81. National Optical Astronomy Observatory NOAO is a national center for optical astronomy in the United States, operated by the Association of Universities for research in astronomy. http://www.noao.edu/

Cerro Tololo NOAO Gemini Science Center Kitt Peak GSMT ... O/IR System This wide-field image of the Crescent Nebula (NGC6888) was taken at the National Science Foundation's 0.9-meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Image credit: T.A. Rector (NRAO/AUI/NSF and NOAO/AURA/NSF) About NOAO Tourist Information News Releases Educational Resources ... Employment Opportunities First volume of Astronomy Education Review complete 2003B Proposal Queue Status NOAO Newsletter #73 NOAO Annual Report, FY 2002 NOAO Science Archive V2.0 Released ... NOAO is the national center for ground-based nighttime astronomy in the United States and is operated by the Association of Universities for Research in Astronomy (AURA), Inc. under cooperative agreement with the National Science Foundation . If you would like information about solar astronomy, visit the National Solar Observatory webmaster@noao.edu

82. NCSA Astronomy Digital Image Library (ADIL) collects astronomical, researchquality images and make them available to the astronomical community, and the general public. Offers Library access, image browse, and FITS links. http://imagelib.ncsa.uiuc.edu/imagelib.html

Introducing the ADIL: Who and What is the ADIL? ADIL News Highlights from the Library Java and the ADIL Topics from the ADIL User's Guide Using ADIL Images Client Viewers How to Deposit Images Finding Images: Query Page Get By Code Contact the ADIL at adil@ncsa.uiuc.edu What's New New Web Address for the ADIL ADIL server upgrade New Experimental AML Server Who and What is the ADIL? The purpose of the Astronomy Digital Image Library (ADIL) is to collect astronomical, research-quality images and make them available to the astronomical community and the general public. Patrons access the Library through the World Wide Web to search for and browse images. Once images are located in the Library, users may download them to their local machines in FITS format for further analysis. The Library provides a number of benefits not only to those looking for images, but also to those who add images to the Library's growing collection. For more on what the ADIL is all about, check the introduction to the ADIL User's Guide The Library is being developed and maintained by the Radio Astronomy Imaging Group at the National Center for Supercomputing Application (NCSA) on the campus of the University of Illinois at Urbana-Champaign (UIUC) . Support has come from: the National Aeronautics and Space Administration (NASA) through Project Horizon, a cooperative agreement with

83. 1st All Astronomy Site organized for education, research and the enjoyment of astronomy. http://www.1st-all-web-site-promotion.com/~1st-all-astronomy/

84. University Of Surrey - Department Of Physics (Research) University of Surrey abridged version of the book Astrophysics , with many links to relevant material on astronomy, astrophysics and cosmology. http://www.ph.surrey.ac.uk/astrophysics/index.html

University of Surrey Department of Physics These pages require a browser that can view frames. To update your browser so it can view these pages, please download the latest versions of either: Internet Explorer

85. New Astronomy Publishes articles in all fields of astronomy and astrophysics theoretical, observational and instrumental. Includes full length research articles and letter articles. The Journal covers solar, planetary, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gammaray. http://www1.elsevier.nl/journals/newast/

Welcome to New Astronomy, the first fully electronic research journal in astronomy and astrophysics, since 1996. With an impact factor of 2.24, New Astronomy is one of the research journals in Astronomy and Astrophysics with the highest impact factors. Quality is maintained by a group of esteemed Receiving Editors Prospective authors are encouraged to submit their articles to New Astronomy. Apart from publishing in a journal with one of the highest impact factor, you will benefit from the following features: Over 50,000 Astronomers and Astrophysicists are reached via the major scientific data base Science Direct Over 20% of these scientists at the most prominent research institutes receive an email-alert about the publication of your article Easy electronic access to your article, immediately after acceptance Your article can be accessed through ADS No page charges Free reprints of your article For any additional information on Elsevier Science’s astronomy program, click here

