Space Telescope Science Institute . ACS Instrument Handbook Cycle 19 . ... Advanced Camera for Surveys Instrument Handbook for Cycle 19 > Chapter 10: Imaging Reference Material > SBC/PR130L . ... 0.04 . ...

Last updated: Wed, 11 Oct 2000 09:07:07 (GMT -0700) Files Transmitted During Summary Period 4717616 Bytes Transmitted During Summary Period 106499688136 Average Files Transmitted Daily 41383 Average Bytes Transmitted Daily 934207791 . ... Jul 1 2000 0.77 1.02 1086454162 36274 | Jul 2 2000 0.97 0.97 1033492856 45617 | Jul 3 2000 0.72 0.73 781279944 34046 | Jul 4 2000 0.83 0.86 914539013 39240 | ... Aug 1 2000 0.77 0.80 853118365 36274 | ... Sep 1 2000 0.65 0.69 730957208 30569 | ...

Next: About this document Up: Old neutron star distribution Previous: References . Figure: Velocity distribution of young pulsars calculated from statistical modelling of evolution of 50,000 binary systems. ... Figure: Equal density contours for the calculated distribution of old neutron stars (in arbitrary units). Figure: Plot of (solid lines), (long-dashed lines) and (short-dashed lines) for the calculated old neutron star space distribution versus limiting distance of the sample . ...

... Индексы солнечной активности . ... Наблюдения NGDC . Солнечные регионы . ... Среднегодичные индексы . ... Июль . ... Июль, 1993 . Визуальные индексы солнечной активности по версии Национального центра геофизических данных . ... 0.00 . ...

... Бренд: Big Figures, Количество предметов: 1 предмет, Пол: для мальчика . ... Артикул: G152LWB43053-506 Цвет: мультицвет Состав: 100% натуральная кожа Параметры изделия: 26x15x6 см Страна дизайна: Италия Страна производства: Румыния . ... Цвет: Желтый . ... Цвет: Золотой . Цвет арматуры: Золото . ... Возраст от лет: 0.7 . ... Цвет: серый . ... Ластик Erich Krause "City XL", цвет: белый - Erich Krause - Erich Krause . ...

... We present a high resolution spectral atlas of the post-AGB star HD56126 associated with IR-source IRAS07134+1005 in comparison to the standard high luminous star Per. The spectra of HD56126 covering the broad spectral region 4010-8790AA at resolving power R=60000 (R=25000 for ?) were obtained with the echelle spectrographs NES and Lynx at the Nasmyth focus of the 6m telescope BTA. Figure 1: . ... HD56126 . ... TiII(11) . ... FeI(557) . ... FeI(485) . ... CeII(157) . ... FeII(151) . ...

... Figure eight, as double four. Figure four, as half of eight. If you skate, you would be great, . If you could make a figure eight. That's a circle that turns 'round upon itself. One times eight is two times four. Four times four is two times eight. ... One times eight is eight, two times eight is 16 . Three times eight is 24, four times eight is 32 . ... Six times eight is 48, seven times eight is 56, . ... And ten times eight is 80, that's true. ... Plus two times eight: . ...

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... Radio Catalog . The corrections in NVSS fluxes leading to the corrected Version 1.1 also result in changes to some of the figures and tables in Kimball Ivezi? ... The results are qualitatively the same. ... The new versions of the figures, along with the original versions (in high resolution), are available here . ... These figures, along with Table 4, continue to motivate t = 0.35 as the optimal separator between "simple" and "complex" sources). ... Complex Sources . ... t NVSS . ... galaxy . ...

Quiet Sun, Grevesse et al. abundances, Arnaud & Raymond 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. ...

. Search this album . Gallery . :: The First 100 Years . :: The 50" Great Melbourne Telescope, 1868-тАж . :: The primary mirror, no longer a perfect figurтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . View full size . Title: The primary mirror, no longer a perfect figure . File name: vest50in1.jpg . Dimensions: 600 x 450 px . Page: 1 2 58 59 60 61 62 63 64 65 66 67 . Powered by Gallery 3.0.9 (Chartres) . Login

... 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). ...

Next: List of Tables Up: No Title Previous: Contents . A dark current CCD exposure with cosmic ray events which are removed with non--linear filters. A) original, (B) 5*5 median filter, (C) 5*1 median filter, and (D) 5*1 recursive filter. Removal of cosmic ray events on a CCD spectral exposure with different techniques: (A) original, (B) median filter, (C) recursive filter and (D) stack comparison. ... Images RINGS and OFFRINGS. ... This image is obtained by the command visual/cube . ...

. 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 .

. Particles position in the equatorial plane, as given by our SPH simulation with gamma=1.2 after19 orbital periods. Postscript version . If you have comments or suggestions, email me at spxhmjb@astro.cf.ac.uk Last update: May 26, 1998 .

. Figure A1. This shows the geometry of a lower support rod when weighted and unweighted by the secondary cage. From this follows the equation . which can be rewritten as . For all cases of interest we have the conditions that << 1 and << 1 so that we can effectively ignore the terms and . Doing this gives us the excellent approximation . Solving this for gives . From the figure we can also see that Z = L sin( a). Combining these last two equations gives .

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... 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 ?.

... FIGURE-1.eps . 2014-09-29 16:05 . ... notes-figures . ... Last Revised: 2014 November 6th . ...