• Asian-Australasian Journal of Animal Sciences
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• 제25권5호
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• pp.621-628
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• 2012

The FAT-1 protein is an n-3 fatty acid desaturase, which can recognize a range of 18- and 20-carbon n-6 substrates and transform n-6 polyunsaturated fatty acids (PUFAs) into n-3 PUFAs while n-3 PUFAs have beneficial effect on human health. Fat1 gene is the coding sequence from Caenorhabditis elegans which might play an important role on lipometabolism. To reveal the function of fat1 gene in bovine fetal fibroblast cells and gain the best cell nuclear donor for transgenic bovines, the codon of fat1 sequence was optimized based on the codon usage frequency preference of bovine muscle protein, and directionally cloned into the eukaryotic expression vector pEF-GFP. After identifying by restrictive enzyme digests with AatII/XbaI and sequencing, the fusion plasmid pEF-GFP-fat1 was identified successfully. The pEF-GFP-fat1 vector was transfected into bovine fetal fibroblast cells mediated by Lipofectamine2000$^{TM}$. The positive bovine fetal fibroblast cells were selected by G418 and detected by RT-PCR. The results showed that a 1,234 bp transcription was amplified by reverse transcription PCR and the positive transgenic fat1 cell line was successfully established. Then the expression level of fat1 gene in positive cells was detected using quantitative PCR, and the catalysis efficiency was detected by gas chromatography. The results demonstrated that the catalysis efficiency of fat1 was significantly high, which can improve the total PUFAs rich in EPA, DHA and DPA. Construction and expression of pEF-GFP-fat1 vector should be helpful for further understanding the mechanism of regulation of fat1 in vitro. It could also be the first step in the production of fat1 transgenic cattle.

• Applied Biological Chemistry
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• 제38권2호
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• pp.111-117
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• 1995

CRP (cAMP receptor protein)은 cAMP와 결합하여 cAMP-CRP 복합체를 형성하여 전사조절의 조절인자로서 작용한다. crp 유전자에 변이를 도입하여 cAMP의 비존재 상태에서 cAMP-CRP와 비슷한 기능을 가진 crp 유전자가 도입된 대장균 MK2001 (crp, cya::km)을 숙주로 사용하여 cAMP 혹은 cGMP의 비존재하에서도 mal 유전자의 발현을 촉진시키는 유전자 sfs (sugar fermentation stimulation) 수 종을 클로닝 하였다. 본 실험에서는 이미 밝혀진 nlp (Ner like protein) 유전자와 같이, sfs의 새로운 유전자를 탐색하여, 그 중 sfs4의 2126 bp 전 염기배열을 결정하고, 잠정적인 sfs4의 promoter 영역에는 CRP 단백질과의 결합 DNA 공통 염기배열(5' AAT TGTGA ACACCA TCACC CGT 3')이 존재함을 확인했다. lacZ 융합 유전자를 작성하여 TP2010R1 MK2001의 균주에서 cAMP를 첨가할 경우 각각 2.3배, 1.8배의 ${\beta}-galactosidase$ 활성이 증가하는 것으로 보아 sfs4는 cAMP-CRP에 의해 발현 조절을 받는 것으로 나타났다.

• 한국작물학회지
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• 제45권5호
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• pp.305-309
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• 2000

Ultra-drying [＜5.0% seed moisture content (SMC)] storage technique is a cost-effective storage method for oily seeds. To decide proper ultra-drying condition for soybean seeds, drying rate was compared three silica gel to seed ratios, two seed sizes with varietal difference, two kinds of container, and three seed amounts per container under :t 23$\pm$1$^{\circ}C$. When the relative humidity (RH) was reduced at the rate of less than 0.1 % a day, silica gel was replaced with dry one by 47 days. Higher silica gel to seed ratios (3:1 and 2:1) dried faster than lower ratio (1:1) until 28 days, but not after 43 days of drying. Also, large seeded variety was dried faster than small seeded variety. Kinds of container and seed amounts per container didn't show differences in drying of soybean seeds. After completion of ultra-drying, percentage germination by standard germination test (SGT) was not different among silica gel to seed ratios, kinds of container, and seed amounts per container, except among seed sizes (varieties). Before SGT, soybean seeds were premoistened using saturated ${CaCl}_2$ for 48 hours and ${NH}_4$Cl for 24 hours in desiccators. To compare germinability between ordinary-dried seeds and ultra-dried seeds, the seeds of seven soybean varieties, which were varying in size from 8.1 to 34.9 g per 100 seeds, were dried using same amount of silica gel under 23$\pm$1$^{\circ}C$. After completion of 76 days of drying, SMCs were reduced to 3.13-3.45% from 7.86-8.82%. SMC after completion of drying was not correlated with 100-seed weight (r=0.556). Before germination tests, soybean seeds were premoistened using saturated salt solutions. Percentage germination was higher with ultra-dried seeds than ordinary-dried seeds in SGT and higher with ordinary-dried seeds than ultra-dried seeds in AAT at the beginning of storage and after 6 months storage, but general trend of percentage germination was not observed among varieties classified by 100-seed weight. From these results, we concluded that further studies are needed to improve ultra-drying storage method for soybean seeds.

