... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Finding the Bivariate Brightness Distribution of galaxies from an H I selected sample . ... A method is presented that will enable the bivariate luminosity/surface brightness distribution of galaxies to be determined from a relatively small H I selected sample. ... PICASSO - an automated galaxy finder . ...

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• HIPASS Bright Galaxy Catalog
• The HIPASS Bright Galaxy Catalog
• livedata / gridzilla distribution

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• Physics 410/510 Observational Cosmology

. Below are links to the theoretical energy distributions of WR stars included in the database of Leitherer et al. (1996; PASP, 108, 996). You can use the links below to read a description of the models (Readme file), and to download the files. Readme file . ftp directory with the individual files All data available for mass FTP at: . ftp ftp.stsci.edu login anonymous password your username cd science/starburst/Schmutz . Last update: December 15, 2001 - Claus Leitherer

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• Spectral Energy Distributions for Massive-star Populations
• STScI Preprint #1290
• NICMOS Parallel Program

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2010 December 27 . One Million Galaxies . Credit: 2MASS , T. H. Jarrett , J. Carpenter, R. Hurt . ... Many galaxies are gravitationally bound together to form clusters , which themselves are loosely bound into superclusters , which in turn are sometimes seen to align over even larger scale structures . ... About APOD | ...

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• The Network Time Protocol (NTP) Distribution
• APOD: 2001 December 6 - Comet Linear (WM1) Brightens
• APOD: 2015 December 11 - The Brightest Spot on Ceres

... The best annual meteor shower is the Geminids, which are expected to peak this year on December 13th at 18h. Some activity will persist until about Dec 15/16. Unfortunately this year's display will be spoiled by a Full Moon at maximum, but you should still see some of the brighter meteors. ... This is a live count of meteor showers based on visual data entered through the IMO electronic report form. ... Saturday, 13 December 2008 19:03 . International Year of Astronomy, Ireland National Node . ...

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• Geminid Meteors
• Armagh Observatory
• Doppler Imaging and Flare Activity on HR1099

... A clear description of El Nino Southern Oscillation and of its consequence on climate in Australia and South America is available at El Nino or ENSO theme pages of the NOAA climate diagnosis center. ( historical comparison of previous elninos with soi indices ) . This image shows cold water upwelling near the coast of Peru (purple) and joining the South Equatorial Current, which flows westward across the Pacific Ocean. ... July 16, 1998 : Satellite image shows pacific stabilizing . ...

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• ESO - About the Science Newsletter
• ESO - ESO-MIDAS Releases and Distribution
• ESO - Science Announcements

... V838 Mon is a member of a new class of eruptive variables which appear as a peculiar novae having late K-M type spectra in their outburst. Before its outburst, it was a wide binary system of B3V type stars. ... The B3V companion was seen in the outburst in the UV spectrum taken with HST (Rauch et al., ... In the latest spectra, the light of B3V companion was predominating in the short-wave photometric bands. ... CCD blue frames of V838 Mon before the eclipse (left) and in the eclipse (right). ...

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• Observational data and reduction
• Spectral energy distribution

ALMA | ... Phase Correction Algorithms | ... On this page, we describe what the phase correction algorithms set out to do and the framework we have developed to optimally use all of the available information. ... We are developing a Bayesian framework to combine all the information we have about the current and future meterological conditions (which are naturally accommodated as priors in a Bayesian scheme) with detailed physical models of the atmosphere. ...

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• Inference of Coefficients for Use in Phase Correction
• Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages
• NVSS Image ftp service (5 August 1998)

... Posts tagged ?Maxwell distribution? Dec 7th, 2007| 03:15 pm | ... There?s only one day in the first week of December with no preprint appearance. Dubbing the week of Dec. 2nd as the first week is hoped to be accepted. ... ArXiv] 1st week, Dec. ... Tags: CMB , cosmic shear , cross-correlation , Hubble constant , Maxwell distribution , Point Process , PSF , SZ , wavelet , X-Atlas . ... Comment . ... Entries RSS . ... vlk on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

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• PAUL J. GREEN - Peer Instruction
• The AstroStat Slog Blog Archive [ArXiv] Pareto Distribution
• SAO Summer Intern Program Projects, 2004

EPIC MOS response Steve Sembay, R.D. Saxton 10 December 2004 1 CCF components Name of CCF VALDATE EVALDATE Blocks changed XSCS ag EMOS1 REDIST 0043.CCF 1999-12-10 2000-07-15 CCD REDISTRIBUTION-n NO EMOS1 REDIST 0044.CCF 2000-07-15 2000-11-09 CCD REDISTRIBUTION-n NO EMOS1 REDIST 0045.CCF 2000-11-09 2001-04-18 CCD REDISTRIBUTION-n NO EMOS1 REDIST 0046.CCF 2001-04-18 2001-08-18 CCD ... This release contains a new set of CCFs which enable rmfgen to generate the correct rmfs. ...

