... Doing Business with ESO > Technology Transfer > Examples of ESO developments that have been taken over by a manufacturer or produced commercially for a wider market . ... ESO for the Public . ... People and Events . ... ESO Press Conferences and Events . ... Developments at ESO . ... Because of the wider applicability of this technology, in 1999 ESO concluded an agreement with the French firm SNLS to manufacture and sell the ESO dewar under license. ... Developments Taken Over by a Manufacturer . ...

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• A lot Chinese names are degenerate. For example, it is hard to identify the
• ESO - Historic examples of ESO-developed technologies
• ESO - Examples of ESO developments that have been used for other similar

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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• Example of how mail is displayed
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• Examples of using the diff command

Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties . ... If necessary, data have been determined for the different crystallographic axes. ... In the following we give some examples of the data and their possible applications. Table: Summary of data measured in the Jena laboratory, which are currently available from the JPDOC. compound . ... amorph. ... Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties root 2003-03-06 ...

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• Database of Optical Properties
• Hydrogenated amorphous carbon
• Silicate minerals

This example shows how to add a few input widgets to a script and how to get data from them. This is a fairly artificial example in that one would normally just use the DIS Expose window for this purpose. ... import RO.Wdg import Tkinter import TUI .Inst.ExposeModel as ExposeModel from TUI .Inst.ExposeStatusWdg import ExposeStatusWdg class ScriptClass(object): Take a series of DIS darks with user input . def __init__(self, sr): Display exposure status and a few user input ...

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• TUI:Scripts:Scripting Tutorial:Get Info
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• Astrophysical Research Consortium Small Aperture Telescope

... The example demontsrates a way how to use the coefficients arrays and the Software . Let us suppose that we have a direction in the S/C frame, determined by the angles u1, u2, where: u1 - angle between vector and X axis (polar angle) u2 - angle on the YZ plane from Y axis (anticlockwise); . ... We use the file 950909t1 (the beginning data 9.09.06), which line 2 interval beginning : date 10.10.95 , time 1.926 thousands of sec, the interval duration is 4.583 thousand of sec. ...

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• Examples of the raw magnetic field information, obtained with the MIF-M
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Name Last modified Size Description . Parent Directory - ppm/ 2009-02-10 15:26 - tif/ 2009-02-10 15:26 - . Apache/2.4.6 (Linux/SUSE) Server at www.astro.louisville.edu Port 80

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• Index of /software/archive/colorspec/colorspec-1.0/examples/ppm
• Index of /software/archive/colorspec/colorspec-1.0/examples/tif
• Index of /software/astroimagej/examples

... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...

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• mcfile
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ASTRONOMICAL YEARBOOK for 2006 (in Russian) . Preface . In the тАЬAstronomical YearbookтАЭ (AY) the ephemerides of the Sun, Moon, major planets and stars computed with the maximum precision in accordance with the resolutions approved by the International Astronomical Union (IAU) are published. ... N.I. Glebova, M.L. Sveshnikov; . ... N.I. Glebova; . ... The data control of the different part of the Yearbook was carried out by N.I. Glebova, N.K. Omelyanchuk, and I.A. Lebedeva. ... N.I. Alehina. ...

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• AY2008 (preface)
• AY (preface)
• AY2011 (preface)

... Eris: More Massive than Pluto . ... Monitoring M2-9 . ... About 2,100 light-years away and over one light-year across, M2-9 is known as a twin jet or butterfly nebula in reference to its striking bipolar symmetry. ... Of course M96 is a spiral galaxy, and counting the faint arms extending beyond the brighter central region it spans 100 thousand light-years or so, about the size of our own Milky Way. vdB 152: Reflection Nebula in Cepheus . ... Reflection nebulas reflect light from a nearby star. ...

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• Haute Provence Star Trails
• Астронет > Haute Provence Star Trails

... Несколько примеров 3-многообразий: тор T^3, сфера S^3, S^3. Их геометрические (например, оптические) своиства. Евклидова и сферическая геометрия и, возмможно, чуть-чуть гиперболическои геометрии. ... Несколько разныкх определений (напр., факторпространство сферы по действию группы Z_p, результат склейки двух полноторий). ... Их геометрические свойства. ... Гиперболическая геометрия на нем. Его расслоение над окружностью со слоем проколотый тор. ...

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• Arithmetic groups (Spring 1997)
• Introduction to dynamical systems (Spring 1999)
• Conference Zeta Functions

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
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Magnification (Power) And Using Eyepieces . ... To determine power in a telescope, divide the focal length of the telescope by the focal length of the eyepiece. By exchanging an eyepiece of one focal length for another, you can increase or decrease the power of the telescope. For example, a 25mm eyepiece used on a telescope with a 1000mm focal length would yield a power of 40x (1000 / 25 = 40) and a 10mm eyepiece used on the same telescope would yield a power of 100x (1000 / 10 = 100). ...

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• The Astronomy Shop - Calendars - by Astronomy Net
• Let Me Be More Clear - an Astronomy Net Exploration Forum Message

. First Name . Last Name . EMail . Phone . Address . Country . [choose yours] Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua And Barbuda Argentina Armenia Aruba .

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• JavaScript Form Validator Documentation

Pulkovo NEO Page . ... NEA Accuracy Estimation . ... The estimation of accuracy of the current CCD observations of asteroids and comets is constantly performed at Pulkovo Observatory. ... The (O-C) values, so called "Observed" minus "Calculated" positions, characterize numerically the observations of any observatory, both professional and amateur, during a short period (one or several close nights). ... So the (O-C) values for these objects nearly entirely define the errors of observations. ...

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• Pulkovo NEO Page: Estimation of Observational Accuracy

Stellarium 0.12.3 . ... Classes . ... Scripting . ... Scripting Engine . ... Script Console . ... Since version 0.10.1, Stellarium includes a scripting feature based on the Qt Scripting Engine . ... Prior to version 0.10.0, Stellarium used a different scripting engine called StratoScript . ... Prior to version 0.10.0, Stellarium had a simple scripting engine, known as StratoScript . ... This script prints "Hello Universe" in the Script Console output window. core.debug( "Hello Universe" ); . ...

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• Stellarium: Plugins
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... Another significant contribution to the crystal energy of metals is the electron-ion interaction or the electron bandstructure energy (E BS ) which is defined by the interaction of valence electrons and the Brillouin zone (BZ) planes. ... The program BRIZ has been developed for 3D visualization of Brillouin zone configurations and intersections of BZ planes with a Fermi sphere[4]. ... 1.75 (electrons/atom). ... 4] Degtyareva V.F., Smirnova I.S.: BRIZ: a vizualization program for Brillouin zone ? ...

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• Spectroscopy of Semiconductors and Dielectrics
• Department of Solid State Physics MIPT
• SPECIALITY 01.04.07 - CONDENSED MATTER PHYSICS SUPPLEMENTARY PROGRAM

... 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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• Calibration data
• Manpage of FITSHDR
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... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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• VISTA - Visible and Infrared Survey Telescope for Astronomy

Turning the Camera Skyward . A reconfigured camera can take wide-field exposures of astronomical objects (constellations, the Milky Way, zodiacal light, moving artificial satellites, meteor showers, variable stars, etc.) to reveal much fainter objects and structures than seen by naked eye. ... This picture reveals objects more than 2.5 times fainter than can be seen by the naked eye, including not only stars but also the Orion nebula (M42), where new stars are being born. ...

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• ASP: The Story of Astronomy
• ASP: Science Fiction Stories with Good Astronomy & Physics
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... Meade Instruments Corporation . ... How to Calculate Power . How to Calculate Power: The magnification, or power, at which a telescope is operating is a function of the focal length of the telescope's main (objective) lens (or primary mirror) and the focal length of the eyepiece employed. ... Example: The Meade DS-2070AT telescope has an objective lens focal length of 700mm; when this telescope is used with a 25mm eyepiece, a power of 700/25 = 28 power (written as "28x") results. ... about meade | ...

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