This diagram illustrates a floating image that overlaps the borders of two paragraphs in normal flow: the paragraph borders are clipped by the non-transparent parts of the image. ... A left-floating image causes the final three lines of the upper paragraph to float along its right side. It causes the first three lines of the following paragraph to do the same, and the remainder of that paragraph flows normally. The paragraph borders shine through the margin area of the image box. ...

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. Name . Last modified . Size . Description . Parent Directory . - . ovl2.png . 25-Jun-2008 20:28 . 8.9K . ovl3.png . 25-Jun-2008 20:28 . 8.4K . ovl4.png . 25-Jun-2008 20:28 . 8.6K . ovl5.png . 25-Jun-2008 20:28 . 8.5K . ovl6.png . 25-Jun-2008 20:28 . 8.5K . ovl7.png . 25-Jun-2008 20:28 . 8.6K . ovl8.png . 25-Jun-2008 20:28 . 8.4K . Apache/2.2.3 (CentOS) Server at www.naic.edu Port 80

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• Index of /~phil/hardware/pdev/fpga/gx/jfft/dlpf/simv/overlap

... 11.05.2000 . ... Credit Copyright: W. Keel and R. White, ( U. Alabama , Tuscaloosa), Hubble Heritage Team ( STScI / AURA ), NASA Explanation: Can this be a spiral galaxy? In fact, NGC 3314 consists of two large spiral galaxies which just happen to almost exactly line-up. ... Publications with keywords: dust - NGC 3314 - galaxy pair - spiral galaxy . Publications with words: dust - NGC 3314 - galaxy pair - spiral galaxy . ... Sculptor Galaxy NGC 134 . NGC 3310: A Starburst Spiral Galaxy . ...

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• Астронет > NGC 3314: When Galaxies Overlap

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2000 May 11 . NGC 3314: When Galaxies Overlap . ... Explanation: Can this be a spiral galaxy? In fact, NGC 3314 consists of two large spiral galaxies which just happen to almost exactly line-up. ... But against the glow of the background galaxy, dark swirling lanes of interstellar dust are also seen to echo the face-on spiral's structure. ...

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• APOD: 2005 May 7 - NGC 3314: When Galaxies Overlap
• APOD: 2011 July 15 - NGC 3314: When Galaxies Overlap

Sloan Digital Sky Survey Telescope Technical Note 19970527 Walter Siegmund . ... Pointing Error Budget . ... The interleaved strips and adjacent stripes overlap about 1 arc minute. ... However, a 2-D pointing accuracy of 3 arc seconds RMS leads to acceptibly uniform overlap and minimises the number of cases that require special handling (Table 3). ... A guide fiber bundle diameter of 16.5 arc seconds and a pointing accuracy of 3 arc sec RMS results in 99% initial success in acquiring guide stars. ...

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Science Vision Drop-outs & Overlaps January 24, 2007 General Discussion (G. Monnet, moderator + Panel chairs) Science Vision Overlaps I. ­ ­ Numerical Simulations Similar to large multi-purpose Instruments Significant operation cost; need for pan-European supercomputing facility II. ... Poitiers, 24 January 2007 Science Vision Dropouts & Overlaps 2 Science Vision Overlaps IV. ... To be addressed in final Science Vision Poitiers, 24 January 2007 Science Vision Dropouts & Overlaps 4 ...

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• Magnitude calibrations
• Astronet - 23-25 January 2007
• DSC_1389

Next: Loading data into Miriad: Up: Reducing 3-mm ATCA observations Previous: Flux density calibrators . When observing at two bands with the ATCA, it is generally sensible to set the two bands so that they do not overlap. ... However having the bands overlap complicates the data reduction process in Miriad . ... Loading data into Miriad : ATLOD . Initial ``fixes'' to millimetre data . ... Bandpass and antenna gain calibration . Flux density bootstrapping . ... Miriad manager . ...

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• casacore: casa::Copy_global_functions_copy Struct Reference
• imcomb
• Version 8.1

STIS Instrument Handbook for Cycle 24 . ... Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 24 > Chapter 12: Special Uses of STIS > 12.2 Long-Slit Echelle Spectroscopy . ... Long-Slit Echelle Spectroscopy . ... Nevertheless, at the price of confusion due to order overlap, the echelle gratings can be used with a long slit to obtain high-resolution spectroscopy of extended objects, or they can be used slitless with a full clear, filtered, or ND aperture. ...

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• UDF Parallels - General Information
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Wavelength-Dependent Selection Effects in Searches for SNRs in Nearby Galaxies Venn diagram depicts optical, radio and X-ray (Chandra) detections of SNRs in five nearby spiral galaxies (M81, M101, NGC 2403, NGC 4736 and NGC 6946) (Limiting LX ? ... 8%) Effects of ambient density and confusion? ... XRB/SNR Associations (e.g., MF16 in NGC 6946, MF22 in M81); also, X-ray counterparts to radio and optical SNRs with "discordant" Xray colors IR (Spitzer) and Radio (Single Dish+VLA) complementary data? ...

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• http://hea-www.harvard.edu/AstroStat/Stat310_1213/dj_20130416.pdf
• The AstroStat Slog funny
• The AstroStat Slog poetry

... ENDFOR ; Find overlaps and tweak rectification wm = reform(wb(0:wi( no-1 ), no-1 )) fm = reform(fn(0:wi( no-1 ), no-1 )) iovr_lo = fltarr(no) iovr_hi = fltarr(no) iovr_lo( no-1 ) = 0 iovr_hi(0) = wi(0) ; work from low wavelength to high wavelength FOR j = no-2,0,-1 DO BEGIN print ,'Order:',j,wb(0,j),wb(wi(j),j) im = n_elements(wm) - 1 k = j + 1 ik = 0 WHILE ( wb(ik,k) LT wb(0,j)+0.001 AND ik LT wi(k) ) DO ik ...

