Next: Splitting and Imaging Up: Primary Beams and Mosaicing Previous: Some Additional Tools . The individual approach images, deconvolves, self-calibrates and restores each pointing separately. ... With the `individual approach', it is possible to deconvolve sources (and thus eliminate their sidelobes - which is the important issue) beyond the limit where Miriad 's primary beam model gives up. ... Splitting and Imaging . Deconvolution, Restoration and Self-Calibration . Image Combination . ...

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... Finally, the individual observations themselves are reduced, using the parameters from the extinction solution. ... That is, the extinction solution can in principle produce results if we observe extinction star 1 only in passband A and star 2 in passband B on night 1, and star 1 only in passband B and star 2 in passband A on night 2. ... Even if the passbands are linked by color terms in the extinction, the solution is possible, because we do obtain mean colors for each star. ...

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... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How do I combine the individual 3-D cubes into a final mosaic? ... Observing Facilities . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... If the individual cubes come from a single offset sequence, the easiest is to use the ESO.SEQ.CUMOFFSETX/Y keywords in the...

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... Meta Index / Home Page / SourceListFile / QUALITY FLAGS . Bad Pixels A point-source will have this flag set if any pixel within the photometry aperture have a corresponding pixel in the quality image with a non-zero value. Similarly, an extended source will have this flag set if any corrsponding pixel in the quality image has a non-zero value. The quality image was added to the image file by omcosflag , and a ``bad'' pixel may either be a damaged or dead one. ...

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Next: Critical Frequencies and Gravitational Previous: Extragalactic Gravitational Wave Background . The number of binaries per frequency decade per solid angle from a separate stellar system (galaxy or cluster of galaxies) is . ... For example, for the Andromeda galaxy M31 ( rad, ) one gets . ... If the angular size of the galaxy is less than the angular resolution of the detector, the critical frequency is independent of the angular resolution, . ...

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Today's APOD | ... Editor's choices for the most educational Astronomy Pictures of the Day about individual stars: . APOD: 2000 June 11 - Sirius: The Brightest Star in the Night . Explanation: Sirius is the brightest star in the night sky. ... As Sirius is 8.7 light years distant, it is not the closest star system - the Alpha Centauri system holds this distinction. ... APOD: 2005 December 4 - Proxima Centauri: The Closest Star . ... APOD: 1999 October 6 - Polaris: The North Star . ... Index | ...

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If you are an educator or astronomer interested in becoming a part of Project ASTRO?, or in using Project ASTRO materials, here are some ways you might get involved with us: . If you live near one of the Project ASTRO National Network Sites , contact the coordinator at your local site to get an application to be a Project ASTRO astronomer or educator. ... Learn More about Project ASTRO Educator-Astronomer Partnerships . ... Return to Project ASTRO: Getting Involved . ...

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. The [+0.0] spectra. The [-1.0] spectra. The [-2.0] spectra. Back to grid page

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In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

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... Radio searches for pulsars associated with supernova remnants. ... The Bologna submillisecond pulsar survey. ... A search for pulsar wind nebulae using pulsar gating. ... Anomalous pulsars and other radio quiet neutron stars in supernova remnants. ... A 16 ms X-ray pulsar in the Crab-like SNR N157B: fast times at 30 Doradus. ... Radio-quiet X-ray pulsars in SNRs and the ``missing'' pulsar problem. ... Searching for X-ray pulsars associated to SNRs in public ROSAT observations. ...

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... In each room, the ash and rubbish is checkedтАж . ... Title: In each room, the ash and rubbish is checked for relics of use, the barrowed into individual piles, one per room. ... In each room, the ash and rubbish is checked for relics of use, the barrowed into individual piles, one per room. ...

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An image of the grand design of spiral galaxy M100 obtained with NASA's Hubble Space Telescope resolves individual stars within the majestic spiral arms. ... Hubble has the ability to resolve individual stars in other galaxies and measure accurately the light from very faint stars. This makes space telescope invaluable for identifying a rare class of pulsating stars, called Cepheid Variable stars embedded within M100's spiral arms. ... 617) 495-7062 . Fax: (617) 495-7356 . ...

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... tghosh@naic.edu Xiaoyu Hong xhong@shao.ac.cn Sergio Colofrancesco sergio.colafrancesco@wits.ac.za Institution ISAS JAXA, Japan NRAO , USA CASS CSIRO, Australia RISC member status institutional institutional institutional , cochair institutional institutional institutional institutional institutional , XC institutional ...

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2015 . ... A priory National teams of countries consist of winners and prizewinners of National Astronomy Olympiad take part in IAO. ... Как правило, каждую страну на IAO страну представляет команда, составленная из победителей и призеров национальной астрономической олмпады. ... In the case of absence of a National team from a country, organizers of IAO may permit any provinces, regions, cities of this country to form the team representing the country. ... National team may consist of: . ...

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... galaxies: bulges galaxies: clusters: general galaxies: clusters: individual: . ... star formation statistics stellar content structure Cosmology ( cosmology :) cosmic background radiation ( cosmology :) cosmological parameters cosmology : miscellaneous cosmology : observations cosmology : theory ( cosmology :) dark ages, reionization, first stars ( cosmology :) dark energy ( cosmology :) dark matter ( cosmology :) diffuse radiation ( cosmology :) distance scale ( cosmology :) early Universe (...

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... 1 |Mathworks |MATLAB new Product |1 |локальная | Individual/Group | 2 |Mathworks |Simulink new Product |1 |локальная | ... 3 |Mathworks |Simscape new Product |1 |локальная | ... 4 |Mathworks |SimElectronics new |1 |локальная | Product | ... 5 |Mathworks |Optimization Toolbox |1 |локальная | new Product | ... 6 |Mathworks |Global Optimization |1 |локальная | Toolbox new Product | ... 7 |Mathworks |Simulink Design |1 |локальная | ... 9 |Mathworks |Parallel Computing |1 |локальная | ...

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... The "GALFA Consortium" is a group of individuals interested in galactic astronomy programs using the Arecibo L-Band Focal Plane Array (ALFA) and who are committed to coordinating efforts to the extent possible in order to maximize science return and program efficiency. ... The GALFA "Coordinating Committee" consists of representatives of GALFA Consortium projects that have been granted telescope time or those in the development stage that have been endorsed by the GALFA Consortium. ...

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... Established in 1996, the goal of the NASA Johnson Space Center Oral History Project (JSC OHP) is to capture history from the individuals who first provided the country and the world with an avenue to space and the moon. ... Alphabetical List A-B C-D E-G H-J K-L M-N O-R S-T U-Z Administrators Aviatrix Herstory Ballistics JSC OHP ISS OHP NACA OHP Experts OHP Space Shuttle Program Earth System Science NASA at 50 STS Recordation Chilean Miners Rescue Shuttle-Mir OHP SCA-SRB OHP C3PO OHP . ...

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Next: Feature enhancement: filtering Up: No Title Previous: Commentary . A sharp contrast is seen between the `crowded' energy map of the modulated oscillations (individual minima and maxima of the signal identified by the Mexican hat wavelet) in section 13 and and the `smooth' presentation of the norm-Morlet transforms of the same data in section 15. ... construct an energy map based on individual events. smooth the map by merging the events that are `close enough' to each other. ...

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