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ASTRONOMICAL INTERFEROMETER

  • Astronomical interferometer
  • Array used for astronomical observations

    An astronomical interferometer or telescope array is a set of separate telescopes, mirror segments, or radio telescope antennas that work together as

    Astronomical interferometer

    Astronomical interferometer

    Astronomical_interferometer

  • Interferometry
  • Measurement method using interference of waves

    absorption or emission associated with a substance or mixture. An astronomical interferometer consists of two or more separate dishes that correlates their

    Interferometry

    Interferometry

    Interferometry

  • Navy Precision Optical Interferometer
  • US Navy astronomical interferometer

    The Navy Precision Optical Interferometer (NPOI) is an American astronomical interferometer, with the world's largest baselines, operated by the Naval

    Navy Precision Optical Interferometer

    Navy Precision Optical Interferometer

    Navy_Precision_Optical_Interferometer

  • Mount Wilson Observatory
  • Astronomical observatory in Los Angeles County, California, US

    telescope was equipped with a special attachment, a 6-meter optical astronomical interferometer developed by Albert A. Michelson, much larger than the one he

    Mount Wilson Observatory

    Mount Wilson Observatory

    Mount_Wilson_Observatory

  • Astronomical optical interferometry
  • Astronomical methodology

    This technique is the basis for astronomical interferometer arrays, which can make measurements of very small astronomical objects if the telescopes are

    Astronomical optical interferometry

    Astronomical_optical_interferometry

  • List of types of interferometers
  • An interferometer is a device for extracting information from the superposition of multiple waves. Air-wedge shearing interferometer Astronomical interferometer

    List of types of interferometers

    List_of_types_of_interferometers

  • Very Large Telescope
  • Telescope in the Atacama Desert, Chile

    that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer also includes a set of four

    Very Large Telescope

    Very Large Telescope

    Very_Large_Telescope

  • Palomar Testbed Interferometer
  • Astronomical instrument in California

    flattened at the poles due to its high rate of rotation. List of astronomical interferometers at visible and infrared wavelengths List of observatories M.

    Palomar Testbed Interferometer

    Palomar Testbed Interferometer

    Palomar_Testbed_Interferometer

  • CHARA array
  • Optical interferometer on Mount Wilson, California

    interferometer, located on Mount Wilson, California. The array consists of six 1-metre (40 in) telescopes operating as an astronomical interferometer

    CHARA array

    CHARA array

    CHARA_array

  • Intensity interferometer
  • Astronomy device

    intensity interferometer is the name given to devices that use the Hanbury Brown and Twiss effect. In astronomy, the most common use of such an astronomical interferometer

    Intensity interferometer

    Intensity_interferometer

  • Mark III Stellar Interferometer
  • The Mark III Stellar Interferometer was a long-baseline optical astronomical interferometer, located at the Mount Wilson Observatory, California, United

    Mark III Stellar Interferometer

    Mark_III_Stellar_Interferometer

  • Jodrell Bank Observatory
  • Astronomical observatory in Cheshire, England

    much, and was donated to the Salford Astronomical Society around 1971. The Multi-Element Radio Linked Interferometer Network (MERLIN) is an array of radio

    Jodrell Bank Observatory

    Jodrell Bank Observatory

    Jodrell_Bank_Observatory

  • Aperture masking interferometry
  • miniature astronomical interferometer. The principal limitation of the technique is that it is applicable only to relatively bright astronomical objects

    Aperture masking interferometry

    Aperture masking interferometry

    Aperture_masking_interferometry

  • Astronomical seeing
  • Atmospheric distortions of light

    scintillation or twinkling Atmospheric seeing causes the fringes in an astronomical interferometer to move rapidly The distribution of atmospheric seeing through

    Astronomical seeing

    Astronomical seeing

    Astronomical_seeing

  • Event horizon (disambiguation)
  • Topics referred to by the same term

    Horizon Telescope, an array of radiotelescopes that form an astronomical interferometer One type of geological horizon Event Horizon Software, the original

    Event horizon (disambiguation)

    Event_horizon_(disambiguation)

