... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• ESO - The European ELT

Arecibo and High Resolution Astronomy . ... Future of HI Astronomy at Arecibo . Future of Radar Astronomy at Arecibo . High Sensitivity VLBI: Neutron Star Astrometry with Arecibo . ... Probing fundamental constant evolution with the Arecibo Telescope . Prospects for future surveys in astronomy . ... Mapping the Future of VLBI Science in the U.S. OH Megamasers, ULIRGs, and Magnetic Fields . ... Radio Synoptic Survey Telescope (RSST) . ... VLBI Plans at Arecibo in the Near Term . ...

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• HISA Poster for the 33rd Annual Meeting of CASCA, May, 2002
• H I Midplane Poster for the 201st Meeting of the AAS, January, 2003
• Diffuse Galactic Light in the Large Magellanic Cloud

Color-magnitude diagrams (CMDs) are presented for the Spitzer SAGE (Surveying the Agents of a Galaxy's Evolution) survey of the Large Magellanic Cloud (LMC). ... Combined with the Two Micron All Sky Survey, the diagrams are used to delineate the evolved stellar populations in the LMC, as well as Galactic foreground and extragalactic background populations. Some 32,000 evolved stars brighter than the tip of the red giant branch are identified. ...

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• The Large Magellanic Cloud's Largest Molecular Cloud Complex: Spitzer Analysis
• Mapping the Cosmic Web
• The Effects of Dust in Simple Environments: Large Magellanic Cloud H II Regions

... Astrophysics Group . Research . Atacama Large Millimetre Array (ALMA) . ... Cosmic Microwave Background (CMB) . ... Galaxy Formation and Evolution . ... The Astrophysics Group is actively involved in the ALMA project , a submillimetre interferometer being built in northern Chile. ... If you are interested in doing research in this area, please visit our Graduate Research Opportunities web pages. ... 2013, Astrophysics Group, Cavendish Laboratory, JJ Thomson Avenue, Cambridge, CB3 0HE . ...

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• Astrophysics Group VSA
• Martin Krause - Large Scale Very Light Jet Simulation
• Astrophysics Group Exploring the Cosmic Dawn

... Infrared Portrait of the Large Magellanic Cloud . ... Credit Copyright: ESA / NASA / JPL-Caltech / STScI Explanation: Cosmic dust clouds ripple across this infrared portrait of our Milky Way's satellite galaxy , the Large Magellanic Cloud. ... The dust temperatures tend to trace star forming activity. ... Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from views in optical images . ... NASA Official: Jay Norris. ... The Large Magellanic Cloud in Ultraviolet...

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• XWare > APOD

. ATLAS is a project to image seven square degrees of sky, in two fields (CDF-S and ELAIS-S1), at radio wavelengths, to an rms of about 15 Jy, making it the widest deep radio survey aver attempted. The fields are chosen to cover the Spitzer Wide-Area IR Extragalactic Survey (SWIRE), and the radio images cut through the dust, to trace the cosmic history of AGN and star-forming galaxies. This page last updated by Ray Norris 5-Mar-2007

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• Australia Telescope National Facility
• Ionized Hydrogen at Large Galactocentric Distances
• Southern Cross Astrophysics Conference Series

... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2016 January 14 . Infrared Portrait of the Large Magellanic Cloud . ... Explanation: Cosmic dust clouds ripple across this infrared portrait of our Milky Way's satellite galaxy , the Large Magellanic Cloud. ... Dominated by dust emission, the Large Magellanic Cloud's infrared appearance is different from views in optical images . ...

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• APOD: 2012 January 15 - Infrared Portrait of the Large Magellanic Cloud
• APOD: 2013 March 23 - Infrared Portrait of the Large Magellanic Cloud
• APOD: 2008 February 16 - Large Binocular Telescope

... 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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• Siding Spring Survey
• Comparison of simulations with the large scale radio galaxy M87.
• Large Magellenic Cloud

. 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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• Description of the RadioAstron project, english version
• Lukash Vladimir Nikolaevich, Astro Space Center (ASC)

... Events . ... COSMOS 2009 - Ireland's Spring Star Party . The Irish Node for the International Year of Astronomy is announcing that this year St PatrickтАЩs Festival celebrations in all major cities in Ireland are endorsing an astronomy theme. In Dublin , this yearтАЩs theme for the festival Parade is тАШ The SkyтАЩs the Limit! тАЩ . ... Monday, 16 March 2009 00:49 . International Year of Astronomy, Ireland National Node . ...

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• Japanese Discover Large Earth Crossing Asteroid
• Southern African Large Telescope (SALT)
• Did the world's largest telescopes survive the earthquake? | OASES Over us All

... Next: Unsupervised Catalog Classification Up: Object Detection and Previous: Classification of Objects . ... Multi-resolution allows for image analysis in terms of different scales. ... This approach is used for the detection (and subsequent analysis) of globular cluster systems around elliptical galaxies, and for image characterization and object trawling in large image databases. ... The applicability of this approach to object detection in large image collections has been investigated. ...

