• 드라이브 ㆍ 컨트롤
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• 제20권2호
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• pp.15-23
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• 2023

In this study, two-dimensional location of crops for auto weeding was detected using deep learning. To construct a dataset for soybean detection, an image-capturing system was developed using a mono camera and single-board computer and the system was mounted on a weeding robot to collect soybean images. A dataset was constructed by extracting RoI (region of interest) from the raw image and each sample was labeled with soybean and the background for classification learning. The deep learning model consisted of four convolutional layers and was trained with a weakly supervised learning method that can provide object localization only using image-level labeling. Localization of the soybean area can be visualized via CAM and the two-dimensional position of the soybean was estimated by clustering the pixels associated with the soybean area and transforming the pixel coordinates to world coordinates. The actual position, which is determined manually as pixel coordinates in the image was evaluated and performances were 6.6(X-axis), 5.1(Y-axis) and 1.2(X-axis), 2.2(Y-axis) for MSE and RMSE about world coordinates, respectively. From the results, we confirmed that the center position of the soybean area derived through deep learning was sufficient for use in automatic weeding systems.

• 생명과학회지
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• 제24권12호
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• pp.1276-1283
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• 2014

조직의 구조 안정성을 유지하는 세포 사이 연접복합체는 multi-PDZ domain protein 1 (MUPP1)을 포함하여 50종류 이상의 단백질로 이루어져 있다. MUPP1은 13개의 PDZ 도메인을 가지는 단백질로서 막경유(transmembrane) 단백질과 세포골격단백질이나 신호단백질 사이에서 scaffold로 작용한다고 알려져 있지만, MUPP1이 어떻게 세포막인접 단백질들을 연결하고 구조 안정화에 기여하는지에 대해 아직 명확히 밝혀지지 않았다. 본 연구에서 MUPP1의 PDZ 도메인과 상호 작용하는 단백질을 규명하기 위하여 효모 two-hybrid 방법을 이용, cell adhesion molecule 1 (Cadm1; SynCAM1, Necl-2 또는 TSLC1로도 알려짐)이 MUPP1과 결합하는 것을 확인하였다. Cadm1은 MUPP1의 2번째 PDZ 도메인과 결합하며, Cadm1의 C-말단에 존재하는 II 형 PDZ-결합모티프(-Y-F-I)가 MUPP1과의 결합에 필수적임을 확인하였다. 또한 MUPP1은 다른 Cadm family 단백질들인 Cadm2, Cadm3, 그리고 Cadm4와도 결합하며, 이러한 단백질간 결합은 glutathione S-transferase (GST) pull-down assay와 공동면역침강으로도 추가 확인하였다. 생쥐의 뇌 파쇄액을 MUPP1 항체로 면역침강하였을 때 Cadm1과 Cadm4가 같이 침강하였다. 이러한 결과들은 MUPP1이 세포 사이 연접에서 Cadms와 세포골격 단백질 사이를 연결한다는 것을 시사한다.

• 한국재료학회지
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• 제8권7호
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• pp.648-652
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• 1998

자동차용 캠 샤프트의 표면경화를 위해 TiG 용접공정에 의한 재용융처리가 실시되었다. 재용융처리는 캠축에 평행한 방향으로 행하여졌다. 캠 샤프트 소재의 조직은 편상의 흑연과 퍼얼라이트의 회주철 조직으로 구성되어 있으나 재용융 처리후 미세한 퍼얼라이트 및 세멘타이트와 구상 오스테나이트의 레데브라이트 조직으로 변화하였다. 캠 샤프트 모재의경도는 HRc 25~28에서 재용융 처리후에는 HRg 53~55정도로 증가하였다. 다층 용융 처리시 비드가 겹치는 경계에서 검은띠가 관찰되었는데 이 검은띠는 흑연으로 판명되었다. 이 검은띠는 전층의 레데브라이트 조직이 변태된 것으로 주로 세멘타이트와 기지조직의 경계에서 생성되었다. 고밀도 에너지인 레이저 용융처리시에도 재흑연화 현상은 TIG의 경우처럼 관찰되었다. 재흑연화 현상의 확인을 위해서 Gleeble 1500을 이용하여 $1100^{\circ}C$와 $1000^{\circ}C$에서 0.5, 1, 3, 5 및 10초동안 유지한 모의실험을 하였다. $1000^{\circ}C$에서 0.5초 유지했을 때도 흑연이 발견된 것으로 보아 재흑연화 현상은 어떠한 재용융 처리 공정을 사용하더라도 피할 수 없는 현상임을 확인할 수 있다.

• 천문학회보
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• 제42권2호
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• pp.74.2-74.2
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• 2017

Faint quasars are important to test the possibility that quasars are the main contributor to the cosmic reionization. However, it has been difficult to find faint quasars due to the lack of deep, wide-field imaging data. In this poster, we present our efforts to find faint quasars in the ELAIS-N1 field through the deep data (iAB ~ 25) obtained by the Subaru Hyper Suprime-Cam (HSC) Strategic Program survey. To select reliable quasar candidate, we also use the near-infrared (NIR) data of the Infrared Medium-deep Survey (IMS) and the UKIRT Infrared Deep Sky Survey (UKIDSS) - Deep Extragalactic Survey (DXS). Using multiple-band color cuts, we select high redshift quasar candidates. To confirm them as high redshift quasars, candidates are observed by the SED camera for QUasars in EArly uNiverse (SQUEAN) instrument in several medium band filters that can sample the redshifted Lyman break efficiency. The quasar sample will be used to study the growth of BH and stellar mass, the relation between the quasar activity and the host galaxy, and their contribution to the cosmic re-ionization.

• 대한한방부인과학회지
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• 제21권4호
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• pp.228-236
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• 2008

Purpose: The purposes of this study is to provide basic informations on oriental medical research and treatment through analysis of breast cancer patients, who visited M $\mu$ integrative cancer center, O O university East-West neo medical center. Methods: Electronic medical records of 106 breast cancer patients who visited oriental medical center from June 2, 2006 to February 28, 2008 were selected to collect clinical data of those patients. Clinical data were analyzed for types of clinical characteristics, and received therapies. For analysis of survival and recurrence, Kaplan-Meier method was used. All the data were processed and analyzed using SPSS version 13.0. Results: Average age of breast cancer patients, who visited oriental medical center was 48.72 ($\pm$10.13). The stage distribution record indicated stage I (5.8%), stage II (7.0%), stage III (5.8%), and stage IV (81.4%). Original purposes of patients were analyzed to be supplementary treatment for western therapy (68.9%), treatment for recurrence prevention (18.9%), and oriental medical treatment (12.2%) in order. While receiving oriental medical treatment, 60.4% of patients received conventional medical treatment simultaneously. Conclusion: Majority of patients who visited oriental medical hospital were stage IV at terminal stage and mainly visited for the purpose of supportive care. Further clinical study of breast cancer patients is needed to validate the effectiveness of oriental medical treatment based on this study.

• 천문학논총
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• 제32권1호
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• pp.225-230
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• 2017

The extragalactic background suggests half the energy generated by stars was reprocessed into the infrared (IR) by dust. At z~1.3, 90% of star formation is obscured by dust. To fully understand the cosmic star formation history, it is critical to investigate infrared emission. AKARI has made deep mid-IR observation using its continuous 9-band filters in the NEP field ($5.4deg^2$), using ~10% of the entire pointed observations available throughout its lifetime. However, there remain 11,000 AKARI infrared sources undetected with the previous CFHT/Megacam imaging (r ~25.9ABmag). Redshift and IR luminosity of these sources are unknown. These sources may contribute significantly to the cosmic star-formation rate density (CSFRD). For example, if they all lie at 1< z <2, the CSFRD will be twice as high at the epoch. We are carrying out deep imaging of the NEP field in 5 broad bands (g, r, i, z, and y) using Hyper Suprime-Camera (HSC), which has 1.5 deg field of view in diameter on Subaru 8m telescope. This will provide photometric redshift information, and thereby IR luminosity for the previously-undetected 11,000 faint AKARI IR sources. Combined with AKARI's mid-IR AGN/SF diagnosis, and accurate midIR luminosity measurement, this will allow a complete census of cosmic star-formation/AGN accretion history obscured by dust.