• Journal of Astronomy and Space Sciences
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• 제25권2호
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• pp.87-100
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• 2008

소백산 천문대의 61cm 망원경에 부착된 bvri CCD 측광 시스템으로 근접쌍성 V523 Cas를 2003년 1월에 4일 밤을 관측하여 792점의 CCD 영상을 얻었다. 이 영상 내에 있는 17개의 BVRI 표준성을 이용하여 소백산 천문대의 bvri 측광계와 Johnson-Cousins의 BVRI 측광계 사이의 변환 관계를 V=v-0.0689(B-V)+0.0063, B-V=1.3197(b-v)-0.1733, V-R=0.9210(v-r)-0.1309, R-I=0.8892(r-i)-0.1055와 같이 구하였다. 이 식을 이용하여 근접쌍성 V523 Cas 근처에 있는 57개 별들의 표준 V등급과 색지수(B-V, V-R, R-I)를 결정하였다.

• 천문학회보
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• 제42권1호
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• pp.58.1-58.1
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• 2017

National Youth Space Center has recently founded the Deokheung Optical Astronomy Observatory (DOAO) 1m Telescope, which accepts community observing applications since 2016. Standardization and calibration of the new observing facility are essential for astronomical research. In this poster, we present standardization processes and preliminary results for photometry of the Johnson-Cousins BVRI filter system. We selected sample data from a night in stable weather condition. After bias, dark, and flat corrections and photometry using ccdred and daophot package of IRAF, we derived standardized band pass parameters including color terms. The corrected photometry results of the BVRI filter system show reduced deviations from the standard magnitudes in the literature. In addition, we calculated atmospheric extinction coefficients and limiting magnitudes of the telescope system. We plan to extend these standardizing processes to flux calibration of narrow band filters, e.g. $H{\alpha}$ filter.

• Journal of Astronomy and Space Sciences
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• 제26권2호
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• pp.157-170
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• 2009

BVRI 표준성 52개를 충북대학교 천문대에서 1-m 망원경과 2K CCD 카메라로 2008년 9-12월 기간에 10일 밤 관측하여 1,322개의 CCD 영상을 얻었다. 우리가 사용한 측광계 bvr과 Johnson-Cousins의 측광계 BVR과 상호 관계를 V = v - 0.0303(B - V) + 0.0466 B - V = 1.3475(b - v) - 0.0251 V - R = 1.0641(v - r) - 0.0125와 같이 구하였다. 이 식을 이용하여 197개 별들의 V, B-V, V-R를 얻었다.

• 천문학회보
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• 제45권1호
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• pp.66.4-67
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• 2020

Gyeonggi science high school for the gifted (GSHS) installed 60cm telescope, which is waiting for student observers. It is essential to understand the characteristics of the photometric system, consisting of telescope, filter, and CCD, to get reliable data. CCD images of SA98 Landolt standard field and M67 were obtained on 19th March 2020. The images of each field were combined by filters, i.e., we ignored the monochromatic atmospheric extinction since the photometric objects themselves are standard stars. 24 standard stars in SA98 field and 12 standard stars in M67 were used to derive the tentative transformation equation between our bv photometric system and Johnson BV photometric system. In this poster, we present the preliminary standardization result for Johnson BV photometric system in GSHS 60cm telescope. The reproductivity is discussed by comparing color coefficients of two fields. We plan to extend this process to Johnsons-Cousins BVRI photometric system and narrow-band filters for flux calibration.

• 천문학회지
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• 제50권3호
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• pp.41-49
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• 2017

We conduct BVRI and R band photometric observations of asteroid (5247) Krylov from January 2016 to April 2016 for 51 nights using the Korea Microlensing Telescope Network (KMTNet). The color indices of (5247) Krylov at the light curve maxima are determined as $B-V=0.841{\pm}0.035$, $V-R=0.418{\pm}0.031$, and $V-I=0.871{\pm}0.031$ where the phase angle is $14.1^{\circ}$. They are acquired after the standardization of BVRI instrumental measurements using the ensemble normalization technique. Based on the color indices, (5247) Krylov is classified as a S-type asteroid. Double periods, that is, a primary period $P_1=82.188{\pm}0.013h$ and a secondary period $P_2=67.13{\pm}0.20h$ are identified from period searches of its R band light curve. The light curve phases with $P_1$ and this indicate that it is a typical Non-Principal Axis (NPA) asteroid. We discuss the possible causes of its NPA rotation.