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         Astronomy Research:     more books (100)
  1. The Particle Physics and Astronomy Research Council Order 1994 (Statutory Instruments: 1994: 425)
  2. A method of slitless absolute spectral photometry for application in reentry research and astronomy by Gale Allen Harvey, 1966

141. NOAO Data Archives
Operated by the Association of Universities for research in astronomy (AURA), Inc. Includes survey programs data archive, and links to other data collections.
http://www.noao.edu/archives.html
NOAO Data Archives
NOAO is operated by the Association of Universities for Research in Astronomy (AURA), Inc. under cooperative agreement with the National Science Foundation
Survey Programs Data Archive
The NOAO Deep Wide-Field Survey is a deep optical and near-infrared wide-field imaging survey that will sample the sky in two 9 square degree fields.
The following additional data collections or other resources are also available. Save-the-Bits (STB): CTIO and KPNO routinely copy and store most data from CCD's and infrared arrays at all their nighttime telescopes. These data are available only by special permission from the Director.
NSO Digital Library
GONG Data Storage and Distribution System (DSDS) : The GONG Data Storage and Distribution System has been developed to store and catalog the data products produced by the GONG pipeline, and to provide the GONG scientific community with tools to access the catalog of data products, to submit a request for these data products, and to distribute data files to those requesting them. Access to these tools is provided through a user's account on a UNIX workstation serving as the GONG Users' Machine. The GONG Data Policy requires that access to data be through this account, obtained by submitting both a

142. George P. McCook
Specializes in mathematic analysis of astronomical data. Chairperson and professor of astronomy at Villanova University. Includes education background and research.
http://www.astronomy.villanova.edu/faculty/mccook/mccook.htm
GEORGE P. McCOOK
Chairperson and Professor of Astronomy
Bachelor Degree of Science
Mathematics, Villanova University, 1959 Master Degree of Arts
Mathematics, Villanova University, 1961 Doctoral Degree
Astronomy, University of Pennsylvania, 1968 Research Interests
Mathematical Analysis of Photometric Data
Design of Microcomputer-controlled data collecting systems
Development of Data Management and Analysis Software
Variable Stars, Protoplanetary Disks in Binary Systems Current Research

143. National Radio Astronomy Observatory
research facility of National Science Foundation, operates many radio telescope observatories.
http://www.nrao.edu/
Monday, June 07, 2004 Quick Links: INFORMATION FOR: General Public Astronomers NRAO Staff USEFUL LINKS: Press Releases Newsletter Meetings/Events Image Gallery ... VLBA Welcome to NRAO!
Previous photo
Next photo The National Radio Astronomy Observatory (NRAO) is one of the world's premier research facilities for radio astronomy. NRAO operates powerful, advanced radio telescopes spanning the western hemisphere. Scientists from around the world use these instruments to probe fundamental questions in astronomy and physics. RADIO IMAGE OF THE DAY Supernova 1993J
Learn more about this image in the NRAO Image Gallery
NRAO NEWS May 3, 2004 - Ethan J. Schreier Named President of Associated Universities, Inc. (AUI News) April 1, 2004 - Radio Astronomers Lift "Fog" on Milky Way's Dark Heart: Black Hole Fits Inside Earth's Orbit March 25, 2004 -

144. University Of Cambridge: Department Of Physics: Astrophysics Group
A wideranging program of research, including the Mullard Radio astronomy Observatory, situated at Lord's Bridge. Group members, research interests, publications, surveys and catalogues, other resources.
http://www.mrao.cam.ac.uk/
Astrophysics Group
Department of Physics University of Cambridge Dept of Physics
The Astrophysics Group
at the Cavendish Laboratory
manages a wide-ranging programme
of research, and runs the
Mullard Radio Astronomy Observatory
situated at Lord's Bridge Information about
Information provided by webman

145. Www.wiley-vch.de
Founded in 1821 by H.C. Schumacher, is the oldest astronomical journal worldwide still being published. Publishes papers on all fields of astronomy and astrophysics and review papers on special and current topics. The journal covers a wide range of issues reaching from cosmology, extragalactic research, cosmic hydrodynamics, stellar physics, interstellar matter, solar and planetary physics to geodetic astronomy.
http://www.wiley-vch.de/berlin/journals/an/index.html
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146. Physics & Astronomy - Research Activity
Physics astronomy » research Activity. Institute for Gravitational research, Particle Physics Experiment, Particle Physics Theory.
http://www.physics.gla.ac.uk/research/
Research Activity
Institute for Gravitational Research
Particle Physics Experiment
Particle Physics Theory
Solid State Physics
Nuclear Physics
Optics
Microwave Thermography Learn more about opportunities in postgraduate research in this department

