「telescope」の共起表現一覧(1語右で並び替え)
該当件数 : 1510件
1979 it was replaced with the Anna L. Nickel | telescope, a 1 meter reflecting telescope. |
appear to have been, in addition to the main | telescope, a transit room, and what was probably a stu |
cius may have noticed them himself without a | telescope a few years before). |
In addition to its | telescope, a 20-inch Cassegrain reflector, it houses a |
The third | telescope, a Coronado PST Hα 40/400 mm, is installed n |
multiple observatories and the Hubble Space | Telescope, a study obtains the exact mass and orbital |
ileoscope uses a 1¼-inch focuser, giving the | telescope a great deal of versatility, since this is t |
Advanced Technology Solar | Telescope a 4m solar telescope. |
The main house had a | telescope, a picture gallery, and an ethnographic muse |
aboard the spacecraft included a Lyman-alpha | telescope, a rubidium-vapor magnetometer, electrostati |
ents, including one 24" Classical cassegrain | telescope, a 14" and 8" Schmidt-Cassegrain telescope, |
ong (China), and OAO (Japan), has a 2m class | telescope, a high dispersion echelle spectrograph, and |
three instruments - an interferometric radio | telescope, a 26-m single-dish antenna, and a solar flu |
ry instruments in use are a 14.5" Cassegrain | telescope, a 12" Schmidt-Cassegrain, a 16" folded Newt |
roken into by thieves who stole the sighting | telescope, a modern replacement has since been install |
a solar | telescope, a telescope especially adapted for viewing |
Microsoft launches its WorldWide | Telescope a free virtual telescope with access to 2 te |
A second | telescope, a 0.6 meter (24 inch) telescope operated by |
The 45m Radio | Telescope: A 45m single-dish radio telescope that oper |
Along with his own | telescope, Abel uses a variety of other telescopes to |
nfrared observations using the Spitzer Space | Telescope, about half of the stars in the cluster have |
He installed a transit | telescope above his college ante-chapel. |
ent of the mission, with the station's solar | telescope activated on 16 January. |
The facility also hosted Michael Schwartz's | telescope, active in supernova patrols, until Tenagra |
A comet seeker is a type of small | telescope adapted especially to searching for comets: |
The VLT | telescope adaptive secondary mirror |
When the 1.8m | telescope additions complete, NPOI also will undertake |
d, European Space Agency member of the Space | Telescope Advisory Team, and Member of Council of the |
Hubble Space | Telescope after servicing by the crew of STS-109 |
eld observation underway by the Hubble Space | Telescope after its 2009 refurbishing. |
The Vatican Advanced Technology | Telescope, aka the VATT, is a 1.8 meter Gregorian tele |
he continued to use the University's 16 inch | telescope, albeit in a rather random fashion. |
de a firm anchor for a microscope, camera or | telescope allowing it to be swiveled in all directions |
mechanism used to move an equatorial mounted | telescope along one axis to keep the telescope in exac |
The observatory has one 0.6 metre Cassegrain | telescope along with a photometer and a CCD camera. |
tation and reassembly of the Merz and Soehne | telescope along with an adequate facility to house it. |
The Nasmyth | telescope, also called Nasmyth-Cassegrain, is a reflec |
A classic zenith | telescope, also known as a zenith sector employs a str |
With the Hubble Space | Telescope also the ultraviolet part of the stellar spe |
n for the proposed Terrestrial Planet Finder | telescope, also to be used on the James Webb Space Tel |
The Kunlun Dark Universe Survey | Telescope, also known as KDUST, is a proposed large su |
tical encoders corrected for errors, and the | telescope also came with auto-guiding CCD and planetar |
omes fixated on watching Olimpia through his | telescope, although her fixed gaze and motionless stan |
ting serving only to carry the weight of the | telescope although there are equatorial versions. |
nts in the objective lens of an astronomical | telescope, although this material had previously been |
lector; an 85cm reflector; a 60/90cm Schmidt | telescope; an 1.26m infrared telescope; and a 2.16m te |
tory was built to house Mr. Witte's personal | telescope, an eight inch refractor made by J. W. Fecke |
the "Father of Geometry") is a planned space | telescope, an M-class mission of the ESA Cosmic Vision |
tenure, with a twelve inch Clarke refractor | telescope and a transit instrument emplaced atop Pupin |
fields and tennis courts, a large reflector | telescope, and a satellite downlink receiver which ena |
(1819-1900), who provided the funds for the | telescope and observatory. |
