... YFIT=A(0)+A(1)*X+A(2)*X^2+.. ... Apr 21, 1988 RWT GSFC use new DETERM_PDP ; Aug 29, 1989 RWT modify for SUN IDL ; Jun 21 1991 GRA CASA cleaned up; tested on SUN, DEC, VAX; ; updated prolog; ; 11 May 94 PJL print a warning if any of the weights are negative ; ;- ;****************************************************************************** pro wpolyfit ,xin,yin, weight , ndeg ,a, yfit , chisqr ; npar = n_params(0) if (npar eq 0) then begin print,' WPOLYFIT ,XIN,YIN, WEIGHT , ...

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• http://www.naic.edu/~tghosh/software/parcheck.pro
• HISA Poster for the 197th Meeting of the AAS, January, 2001
• HISA Poster for the 195th Meeting of the AAS, January, 2000

... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

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Program: CORMAP Purpose: Check whether there is a correlation between two maps Category: ANALYSIS, CALCULATION File: cormap.c Author: M. Vogelaar Keywords: INSET= Give set, subsets: Maximum number of subsets is 2048. BOX= Give box: [entire subset] RANGE= Give range of levels to include in calculation: [all] Input consists of two values. The first value may be greater than the second. See the description for the correct use of this keyword. ... PGCOLOR= Give color 1.. ...

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• http://www.atnf.csiro.au/computing/software/gipsy/tsk/histog.dc1
• http://www.atnf.csiro.au/computing/software/gipsy/tsk/trace.dc1
• Keyin Free-format Input

Next: *period* - Period search Up: *fft* - Period search Previous: A summed or incoherent . The distribution of coefficient values for a single FFT is exponential if the original data contain no periodic signal. ... Significant coefficients will appear beyond the high-value end of the normal distributions. ... xt> fft.histogram_bi=0.5 # if necessary, adjust number for an aesthetic plot xt> ftpplot input table file: rp90_ftp The plot will appear on the screen. ...

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• Mapping Pixel Values to Screen Intensity
• SAOtng Memory Considerations
• Model Spectra for Spectral-Fitting Program

... Calculations of at least two runs with different values of a parameter are required in order to discover to what extent the results depend on the , if at all. ... In order to study how the final statistical distributions depend on the initial functions, the method of Green functions is used. ... Then we can restore any distribution on this parameter (with a certain accuracy) by summing the results for each interval with the appropriate weight. ...

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• Test of the Initial Mass-Ratio Distribution
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• Notes on Monte-Carlo Simulations

... A Bayesian value for may be found simply by treating it as another parameter in our hypothesis space. ... where in the last factor we can drop the conditioning on since it is alone that induces the data . ... Evaluating the appropriate Gaussian integral gives . ... Nevertheless, for realistically large data sets, the distribution is so strongly peaked that it overwhelms any reasonable prior on , and so we assign the Bayesian value of the regularisation constant to be that which maximises . ...

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• OptInt PmWiki : PmWiki / Page File Format

... Routines for accessing I/O ports are in /usr/include/asm/io.h (or linux/include/asm-i386/io.h in the kernel source distribution). ... Before you access any ports, you must give your program permission to do so. This is done by calling the ioperm() function (declared in unistd.h , and defined in the kernel) somewhere near the start of your program (before any I/O port accesses). ... For example, ioperm(0x300, 5, 1) would give access to ports 0x300 through 0x304 (a total of 5 ports). ...

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• Writing programs that use comedi and comedilib
• Determination of atmospheric parameters and calculation of chemical composition
• LWN: Driver porting: dealing with interrupts

... The keywords EXPRTIME and ZEROMAGN set the zero point for magnitudes. ... The program automatically determines a Point Spread Function when it gets proper initial values from the keywords SPROFIL. Initial values may be wrong by 0.1 each, and the program still can converge to the right Point Spread Function. ... The program looks for an initial point spread function into that descriptor at first and it uses data from the keywords SPROFILx when the descriptor DPROFILE is absent. ...

