAR(2) * XDAT RETURN END SUBROUTINE DERVD( XDAT, FPAR, DPAR, NPAR, FOPT ) ....

... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...

... HST Phase II Proposal Instructions for Cycle 20 > Chapter 12: Cosmic OriginsSpectrograph (COS) > REFERENCE INFORMATION > 12.16 WAVECAL Exposure Parameters . ... Table 12.5 lists the exposure times and current settings for the wavelength calibration lamp exposures as a function of spectral element and central wavelength 1 . Table 12.5: WAVECAL Exposure Parameters . ... Exposure Time (seconds) . ... MEDIUM . ... 180 . ... 120 . ... 240 . ... 140 . ... 300 . ... 160 . ...

. This quantity is the physical maximum velocity rotation corrected for inclination, expressed in km/s. It is deduced from the parameter vmaxg after correcting for inclination using incl . This rotation velocity is calculated from both the 21-cm line widths at different levels and/or the available rotation curves (generally H_alpha rotation curves). The rotation of the stellar component is given in the parameter vmaxs . HyperLeda . Questions: prugniel@obs.univ-lyon1.fr

Next: System configuration Up: How to use CONSTRICTOR Previous: Preparation of parameter file Contents . ... DayNumber: Even though this number is in the data, some packet headers have the wrong number and it makes it a whole lot easier to have the user check and enter this number correctly. ... CONSTRICTOR will add a multiple of 24 hours to the time tag when the day number changes. Remember to set the StopTime to, say, 48 hours if you use a DayNumber of one less than the actual day number. ...

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

. Next: Editing Files and Parameters Up: Using IRAF Previous: Editing Text . To display ascii files, use the IRAF command `page' cl> page filename Type ``q'' to exit `page'. Task parameters can be listed with `lparam' cl> lparam qpcopy Table files are displayed using tprint ta> tprint rp90_prd.tab With UNIX-like pipes, these can be used in conjunction with hardcopy print commands like lprint: ta> tprint rp90_prd.tab | lprint . rsdc@cfa.harvard.edu . 1998-06-10

... 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. ...

System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

seeing -- Create a simulated ground-based star image based on a model of atmospheric turbulence seeing output xdim ydim gamma fwhmx fwhmy . output = "" [image] . The name for the output image to be created. xdim = 512 [integer] . The X dimension for the output image. ydim = 512 [integer] . The Y dimension dor the output image. gamma = 1.6666 [real] . ... For a discussion of the significance of this please see the discussion below and the references given. fwhmx = 5.0 [real] . ...

... 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 . ...

... from self-study guide 2 program exercise2 use nag_f77_c_chapter implicit none integer, parameter :: dp = selected_real_kind(12) integer, parameter :: length = 128 real(dp) :: a, ainv real(dp) :: x(length), y(length) ! ... Initialise x and y call init_arrays(ainv, x, y) ! Fourier transform x and y call fourier(x, y) ! ... Call NAG FFT routine ifail = 0 call C06ECF(x, y, n, ifail) if (ifail /= 0) then write(*,*) 'Error in C06ECF: ifail = ',ifail stop end if end subroutine fourier ! ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

... 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 = ...

... 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 . ...

... RC0302+0455 . RC0308+0454 . ... RC0355+0449 . Radio source parameters . ... R.A.(B1950) Dec.( B1950) Freq. ... Parameters of optical candidates for identification . R.A.(J2000) Dec.( J2000) R.A.(B1950) Dec.( B1950) Magn. ... J2000) angle fwhm (X:Y) 03:08:33.98 +04:54:10.5 . ...

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

... Focal reducer main parameters . Focal ratio at the 6m telescope . ... DQE (telescope+SCORPIO+CCD) . 80% in Direct Image mode . 30% in Long Slit mode . 20% in Fabry-Perot mode . Limit magnitude for images . R=26.8 (S/N=5 for Texp=1800 sec, seeing 1.5'') . Limit magnitude for low-resol. spectra . R=24.0 (S/N=10 in continuum, Texp=7200 sec) . ... Size, pixels . ... Pixel size, mkm . ... 83% Plot of the DQE . ...