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Topic: Magdelena Ridge Observatory Interferometer

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	Telescopes
		The Chandra X-ray Observatory is the U.S. follow-on to the Einstein Observatory.
		The observatory has two primary nighttime telescopes: the 60-inch telescope, built in 1908 is home to the HK Project and the Atmospheric Compensation Experiment; and the 100-inch (Hooker) telescope, built in 1917, which is available to the scientific community.
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	www.cv.nrao.edu /fits/www/yp_telescope.html (12332 words)

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	Magdalena Ridge Observatory - Wikipedia, the free encyclopedia
		The observatory is located near the summit of the Magdalena Mountains at an elevation of 10,600 feet (3180 meters) making it the fourth highest observatory in the world.
		The interferometer will consist of an array of ten 1.4-meter telescopes whose images will be optically combined resulting in angular resolution that simulates that of a telescope 400 meters in diameter.
		Magdalena Ridge Observatory is a international scientific collaboration of several universities including the New Mexico Institute of Mining and Technology in Socorro and the University of Cambridge.
	en.wikipedia.org /wiki/Magdalena_Ridge_Observatory (260 words)

	Optical Astronomy
		The CfA operates the Whipple Observatory in Amado, Arizona, and the Oak Ridge Observatory in Harvard, Massachusetts.
		Swift is a three-telescope space observatory (gamma-ray telescope, X-ray telescope, and ultraviolet/optical telescope) for studying gamma ray bursts.
		The Vainu Bappu Observatory (VBO) is the main optical observatory of the Indian Institute of Astrophysics (IIA), and is located in the picturesque neighbourhood of the village of Kavalur in the state of Tamil Nadu.
	www.cv.nrao.edu /fits/www/yp_optical.html (11715 words)

	Magdalena Ridge Observatory Interferometer - Wikipedia, the free encyclopedia
		The Magdalena Ridge Observatory Interferometer will be an optical aperture synthesis array composed of six (possibly up to ten) telescopes, each approximately 1.4 meters in diameter.
		The telescopes making up the astronomical interferometer will be spaced by distances of up to 400 meters and will be optically linked in order to image astronomical objects with great detail—this configuration will simulate the resolving power of a single telescope up to 400 meters in diameter.
		It will be part of the Magdalena Ridge Observatory located in the Magdalena mountains of Socorro county, central New Mexico near South Baldy peak and the Langmuir Laboratory for Atmospheric Research.
	en.wikipedia.org /wiki/Magdalena_Ridge_Observatory_Interferometer (219 words)

	Los Alamos National Laboratory joins the Magdalena Ridge Observatory Consortium (Site not responding. Last check: 2007-10-10)
		Once constructed along the main ridge of the Magdalena Mountains west of Socorro, N.M., the MRO will be a state-of-the-art observatory employing cutting-edge technology to produce detailed images of the far reaches of the universe.
		The observatory will be equipped with three 2.4-meter telescopes -- two fixed and one moveable -- linked by optical interferometry to create the potential resolving power of a single 50-meter telescope.
		Scientists are also looking into the possibility of staging the building of the observatory to have one telescope operational in two years, allowing single-telescope research to begin at the MRO before the construction is complete.
	www.lanl.gov /worldview/news/releases/archive/01-038.shtml (1086 words)

	29 July 2004: Cambridge and New Mexico astrophysicists take the next step towards world’s most ambitious optical ... (Site not responding. Last check: 2007-10-10)
		The Interferometer will be composed of several telescopes, spread out over an area larger than a football pitch and optically linked together to form a single ‘synthetic aperture’ 400 metres in diameter.
		The Interferometer will be a key feature of the Magdalena Ridge Observatory in New Mexico, which is being funded by the United States Congress, administered by the US Office of Naval Research and overseen by the US Naval Research Laboratory.
		The interferometer is expected to be ready (and available) for routine scientific observations in 2008.
	www.admin.cam.ac.uk /news/press/dpp/2004072901 (659 words)