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. < Previous Figure < Main Page < Next Figure . The same as in Fig. 1. In this wavelength range the spectral orders mostly do not overlap. This is why only two spectra from the 1-m SAO telescope show the strong 7224 DIB which is usually intertwined with a telluric line and difficult to cancel out. < Download average spectrum of o Per . < Download average spectrum of reddened stars . < Previous Figure < Main Page < Next Figure .

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... Optical: Nebulosity offset to NE. X-ray: Non-thermal shell, confused by the Vela SNR, with central source, and possible associated pulsar. Point sources: Central X-ray source, with optical nebula, and possible associated pulsar. ... ADS . ... 1998, Nature, 396, 142. -ray observations. ... 1999, ApJ, 519, L177. ... Chandra of central X-ray source. ... Optical observations of central source. ... 2005, ApJ, 619, L163. -ray observations. ... Deep optical observations of compact X-ray source. ...

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• G260.4-3.4

Authors: V.A. Marsakov , T.V. Borkova , . ... It is shown that general populations of globular clusters and metal-poor field stars are components at least of three subsystems occupying different volumes in the Galaxy. The thick disk and proto-disk subsystems are genetically associated with the Galaxy. ... It is argued that heavy-element enrichment and the collapse of the proto-galactic medium occurred mainly in the period between the formation of the proto-disk halo and thick disk subsystems. ...

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... 2004: . Creation of a unique set of the spectral and polarization complex of high resolution in the range of 6-18 GHz, consisting of 64 channels with a 1% analysis stripe was concluded. Based on the combination of key parameters - the frequency overlap and resolution, sensitivity and accuracy of polarization measurements, such a complex is the first instrument of its kind in the practice of solar astronomy. ... Archive . ...

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... October 21, 1997 This Hubble Space Telescope image provides a detailed look at a brilliant "fireworks show" at the center of a collision between two galaxies. ... The respective cores of the twin galaxies are the orange blobs, left and right of image center, crisscrossed by filaments of dark dust. A wide band of chaotic dust, called the overlap region, stretches between the cores of the two galaxies. ...

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The new generation radio interferometer . ... 5000 km on the basis of square kilometer phased arrays. It is shown that this interferometer will have the sensitivity ~ 1 mJy at a frequency 100 MHz. ... VLBI interferometer, Active Galactic Nuclei, cosmology, effective area, sensitivity. ... Для исследований физических условий в активных ядрах галактик и космологических исследований необходимы низкочастотные наблюдения компактных радиоисточников с большой чувствительностью и разрешением. ...

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... 100 6 11 11 0 0 2 9 9 0 0 2 00 00 2 11 90 2 0 7 2 1 6 1 3 3 4 1 3 3 5 2 1 4 2 1 4 7 2 1 1 (a) Aligned Motifs (b) Countings A| - 0.22 0.06 - 0.22 - 0.22 - 0.62 - 1.32 - 1.32 - 1.32 0.98 - 1.32 - 1.32 - 0.22 - 0.62 0.06 0.06 0.28 0.75 C| 0.06 0.75 0.06 - 0.22 0.06 - 1.32 - 1.32 - 1.32 - 1.32 - 1.32 - 1.32 - 1.32 0.62 0.28 0.47 - 0.22 -0 G| 0.28 - 1.32 0.47 - 0.62 - ... AlBio08 An Optimized Counting Graph 7 Probability Weight Matrices Probability function ! ... ATACACA| ...

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... 295, 2003 H. E. Payne, R. I. Jedrzejewski, and R. N. Hook, eds. Merging of Sp ectral Orders from Fib er Echelle Sp ectrographs Petr Skoda Astronomical Institute of the Academy of Sciences of the Czech Republic Herman Hensberge Royal Observatory of Belgium Abstract. We review the data reduction of two fiber-based echelle spectrographs (HEROS and FEROS) with emphasis on the similarity of the inconsistencies between the overlap of spectral orders before merging. ...

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• Automated Software for Slitless Spectroscopy Analysis and Quasar Selection
• A Method for Minimizing Background Offset Errors When Creating Mosaics
• ADASS 2002 Conference Proceedings

. This new view of the historical supernova remnant Cassiopeia A, located 11,000 light-years away, was taken by NASA's NuSTAR. Blue indicates the highest energy X-ray light, where NuSTAR has made the first resolved image ever of this source. Red and green show the lower end of NuSTAR's energy range, which overlaps with NASA's high-resolution Chandra X-ray Observatory. // Credit: NASA/JPL-Caltech/DSS

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... Lyngby, Denmark The flux-flow oscillator (FFO) is a long Josephson junction in which a unidirectional flow of magnetic flux quanta (fluxons) generates millimeter and submillimeter electromagnetic radiation. ... The FFO voltage and thus its frequency is controlled independently by the overlap bias current, Ib, and the so called "control line" inline current, Icl, which creates the magnetic field at the ends of the FFO. ...

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• http://www.cplire.ru/html/lab234/pubs/2003-08.pdf
• http://www.cplire.ru/html/lab234/pubs/2007_13.pdf
• http://www.cplire.ru/nano/publications/JAC251-236.pdf