  • Atacama Large Millimeter Array
  • 66-telescope radio observatory in Chile

    The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile

    Atacama Large Millimeter Array

    Atacama Large Millimeter Array

    Atacama_Large_Millimeter_Array

  • List of astronomical interferometers at visible and infrared wavelengths
  • Here is a list of currently existing astronomical optical interferometers (i.e. operating from visible to mid-infrared wavelengths), and some parameters

    List of astronomical interferometers at visible and infrared wavelengths

    List_of_astronomical_interferometers_at_visible_and_infrared_wavelengths

  • Lovell Telescope
  • Radio telescope at Jodrell Bank Observatory, Cheshire, England

    as an interferometer with the Mark I to carry out a survey of radio sources. The telescope took part in the first transatlantic interferometer experiment

    Lovell Telescope

    Lovell Telescope

    Lovell_Telescope

  • List of largest optical reflecting telescopes
  • designed to be used as optical astronomical interferometers such as the Keck I and II used together as the Keck Interferometer (up to 85 m) can reach higher

    List of largest optical reflecting telescopes

    List of largest optical reflecting telescopes

    List_of_largest_optical_reflecting_telescopes

  • Tau Ceti
  • Single yellow-hued star in the constellation Cetus

    and luminosity of Tau Ceti can be estimated. However, using an astronomical interferometer, measurements of the radius of the star can be made directly

    Tau Ceti

    Tau Ceti

    Tau_Ceti

  • Arecibo Telescope
  • Former radio telescope in Puerto Rico, United States

    hanging 100m-wide subreflector mesh between the dish and the platform. The Astronomical Sciences and Atmospheric Sciences divisions of the NSF had financially

    Arecibo Telescope

    Arecibo Telescope

    Arecibo_Telescope

  • Michelson stellar interferometer
  • Type of array used for astronomical observations

    The Michelson stellar interferometer is one of the earliest astronomical interferometers built and used. The interferometer was proposed by Albert A.

    Michelson stellar interferometer

    Michelson stellar interferometer

    Michelson_stellar_interferometer

  • Aperture synthesis
  • Mixing signals from many telescopes to produce images with high angular resolution

    (or "map") of the source is produced from these measurements. Astronomical interferometers are commonly used for high-resolution optical, infrared, submillimetre

    Aperture synthesis

    Aperture_synthesis

  • Radio telescope
  • Directional radio antenna used in radio astronomy

    a larger antenna, in order to achieve greater resolution. Astronomical radio interferometers usually consist either of arrays of parabolic dishes (e.g

    Radio telescope

    Radio telescope

    Radio_telescope

  • Sirius
  • Brightest star in Earth's night sky

    of 2.063 M☉. The radius of this star has been measured by an astronomical interferometer, giving an estimated angular diameter of 5.936±0.016 mas. The

    Sirius

    Sirius

    Sirius

  • Darwin (spacecraft)
  • 2007 European study concept of an array of space observatories

    three to four metres in diameter, flying in formation as an astronomical interferometer. These telescopes were to redirect light from distant stars and

    Darwin (spacecraft)

    Darwin_(spacecraft)

  • Cosmic Background Imager
  • Astronomical interferometer at Llano de Chajnantor Observatory in Chile (1999–2008)

    The Cosmic Background Imager (or CBI) was a 13-element astronomical interferometer perched at an elevation of 5,080 metres (16,700 feet) at Llano de Chajnantor

    Cosmic Background Imager

    Cosmic Background Imager

    Cosmic_Background_Imager

  • Search for extraterrestrial intelligence
  • Effort to find civilizations not from Earth

    simultaneous access to the interferometer output at the same time. Typically, the ATA snapshot imager (used for astronomical surveys and SETI) is run in

    Search for extraterrestrial intelligence

    Search for extraterrestrial intelligence

    Search_for_extraterrestrial_intelligence

  • MERLIN
  • Observatory

    The Multi-Element Radio Linked Interferometer Network (MERLIN) is an interferometer array of radio telescopes spread across England. The array is run from

