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11篇 您的检索式:作者名="Tarusawa"
    题名 作者 年代 出处 被引量
1Unipla- nar MMIC hybrids-a proposed new MMIC structure 显示文摘HIROTA T TARUSAWA Y OGAWA H 1987IEEE Trans Microwave Theory and Techniques1987,35,6:1
2Uniplanar MMIC hybrids-a proposed new MMIC structure显示文摘HIROTA T TARUSAWA Y OGAWA H 0,,6:1
3CTCF is required for neural development and stochastic expression of clustered Pcdh genes in neurons显示文摘Hirayama T Tarusawa E Yoshimura Y 2012Cell reports2012,2,2:1
4Abnormality of c-kit oncoprotein in certain patients with chronic myelogenous leukemia--potential clinical significance 显示文摘Inokuchi K Yamaguchi H Tarusawa M 2002Leukemia2002,16,2:1
5Quantitative assessment of minimal residual disease in childhood lymphoid malignancies using an allele-specific oligonucleotide real-time quantitative polymerase chain reaction显示文摘TARUSAWA M YASHIMA A ENDO M 2002Int J Hematol2002,75,:1
6Quantitative assessment of minimal residual disease in childhood lymphoid malignancies using an allele-specific oligonucleotide real-time quantitative polymerase chain reaction显示文摘Mitsu Tarusawa Akiko Yashima Mikiya Endo Chihaya Maesawa 2002International Journal of Hematology2002,,2:1
7Large scale in vitro experiment system for 2 GHz exposure显示文摘Takahiro L Ebara H Tarusawa Y 0,,08:1
8Large scale in vitro experiment system for 2 GHz exposure显示文摘Iyama T Ebara H Tarusawa Y 0,,08:1
9Uniplanar MMIC hy- brids : a proposed new MMIC structure 显示文摘Hirota T Tarusawa Y Ogawa H 1987IEEE Trans Microwave Theory Techn1987,35,6:1
10The evaluation of the profile of mood states (POMS) in cancer patients treated by tamagawa hot spring bathing显示文摘Yanagisawa T Noguchi J Tarusawa T 0,,02:1
11Kiso Multi-Fiber Spectroscope Project显示文摘A multi Fiber Spectroscope at Kiso Observatory is under consideration as our next instrument. In this paper we report an overview of our instrument and a scientific target of survey project. We are going to attach multi fiber system at the prime focus of Kiso 150m Schmidt telescope. This telescope has some advantage for our project. First, the effciency in survey for the objects, which number density is 0 1 to 10/degree 2, is higher than other multi object system due to the wide field of view (6 °×6 °). Second, an optics of telescope is well matched to fiber numerical aperture (NA) at an input end of fiber. Moreover, taking a focal ratio degradation (FRD) and scrambling property into account, since the light from object does not move at the entrance slit of spectroscope, we could get spectroscopic data stably with this system. We select a fiber with 100μm core which corresponding to 6 arcsec on focal plane, that is matched with a typical seeing (3 arcsec) at Kiso Observatory and set 150 fibers to one field. For efficient observations, it is necessary to arrange fibers accurately within an accuracy of ±25μm on the curved focal plane during a typical exposure time (1 hour). Therefore we examine a particular positioner specialized for curved surface. We also develop a spectroscope that is suited for a fast focal ratio and proceed with making its design. One of our main key projects with this system is a non biased survey for solar neighbour stars. We are now establishing a new metallicity determination method that easily and reliably measures a metallicity from low dispersion spectra. (see Itoh it et al. 1998) As we consider our main target as Galactic objects and low resolution (R is around 1000), we could observe a star with 17 mag at V band (1 hour exposure).Yasushi Yadoumaru, Nobunari Itoh, Yoshikazu Nakada, Ken’ichi Tarusawa, Takao Soyano Kiso Observatory, Institute of Astronomy, The University of Tokyo and Hiroyuki Mito The Graduate University for Advanced Studies 1999天文研究与技术1999,,S1:0
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