147. IA - BAS
Carries out fundamental research in astronomy, astrophysics, and teaching specialists in this domain.
http://www.astro.bas.bg/
INSTITUTE OF ASTRONOMY Bulgarian 07 Jun Mon, 2004 Administration Staff Sectors News ...
Publications

JD
LAST UPDATE INSTITUTE OF ASTRONOMY
The main activity topic of the Institute of Astronomy is to carry out foundamental research in astronomy and astrophysics and teaching specialists in this domain.
Institute of Astronomy, Bulgarian Academy of Sciences (IA-BAS) was established in 1995 as a successor of the Section of Astronomy and National Astronomical Observatory (SA with NAO, BAS).
Academician Nikola Bonev was the founder and first director of SA, the first collaborator was senior research fellow Dr. Malina Popova. First director of IA-BAS was Prof. Vladimir Shkodrov.
The Institute has two observatories:
National astronomical observatory "Rozhen"

Belogradtchik observatory

148. Physics & Astronomy @ University Of Leicester
General departmental information, as well as information for prospective and current students, and details of ongoing research.
http://www.le.ac.uk/physics/
Physics and Astronomy
T has a national and international reputation for excellence in teaching and research. It achieved the top (Grade 5) research rating in the previous three HEFCE assessments (1992, 1996 and 2002) and was rated excellent in the last Teaching Quality Assessment (1999). ! HOT NEWS !
In the early morning of June 8th this year, the tiny disk of the planet Venus will be seen passing in front of the Sun. The last such "Transit of Venus" occurred in 1882. A variety of events will be held at throughout the day at the National Space Centre in Leicester. Click HERE HERE , and information about the observations being made by astronomers and students in the Department can be found HERE home information for prospective students
information for current students

Last updated: 30th July 2002

149. UD Physics & Astronomy
Offers department directory, latest news, seminar schedules, and event announcements, with overview of the department, curriculum, and research activities.
http://www.physics.udel.edu/
Faculty:
Research Grants: $3 million/yr Department
overview
Undergrad
courses, advising
...

e-BULLETIN BOARD
(Web pages use css files, view with IE 7+, or Mozilla University of Delaware Home Send comments/web errors to: webmaster Physics and Astronomy Home

150. Soumen Mondal's Home Page
Specializes in high angular resolution astronomy. Includes publications and research interests. Department of Space, India.
http://www.prl.ernet.in/~soumen/
Soumen Mondal's home page
Soumen Mondal Astronomy and Astrophysics Division Physical Research Laboratory Ahmedabad-380 009, INDIA Email: soumen@prl.ernet.in Presently I am a Post Doctoral Fellow of Astronomy Division of Physical Research Laboratory , Department of Space , India.
Current research studies : Infrared Instrumentation High speed Near Infrared Photometer
Click here
Dust structure around Wolf-Rayet Star Our high angular resolution studies by lunar occultation at 2.2 micron First discovered stellar pinwheel in the sky by Keck 10m Dust structure around Carbon Mira CW Leo High angular resolution studies by LO Atmosphere of Mira and Semi-regular Variables :
Personal details : My CV : updated on 26. 11.2002 List of Publications (ADS Search) :
Other Link : My home-town My family

Useful links for Astronomy

Useful link for Computers

151. Astronomical Research At The MPIfR/AIUB
In addition, and in notable contrast to other European centres for radio astronomy, Bonn offers a research environment which provides the necessary
http://www.mpifr-bonn.mpg.de/imprs/web3_research.html
Max Planck Institute for Radio Astronomy (MPIfR)
The Institute
radio telescope International co-operations with various institutes like the give the scientists working at the MPIfR access to the whole radio wavelength range usable from the surface of the Earth.
The location of the MPIfR in the same building as the Astronomical Institutes of the University of Bonn encourages joint research activities and provides easy and immediate access for students at the MPIfR to the large number of astronomical courses and seminars held at the university. This has over the years made this location an attractive choice for astronomy students. Research fields The 100 meter telescope is capable for radio observations in different observing modes, like
  • radio continuum - the investigation of galactic and extragalactic sources in broad bands at several wavelengths, spectroscopic investigations of galactic and extra galactic sources