    MERLIN

    MERLIN

    MERLIN

  • LIGO
  • Gravitational wave observatory site

    The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational

    LIGO

    LIGO

    LIGO

  • Antoine Émile Henry Labeyrie
  • French astronomer (born 1943)

    Hypertelescope Lise association, which aims to develop an extremely large astronomical interferometer with spherical geometry that might theoretically show features

    Antoine Émile Henry Labeyrie

    Antoine_Émile_Henry_Labeyrie

  • Lowell Observatory
  • Astronomical observatory and historic landmark in Arizona, US

    Lowell Observatory is an astronomical observatory in Flagstaff, Arizona, United States. Lowell Observatory was established in 1894, placing it among the

    Lowell Observatory

    Lowell Observatory

    Lowell_Observatory

  • Closure phase
  • Observable quantity in imaging astronomical interferometry

    to eliminate the effects of astronomical seeing in optical and infrared observations using astronomical interferometers. A minimum of three antennas

    Closure phase

    Closure_phase

  • Cambridge Optical Aperture Synthesis Telescope
  • English astronomical interferometer observatory

    Optical Aperture Synthesis Telescope, is a multi-element optical astronomical interferometer with baselines of up to 100 metres, which uses aperture synthesis

    Cambridge Optical Aperture Synthesis Telescope

    Cambridge Optical Aperture Synthesis Telescope

    Cambridge_Optical_Aperture_Synthesis_Telescope

  • ISI
  • Topics referred to by the same term

    information on all children in England Infrared Spatial Interferometer, an astronomical interferometer array of three telescopes International Sensitivity

    ISI

    ISI

  • Laser Interferometer Space Antenna
  • European space mission to measure gravitational waves

    The Laser Interferometer Space Antenna (LISA) is a planned European space mission to detect and measure gravitational waves—slight ripples in the fabric

    Laser Interferometer Space Antenna

    Laser Interferometer Space Antenna

    Laser_Interferometer_Space_Antenna

  • Very Large Array
  • Radio astronomy observatory in New Mexico, US

    the equipment, instrumentation, and computing power to function as an interferometer. Each of the massive telescopes is mounted on double parallel railroad

    Very Large Array

    Very Large Array

    Very_Large_Array

  • Radio astronomy
  • Subfield of astronomy that studies celestial objects at radio frequencies

    Pawsey and Ruby Payne-Scott in 1946. The first use of a radio interferometer for an astronomical observation was carried out by Payne-Scott, Pawsey and Lindsay

    Radio astronomy

    Radio astronomy

    Radio_astronomy

  • Combined Array for Research in Millimeter-wave Astronomy
  • Astronomical instrument

    (CARMA) was an astronomical instrument comprising 23 radio telescopes, dedicated in 2006. These telescopes formed an astronomical interferometer where all

    Combined Array for Research in Millimeter-wave Astronomy

    Combined_Array_for_Research_in_Millimeter-wave_Astronomy

  • Lists of telescopes
  • telescopes. List of astronomical interferometers at visible and infrared wavelengths List of astronomical observatories List of highest astronomical observatories

    Lists of telescopes

    Lists of telescopes

    Lists_of_telescopes

  • Telescope
  • Instrument that makes distant objects appear magnified

    images can be computed. Such multi-dish arrays are known as astronomical interferometers and the technique is called aperture synthesis. The 'virtual'

    Telescope

    Telescope

    Telescope

  • Baseline
  • Topics referred to by the same term

    electrocardiogram Baseline (interferometry), the length of an astronomical interferometer The name Baseline may refer to: Baseline (magazine), a magazine

    Baseline

    Baseline

  • Einstein Telescope
  • Proposed gravitational wave detector

    the two arms of each interferometer, unlike 90° in a traditional L-shaped layout. 2L configuration uses 2 pairs of interferometers located in two far separated

    Einstein Telescope

    Einstein_Telescope

  • European Southern Observatory
  • Intergovernmental observatory in Chile

    wavelengths—between infrared light and radio waves. ALMA is an astronomical interferometer initially composed of 66 high-precision antennas and operating