• 천문학회지
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• 제29권spc1호
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• pp.63-64
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• 1996

The nature of distant faint blue field galaxies remains a mystery, despite the fact that much attention has been devoted to this subject in the last decade. Galaxy counts, particularly those in the optical and near ultraviolet bandpasses, have been demonstrated to be well in excess of those expected in the 'no-evolution' scenario. This has usually been taken to imply that galaxies were brighter in the past, presumably due to a higher rate of star formation. More recently, redshift surveys of galaxies as faint as B$\~$24 have shown that the mean redshift of faint blue galaxies is lower than that predicted by standard evolutionary models (de-signed to fit the galaxy counts). The galaxy number count data and redshift data suggest that evolutionary effects are most prominent at the faint end of the galaxy luminosity function. While these data constrain the form of evolution of the overall luminosity function, they do not constrain evolution in individual galaxies. We are carrying out a series of observations as part of a long-term program aimed at a better understanding of the nature and amount of luminosity evolution in individual galaxies. Our study uses the luminosity-linewidth relation (Tully-Fisher relation) for disk galaxies as a tool to study luminosity evolution. Several studies of a related nature are being carried out by other groups. A specific experiment to test a 'no-evolution' hypothesis is presented here. We have used the AUTOFIB multifibre spectro-graph on the 4-metre Anglo-Australian Telescope (AAT) and the Rutgers Fabry-Perot imager on the Cerro Tolalo lnteramerican Observatory (CTIO) 4-metre tele-scope to measure the internal kinematics of a representative sample of faint blue field galaxies in the red-shift range z = 0.15-0.4. The emission line profiles of [OII] and [OIII] in a typical sample galaxy are significantly broader than the instrumental resolution (100-120 km $s^{-l}$), and it is possible to make a reliable de-termination of the linewidth. Detailed and realistic simulations based on the properties of nearby, low-luminosity spirals are used to convert the measured linewidth into an estimate of the characteristic rotation speed, making statistical corrections for the effects of inclination, non-uniform distribution of ionized gas, rotation curve shape, finite fibre aperture, etc.. The (corrected) mean characteristic rotation speed for our distant galaxy sample is compared to the mean rotation speed of local galaxies of comparable blue luminosity and colour. The typical galaxy in our distant sample has a B-band luminosity of about 0.25 L$\ast$ and a colour that corresponds to the Sb-Sd/Im range of Hub-ble types. Details of the AUTOFIB fibre spectroscopic study are described by Rix et al. (1996). Follow-up deep near infrared imaging with the 10-metre Keck tele-scope+ NIRC combination and high angular resolution imaging with the Hubble Space Telescope's WFPC2 are being used to determine the structural and orientation parameters of galaxies on an individual basis. This information is being combined with the spatially resolved CTIO Fabry-Perot data to study the internal kinematics of distant galaxies (Ing et al. 1996). The two main questions addressed by these (preliminary studies) are: 1. Do galaxies of a given luminosity and colour have the same characteristic rotation speed in the distant and local Universe? The distant galaxies in our AUTOFIB sample have a mean characteristic rotation speed of $\~$70 km $s^{-l}$ after correction for measurement bias (Fig. 1); this is inconsistent with the characteristic rotation speed of local galaxies of comparable photometric proper-ties (105 km $s^{-l}$) at the > $99\%$ significance level (Fig. 2). A straightforward explanation for this discrepancy is that faint blue galaxies were about 1-1.5 mag brighter (in the B band) at z $\~$ 0.25 than their present-day counterparts. 2. What is the nature of the internal kinematics of faint field galaxies? The linewidths of these faint galaxies appear to be dominated by the global disk rotation. The larger galaxies in our sample are about 2"-.5" in diameter so one can get direct insight into the nature of their internal velocity field from the $\~$ I" seeing CTIO Fabry-Perot data. A montage of Fabry-Perot data is shown in Fig. 3. The linewidths are too large (by. $5\sigma$) to be caused by turbulence in giant HII regions.

• 지구물리와물리탐사
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• 제20권4호
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• pp.241-267
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• 2017

1945년에 해방된 후부터, 우리나라에서는 지질과학 분야와 자원공학 분야의 전문가들이 서로 협조, 경쟁하면서 두 학문 분야를 발전시켜 왔다. 서로 공유하는 부분이 많은 지구물리 분야와 물리탐사 분야는 범위가 더 넓은 위 두 학문 분야 안에서 각각 자신의 분야를 더욱 깊이 발전시켜 왔다. 1990년대 후반부터 지구물리 분야와 물리탐사 분야의 전문가들은 자신의 분야를 다루는 독립적인 학회가 필요함을 느끼고 학회의 설립을 위한 논의를 거듭하였다. 1997년에 이르러서는 두 분야가 각각 학회를 설립할 것이 아니라, 두 분야를 아우르는 하나의 학회를 설립할 것을 논의한 바 있으나, 결국 1998년에 들어와서는 몇 가지 현실적인 문제로 인해 대한지구물리학회와 한국지구물리탐사학회(이후 한국물리탐사학회로 바꾸었음)를 각각 따로 설립하였다. 양 학회의 설립 후부터 2000년대 중반까지 7 ~ 8 년이 지나는 동안, 양 학회가 다루는 분야들 중 서로 겹치는 분야가 많은 점, 많은 회원이 양 학회 모두의 회원인 점 등의 이유로, 양 학회의 많은 회원들이 양 학회가 통합하여 하나의 학회가 될 것을 바란다는 뜻을 나타내었다. 양 학회의 회장단도 이 의견을 받아들여, 2005년부터 본격적으로 통합을 논의하였고, 결국 2007년에 양 학회가 통합하여, 한국지구물리 물리탐사학회를 설립하였다. 2007년에 통합, 설립한 한국지구물리 물리탐사학회는 그 후부터 계속하여 우리나라의 지질과학 분야, 자원공학 분야의 다른 학회들과 활발히 서로 협조, 경쟁하면서 우리나라의 발전에 크게 기여할 뿐만 아니라, 아시아, 오세아니아, 아메리카 대륙 등 태평양을 둘러싸는 지역들의 외국 학회들과도 긴밀히 협조하면서 세계의 지구물리, 물리탐사 분야의 발전에도 크게 기여하고 있다.