... 30 April 2003 . ... 2003 Paper . SN Ia confidence contours from all sources for Omega Matter and Omega Lambda- Blue contours show 68,95 and 99.7% confidence intervals. ... SN Ia confidence contours from all sources for the equation of state and Omega Matter- Blue contours show the 68, 95 99.7% confidence intervals. ... Coming Soon . ... Best fit model (A), 1-sigma model (B), are shown relative to Concordance Model (C). ... 2003 Paper - w versus Omega_M . ... 2003 Paper - Omega_M versus Omega_L . ...
Разработка, исследование и изготовление мощных полупроводниковых лазеров, излучающих в диапазоне длин волн 800 - 1800 нм. ... 30-летний опыт работы по разработке и изготовлению полупроводниковых лазеров . ... Диапазон длин волн - 800 - 1800 нм . ... Ознакомление с физическими и технологическими принципами работы мощных импульсных полупроводниковых лазеров с интегрированным тиристорным переключателем . ... Мощные импульсные полупроводниковые лазеры - физические основы и практическое применение . ...
Previous Editions of the M111: . ... Severe Space Weather . ... On Line"! ... Any time you have something you'd like to offer - be it a story of how you first got started in astronomy, a star party you just attended, a telescope you just bought, or your favorite constellation, just drop me a line with the story included and I'll be sure to get it posted! ... You can keep an eye on space weather yourself at the National Weather Service's Space Weather Prediction Center, www.swpc.noaa.gov . ...
XMMNewton CCF Release Note XMMCCFREL305 EPICMOS contamination parameters S. Sembay & R. Saxton September 4, 2013 1 CCF components Name of CCF VALDATE List of Blocks changed Change in CAL HB EMOS1 CONTAMINATION 0001.CCF 20000101 CONTAM DEPTH YES EMOS2 CONTAMINATION 0001.CCF 20000101 CONTAM DEPTH YES 2 Change It has become apparent that the response of the MOS cameras (primarily MOS2) has deteriorated at lowenergies (< 1 keV) over the course of the mission. ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0305-1-0.ps.gz -- 145.9 Кб -- 04.09.2013 Похожие документы
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... Why is it so difficult to use ``other people's software''? ... This paper will offer a starting point for software cooperation, centered on the concept of ``minimal software buy-in''. ... We can, for example, try to expose technical impediments to sharing software. And surely the first barrier to using other people's software is ``buy-in'', that is, the effort needed to adopt and use such software. ... For example, distributed objects are being hailed as the key to using other people's software. ...
... Observatory . ... THE HISTORY OF AAAP . ... After introductory remarks by Robert Sanders, founder of the Association, it was moved that the name of the organization be Amateur Astronomers Association of Princeton. ... 2/72 First issue of Sidereal Times, so named by Editor Roxanne Tobin. ... 5/72 Election of officers: Norman Sperling, Director; John Church, Assist. ... Sidereal Times, John gives the following report: . ... Sidereal Times.) ... Amateur Astronomers Association of Princeton Т? 2015. ...
Night of October 24-25, 2011 ============================ CDK20 at Moore Observatory Sum of 100 second exposures Date of observation: 2011-10-25 at 07:03 UTC Sloan filters "g" = blue-green "r" = orange-red "i" = near infrared m74_g_coadd.fits EXPTIME = 5.000000000000E+02 / Maximum equivalent exposure time (s) m74_i_coadd.fits EXPTIME = 7.000000000000E+02 / Maximum equivalent exposure time (s) m74_r_coadd.fits EXPTIME = 5.000000000000E+02 / Maximum equivalent exposure time (s)
... Sizes of spectra The number of spectra that are `spoiled' by overlaps depends on the contrast ratio reached by the MEMS device, the area on the sky covered by an individual spectrum and on the number density of potential spoilers at a given magnitude. ... 4-- NIRSpec contrast and confusion limits 1 low resolution 0.8 0.6 0.4 0.2 0 1 hi resolution 0.8 0.6 0.4 0.2 0 20 Figure 3: Probability that spectra are contaminated at the Galactic pole as a function of the magnitude of the target galaxy. ...
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