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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
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
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
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
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
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
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
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
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
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
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
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
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
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
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)
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
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
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
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
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
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
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
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
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
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
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)
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
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
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
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
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
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
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
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
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
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
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
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
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
telescopes. List of astronomical interferometers at visible and infrared wavelengths List of astronomical observatories List of highest astronomical observatories
Lists_of_telescopes
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
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
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
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
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
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
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
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
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
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
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
the Sagnac interferometer, Zernike phase-contrast interferometer, and the point diffraction interferometer. A common-path interferometer is generally
Common-path_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
Astronomical imaging methods
processes. Aperture masking interferometry Aperture synthesis Astronomical interferometer Bispectral analysis Diffraction-limited system Electronic speckle
Speckle_imaging
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
Welsh physicist (1911–1991)
Radio telescope (Radio window) Astronomical interferometer (History) Very Long Baseline Interferometry (VLBI) Astronomical radio source Radio telescopes
Edward_George_Bowen
Exploration Rover MERLIN – Multi Element Radio Linked Interferometer. A seven-telescope radio interferometer MESSENGER – MErcury Surface, Space ENvironment,
List_of_astronomy_acronyms
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
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
unusual objects until the 1960s. Archaeoastronomy Astronomical chronology Astronomical interferometer Cultural astronomy F. Richard Stephenson History
Historical_astronomy
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
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
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
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)
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
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
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
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
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
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
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
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
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)
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
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