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Park, Young-Hwan,Mishra, Ratnesh Chandra,Yoon, Sunkyung,Kim, Hoki,Park, Changho,Seo, Sang-Tae,Bae, Hanhong The Korean Society of Ginseng 2019 Journal of Ginseng Research Vol.43 No.3
Background: Ginseng (Panax ginseng Meyer) is an invaluable medicinal plant containing various bioactive metabolites (e.g., ginsenosides). Owing to its long cultivation period, ginseng is vulnerable to various biotic constraints. Biological control using endophytes is an important alternative to chemical control. Methods: In this study, endophytic Trichoderma citrinoviride PG87, isolated from mountain-cultivated ginseng, was evaluated for biocontrol activity against six major ginseng pathogens. T. citrinoviride exhibited antagonistic activity with mycoparasitism against all ginseng pathogens, with high endo-1,4-${\beta}$-D-glucanase activity. Results: T. citrinoviride inoculation significantly reduced the disease symptoms caused by Botrytis cinerea and Cylindrocarpon destructans and induced ginsenoside biosynthesis in ginseng plants. T. citrinoviride was formulated as dustable powder and granules. The formulated agents also exhibited significant biocontrol activity and induced ginsenosides production in the controlled environment and mountain area. Conclusion: Our results revealed that T. citrinoviride has great potential as a biological control agent and elicitor of ginsenoside production.
Park, Sunkyung,Lee, Jeong-Eun,Kang, Wonseok,Lee, Sang-Gak,Chun, Moo-Young,Kim, Kang-Min,Yuk, In-Soo,Lee, Jae-Joon,Mace, Gregory N.,Kim, Hwihyun,Kaplan, Kyle F.,Park, Chan,Sok Oh, Jae,Lee, Sungho,Jaffe American Astronomical Society 2018 The Astrophysical journal Supplement series Vol.238 No.2
<P>We present a library of high-resolution (R lambda/Delta lambda similar to 45,000) and high signal-to-noise ratio (S/N >= 200) near-infrared spectra for stars of a wide range of spectral types and luminosity classes. The spectra were obtained with the Immersion GRating INfrared Spectrograph covering the full range of the H (1.496-1.780 mu m) and K (2.080-2.460 mu m) atmospheric windows. The targets were primarily selected for being MK standard stars covering a wide range of effective temperatures and surface gravities, with metallicities close to the solar value. Currently, the library includes flux-calibrated and telluric-absorption-corrected spectra of 84 stars, with prospects for expansion to provide denser coverage of the parametric space. Throughout the H and K atmospheric windows, we identified spectral lines that are sensitive to T-eff or log g and defined corresponding spectral indices. We also provide their equivalent widths (EWs). For those indices, we derive empirical relations between the measured EWs and the stellar atmospheric parameters. Therefore, the derived empirical equations can be used to calculate the T-eff and log g of a star without requiring stellar atmospheric models.</P>