. Departement of Quantum Astrophysics . Head: Kurt V.G. , Prof. ultraviolet spectroscopy of planetary upper atmospheres and interplanetary/interstellar medium; . observations of gamma-bursts and optical identification of their sources; . long-base optical interferometry. Staff: .

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• Theoretical Astrophysics Department

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... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...

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• Galaxy sector, archive 1994
• The study of star formation in KDG61 and KDG64
• Solar system sector, archive 1998

Uranus . ... Miranda . ... 1998 image from HST showing bright clouds html . ... Two views of Uranus' darkspot 107k gif ; 40k jpg . normal and false color views 102k gif ; 40k jpg . ... Infrared image of Uranus B 33k gif . Infrared image of Uranus 2 B 37k gif . Infrared image of Uranus 3 B 56k gif . ... Infrared image of Uranus 5 B 43k gif . Infrared image of Uranus 6 B 34k gif . Infrared image of Uranus 7 B 36k gif . ... Uranus' rings (false color) 78k gif ; 35k jpg ; 211k gif . ...

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• Misc Planetary Picture List
• The Polar Aurora
• Venus Picture List

Jennie Jenkins Will you wear white, oh my dear, oh my dear Oh will you wear white, Jennie Jenkins? I won't wear white For the color 's too bright I'll buy me a fol-de-roldy-tildy-toddy seek-a-double, use-a-cause-a-roll-the-find-me Roll, Jennie Jenkins , roll Will you wear blue , my dear , oh my dear Oh, wear you blue , Jennie Jenkins I won't wear blue The color 's too true Will you wear red, my dear , oh my dear Oh will you wear red, Jennie Jenkins I ...

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• http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/z/zombies/shes_not_there
• http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/g/grant.amy/bridegroom
• http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/s/simon.paul/kodachrome

... Bad Astronomy . ... Mad Science . ... Are colored dwarfs actually colored or are they different kinds of stars? ... Therefore a white dwarf is very bright, and a brown dwarf is very dark. ... Brown dwarfs are a newly discovered type of object, which are midway between stars and planets. ... Several brown dwarfs have been recently discovered orbiting normal stars; you can find more about them at one of my favorite web sites, The Nine Planets , on the page called "Other Solar Systems?" ...

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• Phil Plait's Bad Astronomy: Bitesize Astronomy
• Phil Plait's Bad Astronomy: Misconceptions
• Phil Plait's Bad Astronomy: Misconceptions: What Color is Mars?

... A detailed study of two consecutive bright points observed simultaneously with CDS, EIT and MDI is presented. The analysis of the evolution of the photospheric magnetic features and their coronal counterpart shows that there is a linear dependence between the EIT Fe XII 195? flux and the total magnetic flux of the photospheric bipolarity. ... In a follow-up study, we used wide slit (90arcsec240arcsec) movies of four EIT coronal bright points (BPs) obtained with CDS. ...

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• Coronal Bright Points: Another Oscillating Environment
• Armagh Observatory
• Melotte15 Inside The Heart Nebula | International Year of Astronomy in Ireland

Astronomical Data Analysis Software and Systems X ASP Conference Series, Vol. ... F. A. Primini, and H. E. Payne, eds. ATV: An Image-Display To ol for IDL Aaron J. Barth Harvard-Smithsonian Center for Astrophysics Abstract. ... It works equally well under the Unix, Linux, Windows, and MacOS versions of IDL, and includes features such as interactive control of color stretch, zoom, and image scaling; image blinking; and creation of publication-quality PostScript output. ... 386 Barth Figure 1. window. ...

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• ATV: An Image-Display Tool for IDL
• Recreating Einstein Level One Processing Exposure Masks and Background Maps in
• See Spike Run... Run, Spike, Run

... Package . Class . ... PREV PACKAGE NEXT PACKAGE . FRAMES NO FRAMES All Classes . Class Summary . ... Displays the ImageJ Channels window. ... Implements the Image/Color/Color Picker command. ... This plugin implements the Brightness/Contrast, Window/level and Color Balance commands, all in the Image/Adjust sub-menu. ... ImageJ plugin that does curve fitting using the modified CurveFitter class. ... Implements ImageJ's Paste Control window. ... This is ImageJ's macro recorder. ...

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• University of Louisville Wide Field and Planetary Telescopes
• Colors (ImageJ API)
• IJEventListener (ImageJ API)

... Astrophysics Group . ... Galaxy Formation and Evolution . Publications . ... Very extended cold gas, star formation and outflows in the halo of a bright quasar at z > 6? ,б C. Cicone, R. Maiolino, et al. ... Belfiore, R. Maiolino, K. Bundy et al. 2015,б MNRAS in press (arXiv:1410.7781) . ... 2014, MNRASб in press (arXiv:1409.4764) . ... The dependence of the galaxy mass-metallicity relation on environment and the implied metallicity of the IGM?б  , Y. Peng & R. Maiolino 2014, MNRAS 438, 262 . ...