	Magdalena Ridge Observatory
		Through a cooperative agreement signed in September, 2001, with New Mexico Institute of Mining and Technology, the financial arm for the observatory, NRL was designated as the government lead for the project.
		The Magdalena Ridge Observatory (MRO), a joint endeavor between the university consortium and the Department of Defense, will enable scientists and engineers to determine how to increase sensitivity for ground-based interferometers.
		NPOI is a high-precision, long-baseline optical interferometer that provides highly accurate measurements of star positions.
	www.globalsecurity.org /space/facility/magdalena-ridge.htm (455 words)

	OptInt: MROI
		The Magdalena Ridge Observatory (MRO) project is a collaboration between New Mexico Tech (NMT), the
		The Magdalena Ridge Observatory project is overseen by the
		We are also contracted to deliver the vacuum delay lines for the interferometer, and expect to be involved in delivering other MROI subsystems.
	www.mrao.cam.ac.uk /research/OAS/mroi.html (364 words)

	Physics at Minnesota: Physics and Astronomy Calendar
		The Magdalena Ridge Observatory Interferometer (MROI) is being designed and built at New Mexico Tech in collaboration with the University of Cambridge.
		The completed interferometer will be comprised of ten 1.4m telescopes in four scalable configurations, operating from 600 nm to 2.4 microns.
		We have several of the long lead-time components under contract and will be breaking ground on the interferometer buildings in late spring this year.
	www.physics.umn.edu /calendar/AC/calendar.html?item=1824 (169 words)

	Welcome to Magdalena Ridge Observatory - MRO Interferometer (Site not responding. Last check: 2007-10-10)
		The MRO Interferometer Office is concerned with developing an ambitious multi-element imaging interferometer to operate at wavelengths between 0.6 and 2.4 microns with baselines of up to 400m.
		Its primarily technical and scientific goals are to deliver model-independent images of faint and complex astronomical targets.
		The interferometer is expected to attain first fringes in 2008, and complete commissioning in 2009.
	www.mro.nmt.edu /Interferometer/index.php (171 words)

	NAM 2003 Abstract List, Session 83 (via CobWeb/3.1 planetlab2.cs.unc.edu) (Site not responding. Last check: 2007-10-10)
		We include a more detailed discussion of the use of these detectors at next generation interferometers (the Magdelena Ridge Observatory Interferometer (MROI)), involving their use for group delay fringe tracking and visibility parameter estimation.
		Not only is access to the VLTI and its first generation instruments secure, but participation and access to the 10 x 1.4m Magdalena Ridge Observatory Interferometer is currently being negotiated.
		Abstract: Second-generation interferometers, like the VLTI and the Magdalena Ridge Observatory Interferometer, are set to take spatial interferometry from an experimental basis to that of a facility for the non-specialist interferometer.
	star.arm.ac.uk.cob-web.org:8888 /nam2003/abstracts/abstracts83.html (701 words)

	Cosmos Magazine \| A Publication for the Astronomical and Education Community
		The National Schools Observatory is "a major web-based resource for schools to provide the opportunity to work with professional world-class robotic telescopics".
		The telescope and related instrumentation is run by the Istituto di Radioastronomia (IRA - C.N.R.), sezione di Firenze (former CAISMI), with the assistance of the Osservatorio Astrofisico di Arcetri and the Dipartimento di Astronomia e Scienza dello Spazio of the Universita' di Firenze.
		The Hobby-Eberly telescope (HET) is a new 9 meter telescope, built at the University of Texas McDonald Observatory near Ft. Davis Texas as a result of an international collaboration between the University of Texas at Austin, The Pennsylvania State University and Stanford University in the United States and Ludwig-Maximilians-Universitaet Muenchen, and Goerg-August-Universitaet Goettingen.
	www.cosmosmagazine.tv /telescopes.htm (11964 words)

