... 11.03.1996 . ... A stunning map of this distant, diminutive planet , the first based on direct images, was revealed late last week in a Hubble Space Telescope press release . Above are two opposite hemisphere views of the computer constructed map of Pluto's surface (north is up). ... The map is based on Hubble images made when Pluto was a mere 3 billion miles distant. ... Publications with keywords: Pluto - Hubble space telescope . Publications with words: Pluto - Hubble space telescope . ...

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• Астронет > Hubble Telescope Maps Pluto
• XWare > APOD

... March 11, 1996 . Hubble Telescope Maps Pluto . Credit: A. Stern ( SwRI ), M. Buie ( Lowell Observatory ), NASA , ESA , . ... A stunning map of this distant, diminutive planet , the first based on direct images, was revealed late last week in a Hubble Space Telescope press release . Above are two opposite hemisphere views of the computer constructed map of Pluto's surface (north is up). ... The map is based on Hubble images made when Pluto was a mere 3 billion miles distant. ...

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• APOD: 2002 March 6 - Simulated Galaxy Cluster View
• APOD: 2008 April 28 - Star Forming Region NGC 3582
• APOD: 2013 June 11 - Star Forming Region NGC 3582

... Ignacio Ugarte Urra's PhD thesis topic is the investigation of coronal bright points. In his first paper (in collaboration with Gerry Doyle and Maria Madjarska) he investigated the formation, evolution and decay of a coronal bright point via a spectroscopic analysis of its transition region counterpart and the evolution of the underlying magnetic bipole during 3 days of almost continuous observations. ... In general the bright point has a radiance 4 times higher than that of the network. ...

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• All Ireland Computer Grid
• The Electron Pressure Differential between the Sunspot Plume and the
• M.D. Smith, Research Astronomer

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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• Researches of Astronomy and Space Physics Department
• Explanations to ephemeris for physical observation of the planets for Computer
• Lunar physical observations. Explanations for Computer Ephemeris.

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Computing: Getting started guide [internal access] . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... THE INTERNAL KINEMATICS OF THE MOST LUMINOUS H II REGIONS IN M100 . ... Keywords: ISM: H II regions, ISM: kinematics and dinamics, galaxies: ISM, galaxies: spiral . ...

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• An investigation of the molecular clouds of the Carina HII region/molecular
• Every cloud has a translucent region
• QUANTIFYING THE IONIZING FLUX ESCAPING FROM THE ULTRA-LUMINOUS H II REGIONS IN

EMBARGOED UNTIL: 9:20 AM CST, January 6, 1999 CONTACT: John Biretta Space Telecsope Science Institute, Baltimore, MD (Phone: (410) 338-4917; Internet: biretta@stsci.edu) HUBBLE DETECTS FASTER-THAN-LIGHT MOTION IN GALAXY M87 Astronomers reported today discovering clouds which appear to move many times faster than the speed of light, shooting out from the region of a black hole at the center of the M87 galaxy. ... It's an illusion created by the finite speed of light and rapid motion," Biretta said. ...

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• LABOCA observations of giant molecular clouds in the southwest region of the
• WFPC2 Bright Star Avoidance Regions
• HST Spectral Maps of Accretion Disks in Cataclysmic Binaries

... Pluto's orbit is also highly inclined -- tilted 17 degrees to the orbital plane of the other planets. ... Ground-based observations indicate that Pluto's surface is covered with methane ice and that there is a thin atmosphere that might freeze and fall to the surface as the planet moves away from the Sun. ... This is the first image-based surface map of the solar system's most remote planet, Pluto. ... This is the first surface map of Charon, the moon of the solar system's most remote planet, Pluto....

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• Dayside aurora [Oulu]
• Venus Picture List
• Remote Sensing of Tropical Regions

... Pluto's orbit is also highly inclined -- tilted 17 degrees to the orbital plane of the other planets. ... Ground-based observations indicate that Pluto's surface is covered with methane ice and that there is a thin atmosphere that might freeze and fall to the surface as the planet moves away from the Sun. ... This is the first image-based surface map of the solar system's most remote planet, Pluto. ... This is the first surface map of Charon, the moon of the solar system's most remote planet, Pluto....

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• Radioastronomy reduction procedures
• APOD: June 25, 1996 - A Star Forming Region in the LMC
• The BD+40 region (Abstract)

... OCR by H.Andernach 1/96, to be proof-read) This is the first of a series of papers presenting results of a 10-GHz radio continuum survey of the galactic plane region using the 45-m telescope at Nobeyama. ... Weak Nonthermal Sources: A comparison with the Bonn S-GHz survey reveals a number of weak nonthermal sources near the galactic plane. ... For this reason we conducted a survey of the galactic plane region at 10 GHz using the 45-m radio telescope at the Nobeyama Radio Observatory (NRO). ...

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• RATAN-600 NCP bright radio sources
• The RATAN SNRs Survey
• Source Positions

... Posts tagged ?confidence region? ... Today?s arxiv-stat email included papers by Poetscher and Leeb, who have been working on post model selection inference. Sometimes model selection is misled as a part of statistical inference. Simply, model selection can be considered as a step prior to inference. ... ArXiv] Post Model Selection, Nov. ... Tags: bias , confidence interval , confidence region , coverage , Errors , Estimation , inference , Model Selection . ... Comment . ... Entries RSS . ...

