... Программа izmccd предназначена для высокоточной астрометрической обработки числовых изображений небесных объектов. ... Меню - "Вычисление/Медианный фильтр", либо 12-я кнопка на 2-й панели инструментов. ... телескопа был отснят большой участок неба. а) Копируете все изображения в одну папку. б) Вызываете функцию - меню "Вычисление/Автомат. обработка ", либо 8-я кнопка на 2-й панели инструментов. в) Отмечаете "Определять координаты известных объектов в поле зрения". ... Mx= 0.95100 // "/pix . ...
. XMM-Newton Science Analysis System . eslewchain (eslewchain-1.0.1) [???] . Meta Index / Home Page . EPIC images of name I"rev"_"obsid"_"ra"_"dec"_b"band".ds Where band is the energy band: 1 = 0.2-0.5 keV . 2 = 0.5-1.0 keV . 3 = 1.0-2.0 keV . 4 = 2.0-12.0 keV . 5 = 0.2-2.0 keV . 0 = 0.2-12.0 keV . EPIC exposure maps of name E"rev"_"obsid"_"ra"_"dec"_b"band".ds Only bands 0,4 and 5 are produced. XMM-Newton SOC/SSC -- 2008-10-22
Proposal Identification No.: ... Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: ABSTRACT: Regular Pulsars 6 Hours 45 minutes Continued timing of a millisecond pulsar in a stellar triple system We have discovered and are successfully timing a relatively bright millisecond pulsar in a hierarchical stellar triple system. The inner binary comprises a millisecond pulsar in a 1.6-day orbit with a hot, low-mass white dwarf. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/LorimertagP2822tp.pdf -- 48.8 Кб -- 18.03.2013 Похожие документы
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... In larger sources, the electron distribution may become nearly flat due to the wave-particle interaction, while the conversion efficiency of the particle energy flux into waves reaches 10 - 20%. ... Firstly, we consider the relative effect of the two factors affecting the electron distribution: particle escape from the radio emission source and relaxation of the electron distribution due to wave-particle interaction. ... The particle escape time esc is variable. ...