• Title/Summary/Keyword: EHT1

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MO Studieson on Configuration and Conformation (V). Conformation of Inositol (配置와 形態에 관한 分子軌道論的 硏究 (第5報). 이노시톨의 形態)

  • Ikchoon Lee;Joo Hwan Sohn;Shi Choon Kim;Young Koo Jeon
    • Journal of the Korean Chemical Society
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    • v.23 no.5
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    • pp.271-276
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    • 1979
  • The EHT and CNDO/2 molecular orbital calculations were performed to determine relative stabilities of various conformers of inositol. Our EHT results agree with experimental findings, and correctly predict the destabilizing effect of 1,3-nonbonded interaction of O atoms. In addition, the EHT result show that attractive potential energies between hydroxyl hydrogens and neighboring oxygens are another major factor determining conformational preferences. The inability of CNDO/2 method in predicting correct destabilizing effect of lone pair interaction caused overestimation of stabilization energies for conformers which had 1,3-interactions. The EHT method is superior to the CNDO/2 method for conformational studies of inositols.

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EHT data processing and BH shadow imaging techniques

  • Cho, Ilje
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.1
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    • pp.59.2-59.2
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    • 2019
  • Event Horizon Telescope (EHT) aims to resolve the innermost region to the super massive black hole (SMBH) with its extremely high angular resolution (~20-25 uas) and enhanced sensitivity (down to 1-10 mJy) in concert with the Atacama Large Millimeter/submillimeter Array (ALMA) at 1.3 mm wavelength. This has a great importance as the first observational probe of the black hole shadow which has been theoretically predicted as a ring-like emission affected by the general relativistic effect under a strong gravitational field of SMBH. During the 2017 April 5-11, four nights of EHT observing campaign were carried out towards its primary targets, M87 and $SgrA{\ast}$. To robustly ensure the data processing, independent pipelines for various radio data calibration softwares (e.g., AIPS, HOPS, CASA) have been developed and cross-compared each other. The EHT has also been developing newer interferometric imaging techniques (e.g., eht-imaging-library, SMILI, dynamical imaging), as well as using an established method (CLEAN). With these, the EHT has designed various strategies which will be adopted for convincing imaging results. In this talk, I review how the robustness of EHT data processing and imaging will be validated so that the results can be ensured against well known uncertainties or biases in the interferometric data calibration and imaging.

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Event Horizon Telescope : Earth-sized mm-VLBI array to image supermassive black holes

  • Kim, Jae-Young
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.1
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    • pp.59.1-59.1
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    • 2019
  • Immediate vicinity of a supermassive black hole (SMBH) is an important place to test general relativity in strong gravity regime. Also, this is a place where mass accretion and jet formation actively occurs at the centers of active galaxies. Theoretical studies predict presence of bright ring-like emission encircling an accreting SMBH with a diameter of about 5 Schwarzschild radii, and a flux depression at the center (i.e., BH shadow). Direct imaging of the BH shadow is accordingly of great importance in modern astrophysics. However, the angular sizes of the horizon-scale structures are desperately small (e.g., ~40-50 microarcseconds (uas) diameter for the nearest best candidates). This poses serious challenges to observe them directly. Event Horizon Telescope (EHT) is a global network of sensitive radio telescopes operating at 230 GHz (1.3 mm), providing ultra-high angular resolution of 20 uas by cutting-edge very long baseline interferometry techniques. With this resolution, EHT aims to directly image the nearest SMBHs; M87 and the galactic center Sgr $A{\ast}$ (~40-50 uas diameters). In Spring 2017, the EHT collaboration conducted a global campaign of EHT and multiwavelength observations of M87 and Sgr $A{\ast}$, with addition of the phased ALMA to the 1.3mm VLBI array. In this talk, I review results from past mm-VLBI and EHT observations, provide updates on the results from the 2017 campaign, and future perspectives.

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Downregulation of EHT1 and EEB1 in Saccharomyces cerevisiae Alters the Ester Profile of Wine during Fermentation

  • Yang, Xue;Zhang, Xuenan;He, Xi;Liu, Canzhen;Zhao, Xinjie;Han, Ning
    • Journal of Microbiology and Biotechnology
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    • v.32 no.6
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    • pp.761-767
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    • 2022
  • EHT1 and EEB1 are the key Saccharomyces cerevisiae genes involved in the synthesis of ethyl esters during wine fermentation. We constructed single (Δeht1, Δeeb1) and double (Δeht1Δeeb1) heterogenous mutant strains of the industrial diploid wine yeast EC1118 by disrupting one allele of EHT1 and/or EEB1. In addition, the aromatic profile of wine produced during fermentation of simulated grape juice by these mutant strains was also analyzed. The expression levels of EHT1 and/or EEB1 in the relevant mutants were less than 50% of the wild-type strain when grown in YPD medium and simulated grape juice medium. Compared to the wild-type strain, all mutants produced lower amounts of ethyl esters in the fermented grape juice and also resulted in distinct ethyl ester profiles. ATF2, a gene involved in acetate ester synthesis, was expressed at higher levels in the EEB1 downregulation mutants compared to the wild-type and Δeht1 strains during fermentation, which was consistent with the content of acetate esters. In addition, the production of higher alcohols was also markedly affected by the decrease in EEB1 levels. Compared to EHT1, EEB1 downregulation had a greater impact on the production of acetate esters and higher alcohols, suggesting that controlling EEB1 expression could be an effective means to regulate the content of these aromatic metabolites in wine. Taken together, the synthesis of ethyl esters can be decreased by deleting one allele of EHT1 and EEB1 in the diploid EC1118 strain, which may modify the ester profile of wine more subtly compared to the complete deletion of target genes.

