Network requirements from Ukrainian Physics and Astronomy communities Dr. Peter Berczik Main Astronomical Observatory Ukrainian National Academy of Sciences.

Slides:

Advertisements

Similar presentations

Development of China-VO ZHAO Yongheng NAOC, Beijing Nov

Advertisements

How special are brightest group and cluster galaxies? Anja von der Linden et al., 2007, MNRAS, 379, 867 On the prevalence of radio-loud active galactic.

Return to Hubble: Servicing Mission 4 Dr. Frank Summers Space Telescope Science Institute April 2, 2009.

Astronomy and the Electromagnetic Spectrum

Astrophysics from Space Lecture 1: Introduction Prof. Dr. M. Baes (UGent) Prof. Dr. C. Waelkens (KUL) Academic year

CESAR Educational Astronomy. Objective CESAR (Cooperation through Education in Science and Astronomy Research) will provide students all throughout Europe.

0 THE NETWORK OF ULTRAVIOLET ASTROPHYSICS Inform for the MTR Review to be held in Corfu (September 2007, 10-11) Prepared by: Prof. Ana Inés Gómez de Castro.

Above left: Optical and ultraviolet spectra (in red) of the Sirius-type binary BD , discovered with ROSAT and IUE in The white dwarf is clearly.

MACQUARIE UNIVERSITY, DEPARTMENT OF PHYSICS RESEARCH – ASTRONOMY & ASTROPHYSICS CORE Astronomy and astrophysics research has grown rapidly at Macquarie.

Long-Term Preservation of Astronomical Research Results Robert Hanisch US National Virtual Observatory Space Telescope Science Institute Baltimore, MD.

Light and Telescopes Chapter 5. Radio Interferometry The Very Large Array (VLA): 27 dishes are combined to simulate a large dish of 36 km in diameter.

Brian Schmidt, Paul Francis, Mike Bessell, Stefan Keller.

Online Data Archives for Use In the Classroom Robert Sparks (FNAL/The Prairie School) GLAST/SEU Educator Ambassador Workshop.

Leicester Database & Archive Service J. D. Law-Green, S. W. Poulton, J. Osborne, R. S. Warwick Dept. of Physics & Astronomy, University of Leicester LEDAS.

THE SEARCH OF GIANT RADIO GALAXIES AT DECLINATIONS FROM 3 TO 12 DEGREES Pushchino Radio Astronomy Observatory of Astro Space Center Tyul’bashev S.A., Gliantsev.

The Use of Infrared Color-Color Plots to Identify Rare Objects in the Galactic Mid-Plane Jessica Fuselier Dr. Robert Benjamin, advisor.

A student project. What is a space telescope?  A space telescope is a telescope that orbits around Earth in space.  Like other telescopes they take.

Long-Term Preservation of Astronomical Research Results Robert Hanisch US National Virtual Observatory Space Telescope Science Institute Baltimore, MD.

Introduction of Space Technology. The James Webb Space Telescope The James Webb Space Telescope was previously known as the Next Generation Space Telescope.

Stellar Evolution: from star birth to star death and back again Prof. David Cohen Dept. of Physics and Astronomy.

Hubble Space Telescope Advanced Space Academy Fall 2003 USSRC Proprietary.

Stars and Cells Kathy Cooksey Astronomy Overview.

Science & Technology.

Modern Telescopes Lecture 12. Imaging Astronomy in 19c Photography in 19c revolutionize the astronomy Photography in 19c revolutionize the astronomy 

P olarized R adiation I maging and S pectroscopy M ission Probing cosmic structures and radiation with the ultimate polarimetric spectro-imaging of the.

The Cosmic Simulator Daniel Kasen (UCB & LBNL) Peter Nugent, Rollin Thomas, Julian Borrill & Christina Siegerist.

1 New Frontiers with LSST: leveraging world facilities Tony Tyson Director, LSST Project University of California, Davis Science with the 8-10 m telescopes.

COMPUTER MODELS FOR SKY IMAGE ANALYSIS OF THE INASAN ZVENIGOROD OBSERVATORY Sergei Pirogov ( Institute of Astronomy, Russian Academy of Sciences) VIIth.

IXYZ Frank Marshall NASA/GSFC 25 April 2012 April 25, 20121Implementing Portals of the Universe.

IOP Publishing Lukas Piasecki Regional Manager – Eastern Europe IOP Publishing or Institute of Physics

The Hard X-ray Modulation Telescope Mission

Radio Galaxies and Quasars Powerful natural radio transmitters associated with Giant elliptical galaxies Demo.

Innovations in the Multimission Archive at STScI (MAST) M. Corbin, M. Donahue, C. Imhoff, T. Kimball, K. Levay, P. Padovani, M. Postman, M. Smith, R. Thompson.

