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Journal Articles

Production and synthesis of a novel $$^{191}$$Pt-labeled platinum complex and evaluation of its biodistribution in healthy mice

Omokawa, Marina*; Kimura, Hiroyuki*; Hatsukawa, Yuichi*; Kawashima, Hidekazu*; Tsukada, Kazuaki; Yagi, Yusuke*; Naito, Yuki*; Yasui, Hiroyuki*

Bioorganic & Medicinal Chemistry, 97, p.117557_1 - 117557_6, 2024/01

 Times Cited Count:0 Percentile:0.01(Biochemistry & Molecular Biology)

Journal Articles

Preparation and evaluation of $$^{186/188}$$Re-labeled antibody (A7) for radioimmunotherapy with rhenium(I) tricarbonyl core as a chelate site

Ogawa, Kazuma*; Kawashima, Hidekazu*; Kinuya, Seigo*; Shiba, Kazuhiro*; Onoguchi, Masahisa*; Kimura, Hiroyuki*; Hashimoto, Kazuyuki; Odani, Akira*; Saji, Hideo*

Annals of Nuclear Medicine, 23(10), p.843 - 848, 2009/12

 Times Cited Count:9 Percentile:31.42(Radiology, Nuclear Medicine & Medical Imaging)

Rhenium is one of the most valuable elements for internal radiotherapy because $$^{186/188}$$Re have favorable physical characteristics. However, there are problems when proteins such as antibodies are used as carriers of $$^{186/188}$$Re. Labeling methods require the complicated processes. Therefore, we planned the preparation by a simple method and evaluation of a stable $$^{186/188}$$Re-labeled antibody. For this purpose, we selected $$^{186/188}$$Re(I) tricarbonyl complex as a chelating site. A7 was used as a model protein. $$^{186/188}$$Re-labeled A7 was prepared by directly reacting a $$^{186/188}$$Re(I) tricarbonyl precursor with A7. $$^{186/188}$$Re-(CO)$$_{3}$$-A7 were prepared with radiochemical yields of 23-28%. After purification, $$^{186/188}$$Re-(CO)$$_{3}$$-A7 showed a radiochemical purity of over 95%. In biodistribution experiments, $$^{186/188}$$Re-labeled A7 showed high uptakes in the tumor.

Journal Articles

Neutrino-nucleus reaction cross sections for light element synthesis in supernova explosions

Yoshida, Takashi*; Suzuki, Toshio*; Chiba, Satoshi; Kajino, Toshitaka*; Yokomakura, Hidekazu*; Kimura, Keiichi*; Takamura, Akira*; Hartmann, D.*

Astrophysical Journal, 686(1), p.448 - 466, 2008/10

The neutrino-nucleus reaction cross sections of $$^4$$He and $$^{12}$$C are evaluated using new shell model Hamiltonians. Branching ratios of various decay channels are calculated to evaluate the yields of Li, Be, and B produced through the $$nu$$-process in supernova explosions. The new cross sections enhance the yields of $$^{7}$$Li and $$^{11}$$B produced during the supernova explosion of a 16.2 M$$_odot$$ star model compared to our previous study by factors of 1.3 and 1.2, respectively. On the other hand, the yield of $$^{10}$$B decreases by a factor of three. The yields of $$^{6}$$Li, $$^{9}$$Be, and the radioactive nucleus $$^{10}$$Be are found at a level of 10 to 11 M$$_odot$$. The temperature of $$nu mu, tau$$- and $$bar{nu} mu, tau$$-neutrinos inferred from the supernova contribution of $$^{11}$$B in Galactic chemical evolution models is constrained to be in the range 4.5 MeV to 6.4 MeV. The increase in the $$^{7}$$Li and $$^{11}$$B yields due to neutrino oscillations is demonstrated with the new cross sections.