86. UCLA Physics & Astronomy - RESEARCH GROUPS UCLA Department of Physics astronomy Links to research. ** PLEASENOTE email asg@physics.ucla.edu with new information, corrections http://www.physics.ucla.edu/research/

Home Astronomy Classes Graduate ... People Research Events Resources PLEASE NOTE : email asg@physics.ucla.edu with new information, corrections, updates and additions to this page. This research page is constantly being updated with links to new research going on at UCLA ( last update july 2002) condensed matter physics experimental elementary paticle physics nuclear physics plasma advanced accelerators ... theoretical elementary particles Condensed Matter Physics Hard Condensed Matter Physics Group Soft Condensed M atter Physics Group Hard Condensed Matter Physics Group THEORY Sudip Chakravarty Steve Kivelson Chetan Nayak EXPERIMENTAL Rubin Braunstein Stuart Brown Gil Clark Karoly Holczer Hon-Wen Jiang Kumar Patel Websites: Hard Condensed Matter Group Single Electron Spin Microscope - Karoly Holczer back to top Soft Condensed M atter Physics Group THEORY Robijn Bruinsma

87. US Psionics - Home Page research includes numerology, radionics, millennial studies. Links to astronomy, UFO, and alternative science sites. http://www.uspsionics.com/

The Black Vault Banner Exchange A Zipgate Site Home News Research Products Links In This Section US Psionics About Us About Psionics More Psionics Additional Info ... Peaceful Page II Other Links Psi Software Charles Cosimano Basic Psionics Plans for Psionics devices ... Autogenic course A Bit About US Psionics: US Psionics is an independent research and development entity dedicated to investigating those phenomena and technologies of the world around us that traditional investigators are hesitant to become involved with, either because the subject is TABOO, or because the subject matter is NEW and FRIGHTENING. US Psionics is very aware that the accepted knowledge of today was often the crackpot science of yesterday. Examples of this are our modern acceptance of Anti-Oxidants, Quantum Mechanics, Continental Drift, and Relativity. US Psionics is intent on bringing you the information and products that will enable you to investigate, research, and understand the Psi-oriented and Para-oriented arts and sciences. Be Sure to Review Our Research Projects , Our Numerology Pages , Order a Customized Numerological Talisman , Visit Our Breaking News and Links Pages , and Investigate Our New Product, CYBERSHAMAN . See our free Cybershaman offer below. CyberShaman combines new technology with ancient science . The result is a Psionics / Radionics program so powerful, it must be experienced to be appreciated.

88. UCSC - Department Of Astronomy & Astrophysics Department of astronomy and Astrophysics at UCSC. Site includes descriptions of faculty and student research, information for current and prospective graduate students, and the popular ask an astronomer feature. http://www.astro.ucsc.edu/

Skip Astronomy Home Directory Research ... Online UCSC is one of the world's leading centers for both observational and theoretical research in astronomy and astrophysics. The department includes twenty-two faculty members, whose research interests range from the Solar System and the Milky Way to the most distant galaxies in the Universe and the most fundamental questions of cosmology. There are typically over a dozen postdoctoral researchers in residence, as well as a dedicated and skilled technical staff and a steady stream of visiting scientists. The UCSC department was recently ranked first in the country in research impact, based on citation studies. UCSC is also a leader in astrophysics education. The department currently enrolls about twenty-five students working towards the Ph.D. degree. Graduate students benefit from the low student-faculty ratio in the department and extensive research opportunities, as well as course offerings that cover both theoretical and observational aspects of astronomy. UCSC alumni hold positions at leading universities and research institutes around the world. The department offers an undergraduate minor in Astrophysics, and collaborates with the Physics department to offer an undergraduate major in Astrophysics. The department is involved in several major interdisciplinary research projects. The Center for Adaptive Optics is an NSF Science and Technology Center that is studying new optical correction techniques with applications in both astronomy and vision science. It is based at UCSC, but involves researchers from nearly two dozen academic, governmental, and industrial partners. The Center for the Origin, Dynamics and Evolution of Planets is part of UCSC's branch of the Institute for Geophysics and Planetary Physics. It brings together members of the Astronomy, Earth Sciences, and Physics departments to study planets in our Solar System and around other stars. Members of the Astronomy department interested in cosmology and high energy astrophysics also interact frequently with colleagues in the Physics department and the Santa Cruz Institute for Particle Physics.