Newton built the first practical reflecting | telescope and developed a theory of colour based on th |
July 1723, to test John Hadley's reflecting | telescope, and reported favourably on its performance. |
The | telescope and its camera, including the telescope dome |
urveyor, credited with the inventions of the | telescope and theodolite, and a great popularizer of s |
dozen telescopes, including the Hubble Space | Telescope and large ground-based observatories, have s |
h was published in American Scientist, Sky & | Telescope, and other professional journals. |
was used on the Solar Maximum Mission, Space | Telescope, and Landsat-D Missions, among others. |
The secondary mirror assembly of the Keck | Telescope and its relationship to the primary mirror. |
After gaining a three-inch (76 mm) | telescope and learning to enjoy the hobby of amateur a |
rvatory was built in order to house the Beck | telescope and was dedicated in 1950. |
problem, the development of the Hubble Space | Telescope and for his leadership and development of th |
tions and data captured by the Spitzer Space | Telescope and other telescopes to create a complete pi |
th a 10-inch (250 mm) apochromatic refractor | telescope and German equatorial mount centered under a |
th for the people who designed and built the | telescope, and for the astronomical community. |
olved with such projects as the Hubble Space | Telescope and was the Deputy Project Manager of the Ob |
e star was discovered using the Hubble Space | Telescope and further investigated by the W.M. Keck Ob |
en Ron was in his teenage years, he bought a | telescope and recorded the position of stars. |
Iowa State University's original | telescope and observatory, located northwest of Ames, |
now works at Caltech with the Spitzer Space | Telescope and at NASA as a director. |
the Chandra X-ray Observatory, Spitzer Space | Telescope, and the Herschel Space Observatory. |
tical breadboard prototyping components, and | telescope and microscope attachments. |
He soon acquired a 4-inch (100 mm) | telescope and soon upgraded to a 6-inch (150 mm). |
school has a rare planetarium complete with | telescope and opening-rotating dome roof. |
echanics, Inc. or OMI is a high-end American | telescope and optics instrument manufacturer. |
e possible through his modernizations of the | telescope and his support of Copernicanism, which stat |
scovery was made on the Canada-France-Hawaii | Telescope and the Keck Telescope, both on Mauna Kea in |
instrument was called the Mobile Anisotropy | Telescope and it was positioned at Cerro Toco in the C |
Without this extreme cooling the | telescope and instruments would literally be 'blinded' |
Since the magnification provided by a | telescope and eyepiece is equal to the telescope's foc |
n "equatorial room" containing an equatorial | telescope and a "transit room" containing a transit te |
ired, and there is a gap of 12 m between the | telescope and dome. |
and includes two domes, with a 20" Newtonian | telescope and an 11" Schmidt-Cassegrain telescope insi |
data from the HIRES instrument of the Keck 1 | telescope and the HARPS instrument of ESO's 3.6m teles |
twin four story towers that are topped by a | telescope and a globe. |
ed for the university to construct a Schmidt | telescope and build a dome at Mount Stromlo in Austral |
turbulence generated by the building and the | telescope and to ensure the telescope temperature is a |
ving facilities like the lunar-laser ranging | telescope and the two satellite laser stations. |
referred image (one pathway) by means of one | telescope, and they can add light that has come by the |
the Lebedev "RT-22" 22 meter precision radio | telescope and until 1964 he was the chief scientist fo |
n Dartmouth where he was awarded the Queen's | Telescope and Pembroke College, Cambridge, where he gr |
ed the construction and commissioning of the | telescope, and the Science and Technology Facilities C |
bjects mostly using the 4 m Anglo-Australian | Telescope and plates from the 1.2m (47 in) UK Schmidt |
lished by the Religious Tract Society on the | Telescope and Microscope, The Atmosphere and Atmospher |
ian Observatory operate the Anglo-Australian | Telescope and the UK Schmidt telescopes on behalf of t |
orts of building an indigenous large optical | telescope and a research observatory led to the foundi |
It houses a 24-inch Cassegrain reflecting | telescope and two computer systems: the first controls |
observatory has a 2.12 meter primary mirror | telescope and a 16 inch Meade used for extinction meas |
nia State University using the Spitzer Space | Telescope and the Hubble Space Telescope, as well as t |