152. ACIGA
ACIGA is intended to undertake research and development aimed at improving the performance of present laser interferometer gravitational wave detectors through advanced designs to ultimate limits set by mechanics, quantum mechanics, lasers and optics; and to transfer this into practical designs that can be used in production of commercial products.
http://www.anu.edu.au/Physics/ACIGA/
Welcome to the Australian Consortium for Interferometric Gravitational Astronomy (ACIGA) web page.
A short introduction to gravitational waves, see
Catching gravitational waves
Objectives
In collaboration with the world gravitational wave community, the objectives of ACIGA are to:
  • Undertake research and development aimed at improving the performance of present laser interferometer gravitational wave detectors through advanced designs to ultimate limits set by mechanics, quantum mechanics, lasers and optics;
    Arrange conferences, seminars and workshops as required to compliment and enhance the research of the members of the consortium.
  • Latest News
    LIGO newsletter 2002 ACIGA receives major research funding for the high optical laser power test facillity AIGO, situated at Gingin, Western Australia First meeting of ACIGA (ANZAC Week 2002 at Gingin).
    Management Structure
    ACIGA Board Consists of the representatives of the ACIGA membership including all partners. Acts as an advisory board for all ACIGA operations including input from the International groups and Australian government and industry bodies.
    ACIGA Chairperson
    Prof David E McClelland

    Australian National University
    AIGRC Director
    Prof David G Blair

    University of Western Australia
    Prof Jesper Munch
    University of Adelaide
    Institutions
    ACIGA involves the collaboration of several institutions throughout Australia. Follow the links to find out more information about the research of each institution, employment opportunities, research scholarships and publications.

    153. Astronomical Research At The MPIfR/AIUB
    In addition, and in notable contrast to other European centers for radio astronomy, Bonn offers a research environment which provides the necessary
    http://www.mpifr-bonn.mpg.de/imprs/Web3_Research.html
    Max-Planck Institut for Radio Astronomy (MPIfR)
    The Institute
    radio telescope International co-operations with various institutes like the give the scientists working at the MPIfR access to the whole radio wavelength range usable from the surface of the Earth.
    The location of the MPIfR in the same building as the astronomical institutes of the University of Bonn encourages joint research activities and provides easy and immediate access for students at the MPIfR to the large number of astronomical courses and seminars held at the university. This has over the years made this location an attractive choice for astronomy students. Research fields The 100-m telescope is capable for radio observations in different observing modes, like
    • radio continuum - the investigation of galactic and extragalactic sources in broad bands at several wavelengths, spectroscopic investigations of galactic and extra galactic sources

    154. Icarus
    The official publication of the Division for Planetary Sciences of the American Astronomical Society. It is dedicated to reporting the results of new research observational, experimental, or theoretical concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our solar system or extrasolar systems.
    http://astrosun.tn.cornell.edu/Icarus/
    Icarus has moved to http://icarus.cornell.edu

    155. Physics And Astronomy
    A source of information for undergraduate admissions, current students and staff. A welcome to the department and details of research are also present.
    http://www.sussex.ac.uk/physics/
    Physics and Astronomy
    Welcome to Physics and Astronomy at Sussex
    We provide stimulating teaching and pioneering research in an academic setting that is uniquely interdisciplinary. Our working environment is relaxed and friendly, with a campus set amidst the beautiful South Downs yet only five minutes from the vibrant seaside city of Brighton.

    Related Activities and Interest Groups: events Photo exhibition: Children of Iraq's Wars
    1200 - 1700 Monday, 7 June @ Ground floor (the open space), Arts D
    Experimental Particle Physics Seminar: Neutron EDM - Beyond the Standard Model

    1200 Wednesday, 9 June @ Pevensey 1 - 1A3
    more events...

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    156. Astronomy, Research In Astronomy
    This 2 outside of astronomy. It prepares the student for independent research in astronomy.......Track. research in astronomy.
    http://www.science.leidenuniv.nl/graduateschool/index.php3?m=32&c=67