89. NRAO: Socorro, New Mexico A research facility of the United States National Science Foundation. Site contains an image gallery, an introduction to radio astronomy, and other related information. http://www.aoc.nrao.edu

document.write(dayNames[day] + ", " + monthNames[month] + " "); document.write(date + ", " + year ); document.write(" "); NRAO Home Current Events Public Outreach Frequently Asked Questions Press Releases Introduction to Radio Astronomy For Visitors Official Visitors Tourists Very Large Array Very Long Baseline Array ... Assistant Director's Page Updated 2003-Mar-19 Socorro, New Mexico Socorro, New Mexico, is the home of NRAO operations in New Mexico. Located on the campus of New Mexico Tech , the Array Operations Center houses scientific, engineering, technical, computer and support staff for both the Very Large Array and the Very Long Baseline Array. It includes the control center and correlator for VLBA observations and provides space for the Atacama Large Millimeter Array project. The Very Large Array (VLA) , one of the world's premier astronomical radio observatories, consists of 27 radio antennas in a Y-shaped configuration on the Plains of San Agustin 80 km (50 miles) miles west of Socorro, New Mexico. Each antenna is 25 meters (82 feet) in diameter. The data from the antennas is combined electronically to give the resolution of an antenna 36km (22 miles) across, with the sensitivity of a dish 130 meters (426.5 feet) in diameter. Twilight at The Very Large Array, near Socorro, New Mexico

90. CU Astronomy - Research research Facilities Arecibo Observatory Observatory. SPIGOT SETI, Pulsar,ISM, Gamma rays, Observations, and Theory research Group. WIRE - Wide http://astrosun.tn.cornell.edu/research/

HOME OVERVIEW PEOPLE ACADEMICS RESEARCH Facilities Arecibo Observatory Palomar Observatory SPIF ... WIRE Undergraduate Opportunities NAIC Summer Program PEW REU Space Grant Job Openings EVENTS RESOURCES Research Facilities Arecibo Observatory - Cornell operates this facility near Arecibo, Puerto Rico year round. Arecibo site contains is the world's largest radio telescope. Palomar Observatory - Located on Palomar Mountain in California, Cornell operates the gigantic 200-inch Hale Telescope on a quarter-time basis, sharing the scope with Caltech. SPIF - The Spacecraft Imaging Facility, located on the third floor of the Space Sciences building on the Cornell Campus, provides the image processing and archival facilities needed for maintaining and cataloging the visual data collected by numerous spacecraft. Projects Atacama Telescope - Investigations in the feasibility of a large optical/ infrared telescope in a high altitude plateau in Northern Chile.

91. Swarthmore Women In Astronomy And Physics - Physics And Astronomy REU Reviews Studentwritten reviews of REUs and other summer undergraduate research programs jobs, plus answers to FAQs and useful related links http://d38.dupont01.swarthmore.edu/~wip/reureviews/

The Swarthmore Women in Astronomy and Physics site for reviews of physics and astronomy REUs site has moved to http://www.sccs.swarthmore.edu/org/swap/reureviews/

92. CU Department Of Astronomy : Research research SPIFI South Pole Imaging Fabry-Perot Interferometer. SPIGOT - SETI,Pulsar, ISM, Gamma rays, Observations, and Theory research Group. http://astrosun.tn.cornell.edu/research/index.shtml

Projects Astrophysics and Relativity Theory Group Atacama Telescope ... Job Openings Search Cornell Astronomy: Research Projects Astrophysics and Relativity Theory Group - Faculty and projects associated with theoretical astrophysics and relativity. Atacama Telescope - Investigations in the feasibility of a large optical/ infrared telescope in a high altitude plateau in Northern Chile. Athena - Developing tools for use on the Mars Surveyor lander and rover. Black Holes and Gravitational Waves - Solving Einstein's equations on supercomputers. C-N Galaxy Pair Study - Investigating dark matter in isolated and small groups of galaxy pairs. CONTOUR - An unmanned spacecraft that will analyze the nuclei of three comets from close range. CORMASS - A low-resolution NIR Spectrograph used on the Palomar 60-inch telescope primarily for the study of very low mass stars and brown dwarfs. EGG - Researchers interested in extragalactic study and observational cosmology. FORCAST - A Wide-Field Infrared Camera for SOFIA.

