Next: AO data and AIPS++ Up: Spectral-Line Observing at AO Previous: Useful Stuff . There are currently a number of ways you can convert Arecibo data into other data formats, and a variety of support levels for different data analysis programs. As a result it is feasible to reduce your Arecibo data with a wide range of data reduction software. ... In the following two section we describe spectral line data analysis in two of the available data reduction packages - Analyz and AIPS++. ...

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• Data and Analysis
• The Analysis
• Some Useful Routines for On-Line Data Analysis

... Высококачественный гитарный и инструментальный кабель . Кабель гитарный . ... Краски . В состав набора входит: Краска универсальная акриловая Folk Art, 59 мл . ... Цвет: серый . ... Цвет: . ... Термочувствительный участок не только меняет цвет, если пища слишком горячая (около 43C и выше), но и защищает десны и молочные зубы. ... Если цвет ложки изменился, остудите еду и промойте ложку под холодной водой. Повторяйте до тех пор, пока ложка не перестанет менять цвет. ...

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• Кабель гитарный Analysis-Plus - Analysis-Plus - Analysis-Plus Экраны Draper
• Браслет плетения "Двойной ромб" из серебра - Эстет - Эстет Конструктор Горный
• Цветок искусственный Home-Religion - Home-Religion - Home-Religion Цветок (76

... THE SIMPLEST MODEL. ... 13, Moscow 119992, Russia E-mail: san@sai.msu.ru Abstract: The analysis of the simplest model shows that an asteroid ­ rubble pile evolves, depending on the parameter V2d (where V is the average velocity of fragments and d is the average distance between fragments), either as a conglomerate of "independent mutually gravitating clusters" (when V2d < fm, where f is the gravitational constant and m is the average mass of a fragment) or as a "receding cluster" (when V2d > fm). ...

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• Родионова Жанна Федоровна
• Zhanna F. Rodionova

Dr. Victoria I. Prokhorenko . ... Situation Analysis of The "PROGNOZ" Orbit for Solar- Terrestrial Space Experiments. ... Studies of Satellite Situations Mission. ... A Situation Analysis of the Orbits of the Tail and Auroral Probes in the "INTERBALL" Project. ... Specific Tasks of Multiple Scale Plasma Measurement in Regatta- Cluster System (co-authors S. Savin and L. Zelenyi)- In Book: Proceedings of an International Workshop on Space Plasma Physics Investigations by Cluster and Regatta. ...

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• Wavelet Analysis
• Analysis methods in space physics (Oulu)
• Oulu Space Physics Textbook

Добро пожаловать, Гость . ... В теме В разделе По форуму . ... Темы, интересные всем ? Новости астрономии и космонавтики (Модераторы: Karen , recarrion , LeMay ) ? Einstein@Home S3 Analysis Summary . предыдущая тема следующая тема . ... 0 Пользователей и 1 Гость просматривают эту тему. Гость . ... Появился долгожданный отчет об анализе данных LIGO в конфигурации Science Run 3 (S3), выполненого в рамках проекта Einstein@Home: . ... Ответ #1 : 13.09.2005 [10:44:22] ? ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Last modified . ... 2011-06-09 11:56 . ... 860K . ... 835K . ... Last Revised: 2013 April 25th . ...

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• Abstract 200
• C.J. Butler, Research Astronomer
• DIRECT MASSES FOR BXCIR AND PVTEL VARIABLES

Kholtygin A.F., Shneiwais A.B. Stochastic Data in Astronomy: Fourier Analasis of Strongly Unevaen Time Series . Astrophysics, 48 , 87-100 ( 2005 ) . A detail analysis of the CLEAN algorithm for strongly uneven time series is given. ... The results of our analysis are used for searАhing the harmonic components in line profile variations in the spectra of O8III star lambda Ori A obtained in 2001 with 1 m telescope of the Special Astrophisical Observatory of the Russian Academy of Science. ...

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• Analysis of AstrophysiАal Data
• Wavelet Analysis
• Fourier Analysis

... The large body of near infrared observations presented in Testi et al. (1997; 1998) are analysed with the aim of characterizing the young stellar clusters surrounding Herbig Ae/Be stars. The results confirm the tendency of early Be stars to be surrounded by dense clusters of lower mass "companions", while Ae stars are never found to be associated with conspicuous groups. ... Only the most massive stars (10-20Msun) are found to be associated with dense (10^3 pc^-3) stellar clusters. ...

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• Analysis of the Ext2fs structure
• Traffic Analysis for ge-0/0/3 -- arcrt1
• A homogeneous chemical analysis of the inner Galactic disk from the first data

Next: The STScI NICMOS Calibration Up: No Title Previous: CONICA: The high resolution . The STScI NICMOS Calibration Pipeline . Introduction . ... Dark Current Subtraction . ... Input Data . ... Scalar Background Subtraction . 2-D Background Subtraction . ... Status and Goals of the NICMOS Calibration Plan . ... Photometry . ... Photometric Performance of NICMOS . ... NICMOS Photometry. ... ST-ECF Grism Spectrum Software for NICMOS Grism Data . ... Analysis . ... STScI NICMOS Software . ...