    157. UNL Department Of Physics And Astronomy
    Provides news and a special events calendar, class schedules and descriptions, research group highlights, facilities overview, and departmental directory, history, and general information.
    http://www.physics.unl.edu/
    Calendar of Events Welcome to the Department of Physics and Astronomy at the University of Nebraska-Lincoln Follow the links above to learn about the Department, its academic programs, research and outreach activities. Visit the calendar of events for an up-to-date list of colloquia, seminars and other events happening in the Department.
    Department of Physics and Astronomy
    116 Brace Laboratory
    University of Nebraska-Lincoln
    Lincoln, NE 68588-0111
    Phone: (402) 472-2770
    Fax: (402) 472-2879

    158. Gamma Ray Astrophysics At The NSSTC
    research into gammaray phenomena, such as pulsars, black holes, other galaxies, gamma-ray bursts and exotic astrophysical objects.
    http://gammaray.msfc.nasa.gov
    The Gamma-Ray Astronomy Team Home Page gammaray.nsstc.nasa.gov BATSE
    GLAST Burst Monitor

    Personnel

    Local
    ...
    NASA Home
    The Gamma-Ray Astrophysics Team of the National Space Science and Technology Center welcomes you to its home page. Our group includes scientists and engineers from NASA's Marshall Space Flight Center, Universities Space Research Association (USRA) and the University of Alabama in Huntsville (UAH). We are actively involved in several projects which are designed to investigate the high energy regime of our Solar System and Universe. The primary objectives of our research are to study gamma-ray phenomena such as pulsars black holes other galaxies gamma-ray bursts , and other exotic astrophysical objects.
    Current Projects
    The Compton Gamma Ray Observatory, about to be released from Space Shuttle Atlantis in 1991 April. The eight BATSE detector modules are mounted on the corners of the satellite. Four are visible in the image. T he Burst and Transient Source Experiment. During 9 years of successful operation, the BATSE detectors on the Compton Gamma-Ray Observatory (CGRO) continually recorded observations of gamma-ray bursts, pulsars, and other transient gamma-ray phenomena. Although the CGRO mission was terminated by NASA in June 2000, new science from BATSE and complete data archiving projects continue to occupy members of the GRA team and provide services to the high-energy astrophysics community. The Principal Investigator of this project is

    159. APICS Physics And Astronomy Committee
    The committee affords astronomers and physicists the chance to share expertise in teaching and research. Focus is on undergraduate conference series, lecture tours, and physics and astronomy resources. Lists committee and email contacts.
    http://apwww.stmarys.ca/APICS/
    The APICS Physics and Astronomy Committee
    History The APICS Undergraduate Physics and Astronomy Conference Series (AUPAC) Physics and Astronomy Resources in Atlantic Canada and Beyond
    The Committee
    Chair Craig Bennett Acadia University Secretary and
    Tour Coordinator Adam Sarty Saint Mary's University Past Chair David Tindall Dalhousie University John Lewis Memorial University Pravin Varma Mount Allison University Michael Steinitz Saint Francis Xavier University Francis Weil Abdelhaq Hamza University of New Brunswick Maintained by Malcolm Butler . Last updated February 20, 2003.

    160. LNA/SOAR
    What is the SOAR Telescope (SOuthern Astrophysical research Telescope)? Michigan State University (MSU) and the National Optical astronomy Observatories (NOAO
    http://www.lna.br/soar/soar_e.html
    Last updated:
    April 19, 2004 Home SOAR site A 4.1-meter Telescope Built and Operated as a Brazil/USA partnership. The telescope Instrumentation Gallery of images Links Comments and
    suggestions:
    webmast@lna.br
    What is the SOAR Telescope - ( SO uthern A strophysical R esearch Telescope
    The project is a partnership between Brazil represented by CNPq and USA by the University of North Carolina (UNC), Michigan State University (MSU) and the National Optical Astronomy Observatories (NOAO).
    SOAR is an f/16 Ritchey-Chrétien optical design delivering an 8 arcminute diameter field of view for science with a 50-Hertz tip-tilt stabilized image
    The telescope has dual multi-bay Nasmyth observing ports on the sides of the telescope structure and three bent Cassegrain ports within the telescope itself. The incoming light beam is directed to a specific instrument with the tertiary mirror turret and subsequent fold mirrors. Each Nasmyth port can support an 8-meter telescope class instrument, which allows the SOAR partners to set-up shared use of appropriate instruments. SOAR is situated on Cerro Pachón at an altitude of 2,700 meters above sea level, at the Chilean Andes. The telescope and its white spherical dome sit a few hundred meters from the neighboring 8-meter Gemini South telescope, and within visual range of NOAO’s Cerro Tololo Inter-American Observatory.

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