    European Southern Observatory

    European Southern Observatory

    European_Southern_Observatory

  • List of astronomical instruments
  • Devices for observing, measuring or recording astronomical data

    An astronomical instrument is a device for observing, measuring or recording astronomical data. They are used in the scientific field of astronomy, a natural

    List of astronomical instruments

    List_of_astronomical_instruments

  • Gerard van Belle
  • American astronomer (born 1968)

    Testbed Interferometer to make observations of the rapidly rotating star Altair. He also contributed to practical considerations of operating astronomical interferometers

    Gerard van Belle

    Gerard van Belle

    Gerard_van_Belle

  • Virgo interferometer
  • Gravitational-wave detector in Italy

    interferometer is a large-scale scientific instrument near Pisa, Italy, for detecting gravitational waves. The detector is a Michelson interferometer

    Virgo interferometer

    Virgo interferometer

    Virgo_interferometer

  • Sagnac effect
  • Relativistic effect due to rotation

    Sagnac effect manifests itself in a setup called a ring interferometer or Sagnac interferometer. A beam of light is split and the two beams are made to

    Sagnac effect

    Sagnac effect

    Sagnac_effect

  • NGC 4526
  • Lenticular galaxy in the constellation Virgo

    measuring the rotation of gas molecules around its centre with an astronomical interferometer (in this case the Combined Array for Research in Millimeter-wave

    NGC 4526

    NGC 4526

    NGC_4526

  • Astronomy
  • Scientific study of celestial objects

    objects. A few observatories have been constructed, such as the Laser Interferometer Gravitational Observatory LIGO. LIGO made its first detection on 14

    Astronomy

    Astronomy

    Astronomy

  • James Clerk Maxwell Telescope
  • Radio telescope in Hawaii, US

    Submillimeter Observatory next to it to form the first submillimetre astronomical interferometer. This success was important driving the construction of the later

    James Clerk Maxwell Telescope

    James Clerk Maxwell Telescope

    James_Clerk_Maxwell_Telescope

  • Common-path interferometer
  • the Sagnac interferometer, Zernike phase-contrast interferometer, and the point diffraction interferometer. A common-path interferometer is generally

    Common-path interferometer

    Common-path_interferometer

  • Cambridge Interferometer
  • 214 MHz using the 2-element Long Michelson Interferometer), discovering some of the most interesting astronomical objects known. The telescope was operated

    Cambridge Interferometer

    Cambridge_Interferometer

  • Speckle imaging
  • Astronomical imaging methods

    processes. Aperture masking interferometry Aperture synthesis Astronomical interferometer Bispectral analysis Diffraction-limited system Electronic speckle

    Speckle imaging

    Speckle imaging

    Speckle_imaging

  • Narrabri Stellar Intensity Interferometer
  • Astronomical instrument in New South Wales, Australia (1963–1974)

    The Narrabri Stellar Intensity Interferometer (NSII) was the first astronomical instrument to measure the diameters of a large number of stars at visible

    Narrabri Stellar Intensity Interferometer

    Narrabri_Stellar_Intensity_Interferometer

  • United States Naval Observatory Flagstaff Station
  • Astronomical observatory

    NOFS Director. NPOI is a successful astronomical interferometer of the venerable and proven Michelson interferometer design. As noted, the majority of interferometric

    United States Naval Observatory Flagstaff Station

    United_States_Naval_Observatory_Flagstaff_Station

  • Fabry–Pérot interferometer
  • Optical device with parallel mirrors

    cameras, astronomical equipment, and laser systems. Optical wavemeters and some optical spectrum analyzers use Fabry–Pérot interferometers with different

    Fabry–Pérot interferometer

    Fabry–Pérot interferometer

    Fabry–Pérot_interferometer

  • Australian Square Kilometre Array Pathfinder
  • Radio telescope in Western Australia

    each 12 m (39 ft) in diameter, working together as a single astronomical interferometer with a total collecting area of approximately 4,000 m2 (43,000 sq ft)

