2nd of July 2015 . ATNF Colloquium . ... by Dan Werthimer (University of California, Berkeley) . ... Dan Werthimer will discuss the search for radio, infrared, and optical signals from other civilizations. Berkeley's SETI@home project analyzes Arecibo data using desktop computers from millions of volunteers. SETI@home participants have contributed millions of years of computer time and have formed one of Earth's most powerful supercomputers. ... today * ATNF | ...

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• The Joint Approach
• Pulsar Group PmWiki/Forms
• Basic Processing

Structure Formation : Bright side of the Universe Anatoly Klypin New Mexico State University Also: Stefan Gottloeber (Astrophysikalisches Institut Potsdam) Gustavo Yepes (UAM, Madrid) Cosmological ... -body+hydro simulations Codes: SPH + TREE AMR + shock capturing hydro Physical processes: Compton cooling/heating on CMB Radiative gas cooling Star formation with simple approximations Metal enrichment Energy/momentum feedback from young stars and SN Galaxies too concentrated. ...

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• GRB follow-up team
• Introduction
• The ROSAT Bright Survey: II. Catalogue of all high-galactic latitude RASS

A very important stage in a story of formation of any new science is the shift from discussion of situation which are possible but do not occur in practice due to some reason to recognition of real phenomena of interest. ... We suggest to consider computer viruses as this new specific form of life which is coming in the contact with our form of life. ... Computer life has been created by human being, the role of independent evolution of computer viruses seems to be still negligible. ...

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• Photos from the defense of my master thesis (december 2005)
• Семинар по звездной астрономии

Analysis of general features of the chaotic system behavior and investigation of the properties of concrete chaotic sources. ... Analysis of information properties of chaotic systems and chaotic oscillations as concrete objects for information processing and comunications. ... This hypothesis gives a possibility of designing simple mathematical structures accomplishing various processes of information processing using chaos. ... Activities | ... E-mail: chaos@mail.cplire.ru ...

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• Information Processing with Chaos - Bifurcations Chaos
• Processing Pictures - "InformChaos" Software
• NIST Special Publication 500-223. A Framework for the Development and Assurance

... In the past used to check pn/ MOS cross calibration Example of old vs new pn/ mos Residuals in the form of ratio data / model for PN data on MOS best fitting model Example of old vs new pn/ mos Residuals in the form of ratio data / model for PN data on MOS best fitting model ACIS S3 vs EPIC pn · · Same thing, only now we compare Chandra ACIS S3 with ... Flux cross-cal · · The new HRMA calibration impacts on the ACIS/EPIC flux cross calibration. ...

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• Summary of the algorithm for IMAGING mode data
• XMM-Newton SAS: Watchout Page
• Contrasting optical and X-ray applications

It all started back in 1979 when the diskdrive manufacturer come with the bright idea to make a new transfer protocol. ... This protocol wasn't an ANSI standard, so NCR join Shugart and the ANSI committee X3T9.2 was formed. The new name for the protocol was, Small Computer Systems Interface, SCSI. ... ANSI finished the SCSI standard in 1986. SCSI-II devices was released in 1988 and was an official standard in 1994. ... SCSI is in opposite to IDE/ATA very flexible. ... Datawidth 8 bits. ...

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• NVSS radio survey
• Space-Time with Bound Cluster
• Cluster Analysis

OptInt PmWiki : Pm Wiki / Forms . ... Forms processing can be found in the Cookbook (see below). ... input text name value size= n :) (:input hidden name value :) (:input password name value :) (:input radio name value :) (:input checkbox name value :) (:input select name value label :) (:input default default-name default-value :) (:input submit name value :) (:input textarea name [=value=] rows= n cols= n :) (:input reset name label :) (:input file name label :) (:input image name "src" alt :) . ...

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• Galaxy Evolution: Cosmological evolution of star formation
• Galaxy Evolution: Computing
• NVSS Image ftp service Documentation Help for NVSS Image ftp service

... Информация Руководство и преподаватели Сулейманова Ильмиря Рашитовна . ... Публикации . ... Попов И.П. , Звонов С.Ю. , Сулейманова И.Р. Исследование процессов изготовления осесимметричных конических деталей с заданной толщиной стенки // Вестник КГТУ. ... Сулейманова И.Р. , Звонов С.Ю. Исследование параметров влияющих на процесс вытяжки толстостенной кольцевой заготовки с принудительным утонением // Королевские чтения, , Самара, СГАУ, 2011 г., С. 203 . ...

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• Михеев Владимир Александрович. Публикации
• Сурудин Сергей Викторович. Публикации
• Шляпугин Алексей Геннадьевич. Публикации

... Meade Instruments Corporation . ... Autostar Computer Controllers . 497 Autostar . ... One of the most important advances in telescope control in the past 25 years, the Meade #497 Autostar Computer Controller turns the ETX into an automatic celestial object locating system. ... The #497 Autostar Computer Controller plugs into the control panel of ETX-90EC, ETX-105EC, and ETX-125EC telescopes and enables automatic location of more than 30,000 celestial objects. ... about meade | ... Meade 4M | ...

