... According to the most popular cosmological paradigm, the greater part of the galaxy mass is accumulated in the dark matter halo. ... The polar ring galaxies (PRGs) reveal external rings or disks of gas, dust and stars rotating in a plane roughly perpendicular to the disk of the central galaxy. ... The shape of the dark halo in the model was chosen so as to achieve the best fit to the observed rotation of both galaxies themselves and their polar rings. ... The SPRC-7 galaxy. ...

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• Geodetic measurements group

... Posts tagged ?measurement error? ... Measurement error is ? ... This is how statisticians seem to use it, essentially the bias term. ... Category: Astro , Cross-Cultural , Jargon , Stat , Uncertainty | 8 Comments . ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

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• The AstroStat Slog Blog Archive [ArXiv] Swift and XMM measurement errors, Sep.
• The AstroStat Slog Blog Archive my first AAS. V. measurement error and EM
• Comments on: my first AAS. V. measurement error and EM By: jiangang

... Class . ... ij.plugin. AboutBox (implements ij.plugin. ... BatchConverter (implements java.awt.event.ActionListener, ij.plugin. ... BatchProcesser (implements java.awt.event.ActionListener, java.awt.event.ItemListener, ij.plugin. ... CommandFinder (implements java.awt.event.ActionListener, java.awt.event.ItemListener, java.awt.event.KeyListener, java.awt.event.MouseListener, ij.plugin. ... ImageJ_Updater (implements ij.plugin. ... LUT_Editor (implements java.awt.event.ActionListener, ij.plugin. ...

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• ij.measure Class Hierarchy (ImageJ API)
• ij.macro Class Hierarchy (ImageJ API)
• Class Hierarchy (ImageJ API)

Sloan Digital Sky Survey Telescope Technical Note 19970728 Edward J. Mannery and Walter Siegmund . ... Common corrector mount inspection . ... The corrector nearest the secondary mirror, the common corrector (so named because it is common to both imaging and spectroscopic configuations) is located with respect to the telescope optics support structure by the common corrector mount. ... The fused silica common corrector is 32.5 inches in diameter and is 0.47 inches thick. ...

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• Measurements of 3.5-m Secondary Mirror Motions
• Shack_Hartmann Measurements on the APO 3.5m Telescope
• Primary Mirror Measurements

... 18-1 74 40.5 0.52 Cas A . 18-1 75 38.5 0.49 Cyg A . ...

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• Description of the RadioAstron project, english version

... On-line Data . ... Binary speckle measurements at Calar Alto. I. (Docobo+, 2001) . ... 33660868D We present the first results of our speckle interferometric measurements of binary stars made with the ICCD speckle camera using the 1.52-m telescope of the Observatorio Astronomico Nacional at Calar Alto (Spain) in September, 1999. ... We have used there new speckle measurements to improve the orbital elements for the binaries COU 247 and BU 524 AB. (1 data file). ... Keywords (in text query field) . ...

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• Speckle Measurements with the New Camera of the Astronomical Observatory R. M.
• Results scientific researchs 15
• Scientific seminar of the SSLab Stellar Spectroscopy Laboratory

... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

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• Methods and instruments, general issues
• Results of recent and ongoing site programs
• Media files

... In spite of the good potential possibilities, some of the station "Dnepr" design characteristics did not allow us to apply the usual special IS radar measurement methods. ... Thus for IS signal measurements at the "Dnepr" station, we have developed special methods for recording and processing IS signals in order to determine plasma ionospheric parameters. ... Equations (4-5) from the basis for data post processing to obtain ionosphere parameters. ...

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• East Siberian Center for the Earth's Ionosphere Research. Modernization...

. Webcams . Networking . Weather . Power . System health . Measurements . Seeing at Sun Apr 10 00:24:00 2016 is Unknown . Copyright 2007 2013.

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• . The . MASS . Group .

... 314 Astronomical Data Analysis Software and Systems XIII, eds. F. Ochsenbein, M. Allen, & D. Egret (San Francisco: ASP), 720 . ... The Combined Array for Research in Millimeter-wave Astronomy (CARMA) will be the combination of the BIMA, OVRO, and SZA millimeter arrays, at a new high elevation site (7200', 2200 m). ... CARMA's monitoring system (CAM), is designed to collect monitor data periodically from a set of heterogenous systems and organize these monitor points hierarchically. ...

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• AstroRoute
• Chandra Ground Calibration Raytrace Database and Simulator
• ADASS 2002 Conference Proceedings

Ref: ALMA band 1 horn measures Date: 27/08/2002 Technical note ALMA band n.1 horn measurements Author: Renzo Nesti Summary This document is intended to give pattern and return loss measurements of the ALMA band n.1 horn (31.3-45 GHz) produced by CLOEMA and designed by MECSA and Arcetri. ... Because the measurements have been made by rotating the horn under test on the expected phase centre we conclude that the estimation of the phase centre position does agree well with tests. ...

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• http://www.arcetri.astro.it/~nesti/pdfs/ALMA%20band%202%20horn%20measures.pdf
• NGC1068 (Abstract)
• Microwave Holography of Radioastronomical Antennas

... Spectral regions highlighted by green bars have been used to detemine the тЯиB z тЯй value from H Balmer lines, and the magenta bars highlight the spectral regions used to estimate the magnetic field from metal lines. ... The FORS1 instrument of the ESO Very Large Telescope was used to obtain low resolution circular polarized spectra of nearly a thousand of different stars, with the aim of measuring their mean longitudinal magnetic fields. ...

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• Abstract 192
• CONCLUSIONS
• Conference 98

A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...

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• SPECTROPHOTOMETER FAGOT
• SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM
• HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11

. Webcams . Networking . Weather . Power . System health . Measurements . Seeing at Sat Apr 9 22:26:00 2016 is Unknown . Copyright 2007 2013.

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... Brown University - Vernadsky Institute Microsymposium 38, October 27-29, 2003, Moscow, Russia . ... Moscow State University, Vorobjovy Gory, 119899, Moscow, Russia, gray_pigeon@mail.ru . ... Sternberg State Astronomical Institute, 119899, Moscow, Russia. ... Brown University - Vernadsky Institute Microsymposium 40, 2004, Moscow, Russia . ... Brown University - Vernadsky Institute Microsymposium 42, October 10-12, 2005, Moscow, Russia . ...

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• Gregory G. Michael

Number of spectral channels . ... Spectral channels MSU-SK #1 (#2): . ... 0,54-0,60 (0,54-0,59) µm . ... Ground Resoultion I-IV/V channels . ... Scanning Rate I-IV/V channels . ... Radiation Temperature Measurement Range in Channel V . ... Instrument Error for Radiation Temperatute Measurement in Channel V . ... Ground resolution corresponds to normal flihgt altitude 650 km. For more information send a mail to: info@sputnik.infospace.ru . ...

17. Hot links of Comet WWW site

18. http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/hobbes/incoming/units-os2-2_02.txt

19. MSSA results

20. General Catalogue of Variable Stars: What's new.