... Keyword TIMEDEL missing in Input File . error . The TIMEDEL keyword is missing in the timeseries FITS file, which is necessary to determine the binning factor of the data . ... Hence it is impossible to carry out the variability test. corrective action: Use a different input file . ... The keyword is missing in the input timeseries FITS file which could indicate that there is a problem with the input timeseries FITS file. corrective action: Verify that this is a valid fits file . ...

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... 06aug11:tx sample voltages are displayed for the 1st ipp of the file (.ps) ( .pdf ): . ... Rdev setup for sine wave. 10 millisecond ipp fed into rdev from sps. sine wave= 30MHz+ 11160 hz, amp=14dbm. took 4 files of data (about 60 seconds/file). ... Page 2: Measure phase differences (Data[0] -Tx[0]) for 6000 ipps . ... The measured phase (tx to data) is off by about .5 usecs from the expected time difference. 2nd: phTxSmp[0,ipp+1]-phTxSmp[0,ipp]: The change in tx sample 0 from 1 ipp to the next. ...

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• pntErrVsPlatformMotion
• lbwgain curves nov03
• rotaPlatToSky

... User Guide ] Task: imrm Purpose: Compute rotation measure image from position angle images Categories: image analysis IMRM computes rotation measure and zero wavelength position angle images from at least 2 position angle images at different frequencies. ... Key: in Up to 5 input position angle (positive N -> E) images (in degrees) at different frequencies. ... Default is 0. ... The default is no output RM images. ... This is also true if you give IMRM position angle images at two frequencies only. ...

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• User interface
• impol
• Polarimetric Analysis Tasks

Next Previous Contents . This means that an interrupt happened that no driver expected. ... In many cases you can safely ignore this error message, especially if it only happens once or twice at boot-time. For boot-time messages, look at the messages which are nearby for a clue as to what is going on. For example, if probing is going on, perhaps a probe for a physical device caused that device to issue an interrupt that the driver didn't expect. ...

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• Stream 1/0

... The fitting package in STSDAS (Space Telescope Science Data Analysis System) relies on two basic techniques (one linear and one non-linear) for fitting functions to data. ... Results show that both methods may generate biased coefficients (at the ~few percent level), and over or under-estimate error bars (at the ~10 percent level), in particular from low signal-to-noise data. ... Function coefficient errors are computed directly from the covariance matrix. ... Abscissa is signal-to-noise. ...

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• A Method for Minimizing Background Offset Errors When Creating Mosaics
• ADASS 2002 Conference Proceedings
• Kalman Filtering in Chandra Aspect Determination

The Steady State model of the Universe was proposed in 1948 by Bondi and Gold and by Hoyle. ... At the time the Steady State model was proposed, the Big Bang model was in trouble because the value of the Hubble constant was clearly bigger than the inverse of the age of the Universe. ... Thus the Steady State model has flat spatial sections like the critical density Big Bang model. ... The Steady State model has no adjustable parameters to correct for this error, but the Big Bang does. ...

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• Outputs
• Spectra of Kallas Riech (1980) sources
• THE TEXAS SURVEY: THE PRELIMINARY

... A full set of flatfield frames was taken with the NICMOS arrays during the System Level Thermal Vacuum test, conducted on the ground in August 1996. ... Users are encouraged to recalibrate their data with on-orbit flatfields if the pipeline calibration used thermal vacuum flatfields. Preliminary results from SMOV indicate that variations in the large scale structure of the on-orbit flatfields relative to the thermal vacuum flatfields are of the order of 1-2% in Camera 2, and up to 5% in Camera 1. ...

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• CSPICE Routines: REPMCT_C
• Figure of Merit
• CSPICE Routines: ERRDEV_C

... IPACMAN V2.5 Test Plan (or more) . ... Anyway, results given hereafter are related to one plaform only (the one mentioned on the top). ... specific testcases The following testcases correspond to the minimum set of tests to be run on every new IPACMAN release (alpha, beta, final, .. ... 1/ START IPACMAN . ... Expected result . ... Verify IP: select an IP on disk and run Reports>verify IP . ... IP Diff: select two IPs on disk, and run Reports>IP Diff and check manually the results: verify the . ...

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• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• ESO - Phase 3 Release Validator
• HSTPOLIMA (V2.00) --- February00 --- HSTPOLIMA (V2.00)

... Posts tagged ?systematic error? ... Thanks to L. Lyons? work discussed in [ArXiv] Particle Physics , I found this paper, titled Systematic Errors describing the concept and statistical inference related to systematic errors in the field of particle physics. ... Continue reading ?systematic errors? Tags: coverage , Heinrich , likelihood , Lyons , nuisance parameter , objective priors , p-value , particle physics , statistical error , subjective priors , systematic error . ... Comment . ...

