... Astrophysics Group . ... Surveys and Catalogues . ... The main 7C survey at 151 MHz with resolution 70У?70Тљcosec(declination)Тљarcsec 2 (EWУ?NS) covers a large part of the northern hemisphere above declination 30ТА, excluding the Galactic plane.There is now a final unified non-redundant catalogue for this main survey in ASCII format together with a CDS-style ReadMe file, both available by ftp from MRAO. ... Regions surveyed at resolution 70У?70 cosec(dec) arsec 2 , ftp accesses standardised data: ....

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• Astrophysics Group members - C Haniff
• Astrophysics Group VSA
• Research David Buscher

... Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 . ... Power spectral analysis (PSA) has proven to be an important tool for high spatial resolution measurements from ground based interferometry. ... While many images from HST are far too complicated for PSA, there are a class of scientific problems for which it is a very effective technique for handling the problems created by the HST point spread function. ... Power Spectral Analysis . ...

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• Determining dust temperatures and masses in the Herschel era: The importance of
• Fine Guidance Sensor Instrument Handbook
• Boron in the Very Metal-Poor Star BD-13^o 3442

... 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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• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• How to Piece Together Diffracted Grating Arms for AXAF Flight Data
• NICMOSlook and Calnic C: Slitless Spectra Extraction Tools

... India (1999) xx, PINTofALE: Package for the Interactive Analysis of Line Emission V.Kashyap & J.J.Drake Center for Astrophysics, Cambridge, MA 02138, USA Abstract. ... It is based on a modular set of IDL tools that interact with an atomic database and with observational data. ... The package has been extended to handle analysis of high­resolution X­ray spectra that will be obtained with the Chandra X­Ray Observatory. Key words: X­rays, X­ray Spectroscopy, Stellar Coronae, Analysis Methods 1. ...

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• High Energy Astrophysics
• Michael Juda - Home Page
• Project Tanagra

... Science Publications > Science Announcements > 8th VLTI Summer School: High angular resolution in astrophysics: optical interferometry from theory to observations . ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... Optical/infrared long-baseline interferometry has reached a new stage with the advent of multi-telescope arrays accessible to a broad community of astronomers, most notably VLTI . ...

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• High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
• ESO - Improvement to FLAMES Spectral Resolution and Sensitivity
• ESO - Tomography

... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . Australia Telescope Compact Array . ... Information & tools for observers . ... Virtual Radio Interferometer . ... The ratio above is called the resolution of the telescope. ... An interferometer works most efficiently, in the sense of returning the most information about the intensity and size of the source being observed, for a source whose size is comparable with the telescope's resolution. ...

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• SNR 1987A: highest resolution image ever achieved using the ATCA
• Observations and Data Analysis
• MAPPIT 2: Second Generation High-Resolution Imaging at the AAT

Next: J.E. Chambers, Research Astronomer Up: Research Previous: Research Contents . ... Solar Variability and Climate . Other Activities . ... Applied to data of flares on Gliese866 he was able to estimate the area of hydrogen emitting flare regions as 1-13% of the stellar surface. ... As partners in the project, Armagh Observatory has been asked to contribute to the selection process in exchange for priority access to the data which will eventually flow from the satellite. ...

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• Armagh Observatory

... A homogeneous chemical analysis of the inner Galactic disk from the first data release of Gaia-ESO . ... Gaia-ESO is a public spectroscopic survey designed with this goal in mind. ... These first results highlight the potential of the Gaia-ESO survey to explore areas of the Milky Way still poorly studied, such as the inner disk, and to give new constraints on Galactic chemical evolution models. ... Map of observed targets of the first data release of the Gaia-ESO Survey. ...

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Subject, Object and Problems of Astrophysics. Practical and Theoretical Astrophysics. ... Visual Telescope; Problems Which Are Solved with the Its Help. ... Resolution of Telescopes. ... Effectiveness of Telescope in Respect of Resolution. ... Optical Power of Telescopes for Star-like and Extensive Objects. Boundary Magnitude. Reasons of Light Dissipation in Telescopes. ... Spectral Instruments in Astrophysics. ... Basic Photometrical Ideas, Magnitudes and Their Measurement. ...

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• HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11
• Optical static Fourier spectrometer

reconstruction with Fast Simulation M. Iwasaki University of Oregon At the Sitges meting: tt 6jets 4jets analysis · Charged/Neutral cluster separation with Track- cluster matching · Reconstruction performance in Energy flow analysis · B-tag effect After the meeting: · In FastMC, set the cluster position resolution determined by FullMC · Study Cluster width with FullMC · ...

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Search Site . ... Advanced Search? ... Main goal of our group is to study energy transformation mechanisms in extreme gravitational and magnetic fields of such objects as black holes, pulsars, white dwarfs and flaring stars. Currently, the Group staff is working on the following scientific topics: . Study of rapidly variable astrophysical objects with high temporal resolution . ... Maintained by Sergey Karpov љ-љPart ofљ Special Astrophysical Observatory љwebsite ...

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• Tikhonov's regularization and multiresolution analysis
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... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

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• IRAS01005+7910
• Solar system sector, archive 2011

... 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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• Elena Seifina

... Thermogravimetric and differential thermal analysis . ... TOF-SIMS analysis . Total conductivity, Seebeck coefficient and ion transference number measurements in controlled atmos . ... Processing of ceramic materials, electrode systems and electrochemical cells . ... SIMS analysis is based on exposure of the sample surface with primary ions possessing some definite energy, which is partially consumed by the sample and induces emission of sН-called secondary ions. ... Spatial resolution: 60 nm . ...

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• Laboratory of spectroscopy of defect structures ISSP RAS

Astronomical Data Analysis Software and Systems VII ASP Conference Series, Vol. ... Data Processing 1.1. ... Select Zero Order Sources/Find Observed Target In order to find where the dispersed photons lie, the center of the zero order source position on the sky must be determined, since this is the origin of the spectral coordinates. ... For the HETG grating data, the relevant parts for each source are: zero order, MEG photons, HEG photons, and background photons. ...

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• NICMOS Data Calibration and Analysis
• CONICA: The high resolution near-infrared camera for the ESO VLT
• Index

. Departement of Quantum Astrophysics . Head: Kurt V.G. , Prof. ultraviolet spectroscopy of planetary upper atmospheres and interplanetary/interstellar medium; . observations of gamma-bursts and optical identification of their sources; . long-base optical interferometry. Staff: .

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• Theoretical Astrophysics Department
• Description of the RadioAstron project, english version

18. http://mavr.sao.ru/hq/skai/article/0711.2153v1.pdf

19. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/pagani-cal-2012.pdf

20. Amateur Telescope Makers of Boston