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• The AstroStat Slog PDF
• Watching the Stars go `Round and `Round
• The AstroStat Slog Blog Archive Open and Shut [Equation of the Week]

... This is the truly fun part, observing molecular and atomic gas in star-forming regions with a variety of telescopes. Depending on the temperature and density of the gas, different observations are necessary to study the components of star-forming regions. Because stars form in cool gaseous regions, I most often use radio and sub-mm observations, but I also look for opportunities to make complementary observations using infrared and optical telescopes. ... Copyright 2015 Adele Plunkett. ...

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• ESO - Thesis Topic: Planetary Nebulae and HII regions in the Elliptical Galaxy
• Synthetic Star Forming Region HRDs
• Lots of Small Stars Born in Starburst Region | ESO

... Meta Index / Home Page / Description / Specifying source region shapes . When radiusstyle =`contour', the task calculates the source region shape as an elliptical locus which approximates the contour of the PSF at a given flux value. ... Clearly, in order to calculate the shape of such a flux contour, it is necessary firstly to normalize the PSF to the source brightness and secondly to determine the flux level (in `brightness' units per pixel) at which to find the contour. ...

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• Region file
• Parameters

An Ancient Universe: How Astronomers Know the Vast Scale of Cosmic Time . THE ANCIENT UNIVERSE . c) The Age of Light from the Most Distant Galaxies: The "Time Machine" Effect . ... Thus we are actually seeing these galaxies not as they are today, but as they were billions of years ago. ... The Universe: An Overview | ... The Ancient Universe - The Age of the Expanding Universe - The Age of the Oldest Stars - The Age of Light From Distant Galaxies - The Age of the Chemical Elements | ...

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• ASP: Beacons in the Gloom
• ASP: Miranda: A Jigsaw Puzzle World
• ASP: Star Science in the Autumn Sky

... Flux density at 1 GHz (/Jy): 210 . ... Optical: Large filamentary loop, brightest to the NE, not well defined to the S or W. X-ray: Shell in soft X-rays. Point sources: Several compact radio sources within the boundary of the remnant, including CL4, plus X-ray sources in S. Distance: Optical proper motion and shock velocity gives 0.44 kpc. ... ADS . ... Greidanus & Strom 1992, A&A, 257, 265. ... Shull & Hippelein 1992, ApJ, 383, 714. ... ASCA observations of compact X-ray source in S. ADS . ...

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• G33.6+0.1

... 13, Moscow 119992, Russian Federation, e-mail: busarev@sai.msu.ru; 2 Research Institute Crimean Astrophysical Observatory, p/o Nauchnyi, Crimea 334413, Ukraine, e-mail: prok@crao.crimea.ua Summary: We propose a combined method of astronomical investigations of small or distant planets incorporating registration of a set of integral spectra of an object and their frequency analysis. ... An application of the method is shown on example of asteroid 21 Lutetia. ... 6] Busarev V. V. (2002), Solar Sys. ...

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• Geophysical Research Abstracts

... Astronomers Demonstrate a Global Internet Telescope . ... European and US radio astronomers have demonstrated a new way of observing the Universe – through the Internet! ... This allows imaging of the objects with unprecedented detail, and in real-time, which would have been impossible only a few years ago. ... Surrounded by clouds of dusty gas and emitting strongly in radio waves, the object is poised at the end of its life, heading toward a cataclysmic explosion known as a 'supernova'. ...

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• Planetary Radar: Arecibo Radar Images of Planets
• water ice on mercury
• I-GALFA View of a Galactic Tangent Region

... This program was created for correlating chosen regions in the series of fts images. ... Chosen regions' . ... In this section the program counts the integral for each region of the grid for each image. ... As a matter of fact, the integral is total brightness of the region and it is counted by 'int_tabulated' IDL function. ... In addition, the program will show the count of the regions which correlate with the corresponding region (the brighter region means the bigger count) and its contour. ...

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... Scientific Publications . ... In the autumn of 2016 the scientific journal Computer Optics is planned to be issued with original publications in English (Volume 40 No. ... The journal is included in the List of State Commission for Academic Degrees and Titles of the Ministry of Education and Science of the Russian Federation of the leading peer-reviewed scientific journals and publications, in which basic scientific results of the doctoral thesis in physics and informatics should be published. ...

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• Research and Education Center of Computer Science (REC Cs-208)
• Additional training
• Mikheeva Tatyana Ivanovna

... Data It is now clear that fuzzballs are actually galaxies. ... Using the automatic telescope, we measured the redshifts and brightnesses of a large number of fuzzballs in all regions of the sky. ... Correlation between brightness and redshift Redshifts and Brightnesses 0.005 0.004 0.003 0.002 0.001 0 -0.001 0 -0.002 -0.003 -0.004 -0.005 Redshift of Fuzzball 500 1000 1500 2000 Brightness of Fuzzball The brightnesses and redshifts of all the fuzzballs measured are shown in this graph. ...

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• http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.doc
• http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer2.pdf
• http://www.mso.anu.edu.au/pfrancis/roleplay/ziggy/model_answer3.doc

A team of astronomers has used ALMA to pinpoint the locations of over 100 of the most fertile star-forming galaxies in the early universe. This image shows close-ups of a selection of these galaxies. The ALMA observations, at submillimetre wavelengths, are shown in orange/red and are overlaid on an infrared view of the region as seen by the IRAC camera on the Spitzer Space Telescope. ... ALMA (ESO/NAOJ/NRAO), J. Hodge et al., ... NASA Spitzer Science Center ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1782619C-6102-4D0B-9DCF-FFA5FB5D0C42%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B092843B5-9D5B-4F1D-8917-DAD312D496CF%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B65367468-8CC0-46B1-A662-6CD63A91B5A5%7D