... We derive several relationships to obtain total IR luminosities from IR monochromatic fluxes, and we compare five different star formation rate (SFR) estimators for H II regions in M81 and M51: the UV, HЮБ, and three estimators based on Spitzer data. ... For the entire M81 galaxy, about 50% of the total SF is obscured by dust. ...

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• Terrestrial Silicates Compared to Astronomical Silicates
• Mathematical Analysis of the Iterative/Recursive Algorithm
• compare_table.pro

... Many scientific institutions maintain bibliographies of articles published by their scientists and monitor references made to these publications; these figures are often used to evaluate the effectiveness of the institution. ... a) Identification of papers that are based, at least partly, on new data Publications based on observations can be subdivided into two groups: those presenting new, previously unreported data, and those that make use of already published data. ... Published by . ...

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• Number of papers published using different observatories
• Number of papers published using observational data from different...
• The Cross-correlations

... Different statistical tests are used to compute the probability of a given hypotheses being correct. ... For single quantities, a confidence interval is estimated for the desired significance level. ... When the underlying distribution is normal, the ``Student's'' t and the distributions are used to estimate the confidence intervals for the mean and standard deviation, respectively. ... For this purpose the test variable . ... Special tables give the confidence interval for this test variable. ...

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• Introduction
• HyperLEDA documentation: catalogue of internal kinematics

... Classes . Files . ... File List . File Members . casa . Utilities . ... National Radio Astronomy Observatory 00023 //# 520 Edgemont Road 00024 //# Charlottesville, VA 22903-2475 USA 00025 //# 00026 //# $Id: Compare.h 20551 2009-03-25 00:11:33Z Malte.Marquarding $ 00027 00028 #ifndef CASA _COMPARE_H 00029 #define CASA _COMPARE_H 00030 00031 //# Includes 00032 #include casa /aips.h 00033 #include casa / Utilities /DataType.h 00034 00035 namespace casa { //# NAMESPACE ...

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• colden
• ATNF Daily Astronomy Picture
• tvcycle

... Information about a variety of different calendars for different cultures (e.g., Christian, Jewish, Muslim, Chinese, Hindu etc.) ... In addition, the Chinese had two different ways of interpreting and observing celestial events. One way the Chinese used astronomy was known as lifa; it was a discipline that aimed to understand the regularities and the predictable events in the celestial system through careful, observations, measurements and records. ... back to Teachers' Newsletter Main Page ...

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• ASP: Star Science in the Autumn Sky

Jeff mock supplied 6 different types of filters to use with the high resolution mode of the mock spectrometer. ... Plots were made of the time domain voltage response as well as the frequency domain power response. A decimation of 10 was used for the filter decimation. this gave a filter length of 80 coeff. The plots compare the filter shapes for these filter types (.ps) ( .pdf ) . ... Each color is a different filter type . middle: spectral density reponse for each filter . ...

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• pntErrVsPlatformMotion
• rotaPlatToSky
• Data and Analysis

... DRAFT July 28, 2008, 3:17pm DRAFT X-2 YERMOLAEV AND YERMOLAEV: COMMENT (No abstract for comment) DRAFT July 28, 2008, 3:17pm DRAFT YERMOLAEV AND YERMOLAEV: COMMENT X-3 Recently Zhang et al. [2008] presented a statistical study of sizes and relative geoeffectiveness of ICMEs (bodies of magnetic clouds) and preceding sheaths for 46 events responsible for intense (Dst < -100 nT) geomagnetic storms in 1996-2005 in which only a single ICME was responsible for generating the storm. ... 2008]. ...

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• http://www.iki.rssi.ru/people/y2005.pdf
• http://www.iki.rssi.ru/people/cosr539.pdf
• http://www.iki.rssi.ru/people/qq.pdf

... Different sections of an image may have different exposure. ... The obvious remedy for this is to divide the input image by the exposure map before smoothing. ... If you wish to create a background map in counts per pixel from an XMM exposure in which the exposure time varies significantly between CCDs, then you will need to remultiply the the output image by the exposure map; if however you wish to create a mosaic from several different cameras or pointings, you may wish not to do so. ...

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• Gain correction

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2009 . ... Direct Measurement of the Contribution of Point Sources to the Galactic Ridge X-ray Emission in Record Deep Observations by the Chandra Observatory . ... These demonstrate that electrons generating hard X-ray intensity have been an initiator and main source of flare plasma heating, the particle acceleration and the plasma heating is a system with positive feed back. ...

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• INTERBALL TAIL PROBE SITUATION ANALYSIS
• Comparing Masses Without Use of Gravity
• Energetic Particles

... ME AND MY SCHOOL . SOURCES . THE CHART OF THE DIFFERENCES IN THE SPELLING OF SOME WORDS CONNECTED WITH SCHOOL AND EDUCATIONAL SYSTEM IN BRITAIN AMERICA. ... РАЗЛИЧНЫЕ СТРАНЫ ИМЕЮТ РАЗЛИЧНЫЕ СИСТЕМЫ ОБРАЗОВАНИЯ, НАПРИМЕР ВЕЛИКОБРИТАНИЯ ИЛИ СОЕДИНЕННЫЕ ШТАТЫ. ... ОБО МНЕ И МОЕЙ ШКОЛЕ(ME AND MY SCHOOL), . ... А ТАКЖЕ ВАМ ПРЕДЛАГАЕТСЯ ТАБЛИЦА РАЗЛИЧИЙ В НАПИСАНИИ И ПРОИЗНОШЕНИИ СЛОВ СВЯЗАННЫХ С ОБРАЗОВАТЕЛЬНОЙ СИСТЕМОЙ В США(AMERICAN ENGLISH)И ВЕЛИКОБРИТАНИИ(BRITISH ENGLISH)-THE CHART . ...