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• UHTC Coatings: Ultra High Transmission Coatings, Special Coatings, Telescopes,
• Meade Instruments Corporation - Autostar Computer Controller Instruction Manual
• Meade Instruments Corporation - Magellan II Telescope Computer System

Электронная библиотека астронома-любителя. ... архив RSN . ... Апрель 1998 . ... Дата: 10 апреля 1998 (1998-04-10) От: Alexander Bondugin Тема: Galileo Update - April 9, 1998 Привет всем! ... Дата: 10 апреля 1998 (1998-04-10) От: Alexander Bondugin Тема: Mars Global Surveyor Update - April 9, 1998 Привет всем! ... The feature known as the "Face on Mars" in the Cydonia region was imaged quite successfully on April 5th and its image was released in raw form and in an enhanced form on April 6th. ...

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... Up: Archives and Information Services . ... It is performing astronomical observations at wavelengths from 2.4-240 microns with four instruments; a camera (2.5-18 microns), a photometer (2.5-240 microns), a short-wavelength spectrometer (2.4-45.2 microns) and a long-wavelength spectrometer (43-197 microns). ... The ISO post-mission archive (PMA) is being designed to fully exploit this legacy by providing access to the data across the Internet. ... For each observation the user specifies: . ...

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• Near-IR Imaging of Star-forming Regions with IRAF
• Colophon
• Spiders and Camels and Sybase! Oh, My!

... A faint, dusty rose of the northern sky, emission nebula IC 410 lies about 12,000 light-years away in the constellation Auriga. The cloud of glowing hydrogen gas is over 100 light-years across, sculpted by stellar winds and radiation from embedded open star cluster NGC 1893. ... These "tadpoles" (seen just below center) are regions of denser, cooler gas, and more slowly resist the erosive radiation from the hot stars. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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• Amateur Telescope Makers of Boston ATMoB Observing Awards Program

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

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• Researches of Astronomy and Space Physics Department
• Apparent places of fundamental stars for Computer Ephemeris for 2014
• Apparent places of fundamental stars for Computer Ephemeris for 2015

The original files with the data were in different formats. ... Such files were named "standard data files" and linked to the database. They can be easily transformed to any desirable format by a code. Here we present two simple computer programs of this kind. ... When running the code, you can specify columns in the output file: wavelength, energy (eV) or wavenumber (cm -1 ) as the first column, and complex refractive index or dielectric function as the second and third columns. ...

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... The Wide Field Spectral Imager ( WISPI ) seen here in the Roll Roof Facility provides visible and near-infrared spectra of the sky across 4 degree fields. ... A computer controlled mounting automates the acquisition of 2-D rastered spectral images. ... Light from the sky enters the large 400mm lens at top center, is imaged on the slit, collimated by the smaller 180 mm lens, and diffracted by the grating at the bottom toward the 200mm lens and CCD camera on the right. ... Camera - 200mm f/2 Nikor ED ...

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• University of Louisville Wide Field and Planetary Telescopes
• ImageJ for Astronomy
• ExtendedPlugInFilter (ImageJ API)

The radio-telescope. The radio-telescopes are the great sized constructions. The most spread type of the radio-telescope is a construction the basic element of which is a whole metallic mirror of a parabolic form. The mirror reflects the radiowaves falling on it, so they gather near the focus and are able to be caught by the special unit- irradiator. Then the signal is strengthened and changed into the form convenient for a registration and analysis. ... Back . ...

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• galophotoe
• plutone
• redkoste

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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... Plastic forming and welding of optical elements for laser technologies and optical telecommunications. A set of technological processes of manufacturing of optical elements with sophisticated profiles for laser technologies and optical telecommunications has been developed in the Institute of Solid State Physics . ... тАв€а to form optical surfaces with non-spherical and rather sophisticated profiles, improving essentially effectiveness of laser technologies and optical telecommunications; . ...

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• International Astronomy Olympiad: Form for the short report of National
• Biomimetic method to fabrication of metallic nanostructured€аmesoscopic models
• The VIII Asian-Pacific Astronomy Olympiad, results

... Magnetic Storms . ... Cosmic Rays . ... Energetic Particles . ... Solar fast Particles . We cannot observe the way the distant universe accelerates cosmic rays or produces energetic photons, but acceleration processes also occur on our Sun , though on a much more moderate scale. ... That is why such events are often missed by cosmic ray detectors near the equator, where the lowest energies are excluded by the Earth's magnetic field. ... Should we be concerned about solar energetic radiation? ...

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• Space Research Institute (IKI) Seminar
• The Acceleration of the Aurora
• MARSES Homepage | Project Information

ABSOLUTE PROPER MOTIONS OF 331 OPEN CLUSTERS . ... The proper motions of stars in the fields of 331 open clusters were taken from Four-Million Star Catalog (4M-catalog) of positions and proper motions (Volchkov et al. ... The absolute proper motions for 21 young open clusters have been derived by comparison of precise relative proper motions of individual stars and their corresponding absolute proper motions. ... Sign of proper motions in RA . ... 0.0001 arcsec/yr . ... rms error in RA proper motion . ...

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• Moscow Astronomical Plate Archives: Contents, Digitization, Current and