CLEAN Map ps -- is a plot of the naturally weighted CLEAN image. The lowest contour levels (2 steps) on image is plotted at "clev" levels [Jy/beam], the peak brightness -- "max" values [Jy/beam]. The dashed contours indicate negative flux. The beam is shown in the bottom left corner of the images. The plot is in postscript format.

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Fig. ... Photograph of the Pleiades cluster by E. E. Barnard (1927) , courtesy of the Carnegie Institution of Washington. ... Top left: central cluster in red (POSS E) filter. Top right: central cluster in blue (POSS O) filter. ... Stars on the east side of the cluster generally exhibit E(B-V) ~ 0.03. ... Single underscores represent lower column densities of N (CH + ) ~ 5x10 12 cm -2 . ... Fields and pointings of thesis observations: The WISP field is indicated by the 5њ x 1.7њ diagonal box. ...

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• CIMA Buttons
• GALFACTS Team Ready

... Heliostat is cleaned and wrapped in plastic sтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: Heliostat is cleaned and wrapped in plastic sheeting. Description: The scaffolding is removed, so further access will be impossible until rebuilding is complete. NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... Heliostat is cleaned and wrapped in plastic sheeting. ...

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• Most rooms clean, courtyard looking bare.
• Cleaning the drive is a difficult job.
• Cleaning up

... XI. 2015 acific l ym p i a d Dh aka , Ban g l ad esh G r o u p language English Sky map round. ... Sky from Dhaka. You are given a map of certain region of sky as visible from Dhaka today. The lines drawn indicate boundaries of the constellations. The line shown at the bottom left corner corresponds to 11° in the sky. ... There is a particular binary star in this map, where one component star has yellow colour and other star has blue colour. Mark this star with the letter "B". ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The formation process of a MBF and the associated BP (No. 1 in Table 1), which is formed by bipolar emergence. The top row gives the BP region as seen in AIA 193 at the indicated time. ... The bottom row shows the normalised AIA 193 lightcurve (left), and the positive (middle) and negative (right) magnetic fluxes obtained in the blue and yellow boxes marked in the top two rows. ...

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• Terry Mosely's Bulletins

... title='Салфетки Pampers Baby Fresh Clean 256шт PA-81454789' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> . ... Бра в стиле модерн . ...

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• Рубашка Clean Cut Модель: 28714324 - Clean Cut - Clean Cut Кровать-машина
• Средства для стирки и от накипи Clean home - Clean home - Clean home Pentel
• Краска акриловая наружного применения, цвет кобальт Plaid 01631-PLD - Plaid -

... Imaging techniques II: the galaxy NGC 3621 . ... The three images above show the same HI channel map, ie the hydrogen gas at one particular velocity, of the spiral galaxy NGC 3621 using data from the Australia Telescope Compact Array (ATCA). ... The galaxy NGC 3621 is part of the Local Volume HI Survey (LVHIS) . ... today * ATNF | ... ATCA | ...

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• Computation
• clean
• Deconvolution with CLEAN

... Saturn's Cleanest Moon: Enceladus . ... 25.11.1995 . ... Credit: NASA , JPL , Voyager 2 Explanation: Enceladus orbits Saturn between the smaller Mimas and the larger Tethys . Enceladus is composed mostly of water ice and has the cleanest and purest ice surface in the Solar System . ... The surface also has many unusual groves and relatively few craters, like Jupiter 's moon Ganymede . ... November 1995 . ... 2007 . ... Publications with keywords: Saturn . Publications with words: Saturn . ...

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• XWare > APOD

OSIRIS images of Comet 67P/ChuryumovтАУGerasimenko showing the details of a 0.3-mile-long (500 meters) crack running through the Hapi region. A context image showing the smooth, boulder-strewn Hapi region and the Hathor cliff face to the right is shown in the top left panel. The bottom-left panel indicates the crack extending across Hapi and beyond. The right panel shows the crack where it leaves Hapi and extends into Anuket, with Seth at the uppermost left and Hapi in the lower left. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBD46B601-4168-4478-A4C2-2F9301EBD6E6%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0841AA6D-FBE3-4DD3-B11F-FD55276CF893%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6CBBAB2C-C75D-401A-ADB5-54F82DF295C9%7D

... Clean . ... Flux Sign Expo . ... Flux, mCrab . ... 0.73 PHA . ... The map above is movable . ... Original shows mosaics with all data available. Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. All maps are convolved with instrumental point spread function (PSF) which is Gaussian ( =5'). ... INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ...

