Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000pasj...52....1k&link_type=abstract
Publications of the Astronomical Society of Japan, v.52, p.1.
Astronomy and Astrophysics
Astronomy
77
Ism: Individual (Orion Nebula), Stars: Luminosity Function, Mass Function, Telescopes
Scientific paper
This paper describes the first light and subsequent test observations with the 8.2 m aperture Subaru Telescope constructed at the summit of Mauna Kea. Following the engineering first light, which started 1998 December, the astronomical first light and test observations were carried out in 1999 January with 4 testing instruments under seeing conditions of 0.''2-0.''5 for near-infrared and 0.''3-0.6 for optical wavelengths. The actively supported primary mirror was shown to achieve an overall imaging performance of 0.''1 (FWHM) or better in the absence of any atmospheric disturbance. The pointing accuracy of the telescope is about 1'' rms, and a closed-loop tracking accuracy of <~ 0.''07 rms has been achieved. Infrared images of the Orion Nebula covering {5'}times {5'}, obtained with J, K', and H_2 v=1-0 S(1) filters, have revealed much finer and fainter details of the BN/KL region, the bright bar, and other conspicuous features compared with previous observations. K' band photometry of 516 point sources yielded a luminosity function with a peak at K' ~ 12 mag with a long tail in K' ~ 13 mag down to K' ~ 17 mag, suggesting a fairly large number of young brown dwarfs existing in the Trapezium cluster. Several new features around the Orion BN/KL region are also reported.
Akiyama Masayuki
Ando Hiroyasu
Aoki Tetsuo
Chikada Yoshihiro
Doi Mamoru
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