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• STScI NICMOS Software
• ADASS '97 Program Information
• ADASS '97 Report

... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... 10 (IAUC # 4742) 2/25 13.3 16 j 2/27 13.5(*) 18 lc 2/28 13.8 19 p 3/1 13.2 20 w 3/2 13.5 21 a 3/4 13.8 23 p 3/6 13.3 25 c 3/7 13.3 26 c 3/8 14.1 27 m 3/8 13.3 27 r 3/9 13.4 28 c 3/9 14.1 28 m 3/10 13.6 29 j 3/10 14.0 29 a 3/11 13.6 30 c 3/11 13.5 30 r 3/11 13.7 30 s 3/13 [13.69 CCD Mag.] ...

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... Which sign do you think will have the greatest number of Presidents? ... How many Presidents' birthdays fall under each of the Zodiac signs? ... Which sign has the largest number of Presidents? How many? ... Which sign has the smallest number of Presidents? ... Would you say the birth dates of the Presidents are strongly clustered in one or a few signs? . ...

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... A method to detect non-radial pulsations of CP stars is suggested. ... The opportunity is noted to get an information on spatial structure of non-radial oscillations from the analysis of radial velocities of chemical element lines, concentrated in the spots. To detect and identify the modes of non-radial oscillations of average grades it is suggested to use the methods of line profile analysis applying thee to the lines observed in the local spots on the stellar surface. ...

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• http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p76-p76.pdf
• Spectral energy distribution

... Singular value decomposition of the matrix A is (a) it's decomposition into singularities (b) it's Fourier transform (c) finding the rotation, which transforms it to diagonal form (d) solution of the eigenvalues problem 4. ... Matrix invertion can be calculated by (a) Matlab (b) dividing by determinant (c) calculation of algebraic complements, traslation and dividing by determinant (d) calculation of minors, traslation and dividing by determinant 2 ...

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• Leonid Zotov
• Trudy GAISH, vol. LXV, 1996, Abstracts in English
• Marat Abubekerov - publications list

... ursa in Unknown (configure /etc/snmp/snmpd.local.conf) . ... Max Speed: . ... at which time 'ursa' had been up for 233 days, 1:27:12 . Max . Average . Current . ... 90.0 kB/s (0.4%) . ... 152.0 kB/s (0.6%) . ... 144.0 kB/s (0.6%) . ... Incoming Traffic in Bytes per Second . ... Outgoing Traffic in Bytes per Second . ...

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• Traffic Analysis for ursa (UARNET)

Next: The equilibrium period Up: Evolution of Magnetic Rotators Previous: Evolution of Magnetic Rotators . Analysis of the nature of interaction of a magnetized star with the surrounding plasma allows us to write an approximate evolution equation for the angular momentum of a magnetic rotator in the general form (Lipunov, 1982a[ 98 ]) . where is a specific angular momentum applied by the accretion matter to the rotator. ... The evolution equation ( 4.10.2 ) is approximate. ...

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• The Effect of Relativistic Wind on Accretion Flow Parameters
• Seminars
• Evolutionary Tracks

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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• XV-SPEC
• XV-IMAGE

... Field of interest: data analysis and interpretation of X-ray observations of BHC and NS systems, astrophysics of compact objects and related phenomena: X-ray , optical and radio observations , shocks and stellar winds, emission mechanism, the spectral and timing analysis of the X-ray emission from microquasars ( signature of accreting BH), atoll- and Z-sources ( signature of accreting NS), modeling of INTEGRAL images % . ...

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• Victor Oknyanskij

... Perl . ... IDL is used for data analysis and graphics. ... Advantages of a language that is popular in the real world are the existence of web resources such as tutorials, a wide range of libraries of existing code you can use and modify, and better job prospects for you if you ever want to venture into the real world. ... Most data reduction systems (eg IRAF, MIDAS, Starlink) do not interface well with any programming language: IRAF has itуs own (very clunky) language in which you can write scripts...

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• Raquel Salmeron - Research Interests and Experience
• Marc White - Astrophysicist - The Australian National University

MATHEMATICAL MODELING: . ... This model is developed on the base of the probabilistic description of the collisional aeronomical processes and is realized on a computer as the numerical system (stochastic model). ... Shematovich, V.I., Bisikalo , D.V.             Nonequilibrium processes in the planetary and cometary atmospheres. ... In Russian) . ... Piarnpuu , A. A.; and Shematovich, V. I.       Construction of structural stochastic models of collision processes in rarefied gas media (abstract) . ...

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• Project: PAHs

MINUTES of the RadioAstron Teleconference on December 13, 2011 Yu.Yu. ... IOC status update M. Popov informed the participants on the current IOC results. ... Kovalev added: we continue to observe pulsars and spectral line sources in radiointerferometer mode but only with spacecraft and we are also going to observing pulsars soon with space-ground baselines. ... Kovalev: It is fringe-fitting result. ... In RAFS05 we replace it with K-band observing (maser source Ori KL ­ spectral lines ~100000Jy). ...

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• http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2014,52,391.pdf
• Dubovikov Mikhail Mikhailovich, Astro Space Center (ASC)