93. Welcome To The Oxide Physics Research Programme Web Pages The programme is a collaboration of experimental and theoretical physicists working on the behaviour of correlated electrons in oxide materials. Based in the School of Physics and astronomy at Birmingham University, United Kingdom. Materials of interest include the high temperature cuprate superconductors, nonFermi liquid physics near quantum critical points, unconventional superconductivity in the ruthanates and heavy fermion behaviour in lithium vanadate. http://www.th.ph.bham.ac.uk/oxides/Welcome.html

Welcome to the home page of the Oxide Research programme in the School of physics and astronomy at Birmingham University, United Kingdom. This describes a collaboration of experimental and theoretical physicists and material scientists concerned with the physics of strongly correlated electrons in oxide materials. Materials of interest to us include the high temperature cuprate superconductors, non-Fermi liquid physics near quantum critical points, unconventional superconductivity in the ruthanates and heavy fermion behaviour in lithium vanadate. The work is coordinated by Dr Andy Mackenzie and Dr Andy Schofield. Javascript version of web pages Version of web pages without javascript Research programme Group members ... Contacting us

94. Modern Research By Eduard Westra research done about low mass black holes. On the level of 2nd year astronomy students. http://www.astro.rug.nl/~westra/aoz

In our second year we have to carry out a project about a subject in astronomy. This year we chose for black holes . Now we had to think of a main question, which has become: Do black holes exist in our Universe? To answer this question we divided the question into subquestions. My subquestion is: How can stars evolve into black holes? This question is very important to answer the main question, because the current theories say that IF black holes are created there are three different sizes: very low mass black holes: about 10 to 10 M sun low mass black holes: about 10 to 10 M sun heavy mass black holes: about 10 to 10 M sun If there should be low mass black holes you should think that they have a progenitor of the massrange of a star. Of which kind of an object do you think of when you have an object in the massrange of a star? On the ground of the mass of a black hole you can assume that stars can evolve into low mass black holes. The other two categories will be explained by colleagues of mine. They think that very low mass black holes originate from primordial black holes. About high mass black holes, which will be in the center of galaxies, they have different theories. The subquestion is subsequently devided into four subquestions.

95. ASU Physics & Astronomy | Research Past and current research underway at the Physics and astronomy departmentat Arizona State University. ASU Physics astronomy. http://phyastweb.la.asu.edu/research/

Research is undertaken in Physics and Astronomy in the following areas: Astronomy and Astrophysics Biophysics Condensed Matter Physics: Experiment Condensed Matter Physics: Theory ... Surface Science and Materials Physics For details of each area, including faculty lists and individual topics, projects and publications, click on the above list; alternatively, join the department tour for an overview. Privacy Tempe, AZ 85287 Information@asu.edu Page Contact: phyastweb@asu.edu

96. Jodrell Bank Pulsar Group Home Page As one of the research groups of the Jodrell Bank Observatory, we form part of the Department of Physics and astronomy of the University of Manchester, in the United Kingdom. We have many collaborations with other research groups across the world and, in particular, with the ATNF with whom we are the main partners in the Parkes Multibeam Pulsar Survey http://www.jb.man.ac.uk/~pulsar/index.html

97. ASU Physics & Astronomy | Research - Astronomy And Astrophysics astronomy and astrophysics research at the Physics andastronomy department at Arizona State University. http://phyastweb.la.asu.edu/research/ast/

