. Cosmology . Very Early Universe . Cosmic Microwave Background Anisotropy . Dark Matter Models . Large Scale Structure . High Energy Astrophysics . Active Galactic Nuclei . Astrophysics of Compact Objects . Accretion Disks . Scientific Staff:

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... Astrophysics Group . Research . Star Formation . ... Cosmic Microwave Background (CMB) . ... Galaxy Formation and Evolution . ... In particular, we study the supersonic jets ejected during the star formation process, and the accretion disks surrounding the protostars which allow the stars to grow in mass and in which planets are believed to form. ... Members of the group are also investigating the nature of star formation on galactic scales ? see the pages of the Galaxy Evolution group. ...

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• Astrophysics Group Cosmic Microwave Background (CMB)
• Astrophysics Group Main Projects
• Supernova Remnant (SNR) Catalogue or Catalog of Galactic SNRs

... You are here: start €Ё lbaops €Ё lbamar2008 €Ё v255a . ... VLBI Schedule . ... Observer's Wiki . ... Other VLBI . ... lbaops:lbamar2008:v255a . V255a Setup: . ... Channel 1 . IFP#1-LO 6641 - 6657 MHz USB RCP . ... Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v255/v255a . ... For Hobart the LOs should be set to 468 MHz (IFP#1) and 809 MHz (IFP#2) for the 4 x 16 MHz setup and 809 MHz for the 2 x 16 MHz setup. ... lbaops/lbamar2008/v255a.txt €§ Last modified: 2015/12/18 16:38 (external edit) . ...

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• lbaops:lbanov2008:v255c [ATNF VLBI Wiki]
• lbaops:lbadec2009:v255h [ATNF VLBI Wiki]
• lbaops:lbasep2009:v255f [ATNF VLBI Wiki]

... Using the self-consistent 3D hydrodynamical code in Kobayashi et al. (2007) , we simulate the star formation and chemical enrichment history of the Universe. ... We also predict the rates of supernovae and gamma-ray bursts, and the properties of the host galaxies, which will be observed with the ANU's new SkyMapper telescope. ... Supernova feedback on galaxy formation. ... Feedback from active-galactic nuclei (AGN). ... COALA : Universe Galaxy AGN Star Planet ...

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... Archives . ... Quote of the Week, Aug 31, 2007 . ArXiv] NGC 6397 Deep ACS Imaging, Aug. 29, 2007 . ... Comparison of decision tree methods for finding active objects by Y. Zhao and Y. Zhang . The authors (astronomers) introduced and summarized various decision three methods (REPTree, Random Tree, Decision Stump, Random Forest, J48, NBTree, and AdTree) to the astronomical community. ... Shortcomings of decision tree methods were also described. ... Chandra Blog . ... SAMSI AstroStat Prog. ...

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• Martin Elvis - Home Page
• The AstroStat Slog Blog Archive Background Subtraction, the Sequel [Eqn]
• The AstroStat Slog background

... Morning Session (10:00 am - 1:00 pm) . Invited reviews (40 minutes, including discussion) . ... The Cosmic Microwave Background: Recent Results and Interpretation . ... Joint Discussion (25 minutes talks, including discussion) . 14:30 Early Evolution in the Universe . ... Developments in General Relativity: Black Hole Singularity and Beyond . ... The Highest Energy Cosmic Rays, Gamma Rays and Neutrinos . ... Theoretical Aspects of Ultra High Energy Cosmic Ray Origin and Propagation . ...

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• The Arcetri Spectral Code - E.Landi and M.Landini (1998)
• event - Apache HTTP Server
• Arcetri Star-Formation Group Publications

. 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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• Cosmion-2001
• ADS Abstract Service Results
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. This document is designed to be viewed using Netscape later 5.0 `s Frame features. If you are seeing this message, you are using a frame challenged browser.

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XMM-Newton Science Analysis System . ... The exposure maps suffer from a minor potential double-counting error. If a bad pixel is not known to the DPP, and is not present in the telemetry, and is of the variety that tends to be hot, then it is possible that it has been rejected on-board. Such bad pixels effectively subtract twice their active time from the map, once as an individual bad pixel, and again in the fractional exposure applied to the entire node. XMM-Newton SOC/SSC -- 2006-06-28 ...

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Galaxies are diffuse objects which are imaged against a background of finite brightness and noise. Galaxies which have the maximum contrast with respect to this background are the ones that are first discovered. ... These galaxies have been missed to date but active surveys for them are underway. ... In this page we present several examples of these newly discovered Low Surface Brightness galaxies as well as examples of high surface brightness galaxies. ...