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• Description

. Rus . Eng . Sun images . Magnetic storms online . Sun flares . Geomagnetic activity forecast . Active areas . December : 2007 . mo . tu . we . th . fr . st . su . 1 . 2 . 3 . 4 . 5 . 6 . 7 . 8 . 9 . 10 . 11 . 12 . 13 . 14 . 15 . 16 . 17 . 18 . 19 . 20 . 21 . 22 . 23 . 24 . 25 . 26 . 27 . 28 . 29 . 30 . 31 . No data available . 1953-2016 Laboratory of X-ray astronomy of the Sun, LPI RAS, Russia . Tel.:+7(499)132-65-96, Fax: +7(499)132-65-97 . Design WEBMASTERA.ru .

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• Latest images of the Sun December 11, 2006
• Latest images of the Sun December 01, 2015
• Latest images of the Sun December 11, 2005

... The MIDAS system is available, free of charge, to all non--profit research institutes, whereas other organisations or companies may be charged a nominal fee to cover distribution. Institutes interested in using MIDAS must sign a User Agreement before they receive MIDAS. The necessary forms can be obtained by contacting the Data Analysis Group at ESO/Munich. ... The current system at ESO/Munich is frozen several months prior to the official release. ...

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• Distribution
• Some statistical trends and distributions
• Module Index - Apache HTTP Server

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

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... 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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• Detection of unique bright radio flare of X-ray binary
• interests_kolya_en
• Galaxy sector, archive 2014

XmCCD ----- This distribution includes source code to utilize the Santa Barbara Instrument Group (SBIG) udrv.a library with a Motif-based graphical user interface camera control program. The version of the library also included here is udrv4.0 dated 28 December 2001, provided by Steve Ashe (ashe@dimensional.com and http://dimensional.com/~ashe/) through ftp.dimensional.com/users/ashe . Since the driver and camera control protocols are proprietary, source code is not available for the library. ...

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• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-5.1/README
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-2.0/DEVELOPMENT
• University of Louisville Wide Field and Planetary Telescopes

... Modern aspects of statistical physics and its applications. The seminar welcomes survey talks by senior researchers for the student audience and, more importantly, talks by students of undergraduate and graduate level on their research in progress. ... Olga STETIUKHINA, MSU Math. ... Anna BODROVA, MSU Physics Dept : Size distribution of particles in the rings of Saturn . ... Misha TAMM, MSU Physics Dept : A queue model (continued) . ... Misha TAMM, MSU Physics Dept : A queue model . ...

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• Distributions and Sobolev spaces (Spring 2003)

SDSS CONSTRUCTION ACTIVITIES . ... Construction Punch List: December 27, 1999 . Detail Views of Roof Attachments: December 22, 1999 . ... HVAC and Hoist Work: December 13, 1999 . Moving the Loft: December 6, 1999 . ... Quick Shots of Loft Installation: December 6, 1999 . ... Loft Preparation for Installation: December 1, 1999 . Moving Loft for Prep Work: November 29, 1999 . ... Construction Tarp Installation; Part 2: November 5, 1999 . ... HVAC Installation; Part 3: October 7, 1999 . ...

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• Other Sources of Information

As in the last years, the Ephemerides of Minor Planets for 2015 are prepared by the IAA RAS only in the electronic form. ... Orbital elements of all numbered planets have been determined in IAA all over again on the ground of available observations in the catalog of the Minor Planet Center. ... More detailed information on orbital elements used in the present volume of EMP and their accuracy is given in section "Information on new orbital elements". ... a) information on new orbital elements; . ...

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Next: Search and Retrieval of the AXAF Data Archive on the Web using Java . ... ESA Villafranca . ... The International Ultraviolet Explorer (IUE) mission has produced a large collection of spectroscopic data containing about 104,000 spectra of ca. 9,600 different objects. ... This contribution describes the IUEFA project at Villafranca, and the plans to make the archive available to the scientific community under through the INES (IUE New Extracted Spectra) project. ... Data set . ... 2D spectra . ...

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• Starlink's Software Distribution System
• Indexing and Searching Distributed Astronomical Data Archives
• Distribution of the OPUS Data Processing System

... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

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• http://www.izmiran.rssi.ru/~obridko/papers/313.pdf
• Heliophysical Laboratory of IZMIRAN (Solar-Terrestrial Physics Division)
• О.Г. Бадалян, Г.В. Куклин, В.Н. Обридко