The accurange 3000 distomat was borrowed to evaluate it as a replacement for our current distomats. ... accurange 3000 users manual (.pdf) . ... 28apr11: distance measurements for different sample averages . ... On 28apr11 distance measurements were made with the accurange 3000 distomat. ... Page 1: accurange 3000 distance vs time for 4 sample averages. ... Page 5: accurange 3000 temperate during measurements. the temperature measured for each measurent is plotted. there is no obvious dependencies. ...

... CentralProcessor 0.11 documentation . ... The mssplit utility is used to extract a subset of a measurement set. ... It also has the ability to average channels together while doing so. ... Average a full spectral resolution measurement set down to fewer/wider channels for continuum imaging. ... Any rows with time earlier than this parameter will be excluded during splitting (i.e. they will not be copied to the output measurement set. ... mssplit (Measurement Splitting/Averaging Utility) . ...

... angle (degrees) . inches . ... average . ... range . ... specification . ... tolerance . ... 2ry baffle tip thickness . ... 2ry baffle tip overhang . ...

Uncertainties are a bit different in counting experiments - this lesson explains how. It also covers averaging and how that affects uncertainties. Back Main Uncertainties Page .

Next: Results of follow-up spectroscopy Up: Data reduction Previous: Reduction of the Calar . In the final spectra, redshifts and line fluxes are measured within MIDAS, applying Gaussian fitting to the emission lines. To determine redshifts for individual galaxies, averages are taken over the prominent individual emission lines (mostly H , H , [O III ] 4959,5007 ?) The line [O II ] 3727 ? ... For all spectra, the individual emission line fluxes of the H , [N II ] 6548,6583 ? ...

O.R. Hainaut, ESO, H. Boehnhardt, MPS, and S. Protopapa, UMd . ... MBOSS colour database : colour, absolute magnitude, spectral gradient, dynamical class for each object. mbossData (ASCII) . ... 1998WW31+B, +C refer to the satellites; Warning: measurements reported for the main body (eg 1998WW31) are likely to include measurements of the object together with its satellite(s). ... See the MBOSS-2 paper for details. ... x is the weighted average of all the available measurements, obtained as . ...

Mo deling GRB (and other) p opulations: Some lessons from multilevel mo deling Tom Loredo and Ira Wasserman, Cornell U. Goal: Infer properties of a population from measurements of observables with measurement error and selection effects Multilevel models: · · · Upper level : Draw observables from (adjusted) pop'n dist'n Lower level : Draw measurements from independent data distributions Bayes: ...

Instrument Science Report ACS 02-03 RELATIVE GAIN VALUES AMONG THE FOUR WFC AMPLIFIERS R. C. Bohlin, G. Hartig, & Wm. ... Our method relies on the average absolute gain measurements of the four amplifiers but provides a more accurate determination of their relative gains. 1.INTRODUCTION The absolute gain values for the four ACS WFC amplifiers (A, B, C, & D) have been measured by Martel, Hartig, & Sirianni (2001, MHS) with a typical accuracy of 0.6%. ...

... Armagh Observatory reports that April 2014 was the third warmest April on record at Armagh, that is, since daily temperature measurements at Armagh Observatory began around 1795. ... The mean monthly temperature was 10.5 degrees Celsius, approximately 2 degrees Celsius warmer than the most recent (1981тАУ2010) 30-year average for April. ... This was the third warmest April on record, i.e. since daily temperature measurements at Armagh Observatory began around 1795. ... Last Revised: 2014 May 6th . ...

The technical memorandum: Time and Time Interval Measurement with Application to Computer and Network Performance Evaluation (PostScript) describes a number of techniques for conducting experiments typical of computer network and transmission systems engineering. ... The usual data collected during a performance run of some experiment might include time offsets, time delays, frequency offsets and various error statistics. ...

... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

Magnetic field measurements onboard the Interball Tail spacecraft are carried out by the FM-3I instrument which consists of two flux-gate magnetometers covering two different ranges: [-200, +200] nT and [-1000, +1000] nT. Besides scientific goals, the FM-3I experiment data is used to perform the attitude control of the Interball Tail spacecraft. ... August 22, 1995 . ... October 18, 1995 . Top of the page . ... Back to the Interball Home Page . ...

Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...

OM Background Measurements Nora Loiseau XMM-Newton User Support Group ESAC, Spain XMM-Newton N. Loiseau, 26/04/2005 1 OM Background Measurements, results Background values 0.0350 0.0300 0.0250 values 0.0200 0.0150 0.0100 0.0050 0.0000 W hite UV Gris m V Gris m B V U UVW 1 UVM2 UVW 2 XMM-Newton N. Loiseau, 26/04/2005 2 OM background averages Q LA (Counts/ sec. pix.) Q LA (Counts/sec. sq.arcsec) BPM16274 Diffuse Galactic Zodiacal Light (Counts/sec. sq.arcsec) Light (Counts/ sec. sq.arcsec) thrp. ...

SLAC Jan 2004 CCD Radiation Damage Studies J. Brau, O. Igonkina , N. Sinev, C. Potter (University of Oregon) January 9, 2004 Outline: · Introduction · Neutron and Electron irradiation · Study of SLD VXD3 · Measurement of the trap filling time · Conclusions O. Igonkina for U.Oregon CCD Radiation Damage Studies 1 SLAC Jan 2004 CCD The ... But is it radiation tolerant? ... The study is to be continued O. Igonkina for U.Oregon CCD Radiation Damage Studies 12 ...

Suppose measuring system has 16 electrodes. ... If the measuring system doesn't perform redundant measurements, as the current injection through electrodes n and m is equivalent to the injection through electrodes m and n , corresponding redundant values should be set to zeros as in the following example: POLAR 16 0.000 0.908 0.513 0.313 0.202 0.280 0.752 0.000 0.000 0.869 0.351 0.243 0.297 0.311 0.340 0.000 0.000 0.000 1.358 0.484 0.205 0.212 0.355 1.214 0.000 ... EIT Gallery ...

Once students get the hang of it, they can find and measure the brightness of Delta Cephei in a few minutes. ... of Delta Cephei . ... Oct. ... The following table lists the measurements of Delta Cephei made by one amateur astronomer in autumn 1990. ... 4.0 . ... This activity is a simplified version of one that appeared in Hands-On Astrophysics, a series of activities prepared by the American Association of Variable Star Observers with support from the National Science Foundation. << previous page | ...

... Hartmann Test Using a Screen With Four Holes 2 Hartmann test with four holes screen The theoretical concept of the primary aberrations measurement by four apertures Hartmann test introduced by "Malacara" * and "SalasPeimbert et. al. ... Black curve show the calculated coefficients for phase screens which have 8 modes of Zernike aberrations and red curve show the calculated coefficient for original phase screen. (a) astigmatism 45 (b) astigmatism 090 14 Coma Coma modes of Zernike aberration. ...

... Bojan Nikolic web pages (r. 329) . ... The CASA table tool allows access to all data contained in measurement set format. ... For this reason I have sketched out a simple, python-orientated, wrapper for data access in casata. ... cols = [ "TIME" , "DATA" ] . one gets (unsurprisingly) both the time and the data.. ... msin = "/home/bnikolic/data/almagen/uid___A002_Xa048f_X1.ms" >>> time , visdata = data . ... time , point1 , point2 = data . ... data . ... Accessing measurement set data . ...

... Class . Use . ... Packages that use Measurements . ... Uses of Measurements in ij . Classes in ij that implement Measurements . ... This is an extended image class that supports 8-bit, 16-bit, 32-bit (real) and RGB images. ... Classes in ij.gui that implement Measurements . ... Classes in ij.macro that implement Measurements . ... Implements ImageJ's Process/Enhance Contrast command. class . ... This plugin implements ImageJ's Analyze/Measure and Analyze/Set Measurements commands. class . ...