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| 1 | Id related genes encoding helix-loop-helix proteins are required for G1 progression and are repressed in senescent human fibroblasts显示文摘 | Hara E Yamaguchi T Nojima H Ide T Campisi J Okayama H | 1994 | J Biol Chem1994，269，： | 1 |
| 2 | Estimation of global and regional cardiac tunc tion using 64 slice computed tomography: a comparison study with echocardiography, gated-SPECT and cardiovascular magnetic resonance显示文摘 | Wu Y W Tadamura E Yamamuro M Kanao S Okayama S Ozasa N | 2008 | Int J CardioI2008，128，： | 1 |
| 3 | A simulation for precision airflow control using multi-fan in a plant factory 显示文摘 | OKAYAMA T OKAMURA K PARK J E USHADA M MURASE H | 2008 | Environ Control Bioi2008，46，3： | 1 |
| 4 | Isolation and characterization of proteoglycans synthesized by cultured mesangial sells 显示文摘 | Yaoita E Oguri K Okayama E | 1990 | J Boil Chem1990，265，： | 1 |
| 5 | Rural doctors satisfaction in Japan:a nationwide survey显示文摘 | Matsumoto M Okayama M Kajii E | 2004 | Aust J Rural Health2004，12，2： | 1 |
| 6 | Serotype- specific polysaccharide of Streptococcus mutans contributes to infectivity in cndocarditis显示文摘 | Nagata E Okayama H Ito HO | 2006 | Oral Microbiol Immunol2006，21，6： | 1 |
| 7 | HCV core antigen as an al-ternative to NAT to detect HCV viremia显示文摘 | Raker CAtTabor E Okayama A | 2004 | Transfusion2004，44，2： | 1 |
| 8 | HIDES: a High Dispersion Echelle Spectrograph显示文摘This paper describes a High Dispersion Echelle Spectrograph (HIDES) at the coudé focus of the 188cm reflector of Okayama Astrophysical Observatory, NAOJ. HIDES uses an echelle grating (31 6gr/mm, R=2 14) as the main disperser. Two reflection gratings with the ruling densities of 400gr/mm and 250gr/mm are used for the post cross disperser. The camera consists of five spherical lenses, has the aperture of 200mm diameter, and is designed to achieve spot sizes smaller than 15μm within the image circle of 60mm diameter at wavelengths from 360nm through 900nm without refocusing. A mosaic of two 2K × 4K CCDs with 13 5μm pixel from EEV is employed. The large area of the detectors enables to cover the free spectral range of any order without rotating the echelle. The wavelength coverage in a single exposure is about 200nm with the red cross disperser and mosaiced CCDs. Typical spectral resolution will be 68,000 with 0 76″ slit width. At this resolution one hour exposure will give a detection of a point source at 12 th magnitude at 550nm with the S/N of about 10. | Hideyuki Izumiura Okayama Astrophysical Observatory, National Astronomical Observatory of Japan Honjo 3037 5, Kamogata, Asakuchi, Okayama 719 0232, Japan E mail: izumiura @ oao. nao. ac. jp | 1999 | 天文研究与技术1999，，S1： | 0 |
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