    Australian Square Kilometre Array Pathfinder

    Australian Square Kilometre Array Pathfinder

    Australian_Square_Kilometre_Array_Pathfinder

  • W. M. Keck Observatory
  • Astronomical observatory in Hawaii

    capability. Extremely large telescope Gemini Observatory List of astronomical interferometers at visible and infrared wavelengths List of largest optical reflecting

    W. M. Keck Observatory

    W. M. Keck Observatory

    W._M._Keck_Observatory

  • Large Interferometer For Exoplanets
  • Proposed space mission

    (2024). Large Interferometer For Exoplanets (LIFE). XII. The Detectability of Capstone Biosignatures in the Mid-infrared. Astronomical Journal. Matsuo

    Large Interferometer For Exoplanets

    Large_Interferometer_For_Exoplanets

  • History of the telescope
  • been applied at a number of other astronomical telescope arrays including: the Navy Prototype Optical Interferometer, the CHARA array, and the IOTA array

    History of the telescope

    History of the telescope

    History_of_the_telescope

  • Albert A. Michelson
  • American physicist (1852–1931)

    existence of the luminiferous ether. He later moved on to use astronomical interferometers in the measurement of stellar diameters and in measuring the

    Albert A. Michelson

    Albert A. Michelson

    Albert_A._Michelson

  • Terrestrial Planet Finder
  • NASA concept study of an array of space telescopes

    signatures of life. The two planned architectures were: Infrared astronomical interferometer (TPF-I): Multiple small telescopes on a fixed structure or on

    Terrestrial Planet Finder

    Terrestrial Planet Finder

    Terrestrial_Planet_Finder

  • Smear
  • Topics referred to by the same term

    1990s. Smearing may refer to: Smearing of an image taken by an astronomical interferometer: Bandwidth smearing, a chromatic aberration; Time smearing, a

    Smear

    Smear

  • Angular resolution
  • Ability of any image-forming device to distinguish small details of an object

    for telescopes can be achieved by arrays of telescopes called astronomical interferometers: These instruments can achieve angular resolutions of 0.001 arcsecond

    Angular resolution

    Angular resolution

    Angular_resolution

  • Magdalena Ridge Observatory
  • American astronomical observatory

    of astronomical interferometers at visible and infrared wavelengths List of astronomical observatories Very Large Array — nearby radio Interferometer observatory

    Magdalena Ridge Observatory

    Magdalena Ridge Observatory

    Magdalena_Ridge_Observatory

  • Erciyes University Radio Observatory
  • Observatory

    Türk Telekom in 2000. They are part of a project to build an astronomical interferometer. The radio telescopes operate in the frequencies of 4.5, 11 and

    Erciyes University Radio Observatory

    Erciyes_University_Radio_Observatory

  • Nuller
  • Scientific Electronic Device

    to L band at the Very Large Telescope Interferometer with the Asgard Instrumental suite". Journal of Astronomical Telescopes, Instruments, and Systems

    Nuller

    Nuller

  • Astronomical spectroscopy
  • Measurement of electromagnetic radiation for astronomy

    Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including

    Astronomical spectroscopy

    Astronomical spectroscopy

    Astronomical_spectroscopy

  • Stockert Radio Telescope
  • Observatory

    which has updated the technology and has opened the site to the public. Astronomical observations have been resumed in 2011, primarily for educational purposes

    Stockert Radio Telescope

    Stockert Radio Telescope

    Stockert_Radio_Telescope

  • Hat Creek Radio Observatory
  • Observatory in northern California, USA

    starting in the 1970s when a 2-element interferometer was constructed. From 1980 to 1985 a 3-element interferometer was constructed, with another four antennas

    Hat Creek Radio Observatory

    Hat Creek Radio Observatory

    Hat_Creek_Radio_Observatory

  • List of astronomical observatories
  • This is a partial list of astronomical observatories ordered by name, along with initial dates of operation (where an accurate date is available) and location

    List of astronomical observatories

    List_of_astronomical_observatories

  • Plateau de Bure Interferometer
  • Former astronomical observatory

    The Plateau de Bure Interferometer (PdBI) was a six-antenna interferometer on the Pic de Bure (2550 m) in the French Alps, operated by the Institut de