MO Studies of Configuration and Conformation (Ⅲ). Conformations of Some 2-Substituted Furan, Thiophene and Pyrrole Carbonyl Compounds (配置와 形態에 관한 分子軌道函數論的 硏究 (第3報). Furan, Thiophene 및 Pyrrole 카르보닐 化合物의 2-置換體의 形態)

  • Ikchoon Lee;Shi Choon Kim
    • Journal of the Korean Chemical Society
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    • v.21 no.1
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    • pp.32-37
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    • 1977
  • Conformations of nine 2-substituted furan, thiophene and pyrrole compounds have been studied by EHT methods. The preferred conformations of furan derivatives were trans form, which were mainly stabilized by electrostatic interactions. For thiophenes, electronic conjugation between the ring S and carbonyl oxygen was dominant, while for pyrroles both the electrostatic and conjugation effects were operative in determining the preferred conformations. Results of EHT calculation agreed well with experimentally determined preferences.

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Influence of Drought and High Temperature on the Physiological Response and Yield in Hot Pepper (토양 건조 스트레스와 기온상승에 의한 고추의 생리반응 및 생산량 변화)

  • Lee, Sang Gyu;Lee, Hee Ju;Kim, Sung Kyeom;Mun, Bo heum;Lee, Jin Hyoung;Lee, Hee Su;Do, Kyung Ran
    • Journal of Environmental Science International
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    • v.27 no.4
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    • pp.251-259
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    • 2018
  • This study was conducted to determine the effects of combination of air temperature and soil water content on the growth, physiological disorder rate, and yield of hot peppers. The study was carried out in a typical plastic house (open on one side and with ventilation fans on the other side), which was maintained with gradient air temperature (maximum difference in air temperature: $6^{\circ}C$). The deficit irrigation (DI) treatment commenced 65 days after transplanting. The height of plant and fresh and dry weights of the stem increased at high air temperature (ambient + $6^{\circ}C$, extreme high temperature; EHT). Furthermore, the leaf area decreased significantly with the DI treatment. There were no significant differences in the stem diameter, number of branches, and fresh and dry weights of the leaves among all the treatments. The net photosynthesis rate of the full irrigation (FI) treatment was higher than that of the DI treatment. The photosynthesis rate at ambient air temperature was $19.7{\mu}mol\;CO_2m^{-2}{\cdot}s^{-1}$, the highest among all the treatments; however, the photosynthesis rate of the EHT treatment decreased by 60% ($12.3{\mu}mol\;CO_2m^{-2}{\cdot}s^{-1}$). Additionally, the formation of guard cells in the leaf was abnormal with the EHT treatment, and there was a decrease in translocation efficiency. The effects of air temperature treatment were more pronounced on the physiological disorder rate and yield. The physiological disorder rate of the EHT treatment was the highest under the DI treatment condition. The yield of the AFI (ambient air temperature with full irrigation) treatment was 3,771 kg/10a, the highest among all the treatments; however, the yield of the EHT treatment with DI and FI was 1,282 and 1,327 kg/10a, respectively. These results indicate that growth and physiological disorder rate improved with the EHT treatment; however, there was a decrease in yield. Furthermore, the formation of guard cells was abnormal and malfunctional.

An Ectopic Hamartomatous Thymoma : A Case Report (경부에 발생한 이소성 과오종성 흉선종 1례)

  • Lee, Dong-Jin;Park, Su-Kyung;Kim, Han-Shin;Shin, Mi-Kyung;Chu, Hyung-Ro
    • Korean Journal of Bronchoesophagology
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    • v.14 no.2
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    • pp.48-52
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    • 2008
  • Ectopic Hamartomatous thymoma(EHT) is a rare benign tumor that occurs mainly in the supraclavicular or suprasternal area. Since this entity was first reported by Smith et al. in 1982, less than 50 cases have been reported in the literature. Recognition of EHT is important and needs to be differentiated from high-grade sarcomas such as synovial sarcoma or malignant peripheral nerve sheath tumor because EHT follows a benign clinical course. We experienced a case of ectopic hamartomatous thymoma in the suprasternal area in a 53-year-old man. Here, we present the case with a review of the related literatures.

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Korean activities for mm-VLBI and EHT collaboration

  • Jung, Taehyun;Sohn, Bong Won;Zhao, Guangyao;Cho, Ilje;Kim, Jae-Young
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.1
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    • pp.59.3-59.3
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    • 2019
  • Very Long Baseline Interferometry (VLBI) is a special technique which can provide high angular resolutions of milliarcsecond and sub-milliarcsecond sales in radio astronomical observations. Recently, the mm/sub-mm VLBI observations becomes more widely available and related activities are increasing accordingly. In this talk, I'll introduce ongoing global mm-VLBI activities and EHT collaboration and our (Korean) contributions to them.

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