「photometry」の共起表現(1語右で並び替え)

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e he wrote his dissertation on photoelectric	photometry, a copy of which is available online.
He singlemindedly devoted himself to	photometry and its improvement.
He studied cosmology, stellar convection,	photometry and the Zodiacal light.
He specialized in photoelectric	photometry and held the patent on the Cuffey Iris Photo
lanetary, deep sky, NEO studies, astrometry,	photometry and astrophotography.
der (refractore, diameter 90 mm) both comets	photometry and night observation for public
elescopes which use CCD cameras for imaging,	photometry, and astrometric studies.
In	photometry and radiometry intensity has a different mea
Landolt has worked principally in	photometry and has published a number of widely used li
He worked in astronomical	photometry and spectroscopy and is well known for creat
met discovery and observation, variable star	photometry, and supernova and nova discovery, and color
eroid search programs, gamma ray bursts, CCD	photometry and building state-of-the-art amateur observ
e, and with the modern invention of CCDs and	photometry and automated and computerized search progra
ing infra-red absorption spectrometry, flame	photometry, and investigated the potential of circular
n and other new measurement units for use in	photometry, based on the metre and the Violle candle.
xamples of stray light rejection and precise	photometry because the total brightness from the solar
s-on CCD (charge coupled device) imaging and	photometry by interested students, trained visitors, an
This time he used the Harvard Revised	Photometry catalogue for the positions and brightnesses
ystem became evidient, the UBV Photoelectric	Photometry Catalogue was phased-out in 2000.
The UBV Photoelectric	Photometry Catalogue, or UBV M, is the star brightness
ctroscopic measurements complement the rapid	photometry for selected prime targets.
However, modern photometric	photometry has detected a short "horizontal branch" in
In	photometry, luminous energy is the perceived energy of
s, transit detections of exoplanets, Vilnius	photometry, M-Dwarf star analysis, dynamical system ana
2:	Photometry of WFC images of M81
Brunner William, "Contributions to the	photometry of night sky", Zurich, 1935.
r and photographer, but later specialized in	photometry of variable stars.
used on double stars, parallax measurements,	photometry of variable stars and clusters, and so forth
He mainly worked on the	photometry of galactic star clusters, but also on the a
for their work in the field of photoelectric	photometry of variable stars.
arted a five year collaboration with NASA on	photometry of the Moon and planets using a 12-inch (300
oratory, who specializes in spectroscopy and	photometry of minor planets.
tions of the scientific research: multicolor	photometry of stars, stellar physical parameters, stell
Kosmos 215 performed ultraviolet	photometry of 36 A and B stars from parallel telescopes
for their work in the field of photoelectric	photometry of variable stars.
vidicon systems and early CCD detectors for	photometry of faint stars and galaxies.
am of Rafael Rebolo obtained R & I broadband	photometry on March 19, 1998.
udy of the asteroid by the Ondrejov Asteroid	Photometry Project concludes that a rotational period o
ervatory in 2004 mainly for minor planet CCD	photometry purposes.
active in discovering exoplanets, in stellar	photometry, stellar evolution models, and has been invo
tardome contributed 250 hours of time-series	photometry to this collaboration.
Also,	photometry using 60-cm Cassegrain telescope is made and
lowing her retirement, by D. Owings; and the	photometry was performed under the direction of T. Gehr
th Africa when positional determinations and	photometry were the main interests of the astronomical
This is done using	photometry, which is the practice of measuring the brig

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