    Plateau de Bure Interferometer

    Plateau de Bure Interferometer

    Plateau_de_Bure_Interferometer

  • Gravitational-wave observatory
  • Device used to measure gravitational waves

    present-day generation of laser interferometers has reached the necessary sensitivity to detect gravitational waves from astronomical sources, thus forming the

    Gravitational-wave observatory

    Gravitational-wave observatory

    Gravitational-wave_observatory

  • Green Bank Interferometer
  • Former radio telescope in Green Bank, West Virginia

    with the Green Bank Interferometer". American Astronomical Society, 191st AAS Meeting, Id.110.17; Bulletin of the American Astronomical Society. 29: 110

    Green Bank Interferometer

    Green Bank Interferometer

    Green_Bank_Interferometer

  • Kernel-phase
  • Kernel-phases are observable quantities used in high resolution astronomical imaging used for superresolution image creation. It can be seen as a generalization

    Kernel-phase

    Kernel-phase

  • Very-long-baseline interferometry
  • Comparing widely separated telescope wavefronts

    interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. In VLBI a signal from an astronomical radio source, such as a quasar

    Very-long-baseline interferometry

    Very-long-baseline interferometry

    Very-long-baseline_interferometry

  • Hongmeng project
  • Reza; Chen, Xuelei; "An Imaging Algorithm for a Lunar Orbit Interferometer Array", Astronomical Journal, 156,43 (2018) https://iopscience.iop.org/article/10

    Hongmeng project

    Hongmeng project

    Hongmeng_project

  • TAMA 300
  • Gravitational wave detector

    a Fabry–Pérot Michelson interferometer (FPMI) with power recycling. It is officially known as the 300m Laser Interferometer Gravitational Wave Antenna

    TAMA 300

    TAMA 300

    TAMA_300

  • Altair
  • Brightest star in the constellation Aquila

    "The stellar interferometer at Narrabri Observatory-II. The angular diameters of 15 stars". Monthly Notices of the Royal Astronomical Society. 137 (4):

    Altair

    Altair

    Altair

  • Radio window
  • Region of the radio spectrum

    upper limit of the radio window towards the 1 THz optimum, since the astronomical objects give spectral lines of greater intensity in the higher frequency

    Radio window

    Radio window

    Radio_window

  • Edward George Bowen
  • Welsh physicist (1911–1991)

    Radio telescope (Radio window) Astronomical interferometer (History) Very Long Baseline Interferometry (VLBI) Astronomical radio source Radio telescopes

    Edward George Bowen

    Edward George Bowen

    Edward_George_Bowen

  • List of astronomy acronyms
  • Exploration Rover MERLIN – Multi Element Radio Linked Interferometer. A seven-telescope radio interferometer MESSENGER – MErcury Surface, Space ENvironment,

    List of astronomy acronyms

    List_of_astronomy_acronyms

  • John Gatenby Bolton
  • British-Australian astronomer (1922–1993)

    electronics and the ideas that would help him later to build a sea-cliff interferometer. As World War 2 ended in 1945, HMS Unicorn shuttled cargo and personnel

    John Gatenby Bolton

    John Gatenby Bolton

    John_Gatenby_Bolton

  • OVRO 40 meter Telescope
  • Radio telescope in California

    Science Foundation, as a prototype for a planned astronomical interferometer at Owens Valley. The interferometer was to incorporate eight dishes moving on rails

    OVRO 40 meter Telescope

    OVRO 40 meter Telescope

    OVRO_40_meter_Telescope

  • Historical astronomy
  • unusual objects until the 1960s. Archaeoastronomy Astronomical chronology Astronomical interferometer Cultural astronomy F. Richard Stephenson History

    Historical astronomy

    Historical_astronomy

  • Palomar Observatory
  • Astronomical observatory in Southern California

    Gattini-IR telescope. Decommissioned instruments include the Palomar Testbed Interferometer and the first telescopes at the observatory, an 18-inch (46 cm) Schmidt

    Palomar Observatory

    Palomar Observatory

    Palomar_Observatory

  • Betelgeuse
  • Red supergiant star in the constellation Orion

    1920, Albert A. Michelson and Francis G. Pease mounted a six-meter interferometer on the front of the 2.5-meter telescope at Mount Wilson Observatory