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• The AstroStat Slog measurement error
• The AstroStat Slog Blog Archive different views
• Multi-Rsh parallelized rsh program

... 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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• APOD: December 30, 1998 - Supernova 1994D and the Unexpected Universe
• APOD: 2000 March 12 - Supernova 1994D and the Unexpected Universe
• mod_dumpio - Apache HTTP Server

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2015 May 31 . Supernova 1994D and the Unexpected Universe . Image Credit: High-Z Supernova Search Team , HST , NASA . Explanation: Long ago, far away, a star exploded. ... Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... About APOD | ...

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• APOD: 2004 January 20 - Unexpected Galaxy String in the Early Universe
• APOD: 2009 September 8 - Unexpected Impact on Jupiter
• APOD: 2008 January 1 - Rays from an Unexpected Aurora

... Bojan Nikolic web pages home . ... For some numerical experiments with CASA , I have recently been recompiling some parts of this package. ... That is before even touching the code! ... I used the SCons build system to build the CASACORE libraries. ... Apparently missing include for strlen: --- a/code/display/Display/Options.cc +++ b/code/display/Display/Options.cc @@ -30,6 +30,7 @@ #include <sys/stat.h> #include <iostream> #include <dirent.h> +#include <string.h> namespace casa { namespace viewer {...

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• How de-focusing makes wavefront errors more apparent Bojan Nikolic web pages
• Limits on Phase Correction Performance Due to Differences Between Astronomical

Astronomy Picture of the Day . ... 31.05.2015 . ... Credit Copyright: High-Z Supernova Search Team , HST , NASA Explanation: Long ago, far away, a star exploded. Supernova 1994D , visible as the bright spot on the lower left, occurred in the outskirts of disk galaxy NGC 4526 . Supernova 1994D was not of interest for how different it was, but rather for how similar it was to other supernovae . ... Publications with keywords: supernova - cosmology . ... A Supernova through Galaxy Dust . ...

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• Астронет > Supernova 1994D and the Unexpected Universe
• Unexpected Galaxy String in the Early Universe

... It can be a good idea to periodically check for bad blocks. ... It outputs a list of the numbers of all bad blocks it can find. ... The following example will show how this could be done. $ badblocks /dev/fd0H1440 1440 > bad-blocks . fsck -t ext2 -l bad-blocks /dev/fd0H1440 . ... Pass 1: Checking inodes, blocks, and sizes . ... Pass 5: Checking group summary information. /dev/fd0H1440: ***** FILE SYSTEM WAS MODIFIED ***** . dev/fd0H1440: 11/360 files, 63/1440 blocks . ...

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• Observations and Data Reduction
• Influence of Climate Variables on Tree-Ring Widths of Different Species
• Leonids 2006

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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... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . ... ISS 45/46 . ... The crew training without the actual science hardware before the first session of operation with this science hardware (for which there is a virtual manual) with a log file generated; . ... HISTORY . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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• S.P.Korolev RSC Energia - ECOLOGICAL MONITORING

... hstpolima: Reduce linear polarization data for HST instruments (currently FOC, NICMOS and WFPC2 are supported). ... Images for the three Stokes parameters (I,Q and U), the linear polarization and position angle and their error images are output. hstpolpoints: Reduce linear polarization data for HST instruments for a set of circular apertures. ... There is a web page http://www.stecf.org/software/impol/ briefly describing the package and giving example polarization maps for HST and model data. ...

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• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)

To print commands and their arguments as they are executed: cat example #!/bin/sh TEST1=result1 TEST2=result2 if [ $TEST1 = "result2" ] then echo $TEST1 fi if [ $TEST1 = "result1" ] then echo $TEST1 fi if [ $test3 = "whosit" ] then echo fail here cos it's wrong fi . This is a script called example which has an error in it; the variable $test3 is not set so the 3rd and last test [ command will fail. Running the script produces: example result1 [: argument expected . ...

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• Did You Know?
• Index of manual pages: E
• Example of using an if construct

... Appendix: Effect of errors in the encoder roller and drive disk on tracking. ... Servo error. ... Table 1: Tracking error budget Component Component error (nm RMS ) Effect (mas RMS ) Az axis wobble Drive disk high freq. error 200 17.17 Guide roller error 50 8.58 Lower bearing high freq./nonrep. error 50 4.29 Alt axis wobble Bearing high freq./nonrep. error 50 4.86 Az encoding error Drive disk high freq error 200 4.59 Encoder capstan error 50 5.73 Encoder ...

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• Tracking error budget
• Mirror Controller Version History
• Fiber-optic plug rotation

For a sample of 16 people, the error would be 4/16 = 25%. This a large error since the range of YES vs NO is from 0-100% if 12 people answered yes and 4 people answered no then your result would be: . Percentage yes = 75 +/- 25% . ... For a sample fo 1000 people, the error would be SQRT(1000)/1000 = 33/1000 = 3%. If 750 answered yes and 250 answered no then your result would be: . ... Conclusion: Always ask what the measuring errors are!! Previous Lecture Next Lecture Course Page ...

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