... Астрософт (Модератор: tlgleonid ) > . Reference stars в программе MaxIm DL . ... Благодарностей: 0 . ... 21 Июнь 2009, 10:23:08 ? В программе MaxIm DL (Version 4.58) столкнулась с тем, что при фотометрировании не могу отметить больше чем 8 звезд сравнения (ref). ... Ответ #1 : 21 Июнь 2009, 13:10:42 ? ... А блеск исследуемых звезд вычисляется из среднего по всем звездам сравнения. ... Цитата: Protozvezda от 28 Июнь 2009, 02:44:42 Не хотели ли бы Вы подключиться к моей программе наблюдений? ...

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... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

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... This is commonly referred to as CPM (cost per thousand impressions).We pay you a percentage of revenues for the ads that you and your friends view with Harry, based on current CPM rates.You will get 75% of total revenue generated from your viewing.. ... REMEMBER: for every one hour the program on Your screen You'll get paid $0.50. And when You recommend those program to Your friends, reffering to Your personal ID, You'll get paid $0.10 for every hour the program open on Your's friends computer. ...

... Sayh al Uhaymir (SaU) 085, a 112 g carbonaceous chondrite, was found in the desert of Oman on January 11, 2002. ... In SaU 085, the matrix /(chondrule+aggregates) ratio is 0.77, similar to Allende and Mokoia, both oxidized CV chondrites, but also similar to the reduced CV chondrites [1]. ... Some FeO-rich augites and diopsides from the SaU 085 matrix have high NiO contents similar to CK chondrites (0.7-3.3 wt% NiO) (Fig. 2), additional evidence for this oxidized type of CV chondrite. ... Fig. ...

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RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope 's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication SSRT - Siberian Solar Radio Telescope . ...

We present a catalogue of galaxies for which spatially resolved data on their internal kinematics have been published; there is no apriori restriction regarding their morphological type. The catalogue lists the references to the articles where the data are published, as well as a coded description of these data: observed emission (E) or absorption (A) data, optical (O) or radio (R) data, velocity (V) or velocity dispersion (D), radial profile (1) or 2D field (2). ...