Antarctic Submillimeter | Telescope and Remote Observatory, or AST/RO, is a 1.7 |
The dome acted as a shield for the | telescope and blocked out any unwanted energy rays. |
The observation tower had a 400x | telescope and an 18 million candlepower searchlight in |
, which houses a 22-inch (560 mm) reflecting | telescope and is used for research (primarily of binar |
ASTRA offered to repair the | telescope and drive if the then Monklands District Cou |
, and integration of the Hopkins Ultraviolet | Telescope and the Astro Observatory. |
nclude the Minnesota 1.5 meter, the Jamieson | telescope and a robotic telescope operated from South |
at Observatories, including the Hubble Space | Telescope and the Spitzer Space Telescope. |
and Goddard Space Flight Center designed the | telescope and the spacecraft, respectively. |
follow-up observations with the Hubble Space | Telescope and the European Southern Observatory's Very |
s caught spying on Oklahoma practices with a | telescope and a camera. |
NOT, the WHT, the DOT, the SST, the Mercator | Telescope and the ING |
ts through a modern 40 cm schmidt-cassegrain | telescope and a historic 29 cm refractor telescope bui |
sed on observations made by the Hubble Space | Telescope and Gemini Observatory on Cerro Pachon in Ch |
ical Observatory, home of a 67/92-cm Schmidt | telescope and the 182-cm telescope dedicated to Nichol |
trument's manufacturers, as inscribed on the | telescope and on the pendulum box-G. |
William Herschel | Telescope and the DOT |
in the nearby area include the Greek NESTOR | telescope and the Italian NEMO telescope, which are bo |
The Swiss Euler 1.2m | Telescope and the Mercator Telescope were part of the |
e four separate telescopes of the Very Large | Telescope, and the Large Binocular Telescope. |
he name comes from Astronomy with a Neutrino | Telescope and Abyss environmental RESearch project; th |
Hill Observatory houses the Canopus 1 metre | telescope and is situated approximately 12 km from Hob |
A 1-meter radio | telescope and a space theatre are planned to be constr |
rs to erect a 0.5 metre (20 inch) reflecting | telescope, and 0.25 metre refracting telescope on the |
reelanced for astronomy magazines such Sky & | Telescope and Astronomy. |
This observatory hosts a 1.2m infrared | telescope and also several aeronomy experiments. |
mpers have access to a 12", 20", 40" and 60" | telescope, and on the nearby Mount Bigelow site, a 61" |
etected in 2009 by the Fermi Gamma-ray Space | Telescope and by the AGILE satellite. |
tory, equipped with a seven-inche refracting | telescope and two smaller telescopes, forms one of the |
a very long spiral staircase leading to the | telescope and a balcony called "The Bok Walk". |
s used by the ancient Assyrians as part of a | telescope, and that this explains their knowledge of a |
from multiple wavelengths from Hubble, ESO's | telescope and NASA's Chandra and used virtual observat |
ryostat of the payload module surrounded the | telescope and science instrument with a large dewar co |
The | telescope and related instrumentation were run by the |
t the NICMOS instrument for the Hubble Space | Telescope and the MIPS instrument for the Spitzer Spac |
He designed the massive radar / radio | telescope and oversaw its construction in the karst fo |
ics imager (e.g., a refracting or reflecting | telescope, and therefore is normally not favored at wa |
that amount would go the construction of the | telescope and observatory; the other half to a permane |
xisting 15-metre (49 ft) James Clerk Maxwell | Telescope and 10.4-metre (34.1 ft) Caltech Submillimet |
pact has been studied by NASA's Hubble Space | Telescope, and the study suggests that the observed in |
t subsequent observation by the Hubble Space | Telescope and the VLT has shown that the objects move |
stained glass, images from the Hubble Space | Telescope, and the Discovery Pavilion, an educational |
s equipped with a 6-inch (150 mm) refracting | telescope and was the site of E. E. Barnard's earliest |
Sputnik 1 and Voyager 2 to the Hubble Space | Telescope and International Space Station, as are exte |
ty, which introduced the idea of the network | telescope and provided major empirical results regardi |
y maintains an eight-inch Schmidt-Cassegrain | telescope and a solar telescope. |
comes the first to study a comet through the | telescope and gives the first description of the nucle |
displays some of the characteristics of the | telescope and the site. |
tronomers at the Vatican Advanced Technology | Telescope announced the discovery of a small moon orbi |
