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20012013
most citedThe AzTEC mm-Wavelength Camera

161 citations · 424 across the 8 of their papers we have counts for

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astro-ph2008★ 161 cited

The AzTEC mm-Wavelength Camera

G. W. Wilson, J. E. Austermann, T. A. Perera +13

AzTEC is a mm-wavelength bolometric camera utilizing 144 silicon nitride micromesh detectors. Herein we describe the AzTEC instrument architecture and its use as an astronomical in…

astro-ph2006★ 1 cited

Interplay between diffusion, accretion and nuclear reactions in the atmospheres of Sirius and Przybylski's star

Alexander Yushchenko, Vera Gopka, Stephane Goriely +8

The abundance anomalies in chemically peculiar B-F stars are usually explained by diffusion of chemical elements in the stable atmospheres of these stars. But it is well known that…

astro-ph2004★ 25 cited

Thorium-rich halo star HD221170: further evidence against the universality of the r-process

Alexander Yushchenko, Vera Gopka, Stephane Goriely +6

We report the abundance determination in the atmosphere of the bright halo star HD221170. The spectra were taken with the Terskol Observatory's 2.0-m telescope with a resolution R=…

astro-ph2003★ 11 cited

Raman Scattered He II 6545 Line in the Symbiotic Star V1016 Cygni

Hee-Won Lee, Young-Jong Sohn, Young Woon Kang +1

We present a spectrum of the symbiotic star V1016 Cyg observed with the 3.6 m Canada-France-Hawaii Telescope, in order to illustrate a method to measure the covering factor of the…

astro-ph2003★ 41 cited

Probing the Spatial Distribution of Extrasolar Planets with Gravitational Microlensing

Cheongho Han, Young Woon Kang

Under the current microlensing planet search strategy of monitoring events caused by stellar-mass lenses, only planets located within a narrow region of separations from central st…

astro-ph2001★ 1 cited

Astrometric Detection of Double Gravitational Microlensing Events

Cheongho Han, Byeong-Gon Park, Wonyong Han +1

If a gravitational microlensing event is caused by a widely separated binary lens and the source approaches both lens components, the source flux is successively magnified by the i…