「Photometry」の共起表現一覧(1語右で並び替え)

Photometry

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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