s of galaxies drawn from NASA's Hubble Space | Telescope archive. |
To view it, binoculars or a | telescope are necessary, as it is too faint to be visi |
be to the question of whether the walls of a | telescope are made of metal or cardboard. |
imary instruments for the 40-inch (1,000 mm) | telescope are a 2048x2048 SITe CCD for direct imaging |
klin for whom he made a set of magnets and a | telescope around 1758. |
The discovery was made with a | telescope array at the South African Astronomical Obse |
The Pachmarhi | telescope array stands at Pachmarhi, Madhya Pradesh, I |
For a very different science goal, the Allen | Telescope Array has offered to provide the downlink fo |
y Solar Array (OVSA) is a astronomical radio | telescope array with main interests in studying the ph |
Telescope Array Project | |
Air Shower Array (AGASA) experiments is the | Telescope Array Project which began data collection in |
The Pachmarhi | Telescope Array or Pachmarhi Array of Cerenkov Telesco |
Multi-spectral solar | telescope array (MSSTA), a rocket launched payload of |
Design of the Cherenkov | Telescope Array, a matrix of Cherenkov Telescopes ten |
The Multi-spectral solar | telescope array, or MSSTA, was a sounding rocket paylo |
e painting, and I don't think even the Sky & | Telescope article is that speculative. |
Sun Gun | Telescope, as featured in the August 1999 issue of Sci |
e appeared in Astronomy Magazine and Sky and | Telescope as well as an astronomy textbook for German |
Keck telescopes (the world's largest optical | telescope as of 2005) to measure the spectra and hence |
e spare RSU would not impact the life of the | telescope, as it had been fully refurbished on the gro |
mining the faintest stars visible in a small | telescope as there are a wide range of stellar magnitu |
2 with a 0.91-m reflector and 0.50-m Schmidt | telescope as a branch station of the Tokyo Astronomica |
Chajnantor is an ideal location for such a | telescope, as the region is one of the driest on the p |
The | telescope as seen in May 2008. |
try, and also operates the Sheshan 25m radio | telescope as part of the Chinese VLBI array and the EV |
performed by eye, the CCD camera makes this | telescope as powerful as a 100-inch (2.5 meter) telesc |
When he was 14 he received a 60 mm | telescope as a Christmas present: the first of nearly |
much lighter, unaberrated mirror and optical | telescope assembly. |
rther study of the system using Hubble Space | Telescope astrometry revised the mass of HD 38529 c do |
with astrometric data from the Hubble Space | Telescope, astronomers have determined the orbital inc |
ble-light wavelengths, use of the Very Large | Telescope at Cerro Paranal has revealed the presence o |
n equatorial mount for the 8-inch refracting | telescope at Aldershot Observatory. |
Originally the Vacuum Tower | Telescope at Sacramento Peak, it was renamed in 1998 i |
William Lassell in 1862 using his four-foot | telescope at Malta, and by M. Trouvelot from Cambridge |
81 on a plate taken with the 1.2m UK Schmidt | telescope at Siding Spring, Australia. |
It is operated at the MPI/ESO 2.2m | telescope at the La Silla Observatory. |
c plates taken by Tom Gehrels on the Schmidt | telescope at the Palomar observatory. |
Pierce, established the McMath-Pierce Solar | Telescope at Kitt Peak Observatory near Tucson, Arizon |
RA is the World's highest angular resolution | telescope at near-infrared wavelengths. |
spectrograph mounted on the ESO's 3.6 meter | telescope at La Silla, Chile. |
es brighter than normal by the Magellan-Clay | telescope at Las Campanas Observatory in Chile. |
uthland Astronomical Society Observatory and | telescope at the Southland Museum and Art Gallery, wit |
One antenna of the One-Mile | Telescope at the observatory |
The Northumberland | Telescope at Cambridge Observatory, The Observatory 60 |
Danish 1.54m | telescope at ESO, La Silla, Chile |
It was mounted on the ESO 3.6m | telescope at La Silla Observatory. |
Milton L. Humason using the 100-inch (2.5 m) | telescope at Mount Wilson Observatory. |
by the HARPS spectrograph on ESO's 3.6-metre | telescope at La Silla, GJ1214b is the second super-Ear |
taken by Tom Gehrels with the Samuel Oschin | telescope at the Palomar Observatory, it was given the |
h African Astronomical Observatory 1.0 meter | telescope at Sutherland, South Africa |
from CT Chamaeleontis, using the Very Large | Telescope at the European Southern Observatory. |
being deputy astronomer of the U.K. Schmidt | telescope at Siding Spring, with which this minor plan |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |
こんにちは ゲスト さん
ログイン |
Weblio会員(無料)になると 検索履歴を保存できる! 語彙力診断の実施回数増加! |