    Betelgeuse

    Betelgeuse

    Betelgeuse

  • Large Binocular Telescope
  • Telescope for optical astronomy

    Advanced Technology Telescope Extremely large telescope List of astronomical interferometers at visible and infrared wavelengths List of largest optical reflecting

    Large Binocular Telescope

    Large Binocular Telescope

    Large_Binocular_Telescope

  • GRAVITY (Very Large Telescope)
  • GRAVITY is an instrument on the Very Large Telescope

    VLTI GRAVITY GRAVITY is an instrument on the interferometer of the Very Large Telescope (VLTI). It either combines the light of the four Unit Telescopes

    GRAVITY (Very Large Telescope)

    GRAVITY (Very Large Telescope)

    GRAVITY_(Very_Large_Telescope)

  • Tianlai experiment
  • Chinese radio astronomy experiment

    and performance of a prototype transit radio interferometer, Monthly Notices of the Royal Astronomical Society, Volume 506, Issue 3, September 2021,

    Tianlai experiment

    Tianlai experiment

    Tianlai_experiment

  • Infrared astronomy
  • Observation of infrared wavelengths

    infrared telescopes are combined to form astronomical interferometers. The effective resolution of an interferometer is set by the distance between the telescopes

    Infrared astronomy

    Infrared_astronomy

  • HR 8799 e
  • Jovian planet orbiting HR 8799

    Observatory announced the result of their Very Large Telescope astronomical interferometer (VLTI) imaging of HR 8799 e employing the GRAVITY instrument

    HR 8799 e

    HR 8799 e

    HR_8799_e

  • Anderson Mesa Station
  • Astronomical observatory in Arizona, US

    Anderson Mesa Station is an astronomical observatory established in 1959 as a dark-sky observing site for Lowell Observatory. It is located at Anderson

    Anderson Mesa Station

    Anderson_Mesa_Station

  • Great Observatories program
  • Series of NASA satellites

    much higher resolution than by Hubble from the ground using astronomical interferometers or adaptive optics. Larger ground-based telescopes have only

    Great Observatories program

    Great Observatories program

    Great_Observatories_program

  • Canadian Hydrogen Intensity Mapping Experiment
  • Canadian radio telescope

    high-redshift universe. The instrument is a hybrid semi-cylindrical interferometer designed to measure the large scale neutral hydrogen power spectrum

    Canadian Hydrogen Intensity Mapping Experiment

    Canadian Hydrogen Intensity Mapping Experiment

    Canadian_Hydrogen_Intensity_Mapping_Experiment

  • Observational astronomy
  • Division of astronomy

    of observing celestial objects with the use of telescopes and other astronomical instruments. As a science, the study of astronomy does not rely on direct

    Observational astronomy

    Observational astronomy

    Observational_astronomy

  • Green Bank Observatory
  • American astronomical observatory

    (previously National Radio Astronomy Observatory, Green Bank) is an astronomical observatory located in the National Radio Quiet Zone in Green Bank, West

    Green Bank Observatory

    Green Bank Observatory

    Green_Bank_Observatory

  • Astronomical Observatory (University of Illinois Urbana-Champaign)
  • Observatory in Urbana, Illinois, U.S.

    The University of Illinois Astronomical Observatory, located at 901 S. Mathews Avenue in Urbana, Illinois, on the campus of the University of Illinois

    Astronomical Observatory (University of Illinois Urbana-Champaign)

    Astronomical Observatory (University of Illinois Urbana-Champaign)

    Astronomical_Observatory_(University_of_Illinois_Urbana-Champaign)

  • United States Naval Observatory
  • Scientific agency in the United States

    near Flagstaff. This facility now oversees the Navy Precision Optical Interferometer. By the early 1870s the USNO daily noon-time signal was distributed

    United States Naval Observatory

    United States Naval Observatory

    United_States_Naval_Observatory

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ASTRONOMICAL INTERFEROMETER

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ASTRONOMICAL INTERFEROMETER