... Meta Index / Home Page This section documents warnings and errors generated by this task (if any). ... error . ... No variance image was supplied, so the task has tried to use the inset as its own variance image. ... The user has set smoothstyle =`adaptive' and withuserwidths =`yes', but hasn't supplied any convolvers in userwidths . ... The user probably ought to check the output to make sure that it looks ok. corrective action: Such pixels are set to zero. negativeValuesInVarianceOutput . ...

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... Abstract Fetch from the kernel pool the double precision values of an item associated with a body. ... It's an error to supply an output array that is too small to hold all of the values associated with the requested kernel variable. Detailed_Output dim is the number of values returned; this is always the number of values associated with the requested kernel variable unless an error has been signaled. values is the array of values associated with the requested kernel variable. ...

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• CSPICE Routines: BODVCD_C
• CSPICE Routines: GDPOOL_C
• CSPICE Routines: EKUCEC_C

Starting generation of Calibration File FS version = 0009.0004.0017 time_zero = 3171600 Rack type is MK3/4 Found #103 errors of type = ERROR qk -211 Tsys value for device ve overflowed or were less than zero. Found #73 errors of type = ERROR qg -303 Track 21 parity errors exceed threshold. ... Found #34 errors of type = ERROR ch -336 Enabled tracks do not check with requested tracks Found #30 errors of type = ERROR qg -304 Track 19 sync errors exceed threshold. ...

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• Error Handling
• Task Parameters
• Tools - Mathematical functions

The examples of the errors. ... Observations with ordinary values of the "Mean error of single observation" Obj Code DT RA (O-C) DEC (O-C) mag z h m s " ° ' " " ° 3907 761 1998 08 24.383673 3 17 44.739 0.28 +30 46 00.84 -0.08 15.8 18 3907 761 1998 08 24.409133 3 17 46.152 0.28 +30 46 10.85 0.12 15.8 11 3907 761 1998 08 25.392523 3 18 40.107 0.33 +30 52 27.69 0.04 15.4 15 Total mean value of 3 observations 0.297?0.017 0.027?0.058 Mean error of single observation 0.029 0.101 COMMENT. ...

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• Pulkovo NEO Page: Estimation of Accuracy of the Observations

... The ruze formula gives the fractional gain caused by errors in the surface: fracgain=exp(-(4*pi*delta/lambda)^2) ... delta=rms surface error,lambda=wavelength The fractional gain is gainMeasured/gainExpected . ... The gains we measured include losses from pointing errors, pitch/roll/focus (prf) errors, and errors from the surface. ... Figure 7 shows the fractional gain from the pitch/roll/focus errors. Figure 8 shows the measured gain corrected for the pitch/roll/focus errors. ... Figure 11. ...

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• http://www.naic.edu/~phil/pnt/pntchk_nov06.html
• http://www.naic.edu/~phil/callbn/calvaljan02/lbncalvaluejan02.html
• measured_operating_values

SUBROUTINE TAP_ERMES ( TEXT, TEXLEN, STATUS ) . Return an error message associated with a TAP status value. SUBROUTINE TAP_ERROR ( TAP_ROUTN, NAME, TEXT, STATUS ) . Report an error message. ... Report an error message associated with a TAP status value. ... Purpose: return an error message associated with a TAP status value. ... TEXT = CHARACTER * ( * ) (Given) TAP error message text. ... Invocation: CALL TAP_REP( NAME, TEXT, STATUS ) Description: An error message is built in the form: !! ...

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• Simon Jeffery's Software Store: TAP global constants
• Armagh Observatory

Next: Reduction procedure Up: Extinction and transformation Previous: Strategy . Standard stars can be included in the extinction solution, if one is careful. The problem is that there are usually appreciable ``conformity errors'' due to mismatch between the instrumental and the standard passbands [ 16 ]. ... Thus, it is wrong to assume that the transformation between the instrumental system and the standard system is exact, even if there were no measurement error in either system [ 1 ]. ...

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• Application Commands
• Values, Variables, and Literals
• Nonlinearity

... Астронет | ... планета Астронет | ... Астрономия в России | ... История астрономии . ... Любительская астрономия . ... Кривая блеска GRB 030329 . ... Includes most data through GCN 2276 . Light curve of posted GCN observations of GRB030329, including AAVSO observations, by Melissa Nysewander (UNC-Chapel Hill) . ... Публикации с ключевыми словами: гамма-всплески - оптические ореолы гамма-всплесков . ... Самый далекий, самый желанный . GRB 090423: самый далекий взрыв . ...