World Space Observatory/ UV: Status report ( materials for the presentation of Mr. Yu.Nosenko ) Mr. Yu.Nosenko ) WSO/UV is an international space observatory.

VII th Bulgarian-Serbian Astronomical Conference (VII BSAC): 1- 4 June, 2010, Chepelare, Bulgaria DIGITIZING OF THE ASTRONOMICAL PHOTO PLATES IN THE NATIONAL.

Research Networks and Astronomy Richard Schilizzi Joint Institute for VLBI in Europe

The Sloan Digital Sky Survey ImgCutout: The universe at your fingertips Maria A. Nieto-Santisteban Johns Hopkins University

The Virtual Observatory Europe and the VO: the Astrophysical Virtual Observatory and the EURO-VO Astrophysical Virtual Observatory and the EURO-VO Paolo.

Prospects for observing quasar jets with the Space Interferometry Mission Ann E. Wehrle Space Science Institute, La Canada Flintridge, CA, and Boulder,

Nov Common Archive Observation Model What is CAOM and why should MAST use it? Brian McLean.

Advanced Technologies in Education Virtual Observatory 1 Virtual Observatory: D-Space Project Athens, 14 November 2004 Elena Tavlaki Head of Research Programs.

CELT Science Case. CELT Science Justification Process Put together a Science Working Group –Bolte, Chuck Steidel, Andrea Ghez, Mike Brown, Judy Cohen,

Investigation of different types radio sources by IPS method at 111MHz S.A.Tyul’bashev Pushchino Radio Astronomy Observatory, Astro Space Center of P.N.Lebedev.

G. Miknaitis SC2006, Tampa, FL Observational Cosmology at Fermilab: Sloan Digital Sky Survey Dark Energy Survey SNAP Gajus Miknaitis EAG, Fermilab.

What Does the Infrared Have to Do With Space?

The Large Synoptic Survey Telescope: The power of wide-field imaging Michael Strauss, Princeton University.

Application of Decision Trees Decision trees have been used in many areas. One notable area is star-galaxy classification. As an example, the Space Telescope.

Data Archives: Migration and Maintenance Douglas J. Mink Telescope Data Center Smithsonian Astrophysical Observatory NSF

Theme 6 – Space Telescopes and Adaptive Optics ASTR 101 Prof. Dave Hanes.

X-ray sky survey of bright, serendipitous sources with 2XMMi at the AIP Speaker: Alexander Kolodzig Origin: Humboldt-Uni Berlin, Germany Institute:AIP.

Sharing scientific data: astronomy as a case study for a change in paradigm Présenté par Françoise Genova.

A llen A rray T elescope Low Hanging Fruit in The New Radio Sky or Radio Surveys and Transients with the Allen Telescope Array or The Same Road Twice Geoffrey.

Anomalously Blue Elliptical Galaxies in the Sloan Survey Mentor: Dr. Mike Fanelli, UNT Collaborators: Dr. Pam Marcum, TCU & NASA Headquarters Dr. Christian.

What is Astronomy? An overview..

The European Hubble Space Telescope Legacy Archive Wolfram Freudling.

FIRST LIGHT A selection of future facilities relevant to the formation and evolution of galaxies Wavelength Sensitivity Spatial resolution.

Wide-field Infrared Survey Explorer (WISE) is a NASA infrared- wavelength astronomical space telescope launched on December 14, 2009 It’s an Earth-orbiting.

Color Magnitude Diagram VG. So we want a color magnitude diagram for AGN so that by looking at the color of an AGN we can get its luminosity –But AGN.

Moving towards the Virtual Observatory Paolo Padovani, ST-ECF/ESO

Canadian contributions to space exploration

6.3 Telescopes and the Atmosphere

Planning Observations

Long-Term Preservation of Astronomical Research Results

What is Astronomy? An overview..

Space Technology 8.E.4B.5 Obtain and communicate information to describe how data from technologies (including telescopes, spectroscopes, satellites,

What is Astronomy? An overview..

Science Notes: Stnd 24 Date Standard 24: 8.ETS1.2

Science Notes: Stnd 24 Date Standard 24: 8.ETS1.2

The hubble telescope Carlota.

What is Astronomy? An overview..