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... 2006 December 12 . Light Deposits Indicate Water Flowing on Mars . ... Explanation: What's creating light-toned deposits on Mars? ... One clear case is shown above , where the same crater on Mars is shown as photographed in 1999 August and again in 2005 September. ... Apparent tributaries near the bottom bolster the leading hypothesis that water gushed out of the crater wall, flowed down the crater, and soon evaporated into the thin Martian atmosphere . ... About APOD | ...

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• APOD: Galileo Views Ganymede
• APOD: November 25, 1995 - Saturn's Cleanest Moon: Enceladus
• APOD: 2005 June 6 - Saturn: Dirty Rings and a Clean Moon

The HST images of GRB 990123. HST has observed this field in the 50CCD (open) filter on the 8 February 1999, 23 March 1999, and the 7 February 2000, or 16, 59 and 380 days after outburst. ... On the left in the above image is the February 1999 image of GRB 990123, on the right the difference between that image and the February 2000 image. ... On the left in the above image is the March 1999 image of GRB 990123, on the right the difference between that image and the February 2000 image. ... 1999). ...

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• Superluminal Motion in the M87 Jet
• Deconvolution

... Please note that throughout this exercise you need some patience since the PEARL procedures use the Direct Fourier Transform which is quite slow for the size of map we are trying to work with! . ... Initial chisq= 24.980139 . SVD: will edit 0 singular values! ... Click Update to add the selected number of CLEAN component to the current model (which was empty at the start), self-calibrate the phases, subtract the CLEAN components from the data, and re-display the updated residual and final maps. ...

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• BL Lacs
• Official Homepage of Sebastian Deiries
• NPOI Lab

... Previous: ESO C Library for an Image Processing Software Environment (eclipse) . ... A new CLEAN-type algorithm searches for model components not in the dirty image but in the multi-resolution wavelet transform of the dirty image based on the dirty beam. ... The improvement of this prototype Wavelet CLEAN, which does convolve with the dirty beam, can be attributed to a suppression of noise and aliasing in the dirty image by use of information in the sidelobes of the whole image domain. ...

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• Determination of the Permissible Solutions Area by Image Reconstruction from a
• Restoration of HST WFPC2 Images in Gyro-Hold Mode
• Data Acquisition by Switching

... 1 2 3, Nothing's for free 4 5 6, Pick up the sticks and go home. ... What's left when the locks have all been broken, young children of authority? ... 1 2 3, Nothing's for free 4 5 6, Pick up the sticks and go home. the basement lies within us, the fear comes through the door there's nothing left between us, the fear becomes a roar Once that wheel is in motion, don't lose what you have found. I'm talking about the burning wheel of tongues, everything that makes it go around. ...

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• Dynamic HTML in Communicator
• Long description for example showing caption to the left of a table
• Long description for example illustrating positioning with respect to a

... This section describes three functions which have been created to cleanup defects in images. The first two functions for cleaning rows and columns are particularly useful for CCD--images. ... These can often be removed with the commands: MODIFY/COLUMN INPUT OUTPUT [C or V] [columns] . ... This is particularly useful for removing the permanent defects which may exist in the CCD--frames and which cannot be removed by the MODIFY/COLUMN or MODIFY/ROW commands. ...

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• Input Data and Preprocessing
• Progress Bars
• New galactic sources

... 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). ...

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• Sun image
• Evidences of supercritical accretion onto black hole in SS433
• Figure 1

... The fact that the gray residual is scaled 2.5 times the gravity and model means disturbances are more apparent. ... Start and stop times are indicated in the lower corners of the graph.In this first picture, you see the earthquake off New Guinea at 3:55 UTC 2009-04-01 (we saw it 20 minutes later). ... However, gravity does not directly mean displacement, so some scaling factor has yet to be applied--do not take the 0.5 m literally--it may be closer to 0.3 m. The green is barometer. ...

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• Figure 9
• default
• TUI:Guiding:NA2 Guider

... Distribution of orbital elements for the RR Lyrae stars. Results for stars with [Fe/H ] > -0.95 (left column), [Fe/H ] < 0.95 and V res < 290 km/s (middle column), and [Fe/H] < -0.95 and V res > 290 km/s (right column) are shown separately. In the top row, we have plotted normal curves fitting the distributions. ... next figure | privious figure . ...

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• Vladimir Marsakov Abstracts
• F-stars in galactic disk, figures

... When the cursor is moved across the image (using the left-mouse button) a profile, from the cursor-position upwards to the height of the spectrum extraction-region height, is drawn at the bottom of the image. A new spectrum is selected by centering the cursor (either by moving the mouse or by using the arrow keys on the right of the key-board) over the approximate centre of the corresponding zeroth-order feature and either clicking the left-mouse button or hitting the return key. ...

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• The spectrum-selection window (old method)
• Cleaning lightcurves
• Details about the pattern recognition