排序方式： 共有5条查询结果，搜索用时 0 毫秒
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J. Schneider A. Boccaletti D. Mawet P. Baudoz J.-L. Beuzit R. Doyon M. Marley D. Stam G. Tinetti W. Traub J. Trauger A. Aylward J. Y-K. Cho C.-U. Keller S. Udry 《Experimental Astronomy》2009,23(1):357-377
The Super-Earth Explorer is an Off-Axis Space Telescope (SEE-COAST) designed for high contrast imaging. Its scientific objective is to make the physico-chemical characterization of exoplanets possibly down to 2 Earth radii. For that purpose it will analyze the spectral and polarimetric properties of the parent starlight reflected by the planets, in the wavelength range 400–1,250 nm. 相似文献
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J.-L. Beuzit L. Demailly E. Gendron P. Gigan F. Lacombe D. Rouan N. Hubin D. Bonaccini E. Prieto F. Chazallet D. Rabaud P.-Y. Madec G. Rousset R. Hofmann F. Eisenhauer 《Experimental Astronomy》1997,7(4):285-292
ADONIS is an adaptive optics (AO) user friendly instrument offered to the European astronomical community on the ESO 3.6-m telescope at La Silla. It is an upgraded version of COME-ON-PLUS, the VLT AO prototype, which already produced significative astrophysical results in a wide range of fields, from planetology to extragalactic astrophysics. ADONIS is now allowing the astronomer to use adaptive optics as a common user instrument thanks to the implementation of an open artificial intelligence software that handles the large number of parameters needed to optimise the AO correction. We will describe the ADONIS system, including the two dedicated infrared cameras, summarize its performances and discuss the observing procedures. 相似文献
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Mazeh T Naef D Torres G Latham DW Mayor M Beuzit JL Brown TM Buchhave L Burnet M Carney BW Charbonneau D Drukier GA Laird JB Pepe F Perrier C Queloz D Santos NC Sivan JP Udry S Zucker S 《The Astrophysical journal》2000,536(1):L55-L58
Three new silicon-bearing radicals of astrophysical interest, SiCCH and the two nearly isoenergetic isomers SiCN and SiNC, were detected in a laboratory discharge in their X2Pi ground states by Fourier transform microwave and millimeter-wave absorption spectroscopy. Hyperfine structure was observed in the low rotational transitions of the (2)Pi(1/2) ladder, and well-resolved Lambda-doubling was observed in both fine-structure ladders. With the spectroscopic constants derived from the laboratory measurements, the spectra of all three can be calculated to an uncertainty of less than 0.1 km s(-1) in equivalent radial velocity over the entire range of interest to radio astronomers. SiCN, with a dipole moment of 2.9 D, is probably the most promising of the three for astronomical discovery. 相似文献
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Jehin Emmanuel Boehnhardt Hermann Sekanina Zdenek Bonfils Xavier Schütz Oliver Beuzit Jean-Luc Billeres Malvina Garradd Gordon J. Leisy Pierre Marchis Franck Más Antonio Origlia Livia Scarpa Daniel Thomas Daniel Tozzi Gian Paolo 《Earth, Moon, and Planets》2002,90(1-4):147-151
Comet C/2001 A2 experienced several splitting events duringits 2001 perihelion passage. The first break-upevent was observed
in March 2001 (IAUC 7616).In this paper we report the first results of ourextensive imaging and spectroscopic monitoring campaignwith
ESO telescopes over several weeks before andafter the perihelion passage on May 25 2001. 相似文献
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