Presentation transcript:

Network requirements from Ukrainian Physics and Astronomy communities Dr. Peter Berczik Main Astronomical Observatory Ukrainian National Academy of Sciences

Plan: 1. Status… 2. Problems… 3. Requirements… 4. Conclusions…

Ukrainian National Academy of Sciences ~30,000 scientific workers in 166 institutes

Physics and Astronomy division of Ukr. Nat. Acad. of Sci. ~7,500 scientific workers in 24 institutes

Institute profiles Astrophysics, Cosmology (Prof. Yuri Izotov) Astrophysics, Cosmology (Prof. Yuri Izotov) Geophysics (Prof. Yaroslav Yatskiv) Geophysics (Prof. Yaroslav Yatskiv) Space Physics (Dr. ) Space Physics (Dr. Vladimir Kuz’kov) High Energy Physics (Prof. Laszlo Jenkovszky) High Energy Physics (Prof. Laszlo Jenkovszky) Atomic and Nuclear Physics Atomic and Nuclear Physics Atmospheric and Oceanic Physics Atmospheric and Oceanic Physics Biological and Medical Physics Biological and Medical Physics Chemical Physics Chemical Physics General and Classical Physics, Fluid Dynamics General and Classical Physics, Fluid Dynamics Optics, Plasma Physics Optics, Plasma Physics Quantum Physics Quantum Physics Mathematical Physics Mathematical Physics

Internet connection of our division

Problems: Ukraine state budget: ~11 billion USD Ukraine state budget: ~11 billion USD Population: ~48 million Population: ~48 million UNAS budget: ~75 million USD UNAS budget: ~75 million USD Typical institute budget: ~450 k USD Typical institute budget: ~450 k USD Typical money for one scientists: Typical money for one scientists: 450 k USD/200/12 ~190 USD/month

Problems: No direct money for “INET” payments in academic budget!!! No direct money for “INET” payments in academic budget!!! No direct money for communication infrastructure development in academic budget!!! No direct money for communication infrastructure development in academic budget!!! The INET connection is a own problem of institutes, no have any free or “centralized academic network” services. The INET connection is a own problem of institutes, no have any free or “centralized academic network” services.

Requirements… INET for library services. The common “everyday task”. INET for library services. The common “everyday task”. – ~100 MB/day –ApJ, AJ, A&A, MNRAS… ~100 MB/day – ~100 MB/day

Requirements… Online catalogs and databases. “Virtual Observatory”… Online catalogs and databases. “Virtual Observatory”… – Hubble Data Archive (HDA) ~5.2 TB

Requirements… Other online catalogs and databases… Other online catalogs and databases… –The Digitized Sky Survey (DSS). The Catalogs and Surveys Branch of the STScI has been digitizing the photographic Sky Survey plates from the Palomar and UK Schmidt telescopes in order to support HST operations and provide a service to the astronomical community. Archive users can easily retrieve image data for any part of the sky. –The Sloan Digital Sky Survey (SDSS) is using a dedicated 2.5 m telescope and a large format CCD camera to obtain images of over 10,000 square degrees of high Galactic latitude sky in five broad bands (u', g', r', i' and z', centered at 3540, 4770, 6230, 7630, and 9130 A, respectively). The first data release, planned for June 2001, includes: imaging data containing a searchable catalog, images in several formats (FITS and JPEG), and spectra in both FITS format and GIF spectra with line identifications. This first public data release will contain over 500 square degrees of sky.

Requirements… Other online catalogs and databases… Other online catalogs and databases… –The Far Ultraviolet Exporer (FUSE) covers the A spectral region. This active mission contains high resolution spectra of hot and cool stars, AGNs, supernova remnants, planetary nebulae, solar system objects and the interstellar medium. The International Ultraviolet Explorer (IUE) Final Archive, which contains over 104,000 spectra of approximately 10,000 individual astronomical sources (covering the 1, ,350 A range). The Extreme Ultraviolet Explorer (EUVE) Archive, which at present contains spectroscopic observations (in the A range) of about 300 sources, mostly Galactic. The Ultraviolet Imaging Telescope (UIT) Archive, which contains 1,579 images of 259 targets (covering the 1, ,300 A range) obtained by UIT as part of the ASTRO-1 and ASTRO-2 missions. –The Faint Images of the Radio Sky at Twenty-centimeters (FIRST) Archive. The FIRST project is designed to produce a radio survey at 20 cm (1.4 GHz) of over 10,000 square degrees down to a flux of 1 mJy.

First permanent GPS network in Ukraine (NATO NIG: ) Daily transfer ~10 – 20 MB, but in ~1h -> need min. 64 Kbps channels!!!

Optical communication experiments with geostationary satellite

Telecommunication satellite ARTEMIS was launched on 12 July He has RF channels and SILEX device (Semiconductor Laser Inter Satellite Link Experiment) worked at 2 Mbps and 50 Mbps rates. ESA constructed the optical ground station at Tenerife Observatory, Canary islands for ground test of SILEX.

ESA and MAO proposed common experiment V.Kuz’kov, M.Medvedskij, D.Yatskiv, V.Nedashkovsky, Yu.Gluschenko, V.Suberljak, M.Peretytko, N.Eremenko.

Conclusions… We need a high band INET channels (> 2 Mbps) in all academic institutes for everyday scientific work – everyday scientific work – BUT without extra payment!!! BUT without extra payment!!!