Zobrazeno 1 - 10
of 440
pro vyhledávání: '"C. Roddier"'
Publikováno v:
Icarus; November 2000, Vol. 148 Issue: 1 p320-320, 1p
Autor:
Akbari Zadeh, Naghmeh1 (AUTHOR) naghmeh.akbari@dkit.ie, Ryan, Peter1 (AUTHOR) peter.ryan@dkit.ie, Kennedy, David M.2 (AUTHOR) david.kennedy@tudublin.ie, O'Rourke, Fergal1 (AUTHOR) fergal.orourke@dkit.ie
Publikováno v:
Energies (19961073). Jan2025, Vol. 18 Issue 1, p22. 32p.
Autor:
J. L. Beuzit, M. C. Hainaut, Eduardo L. Martín, Francois Roddier, T. Forveille, Michel Mayor, C. Roddier, C. Perrier, X. Delfosse, D. Segransan, Stéphane Udry
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 425, pp.997-1008
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 425, pp.997-1008
We present some results of a CFHT adaptive optics search for companions to nearby dwarfs. We identify 21 new components in solar neighbourhood systems, of which 13 were found while surveying a volume-limited sample of M dwarfs within 12pc. We are obt
Publikováno v:
Adaptive Optics.
Summary not available.
Autor:
F. Roddier, C. Roddier
Publikováno v:
Publications of the Astronomical Society of the Pacific. 109:815
The detection of faint light sources very close to a bright star is primarily limited by light scattered by the Earth's atmosphere. This source of scattered light can now be reduced by means of adaptive optics, or totally eliminated by using a telesc
Autor:
Volkov, A. S.1 (AUTHOR), Khviyuzov, S. S.2 (AUTHOR) khviyuzov.s@yandex.ru
Publikováno v:
Journal of Applied Spectroscopy. Jan2024, Vol. 90 Issue 6, p1259-1266. 8p.
Publikováno v:
Journal of Marine Science & Engineering; Dec2024, Vol. 12 Issue 12, p2198, 20p
Publikováno v:
Optics Communications. 24:281-284
Theoretical transfer functions for astronomical speckle interferometry, through a defocused telescope, have been computed assuming a log-normal complex amplitude for the incoming wavefront. They are found in reasonable agreement with recently publish
Autor:
C. Roddier, F. Roddier
Publikováno v:
International Astronomical Union Colloquium. 49:175-185
In optical astronomy, images are highly degraded by atmospheric turbulence. The diameter of the seeing disk may vary from 0.2 arcseconds to 10 arcseconds or more according to weather conditions. A typical diameter is of the order of 2 arcseconds whic
Publikováno v:
Optica Acta: International Journal of Optics. 26:583-595
Measurements of the energy spectra of infra-red images of stellar point sources were made at the Coude focus of the 3·8 m telescope at Kitt Peak National Observatory, U.S.A. A scanning slit was used to record the irradiance distribution in the image