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• Noise distributions
• In Case of Trouble
• Password Formats - Apache HTTP Server

ChangeLog for htrframes =============================== Version 1.2.1 - 2004-03-15 (CG) ------------- - DISTRIBUTION set to SOC, since package should remain internal Version 1.2 - 2002-05-24 ( JDR ) ----------- - uses OAL to convert time values to MET Version 1.1 - 2002-05-08 ( JDR ) ----------- - requires new-format ODF, hence the major ...

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• http://xmm.vilspa.esa.es/sas/6.1.0/doc/htrframes/ChangeLog
• Null-hypothesis probability distribution for a weighted sum of Poissonian
• Description

... Abstract Return the character value of a kernel variable from the kernel pool. ... Brief_I/O VARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- name I Name of the variable whose value is to be returned. start I Which component to start retrieving for name room I The largest number of values to return. lenout I The length of the output string. n O Number of values returned for name. cvals O Values associated with name. found O True if variable is in pool. ...

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• WFC3 Instrument Handbook
• CSPICE Routines: GDPOOL_C
• Create a Program Using the JWST Mosaic Tool in APT

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• ESO - Negative pixel values in the 2D spectrum image are not being ignored by
• ESO - How do I interpret the SEQ TIME keyword values?
• Working with

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

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• AstroAsciiData
• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)

A completely new possibility of Fortran 90 is recursion. Note that it requires that you give a new property RESULT for the output variable in the function declaration. ... Here follows two examples, first recursive calculation of the factorial, then recursive calculations of the Fibonacci-numbers. ... The listings of the routines follow, the output variables are called FAC_RESULT and FIBO_RESULT , respectively. ... Not only functions but also subroutines can be recursive. ...

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• Tutorial on Fortran 90, Digital UNIX
• Keyword arguments and default arguments
• Argument association

.

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DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• Format Documentation of *.wdc Files
• Format Documentation of kpyymm.tab Files
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

... Apache HTTP Server Version 2.4 . ... Notes about the password encryption formats generated and understood by Apache. ... MD5 . apr1$" + the result of an Apache-specific algorithm using an iterated (1,000 times) MD5 digest of various combinations of a random 32-bit salt and the password. ... Insecure. $ htpasswd -nbB myName myPassword . ... Since the MD5 function is commonly available, other software can populate a database with encrypted passwords that are usable by Apache digest authentication. ...

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• Clumpy dust disks
• Color Values
• CHIANTI atomic database

... Accurate identification of physical binary star systems has become of increasing interest in recent years. ... Identification of physical binary star systems, with an estimated reliability of such identifications based on the theory of probability, is also important for current and future efforts to find binary star systems that are candidates for observations with the aim of determining their orbits and component masses. ... probability of the proximity of proper motions and ; . ...

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• Using Massively Parallel Processing of a NLTE Spectrum Synthetic Code and an
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• A Method for Visualizing Time Variability in X-Ray Images

... Reference ID: CHU . Driver ID: CHU . Serial Port: /dev/chu u ; 300 baud, 8-bits, no parity . ... Unlike the NIST time services, whose timecode requires quite specialized hardware to interpret, the CHU timecode can be received directly via a serial port after demodulation. ... The time1 fudge option can be used to set the CHU propagation delay, compensate for inherent latencies in the serial port hardware and operating system. ... Not used by this driver. stratum number . ...

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• The Network Time Protocol (NTP) Distribution
• Creating a watermark effect
• HSV is Groo-V!

... FIELD | ... METHOD . ... static int . ... Set this flag to have the ImageProcessor that is passed to the run() method converted to a FloatProcessor. static int . ... Set this flag if the filter wants its run() method to be called for all the slices in a stack. static int . ... Set this flag if the filter does not want its run method called. static int . ... Set this flag if the setup method of the filter should be called again after the calls to the run(ip) have finished. static int . ...

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• Interpreter (ImageJ API)
• RankFilters (ImageJ API)
• EDM (ImageJ API)

... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...

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