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• Surveys & Large-Scale Data Management
• ADASS 2003 Conference Proceedings
• On-line Access to Very Large Catalogues

... Tonight's Sky . ... The Magazine . ... Observing . ... Magazine . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... large (8 inches or larger) . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ... Astronomy Magazine . ...

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• very large telescope | Astronomy.com
• large magellanic cloud | Astronomy.com
• Observing springtime deep-sky objects with a large telescope | Astronomy.com

... Large . ... Normal . ... Thumbnails . ... Enter: Large | ... Contents with thumbnails: Large | ... Florence streets . ... Rome. ... Sunday, 12 September. ... Monday, 13 September. ... Tuesday, 14 September. ... Wednesday, 15 September. ... Thuesday, 16 September. ... Friday, 17 September. ... Saturday, 18 September. ... There's also index of the complete set of photos with thumbnails. ... return to photo album contents | ...

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• Photo album: Japan: Kyoto and Nara, August 1997
• Image: We are walking to large Buddhist temple near Kyoto station
• Image: Slope of the hill is covered by large stone staircase. Deers everywhere.

The Cosmic InfraRed Background (CIRB) is the radiation from stars in many faint galaxies. ... The near-infrared (wavelengths near 2-3 microns) and optical (wavelengths near 500 nm) part of this extragalactic background light is just starlight redshifted into the infrared. But some starlight is absorbed by dust and re-emitted in the far-infrared (wavelengths near 100 microns). ... The CMB is by far the largest of these radiation fields, with a total intensity of 996 nW/m 2 /sr. ... Part 2 | ...

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• Large Scale Survey Project URL's
• SUMSS: A Wide-Field Radio Imaging Survey of the Southern Sky
• Removing Cosmic Ray Hits

... We present 7mm observations of the dusty disk surrounding the 10 Myr old 1.5 Msun pre-main-sequence star CQ Tauri obtained at the Very Large Array with 0.8 arcsecond resolution and 0.1 mJy rms sensitivity. ... We find that the disk radius is constrained to the range 100 to 300 AU, depending on the steepness of the disk surface density distribution. The power law index of the dust opacity coefficient, beta, is constrained to be 0.5 to 0.7. ...

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• IRAS Image Of The Large Magellanic Cloud
• Optical System
• Arcetri Solar Physics Group: High Resolution Studies

Within the Hubble Ultra Deep Field there are approximately 10,000 discrete objects. ... Most of these objects are very small and likely have masses in the range of 10 5 to 10 7 solar masses. Note the mass of the Milky Way galaxy is 10 12 solar masses. ... Finally, for you cosmologists/experts out there this ultra deep field is quite consistent with what was seen in the original Hubble Deep Field 5) don't necessarily have small angular diameters. ...

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• The Galaxy Gallery: Messier Objects
• Solar Energy: Large Scale Production

Imaging with the GLAST Large Area Telescope ' J. Chiang JSM , 1 August 2007 $ 1 Imaging Using the GLAST Large - Area Telescop e Jim Chiang Stanford Linear Accelerator Center % Imaging with the GLAST Large Area Telescope ' J. Chiang JSM , 1 August 2007 $ 2 The GLAST Large Area Telescop e % Imaging with the ... Distinguishing a collection of weak point sources from diffuse, extended emission. ...

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• The Chandra Multiwavelength Project (ChaMP)
• To compress and display a large (e.g. ROSAT) image
• *imcopy* - Extract a small image file from a larger image

... We can help students grasp the significance of Hubble's extremely keen eye, and learn a bit about angles and math in the process, with the following in-class activity. ... Looking through binoculars or telescopes allows us to magnify a small section of the sky. To measure sizes or distances in that small section, astronomers divide a degree into 60 smaller pieces called arcminutes, and further subdivide minutes into 60 smaller sections called arcseconds. ... 30 feet = . ... 36 seconds . ...

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• ASP: Cosmic Collisions
• ASP: More About Deep Space Objects and Cosmic Terms
• ASP: An Ancient Universe - Andromeda

Общая Астрономическая Конференция > Форумы общей направленности > Любые вопросы от новичков . Supernovae - Microwave Background - Large-Scale clustering . ... Поиск . ... Созвездия (поиск и описание) .. Созвездия южного неба (поиск и описание) .. Осенние созвездия (поиск и описание) .. Летние созвездия (поиск и описание) .. ... Double Cluster (Хи и Аш Персея (Chi & h Persei), NGC 869 и NGC 884) и скопления вокруг него Звездные ассоциации - астеризмы (поиск и описание) .. ...

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• Supernovae - Microwave Background - Large-Scale clustering [Архив] - Общая

... Telescopes . ... 2002: . A quartz echelle spectrograph with a large diameter of the collimated beam (NES) equipped with a CCD (2048x2048 elements) was designed, manufactured and put into operation in the Nasmyth focus of the 6-m telescope. ... We have developed and tested the model of a new-generation three-element broadband radiometric matrix system at the RATAN-600 extremely short wavelength of 1 cm, allowing a large replication to over 100 elements. ...

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• Large telescopes application form
• Metagalaxy sector, archive 2011
• Discovery of enrichment of the envelopes of post-AGB stars with heavy metals