Astronomy and Astrophysics P.A. Aannestad, D. Burstein, A.P. Cowley, J. J. Hester, S.C. Odewahn (Academic Professional), P.A. Scowen (Academic Professional), S.G. Starrfield, L.L. Stryker (ASU West Campus), R.A. Windhorst, S. Wyckoff Arizona State University is one of the most active and dynamic centers of astronomical research of its size in the nation. The astronomy group consists of eight full-time faculty members plus two academic professionals, several affiliated faculty and postdoctoral fellows. The group's research spans a wide variety of topics in observational astronomy and theoretical astrophysics, including the solar system, the structure and physics of the interstellar medium, novae and cataclysmic variables, compact objects, galactic structure, and cosmology. ASU's astronomers enjoy national and international prominence for their work, and are involved in collaborations with researchers around the world. Among the most important strengths of ASU's program is the access students have to a wealth of nearby resources. The state of Arizona is home to numerous world-class astronomical observing facilities, all within a four-hour drive of the Tempe campus. ASU astronomers are formally associated with the

98. AstroWeb: Astronomy/Astrophysics On The Internet Nearly 3000 links in 36 distinct subject areas, such as telescopes, libraries, images, conferences, research and researchers. http://www.stsci.edu/astroweb/astronomy.html

AstroWeb: Astronomy/Astrophysics on the Internet Welcome to AstroWeb - a collection of pointers to astronomy-related information available on the Internet. The database is maintained by the AstroWeb Consortium , a collaboration involving 9 individuals at 7 institutions. In addition to classified lists of resource records, the Consortium also provides a utility to search the AstroWeb database: (WAIS search help) Most of the URLs in the database are tested three times a day to verify aliveness (see "AstroWeb Dead URLs" and "AstroWeb Unreliable URLs" ). The Consortium will be pleased to accept contributions of new resource records. You can use HTML forms to submit an addition or change to the Astroweb database review pending submissions review Astroweb records changed in the past month or send EMail to the Consortium This NRAO version of AstroWeb is recomputed at about 09:10 UTC each day, if the master database has been changed. Neither the individuals involved in the AstroWeb Consortium, nor their affiliated institutions, accept any responsibility for the contents or availability of information located at other Internet sites. 1/27/2003 2:57:25 PM The AstroWeb master database currently contains 3069 distinct resource records: Category Records Observing resources Telescopes Astronomical survey projects Telescope observing schedules Metereological information Data Resources Data and Archive Centers Astronomy Information Systems Publication-related Resources Abstracts of Astronomical Publications Full-texts of Astronomical Publications Astronomical Bibliographical Services Astronomy-related Libraries ... Other library resources People-related Resources

99. UW Astronomy -- Research UW Astro Home University of Washington astronomy Department research.This page describes ongoing research at the University of Washington. http://www.astro.washington.edu/dept/research.html

University of Washington Astronomy Department Research This page describes ongoing research at the University of Washington. Find more about the particular research interests of many of the faculty, staff and graduate students by looking at their individual home pages RESEARCH ACTIVITIES OF UW ASTRONOMY FACULTY This page describes the research interests of the department's faculty and postdocs, with links to personal homepages. Annual Report (pdf) UW Astrobiology Program The UW Astronomy department is a member of the new astrobiology program. Observational Facilities This page describes the observing resources that the UW Astronomy department is directly associated with. The HPCC (High Performance Computing and Communications) Group Stardust A NASA Discovery mission to collect samples from a comet and bring them back to Earth. Dr. Don Brownlee is the Principal Investigator. The MaCHO Alert Homepage Finding charts and coordinates of microlensing events in progress, maintained by the MaCHO collaboration at the University of Washington Astronomy Department ( Dr. Chris Stubbs

100. Montana State University Physics And Astronomy Education Research Group research pages and description of Ph.D. program in physics education research. http://www.physics.montana.edu/physed/

A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z

Page 5     81-100 of 194    Back | 1  | 2  | 3  | 4  | 5  | 6  | 7  | 8  | 9  | 10  | Next 20