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• Galaxy Gallery Page IV: The Movies
• Astro-2 and the UIT Experiment

. R=4.7k-10 kOhm . Ca=Cc=2*Cb . Cb=Cd=1/(2*sqr(2)*pi*Fc*R) . Units: R [Ohm], Cx [F], Fc [Hz] . Contributor: Joakim жgren Source: ? Please send any comments to Joakim жgren .

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• HwB: Active Filter: Butterworth 12dB Highpass
• HwB: Active Filter: Butterworth 6dB Highpass
• HwB: Active Filter: Butterworth 6dB Lowpass

Next: Code II: Unknown Up: Image Restorations of High Previous: Construction of Algorithms . ... The positions of the designated point sources ( ) must be given as well as initial amplitudes for and . ... The integrated flux of the point sources ( ) plus that of the distributed emission ( ) is constrained to equal that of the observed image ( ). ... This is investigated in Fig. 1 where all emission derives from point sources but only one - the brightest - is designated as such. ...

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• Hubble Science Legacy Workshop Program
• Comments [Comments]
• STScI Active Galaxies Lunch Talk Series

... Астронет | ... планета Астронет | ... S. Alba Villegas; R. Freire Ferrero . ... New insights on late-A and early-F star activity . ... Formation and stability of the galactic shock waves . ... Dispersion of electromagnetic waves in active moving plasma . ... N. G. Bochkarev; A. N. Burenkov; A. I. Shapovalova . ... The luminosity function of quasars (active galactic nuclei) in a merging model with the eddington limit taken into account . ... About the euro-asian astronomical society . ...

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• Active Galaxy NGC 1275
• Астронет > Active Galaxy NGC 1275
• NGC 3603: An Active Star Cluster

Main Program Travel Where to go in Moscow Information . ... The 2014 year marks the 100th anniversary of Yakov Zeldovich . ... John Carlstrom (University of Chicago) . ... Lyman Page (Princeton University) . ... The conference will be held at the Space Research Institute (IKI) in Moscow, Russia, on June 16-20, 2014 . ... International Conference: Cosmology and High Energy Astrophysics (Zeldovich-90) 20-24 Dec 2004, Moscow, Russia . ... 2014 Space Research Institute, Moscow Русская версия ...

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• Kvant Astrophysical module
• Zeldovich-90: COSMOLOGY AND HIGH ENERGY ASTROPHYSICS
• Астрофизические ссылки

... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

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• astro-ph abstracts (body) search for 'dichotomy' all years (1992-2001)
• astro-ph authors/title/abstract search for 'galaxy cluster' (skipped 200) all
• astro-ph abstracts (body) search for 'high redshift radio ' all years

... The department was founded in late sixties by Prof. D.Ya.Martynov, who for many years was also the director of Sternberg Astronomical Institute. At present time, the head of the department is Prof. A.M.Cherepashchuk, a pupil of D.Ya.Martynov and his successor as the director of SAI. Since Prof. Martynov, the scientific activity of the department was primarily related to binary stars. ... The department consists of 15 members most of which have Ph.D. in Astrophysics. ...

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... The Search for Stellar Origins from Antiquity to the 21st Century . Dr. Charles Lada, Harvard-Smithsonian Center for Astrophysics . ... In this talk, "The Search for Stellar Origins from Antiquity to the 21st Century," Dr. Lada will explore the question of why it took so long for star formation to become an active branch of astronomical research. ... ground-based and space-based telescopes. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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... Tonight's Sky . ... Sky this Month . ... Astronomy for Kids . ... Hubble sees NGC 7090 т?? an active star-forming galaxy . ... This image portrays a beautiful view of the galaxy NGC 7090, as seen by the NASA/ESA Hubble Space Telescope. ... This image portrays a beautiful view of galaxy NGC 7090, as seen by the NASA/ESA Hubble Space Telescope. ... These structures trace the location of ongoing star formation, visual confirmation of recent studies that classify NGC 7090 as an active star-forming...

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• Overfed black holes shut down galactic star-making | Astronomy.com
• Active supermassive black holes revealed in merging galaxies | Astronomy.com
• A new type of active galaxy | Astronomy.com

At the National and International level, NAIC's interest is well represented by Dr. Thomas Gergeley (Electromagnetic Spectrum Manager, NSF ), Dr. Donald Backer (Chairman of CORF ), Dr. Darrel T. Emerson (Chairman of IUCAF ). ... NAIC also takes active part through filling comments in all relevant public proceedings of the Federal Communications Commission ( FCC ). ... NAIC's interference guidelines as per PRCZ. A text version of FCC's Report and Order for establishing the PRCZ. ...

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• Proposed E-ALFA Organizational Structure
• ASPH 405: Extragalactic Astrophysics, Winter 1999