	[82.08] Design and Test of an Instrument for Measuring Microthermal Seeing on Magdalena Ridge (Site not responding. Last check: 2007-10-10)
		The Magdalena Ridge Observatory Interferometer is an ambitious multi-element imaging interferometer being built by New Mexico Tech that is located west of Socorro in the Magdalena Mountains at an altitude of 10,500 ft. The performance of the interferometer is impacted by the seeing quality from atmospheric effects.
		The rapid temperature measurements are directly related to the local turbulence which in turn is responsible for the ground-level astronomical seeing.
		Los Alamos National Laboratory and the Magdalena Ridge Observatory are financially supporting this research.
	www.aas.org /publications/baas/v37n4/aas207/1080.htm (250 words)

	Research Facilities at NMT (Site not responding. Last check: 2007-10-10)
		The The National Radio Astronomy Observatory (NRAO) has its Array Operations Center on the New Mexico Tech campus.
		NM Tech is a founding partner in the recently funded Magdalena Ridge Observatory.
		The interferometer will be able to resolve angles smaller than a thousandth of an arcsecond, comparable to the VLBA.
	www.physics.nmt.edu /Research/facilities.html (549 words)

	Infrared Astronomy Resources (via CobWeb/3.1 planetlab2.cs.unc.edu) (Site not responding. Last check: 2007-10-10)
		The Infrared Space Observatory (ISO) is an ESA (European Space Agency) mission with the participation of ISAS (Japan) and NASA (USA).
		Details of the research and teaching interests of the group, as well as information on the Liverpool Telescope project - a fully-robotic 2m telescope to be situated at the Observatorio del Roque de los Muchachos, La Palma.
		VISTA is the Visible and Infrared Telescope for Astronomy: a 4-m Wide Field Survey telescope for the Southern Hemisphere, being built at Cerro Paranal, close to ESO VLT, by a consortium of 18 UK universities.
	cdsweb.u-strasbg.fr.cob-web.org:8888 /astroweb/infrared.html (6812 words)

	Observatories and Telescopes Resources
		AKARI (formerly ASTRO-F) is an infrared sky survey mission from Institute of Space and Astronautical Science (ISAS) of the Japan Aerospace eXploration Agency (JAXA) with the participation of the European Space Agency (ESA).
		This configuration will provide high resolution interferometry in the visible spectral region as well as the K spectral band (2.2 micron), with a limiting resolution of 0.2 milliarcsec in the visible.
		The original low frequency telescope was superseded in 1976 by a 14-m diameter radome-enclosed antenna for use at high radio frequencies (mm wavelengths), built primarily to study the physics and chemistry of interstellar clouds, circumstellar envelopes, planetary atmospheres, and comets.
	cdsweb.u-strasbg.fr /astroweb/telescope.html (9231 words)

	Mro (via CobWeb/3.1 planetlab2.cs.unc.edu) (Site not responding. Last check: 2007-10-10)
		Hokuriku Broadcasting System, broadcasting station in Ishikawa Prefecture, Japan
		Magdelena Ridge Observatory, site of the Magdelena Ridge Observatory Interferometer
		Please check back often as new enhancements are frequently being created
	www.seattleluxury.com.cob-web.org:8888 /encyclopedia/entry/MRO (122 words)

	[82.14] Magdalena Ridge Observatory Interferometer Science Mission and Design Requirements (Site not responding. Last check: 2007-10-10)
		The science reference mission for the interferometer, from which we derive the design requirements, has three main components: the study of stellar and planetary formation, developing a better understanding of physical processes at various stages of stellar evolution, and characterization of the innermost regions of active galactic nuclei.
		A discussion of each of these key areas and the subsequent design requirements they place on the interferometer will be presented.
		Construction of the facility will begin in April, 2006 with expected first fringes in 2008.
	www.aas.org /publications/baas/v37n4/aas207/1960.htm (168 words)

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