In-Ohk Ouh, Min Jung Kim, Kwang wook Kim, Hee ji Lim, Ye Jin Yang, Hu-Jang Lee, Woo H. Kim, Phil-Ok Koh, Seo Young Moon, Kyoung Hwa Choi, Yoo-Kyoung Lee, Kwang Il Park
This study evaluated the immunogenicity of the Bacillus Calmette-Guérin (BCG) vaccine in a guinea pig model to refine preclinical assessment methods. 24 guinea pigs were divided into four groups for immunohistochemical, histopathological, and molecular analyses, including qRT-PCR and ELISA. The ELISA results revealed significant elevations in interleukin 2 (IL-2), interferon-gamma (IFN- ), and tuberculosis-specific antibodies in vaccinated guinea pigs, particularly γ notable after 6 weeks. Although lung cytokine levels remained unchanged, spleen gene expression showed significant differences in interleukin-17, interleukin-12, interleukin-1β, and C-X-C motif chemokine ligand 10 after 6 weeks. Immunohistochemistry revealed peak IL-2 expression at 8 weeks and significant IFN-γ and TNF-α expression at 6 weeks. This study confirmed the effectiveness of BCG vaccine in guinea pigs, providing crucial insights for future tuberculosis vaccine development and standardizing immune response indicators.
Aqueous Zn-ion batteries (ZIBs) are very attractive owing to their high safety and low cost. Among various cathode materials, organic materials-based electrodes incorporating various redox functional groups have gained significant attention in the field of ZIBs due to their benefits of a tunable structural design, facility, eco-friendly, and possibility of multivalent energy storage. Herein, we demonstrate the nanostructured organic active materials deposited onto the CNT networks (HyPT@ CNT) for flexible ZIBs. This HyPT nanorods were obtained reassemblying the herringbone structured 3,4,9,10-tetracarboxylic dianhydride through a hydrothermal process in the presence of acid. These HyPT@CNT hybrids were electronically conductive and redox active, as well as could be fabricated into a flexible electrode achieving flexibility from mechanical integrity of robust networked structure. The as-fabricated flexible ZIBs delivered the high capacity of 100 Ah g− 1 at a current density of 0.1 A g− 1 and long-term cycling performance exceeding 5000 cycles. Consequently, these electrochemical performances are associated with the redox reactivity of carbonyl groups as verified by spectroscopic and electrochemical characterizations and the hybridization of HyPT nanorods with CNT networks.
Myungshin Im, Yonggi Kim, Chung-Uk Lee, Hee-Won Lee, Soojong Pak, Hyunjin Shim, Hyun-Il Sung, Wonseok Kang, Taewoo Kim, Jeong-Eun Heo, Tobias C. Hinse, Masateru Ishiguro, Gu Lim, Cuc T. K. LY, Gregory S. H. Paek, Jinguk Seo, Joh-na Yoon, Jong-Hak Woo, Hojae Ahn, Hojin Cho, Changsu Choi, Jimin Han, Sungyong Hwang, Tae-Geun Ji, Seong-Kook J. Lee, Sumin Lee, Sunwoo Lee, Changgon Kim, Dohoon Kim, Joonho Kim, Sophia Kim, Mankeun Jeong, Bomi Park, Insu Paek, Dohyeong Kim, Changbom Park
Even in an era where 8-meter class telescopes are common, small telescopes are considered very valuable research facilities since they are available for rapid follow-up or long term monitoring observations. To maximize the usefulness of small telescopes in Korea, we established the SomangNet, a network of 0.4{1.0 m class optical telescopes operated by Korean institutions, in 2020. Here, we give an overview of the project, describing the current participating telescopes, its scientic scope and operation mode, and the prospects for future activities. SomangNet currently includes 10 telescopes that are located in Australia, USA, and Chile as well as in Korea. The operation of many of these telescopes currently relies on operators, and we plan to upgrade them for remote or robotic operation. The latest SomangNet science projects include monitoring and follow-up observational studies of galaxies, supernovae, active galactic nuclei, symbiotic stars, solar system objects, neutrino/gravitational-wave sources, and exoplanets.
Yongjung Kim, Myungshin Im, Yiseul Jeon, Minjin Kim, Soojong Pak, Minhee Hyun, Yoon Chan Taak, Suhyun Shin, Gu Lim, Gregory S. H. Paek, Insu Paek, Linhua Jiang, Changsu Choi, Jueun Hong, Tae-Geun Ji, Hyunsung D. Jun, Marios Karouzos, Dohyeong Kim, Duho Kim, Jae-Woo Kim, Ji Hoon Kim, Hye-In Lee, Seong-Kook Lee, Won-Kee Park, Yongmin Yoon, Seoyeon Byeon, Sungyong Hwang, Joonho Kim, Sophia Kim, Woojin Park
Metal matrix composites(MMC) can obtain mechanical characteristics of application purposes that a single material is difficult to obtain. Al2 O3/AC8A composites were fabricated by low pressure infiltration process. The purpose is establishing the optimal casting conditions for composite preparation under low pressure. It is known the inorganic binder help infiltration. Therefore Al2O3 fiber preform's optimum sinter temperature is 1160℃, added inorganic binder is mixed binder(SiO2 sol:Al2O3 sol=5:2). And three fibers have been compared (Al2O3 80%/SiO2 20%, Al2O3 80%/SiO2 10% and Al2O3 97%/SiO2 3%). Al2O3/AC8A composites was made by each melting temperatures(650℃, 700℃, 750℃) and wear test was performed about effect of temperatures, kind of fiber, matrix and composites, aging time. Wear test is Ball on disk wear test. The resistance increased with the low melting temperature and Al2O3 80%/SiO2 20% fiber.
I.-G. Shin, Y.-H. Ryu, A. Udalski, M. Albrow, S.-M. Cha, J.-Y. Choi, S.-J. Chung, C. Han, K.-H. Hwang, Y. K. Jung, D.-J. Kim, S.-L. Kim, C.-U. Lee, Y. Lee, B.-G. Park, H. Park, R. W. Pogge, J. C. Yee, P. Pietrukowicz, P. Mroz, S. Koz lowski, R. Poleski, J. Skowron, I. Soszynski, M. K. Szymanski, K. Ulaczyk, L. Wyrzykowski, M. Pawlak, A. Gould
We report the characterization of a massive (mp = 3:91:4Mjup) microlensing planet (OGLE- 2015-BLG-0954Lb) orbiting an M dwarf host (M = 0:33 0:12M) at a distance toward the Galactic bulge of 0:6+0:4 0:2 kpc, which is extremely nearby by microlensing standards. The planet-host projected separation is a? 1:2AU. The characterization was made possible by the wide-eld (4 deg2) high cadence ( = 6 hr1) monitoring of the Korea Microlensing Telescope Network (KMTNet), which had two of its three telescopes in commissioning operations at the time of the planetary anomaly. The source crossing time t = 16 min is among the shortest ever published. The high-cadence, wide-eld observations that are the hallmark of KMTNet are the only way to routinely capture such short crossings. High-cadence resolution of short caustic crossings will preferentially lead to mass and distance measurements for the lens. This is because the short crossing time typically implies a nearby lens, which enables the measurement of additional eects (bright lens and/or microlens parallax). When combined with the measured crossing time, these eects can yield planet/host masses and distance.