... Protective equipment: . ... Employers should use this information only as a supplement to other information gathered by them, and should make independent judgement of suitability of this information to ensure proper use and protect the health and safety of employees. This information is furnished without warranty, and any use of the product not in conformance with this Material Safety Data Sheet, or in combination with any other product or process, is the responsibility of the user. ...

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• ZnTe Safety Data Sheet
• CdSe Safety Data Sheet
• ZnSe Safety Data Sheet

... Classes . Files . ... File List . File Members . measures . ... It is a simple 00060 // container with the selected method, and the mean epoch . br 00061 // The method is selected from one of the following: 00062 // ul 00063 // li Aberration ::STANDARD (at 1995/09/04 the IAU1980 definition) 00064 // li Aberration ::NONE 00065 // li Aberration ::B1950 00066 // /ul 00067 // Epochs can be specified as the MJD (with defined constants MeasData::MJD2000 00068 // and MeasData ...

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• casacore: casa::Aberration Class Reference
• casacore: measures/Measures/SolarPos.h Source File
• casacore: casa::SolarPos Class Reference

... The SDSS 3D Universe Map . ... 28.10.2003 . ... Credit Copyright: Sloan Digital Sky Survey Team , NASA , NSF , DOE Explanation: The latest map of the cosmos again indicates that dark matter and dark energy dominate our universe. The Sloan Digital Sky Survey (SDSS) is on its way to measuring the distances to over one million galaxies . ... October 2003 . ... 2003 2004 . ... Publications with keywords: SDSS - universe - dark energy . Publications with words: SDSS - universe - dark energy . ...

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• Journal "Peremennye Zvezdy"
• JKCS041: The Farthest Galaxy Cluster Yet Measured
• Астронет > JKCS041: The Farthest Galaxy Cluster Yet Measured

Download Izmccd (~2.7 MB). ... If you want to calculate equatorial coordinates of object: . Click the " File " menu, and then click " Open " ; or press  on toolbar. Choose a file with image. ... Also see section " Viewing of image ". ... Before, if it is necessary, you must make an account dark current and flat field (See section " Preliminary processing of images ".) ... Measure the marked stars. ... Click the " Calculations " menu, and then click " Coordinates " or . ...

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An image of the grand design of spiral galaxy M100 obtained with NASA's Hubble Space Telescope resolves individual stars within the majestic spiral arms. ... Hubble has the ability to resolve individual stars in other galaxies and measure accurately the light from very faint stars. This makes space telescope invaluable for identifying a rare class of pulsating stars, called Cepheid Variable stars embedded within M100's spiral arms. ... 617) 495-7062 . Fax: (617) 495-7356 . ...

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• PINTofALE EXAMPLE SESSION: via Dracia
• Watching the Stars go `Round and `Round
• The AstroStat Slog identification

... LABORATORY OF RADIO ASTRONOMICAL OBSERVATIONS . Radio sources identification is one of the most important tasks of the current radio astrophysics. ... Optical idetification. ... Optical identifications of subsample of steep spectra radio sources from RC catalog using 6m SAO telescope of SAO RAS: optical observations. ... Astronomy Reports. ... Identification of radio sources with data of various radio catalogs allows one to construct continual spectrum of the object and its radio structure. ...

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• Radial velocity of the IRAS04296
• Atlas and list of identified lines
• Absorption bands identified with DIBs

... An interactive IRAF task for the analysis of Extreme Ultraviolet Explorer ( EUVE ) emission line spectra is presented. The line flux in extracted spectra may be measured by multiple techniques, including fitting individual lines. ... To aid in identifying lines, the positions of known lines may be marked on the spectrum during the fitting process. Also, model EUVE spectra may be constructed and overlaid using plasma emissivities and source emission measures supplied by the user. ...

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• Identification and Analysis of Binary Star Systems using Probability Theory
• ADASS 2003 Conference Proceedings

... Edit: manual editing using boxes . Window: specify plot range with a box . ... Mean: place a box and have the mean and rms values computed . Identify: click data points and have them identified . H-Line: display a horizontal line and move it for measuring purposes . V-Line: display a vertical line and move it for measuring purposes . FIT: display a widget for fitting various functions to the displayed data ...

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• Identifications and Efficiency
• Sample Identification
• First Rotation Period of Kuiper Belt Object Measured (ESO PR Photo 41/98)

... Activity 3: Measuring the Position of the Sun in the Sky . Purpose: To give students the opportunity to measure the position of the Sun in the sky using simple tools and methods. ... Alternatively, you may have students devise their own methods of relative measurement and apply them to measuring the position of the Sun in the sky. ... Rangi is the sky, and when the Sun is near Rangi's head it is summer in New Zealand. ... Read the Maori story to students. ... back to Teachers' Newsletter Main Page ...