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• ALMA Phase Calibration Techniques at the Cavendish Astrophysics Group
• Astrophysics Group Stars ? Birth and Death
• Astrophysics Group Surface Imaging of Betelgeuse

. eng || rus . Home . Projects . Research . Publications . Astronomy Letters . Conferences . SRG Project . RSDC . Contacts . Theory and observations . INTEGRAL All-sky survey . Bright X-Ray pulsars with INTEGRAL . X-ray survey for galaxy clusters using archival ROSAT observations 400 deg 2 cluster survey . Observations of gamma-ray burst afterglows with RTT150 telescope . Optical identifications of hard X-ray sources . 2016 IKI RAN

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• High Energy Astrophysics Today and Tomorrow
• INTEGRAL 9-year Galactic Survey

The Astronomy Shop . ... Shop | ... Cards | ... Sold in sets of 8 cards (two of each image) with envelopes in a Keepsake Wallet. ... Starbirth Clouds in M-16, Starbirth in the Trifid Nebula, Live Cycle of Stars in Galactic Nebula NGC 3603, and Inside the Lagoon Nebula. ... Majestic Spiral Galaxy NGC 4414, A Grazing Encounter of Two Spiral Galaxies, Infant Stars Ring Core of Galaxy NGC 4314, and Galactic Silhouettes. ... We have bulk pricing available. ... www.astronomy.net . About Astronomy Net | ...

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• You Can Make Stellar Images Brighter - an Astronomy Net Article
• Experiment With Font Color - an Astronomy Net Exploration Forum Message
• Color Filters - an Astronomy Net Eyepieces Forum Message

. Welcome to X-Ray WWW Server . at Sternberg Astronomical Institute . This page was designed by Sergey Nazin . Send questions and comments to leng@sai.msu.su

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• UBV light curves (van den Bergh, 1976)
• References
• color.sty

... Colors of Sunlight . S-4A.Color Expts. ... Here is your opportunity to demonstrate the three-color theory by using your computer. I am indebted for this to Joe Burns , on whose color demonstration file it is based. ... You see below two tables with colored fields. ... blue . ... D0FBFF gives the intensity of the three colors which make up the background: D0 is the intensity of red , FB is the intensity of green and the second FF is the intensity of blue , the maximum blue you can get. ...

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• The Many Colors of Sunlight
• Experimentando con los Colores
• The Polar Aurora

... The theater "U Nikitskikh Vorot" is located at the Nikitskiye Vorota (Nikita Gate) Square, at the intersection of the Nikitskiy (formerly Suvorovckiy) Boulevard and the Bolshaya Nikitskaya (formerly Gerzen) Street. ... 1) From "Arbatskaya" metro station (any of the two). ... Then walk for 5-6 minutes on the right side of the Nikitskiy Boulevard in the direction of the Pushkinskaya Square until you see the theater's front porch. ... BACK to "U Nikitskikh Vorot" theatre page . ...

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. The measuring unit of the electrical impedance tomograph. The belt with electrodes for measurements on thorax . The EIT animation reconstructed from the data measured on the volunteer's thorax: . Right . Anterior . The animation represents one respiratory cycle, the cardiac pulsations are visible also. The static visualization is demonstrated: 1 - spinal column, 2 and 3 - right and left lungs, 4 - heart. The brightest colors correspond to highest conductivity .

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• Actor Prolog. An Example of Web Agent Report.

... Meta Index / Home Page / Description xcolorcod provides a list of pre-defined color tables that is identical to the internal color maps of the image displayer Ds9 . ... LEVEL . ... RED . ... The table can also be regarded as defining three separate curves for the three basic colors red, green, and blue and piecewise linear interpolation is carried out for intermediate LEVEL values. ... 0 So a pixel with a scalar value of e.g. will be assigned a color with 50% red, 17% green, and no blue intensity. ...

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• XMM-Newton Trainee Project 2004
• Source lies near to a bright source - bit 6
• Analysis of very bright sources

The revision of the MASS/DIMM star catalogue N. Shatsky, V. Kornilov March 16, 2008 Abstract The compilation of the (updated) version of the MASS (MASS/DIMM) device target catalogue is described. ... Then the list was cleaned according to following criteria: I. Remove stars too faint for a MASS device. ... Here the color equation of the Sternb erg device was taken: M AS S mag = V mag + 0.45 (B - V ); stars with M AS S mag > 3.2 were removed. ... This was made based on the GCVS4.2 catalogue data. ...

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Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...

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• http://selena.sai.msu.ru/Shev/Publications/m44_75_shevchenko_etal.pdf
• http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf
• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

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