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... Take a particularly simple signal: a cosine wave. ... Now, we are going to stretch and shrink the wavelet along the time axis (we assume the data is in the time domain), and at each time compare the shape of the signal to that of the wavelet. ... Figure 3: The wavelet (dotted line) is translated rela tive to the signal (solid line). ... Figure 4: The dashed line plots the `match' between the wavelets (dotted line) and the signal (solid line) as a function of time. ...

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• Analysis of a multiperiodic signal
• Publications
• Image: Nijo castle, Shogun palace. The main building. Comparing to temples and

... Up: Data Analysis Tools, Techniques, and Software . Previous: An Automatic Astronomical Classifier Based on Topological Neural Networks . ... Teuben, P. J., Wolfire, M. G., Pound, M. W., & Mundy, L. G. 2000, in ASP Conf. ... P. J. Teuben, M. G. Wolfire, M. W. Pound, L. G. Mundy . ... We have assembled a cluster of Intel-Pentium based PCs running Linux to compute a large set of Photodissociation Region (PDR) and Dust Continuum models. ... 2000). ... Teuben, P. J. 2000, BIMA memo (in preparation) . ...

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• ADASS Conference Series
• Classification of Objects in the Guide Star Catalog
• Cost-Effective System Management

The Special Astrophysical Observatory of Russian Academy of Sciences is one of the leading center of stellar magnetism study. ... Our observatory every 3-5 years holds an International Conference "Magnetic Stars" during past 30 years. ... The conference proceedings were published in book "Stellar Magnetism", Editors-in-chief Yu.V. Glagolevskij and I.I. Romanyuk (Saint Petersburg, Nauka, 1992), 270 pages. ... Conferences . History . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...

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• Description of algorithm
• Database "Stellar Spectra"
• THE MEASUREMENT OF MAGNETIC FIELDS IN THE SOLAR ATMOSPHERE ABOVE SUNSPOTS USING

... 2008. ... Phys. Rev. B 47, 7312 (1993) and F. Evers et al., ... k F d e2 (1) The experimental data are compared with Eq. (2) in Fig. 1 where we plotted the experimental and theoretical dependences of xx(1/2)kF on d (let us remind that kF = 4 n ). The experimental points exhibit a large spread not very far from the theoretical line. ... REFERENCES m Fig. 2. xx(1/2)n2 versus the spacer thickness d. The gles are the experimental data, and the solid line is the fit of the data in the log­log scale. ...

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• http://www.issp.ac.ru/lek/shovkun/abs17.html
• http://www.issp.ac.ru/lek/zverev/art69-RE.pdf
• http://www.issp.ac.ru/lek/murzin/art38E.pdf

My research interests are focussed on the theory and modelling of accretion processes as well as star and planet formation mechanisms. I am particularly interested in the stability properties of accretion discs, the generation of MHD turbulence and associated angular momentum transport, disk - planet interactions and the origin and characteristics of jets and winds from accreting systems . ... These results have been published in Salmeron & Wardle, 2005, M.N.R.A.S., 361: 45-69. ...

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• COALA - Computational Astrophysics Laboratory

... Archives . ... A number of practical Bayesian data analysis books are available these days. ... Bayesian Computation with R . ... If an young astronomer likes to enter the competition posted below because of sophisticated data requiring non traditional statistical modeling, this book can be a good starting. ... The other book is . ... There are other practical real data sets to illustrate Bayesian computations in the book and these example data sets are found from the book website . ... Chandra Blog...

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• The Orion OB1 Association
• The AstroStat Slog VO
• How did I collect the tweets from the 219th meeting of the AAS

... January 13, 1997 . Sunspots: Magnetic Depressions . ... Explanation : Our Sun has spots! These spots appear dark in photographs like the one above, but in fact sunspots are quite bright - they are just dark compared to the rest of the Sun. ... This field slows energy from entering the sunspot region, causing sunspots to appear cooler, darker, and lower than the surrounding surface. ... The Sun and sunspots should never be looked at directly . ... About APOD > . ...

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• APOD: March 22, 1998 - Sunspots: Magnetic Depressions
• APOD: 2004 July 25 - A Solar Filament Lifts Off
• APOD: 2000 August 9 - A Solar Filament Lifts Off

... A homogeneous chemical analysis of the inner Galactic disk from the first data release of Gaia-ESO . ... Gaia-ESO is a public spectroscopic survey designed with this goal in mind. ... These first results highlight the potential of the Gaia-ESO survey to explore areas of the Milky Way still poorly studied, such as the inner disk, and to give new constraints on Galactic chemical evolution models. ... Map of observed targets of the first data release of the Gaia-ESO Survey. ...

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• Ionized outflows in z~2.4 quasar host galaxies
• Serpmap (Abstract)

... In order to compare the number of different evolutionary stages obtained and X-ray luminosity of the chosen X-ray sources with the observed galactic values we use the sum of C/O+O/C , where C and O are the calculated and observed values of a given binary type, respectively. If we make comparison for a number of different binary species (for example, we compare the number of CV, number of X-ray pulsars,   total X-ray luminosity of LMXB, etc.), we write this criterion in the form: . ...

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• Basic Observational Data for Determination of f(q) and
• Nomenclature
• E-P transitions for different orbits

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

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