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Collection of the orbital elements | ... The errors of the spacecraft motion extrapolation outside the measuring time interval were estimated by using the comparison of SC positions calclulated by the forward integration ( extrapolation method) and backward integration ( interpolation methods). ... The character of these time shift of the ascending nodes ( D Tn) corresponds to the orbiting period errors, which arise during SC motion extrapolation outside the measuring intervals. ... INTERBALL mission ...

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• The INTERBALL Tail PROBE orbital elements
• About modification of the INTERBALL orbital elements
• DOK-2 Results Page

Astronomy Terms - To Help You Study The Universe . Articles | ... Learning about the universe, or the study of astronomy, can be fun for the individual or for the whole family. ... Learning a few simple terms will help you with this fascinating study. ... You will use a telescope or binoculars for your observation of the sky at night. ... Celestial Terms . ... Meteor or a shooting star – the light caused when a meteoroid burns up in Earth's . ... www.astronomy.net . About Astronomy Net | ...

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• Measuring Resolution - an Astronomy Net ATM Forum Message

This illustration shows the disk of our Milky Way Galaxy surrounded by a fain, extended halo of old stars. Astronomers using the Hubble Space Telescope to observe the nearby Andromeda Galaxy serendipitously identified a dozen foreground stars in the Milky Way halo. They measured the first sideways motions (represented by the arrows) for such distant halo stars. The motions indicate the possible presence of a shell in the halo, which may have formed from the accretion of a dwarf galaxy. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE5028013-E99A-40AC-8F7C-A74700FBF1F1%7D
• NASAт??s MAVEN mission identifies links in chain leading to atmospheric loss |
• Clearing the cosmic fog: The most distant galaxy ever measured | Astronomy.com

... This file table3 82 660 Observed wavelengths, laboratory values and identifications -------------------------------------------------------------------------------- Byte-by-byte Description ... Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- SpOrd Spectrum order 5- 12 F8.3 0.1nm SolLam Wavelength determination of all solar and telluric lines measurable on the ... Note (6): J: Junkes et al., ...

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• Astronomical Catalogues

. Home . News . Gallery . Events . Twitter . Press Releases . Links . Contact Us . Calendar . Press & Web Coverage . Previous . Next . List . Taken on the 24th November by John McConnell. It shows the ISS and an unidentified satellite . Friday, 2 January 2009 23:14 . International Year of Astronomy, Ireland National Node . [Back To Top] .

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• Media Coverage
• IDLINES: identifying spectral lines
• Armagh Observatory

... Observations of GRB afterglows with Russian-Turkish 1.5-m Telescope (RTT150) . ... The afterglow light curve was measured in detail starting from about 5 h after the GRB and over five ensuing nights. In addition, upper limits were obtained on the rapid variability of the afterglow on the first night of observations and the history of afterglow color variations was measured in detail. ... 2007) : . ... Astronomy Letters, 33, 797 (2007) , arXiv:0802.1635 , The original text in Rissian . ...

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Restoring of magnetic field . These plots also were generated during attitude quality tests. On the lowest panel the measured magnetic field are ploted. ... Two upper graphs are the results of application of the attitude parameters to the measured magnetic field. To obtaining a good results, some additional procedures should be executed. ... There are not any amplitude or phase breaks and gaps in the restored magnetic field. ...

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• ENERGETIC PARTICLE EXPERIMENT DOK-2
• Trigonometry--what it is good for?
• (EHIPS) Applying to Australian data

This section of AMPLE provides a means for identification of minor planets. ... Due to special organization of the package, AMPLE permits the identification to be reliable fulfilled THROUGHOUT the TITLE YEAR. ... In such cases the result of identification depends on where the nearest opposition of inspected planet is situated, within basic interval lasted from November of preceding year to February of subsequent one or without it. ...

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. RC-archive . RC0907+0436 . RC0908+0451 . RC0934+0505 . RC0942+0447 . RC0945+0454 . The R-band contours (BTA) superposed . on 1490MHz image (VLA) ps . The map (1490MHz,VLA) superposed . on the R-band image (BTA) ps . Last updated 30 Jul 2001

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. Для работы с системой необходима идентификация пользователя. Введите, пожалуйста, Ваш идентификатор и пароль. Идентификатор: . Пароль: . Если Вы еще не зарегистрировались в системе, воспользуйтесь нижеприведенной формой. Введите, пожалуйста, Ваш идентификатор (состоящий только из букв и цифр) и пароль. Идентификатор: . Пароль: . Еще раз пароль: .

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• Thomson's method of spectral estimation

... A. A. Berezhnoy1,2, N. Hasebe1, M. Kobayashi1, G. Michael3 and N. Yamashita1 1Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan 2Sternberg Astronomical Institute, Moscow, Russia 3German Aerospace Center, Institute for planetary research, Berlin, Germany Abstract: The quality of Lunar Prospector measurements of elemental composition of the lunar surface is checked by comparison between remote sensing and returned sample collection data sets. ...

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• http://selena.sai.msu.ru/Greg/Publications/ms38/ms067.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf