... Each bin is associated with a start time (which is equal to the end time of the previous bin, if there is one), and end time (which is equal to the start time of the following bin, if there is one) and an attitude. ... This attempt is either successful or unsuccessful (logical returned value of the oal call, or null value in the atthkset column). evproject begins a new attitude bin if any of the following occur: . ... The attitude of each new `successful' bin is set to the baseline attitude. ...

... The normalised WHT optical spectrum of KIC 10449976 fitted with the model described in 3 optimized for abundances of C, N, Si and Ne, together with line identifications. ... Optical spectroscopy of the blue star KIC 10449976 shows that it is an extremely helium-rich subdwarf with effective temperature T eff = 40 000 300 K and surface gravity log g = 5.3 0.1. ... Kepler photometry of KIC 10449976 in both long and short cadence modes shows evidence for a periodic modulation on a timescale of 3.9 days....

... Also the measured signals are a#ected by detector transients, altering the final results considerably. ... The sequence is bounded by two measurements of the FCS , to fix the responsivity for the baseline correction 0 200 400 600 800 1000 measurement time [s] 0.00 0.02 0.04 0.06 0.08 0.10 Volt/second bg source fitted baseline 2. FCS 1. FCS source initial drifting signal corrected signal bg FCS source background signal internal calibration signal source signal corrected ...

O ptimal transport : T heory and A pplications . ... Names of participants of the OTARIE project are underlined . ... That code was never made public. ... WANN (Weighted Approximate Nearest Neighbors) is a library of C++ classes for weighted nearest neighbor search: given the set P of points p 1 , p 2 , , p N endowed with weights w 1 , w 2 , , w N and a query point q , find p k such that | ... WANN is part of a multipurpose library for numerical transport optimization developed in the OTARIE project. ...

The creation of the database of images of old analogue magnetograms of Geophysical Observatory "Paratunka", Kamchatka, Russia, 1967-2006 VarSITI / SCOSTEP Project Final Report ­ 2014 1. INTRODUCTION Magnet ic field variat ions show the processes in the Sun-Earth system. ... These data are contained in analogue magnetograms obtained at the observatories during the last century. ... The usual so lut ion of these problems is to obtain the graphic images of magnetograms. ...

... Sighting the telescope, first at the tree and then at pole B, you measure the angle A of the triangle ABC, equal to the difference between the numbers you have read from the azimuth plate.. ... Why triangles? ... One large surveying project of the 1800s was the " Great Trigonometric Survey " of British India. ... Everest was the one who commisioned and first used those giant theodolites; they are now on display in the Museum of the Survey of India in Dehra Dum. ... Everest . ...

OSLO LT V5.4 Optical Software For Layout And Optimization . Articles | ... Has anyone out there tried to raytrace a telescope design? ... OSLO LT keeps track of the optical path length each ray travels, so it knows the phase relationship of the light as it travels through the telescope. ... Through the use of OSLO LT, I've been able to refine the optical design of the telescope I'm working on. ... www.astronomy.net . About Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

Note that these are 'General' ICDs giving information about protocols, not specific ICDs giving details of the full interfaces between specific Gemini systems. ... Document . ... The System Command Interface (PS) . ... The Baseline Attribute/Value Interface (PS) . ... Baseline DHS interface (PS) . ... System Status and Alarms Interface (PS) . ... Wavefront Sensing Information Interface (PS) . ... ICS/TCS Direct Control Interface (PS) . ... Telescope Tube Mass Balance f/16 IR Top End Config. ...

... Sighting the telescope, first at the tree and then at pole B, you measure the angle A of the triangle ABC, equal to the difference between the numbers you have read from the azimuth plate.. ... Why triangles? ... One large surveying project of the 1800s was the " Great Trigonometric Survey " of British India. ... Everest was the one who commisioned and first used those giant theodolites; they are now on display in the Museum of the Survey of India in Dehra Dum. ... Everest . ...

Quiet Sun, Grevesse et al. abundances, Arnaud & Rothenflug ion balances . Figure 1: Emission Measures (EM) [cm -5 ] derived from combining all lines for particular ions, for the Active and Quiet Sun regions observed by SERTS. Error bars have been shown when multiple lines from the same ion have been combined to produce a single ion-averaged EM. ... Following Brosius et al. (1996), we have assumed solar coronal abundances derived by Feldman et al. ...

... The OVERLAY element is used to overlay images on top of a base figure. ... UNITS . Specifies the choice of units for width and height: units=pixels (the default) specifies pixels, while units=en specifies en units (a typographical unit equal to half the point size). ... X increases to the right, and is given in pixels or en units (according to the value of the UNITS attribute). ... HEIGHT . Specifies the desired height in pixels or en units (according to the value of the UNITS attribute). ...

. F IGURE . 7. The age distribution of the globular clusters of (a) Galactic origin and (b) accreted by the Galaxy. Different shadings are used to show the thick disk and prot-disk halo clusters. The curves are Gaussian fits to the corresponding histograms. Data was taken from ( Borkova Marsakov, 2000 ). discussion in the text | privious figure | next figure .

SKA ­ TDT Group On Phase Computation during Folding C.Baffa, E.Giani January 2014 The last part of pulsar search algorithm, as in the SKA TDT group approach, is the verification and optimization of pulsar parameters candidates identified in the previous phases. ... As the phase errors are expressed as fractions of the full period (in our case 44 measurement of 50 s), it is evident that the maximum integration time compatible with single precision phase computation is very short. ...

... 02-Mar-2006 14:49 . ... OptiM_Setup/ . ... 29-Jan-2003 16:24 . 2.0K . ... 03-Feb-2003 12:45 . ...

... Астронет | ... Обзоры astro-ph | ... A&ATr | ... планета Астронет | ... Словарь | ... О словаре . ... Термин "baseline" . baseline : . базис . ... east-west baseline : . базис (радиоинтерферометра), ориентированный в направлении запад-восток . ... fixed baseline : . постоянный базис (радиоинтерферометра) . long baseline : . большой базис (радиоинтерферометра) . Вернуться в словарь . ...

... Parent Directory 06-Jun-2002 17:31 - 30dor. gif 22-Jul-2002 09:35 397k 30dor.txt 22-Jul-2002 09:35 2k 47tuc. gif 22-Jul-2002 09:35 78k 47tuc.txt 22-Jul-2002 09:35 2k dem192.txt 22-Jul-2002 09:35 2k dem192_u.jpg 22-Jul-2002 09:35 139k hkhiper.jpg 22-Jul-2002 09:36 234k hkiper.txt 22-Jul-2002 09:35 2k lmc-1. gif 22-Jul-2002 09:35 56k lmcstcl. gif 22-Jul-2002 09:36 130k lmcstcl.txt ...

. Figure 2. The same as in figure 1 but for dependence of the FD onset (?To, panels a,b) and peak (?Tp, panels c,d) transit times on the eruptive magnetic flux ?.

... There are two stars in the binary system: a donor star on the right and a black hole on the left (an infinitely small point in the center of a complex figure). ... The wind is ejected as a hollow cone; it has a funnel (the funnel opening angle in the figure) and thick walls (wall opening angle in the figure). The observer looks at the whole system and the supercritical disk from the right, and sees everything up to the wind photosphere (the red color in the figure). ...

. Приложение к лекции для студентов . Верходанов О.В. Рис.12. Пример работы алгоритма чистки. На верхнем рисунке приводится модельное изображение, на среднем - грязная карта, на нижнем - изображение, восстановленное с помощью CLEAN. Рисунок воспроизведен из работы Стиэра и др. (1984). vo @ sao.ru ( Oleg Verkhodanov ) .

... ARTICLE: The Adventurous Search For The Astronomical Unit . ... Kepler himself had suggested to use the rare occasions of Venus transiting (crossing) the solar disk to measure our distance to the planet. ... Due to the orbital inclination of Venus against the ecliptic of 3.5°, a Venus transit is so rare that it happens only at intervals of 121.5 years, 8 years, 105.5 years, 8 years and so on. ... Crabtree witnessing the transit of Venus 1639 . ... Transits of Venus - The Quest for the Solar Parallax...