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parameter estimates and variances Bayesian Gaussian Aperture Photometry -- updated notes Ї Model Selection Model Selection Ї Ї Ї Ї Ї p-values and Hypothesis Tests Type I, Type II, and other errors Analysis Design Upper Limits Hypothesis Tests , Likelihood Ratio Tests , and posterior predictive pvalues Odds ratios, Bayes Factors AIC/BIC/DIC/WAIC/HQIC/MDL Ї Ї p-values Ї Ї p=Pr(T T(D)|H) What ... The difference between significant and not significant is not significant." ...

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• The AstroStat Slog p-value
• The AstroStat Slog systematic error
• Mapping Pixel Values to Screen Intensity

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

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• Keywords_289

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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• API Help
• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)
• Auxilliary data

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

... Make up at least 5 data points, each with an x value, a y value and an uncertainty in the y value. ... Right-click on the top of the column containing the x-data and drag your mouse to the bottom of the column to select it. ... You must first enter the Positive Error Value (the `up error bars') ґ click at top of the column of y error values and drag down to select all of the values (in the above screenshot the y error values are in the column labeled ). ... Let's try fitting a straight line. ...

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• http://www.mso.anu.edu.au/~akarakas/Teaching/readme

... Apache HTTP Server Version 2.4 . ... Although the Apache HTTP Server provides generic error responses in the event of 4xx or 5xx HTTP status codes, these responses are rather stark, uninformative, and can be intimidating to site users. ... Additionally, a set of values are provided, so that the error document can be customized further based on the values of these variables, using Server Side Includes . ... Customizing Error Responses . ... ErrorDocument 500 http://error.example.com/server_error.html...

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• Color Values
• Displaying Errors with the JavaScript Console
• CHIANTI atomic database

First, we'll set up values for Mail :: Bulkmail # #################### define package Mail :: Bulkmail # server _class stores the server object that we're going to use. #uncomment the DummyServer line and comment out the Server line for debugging server _class = Mail :: Bulkmail :: Server # server _class = Mail :: Bulkmail :: DummyServer #log our errors ERRFILE = / Mail::Bulkmail might as well use it. ...

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• http://hea.iki.rssi.ru/conf/hea2007/scripts/gen_validatorv2.js~
• INTEGRAL 9-year Galactic Survey

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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• Processing the "Face on Mars" Images
• Identities
• ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM

... Here is an example of the output header of CATS data. ... SIMPLE=T / BITPIX=8 / character information NAXIS=0 / no image data array present EXTEND=T / may be standard extensions OBJECT= CATS SEARCH / CATS search result ORIGIN=SAO RAS DATE=01/01/1997 / date of file creation END XTENSION=TABLE / F-file table extension BITPIX=8 / 8-bits ... NAXIS1=93 / No. of characters per row NAXIS2=1000 / the number of lines (sources) TFIELDS=10 / there are 16 fields per row EXTNAME= CATS / object name: ...

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• comedi_loglevel
• Mathematics: <math.h>
• exit()

Sloan Digital Sky Survey Telescope Technical Note 19970527 Walter Siegmund . ... Pointing Error Budget . ... The interleaved strips and adjacent stripes overlap about 1 arc minute. ... However, a 2-D pointing accuracy of 3 arc seconds RMS leads to acceptibly uniform overlap and minimises the number of cases that require special handling (Table 3). ... A guide fiber bundle diameter of 16.5 arc seconds and a pointing accuracy of 3 arc sec RMS results in 99% initial success in acquiring guide stars. ...

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• mirror
• TUI:TUI Menu:Preferences Window
• TUI:Telescope:Slew Window:Options:Calibrate

... B data of V 616 Mon (A 0620-00) # in UBV system - calculated by Shugarov from photgraphic values, # observed in Krimea # Ref : Переменные звезды 20, 251-254 , 1976 # Ref : Peremennye zvezdy 20, 251-254 , 1976 # Ref : Variable Stars 20, 251-254 , 1976 # translated to LF by G.V.Lipunova # LF = log flux flux = erg/cm^2/sec # 1=day, JD; 2=B; 3=error(1 sigma); 4=B,LF; 5=B-error,LF # 1 2 3 4 5 #2421614.225 12.39* 0.1 2442661.576 11.58 ...

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Download Izmccd (~2.7 MB). ... for 1-5 bytes is number of a numbered minor planet, . ... Positions 1-80 file "mpcreportiz.txt" are similar to positions of file "mpcreport.txt". 83-95 ? errors of unit weight, . ... If this tag is " 1 0 " , this record contains results of measurements of an image of object (approximation by "PSF"),? . ... 57-66 ? error in X (pixels), for first star in a multicentric image, for subsequent it is error in (distance between first star in the image and this), . ...

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