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Volumn 306, Issue 5705, 2004, Pages 2224-2227

Detection of a deep 3-μm absorption feature in the spectrum of Amalthea (JV)

Author keywords

[No Author keywords available]

Indexed keywords

ABSORPTION; INFRARED DETECTORS; MINERALS; ORBITS; PLANETS;

EID: 11144293483     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1105427     Document Type: Article
Times cited : (23)

References (31)
  • 1
    • 0003149264 scopus 로고
    • D. Morrison, Ed. (Univ. of Arizona Press, Tucson)
    • J. B. Pollack, F. Fanale, in Satellites of Jupiter, D. Morrison, Ed. (Univ. of Arizona Press, Tucson, 1982), pp. 872-910.
    • (1982) Satellites of Jupiter , pp. 872-910
    • Pollack, J.B.1    Fanale, F.2
  • 6
    • 0001281771 scopus 로고    scopus 로고
    • P. C. Thomas et al., Icarus 135, 360 (1998).
    • (1998) Icarus , vol.135 , pp. 360
    • Thomas, P.C.1
  • 12
    • 11144254751 scopus 로고    scopus 로고
    • note
    • The intensity of the scattered light from Jupiter was about five times that of the background sky level and was 20% of the peak intensity of the object in J band. It was about half of the background and 10% of the peak intensity of the object in H band. A linear function was fitted to the scattered light, which was thus subtracted from the background. The errors of the photometry include the possible incompleteness of the removal of scattered light.
  • 14
  • 26
    • 0010533725 scopus 로고    scopus 로고
    • W. F. Bottke Jr., A. Cellino, P. Paolicchi, R. P. Binzel, Eds. (Univ. of Arizona Press, Tucson)
    • A. S. Rivkin, E. S. Howell, F. Vilas, L. A. Lebofsky, in Asteroids III, W. F. Bottke Jr., A. Cellino, P. Paolicchi, R. P. Binzel, Eds. (Univ. of Arizona Press, Tucson, 2002), pp. 235-253.
    • (2002) Asteroids III , pp. 235-253
    • Rivkin, A.S.1    Howell, E.S.2    Vilas, F.3    Lebofsky, L.A.4
  • 31
    • 11144340037 scopus 로고    scopus 로고
    • notre
    • We thank the Subaru adaptive optics team, the IRCS team, and M. Goto, who made the observations possible. This report is partly based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.