Journal Articles

Neutrino-nucleus reaction cross sections for light element synthesis in supernova explosions

Yoshida, Takashi*; Suzuki, Toshio*; Chiba, Satoshi; Kajino, Toshitaka*; Yokomakura, Hidekazu*; Kimura, Keiichi*; Takamura, Akira*; Hartmann, D. H.*

Astrophysical Journal, 686(1), p.448 - 466, 2008/10

 Times Cited Count:92 Percentile:89.6(Astronomy & Astrophysics)

The neutrino-nucleus reaction cross sections of $$^4$$He and $$^{12}$$C are evaluated using new shell model Hamiltonians. The new cross sections enhance the yields of $$^7$$Li and $$^{11}$$B produced during the supernova explosion of a 16.2 $$M_odot$$ star model compared to the case using the conventional cross sections by about 10%. On the other hand, the yield of $$^{10}$$B decreases by a factor of two. The yields of $$^6$$Li, $$^9$$Be, and the radioactive nucleus $$^{10}$$Be are found at a level of $$sim 10^{-11} M_odot$$. The temperature of $$nu_{mu,tau}$$- and $$bar{nu}_{mu,tau}$$-neutrinos inferred from the supernova contribution of $$^{11}$$B in Galactic chemical evolution models is constrained to be in the range 4.3 MeV to 6.5 MeV. The increase in the $$^7$$Li and $$^{11}$$B yields due to neutrino oscillations is demonstrated with the new cross sections.

Journal Articles

Structure study of thin films by employing anomalous dispersion of synchrotron X-rays

Mizuki, Junichiro; Kimura, Hidekazu*

Oyo Butsuri, 68(11), p.1271 - 1274, 1999/11

no abstracts in English

Journal Articles

The XAFS beamline BL01B1 at SPring-8

Uruga, Tomoya*; Tanida, Hajime*; Yoneda, Yasuhiro; Takeshita, Kunikazu*; Emura, Shuichi*; Takahashi, Masao*; Harada, Makoto*; Nishihata, Yasuo; Kubozono, Yoshihiro*; Tanaka, Tsunehiro*; et al.

Journal of Synchrotron Radiation, 6(Part3), p.143 - 145, 1999/05

An x-ray absorption fine-structure (XAFS) spectroscopy beamline, BL01B1, was installed at a bending magnet source at SPring-8 and has been open to users since October 1997. It was designed for XAFS experiments covering a wide energy range. Position tables and automatical control programs were established to adjust the x-ray optics and achieve the designed performance of the beamline under each experimental condition. This has enabled conventional XAFS measurements to be made with a good data quality from 4.5 to 110 keV.

Journal Articles

Eu ${it K}$-XAFS of europium dioxymonocyanamide with the convension He$$^+$$ ion yield method

Takahashi, Masao*; Harada, Makoto*; Watanabe, Iwao*; Uruga, Tomoya*; Tanida, Hajime*; Yoneda, Yasuhiro; Emura, Shuichi*; Tanaka, Tsunehiro*; Kimura, Hidekazu*; Kubozono, Yoshihiro*; et al.

Journal of Synchrotron Radiation, 6(3), p.222 - 224, 1999/05

 Times Cited Count:11 Percentile:61.16(Instruments & Instrumentation)

no abstracts in English

Oral presentation

Preparation of $$^{188}$$Re-labeled antibody (A7) by a simple method using rhenium(I) tricarbonyl complex

Ogawa, Kazuma*; Kawashima, Hidekazu*; Kinuya, Seigo*; Yoshimoto, Mitsuyoshi*; Shiba, Kazuhiro*; Kimura, Hiroyuki*; Hashimoto, Kazuyuki; Mori, Hirofumi*; Saji, Hideo*

no journal, , 

$$^{188}$$Re is one of the most useful radionuclides for internal radiotherapy. However, there is a problem when protein such as antibody is used as a carrier of $$^{188}$$Re. The labeling method using bifunctional chelating agents require the conjugation of $$^{188}$$Re-complex to protein after radiolabeling with the bifunctional chelating agent. Then, we planned the preparation of a stable $$^{188}$$Re-labeled protein by a simple method. A7 monoclonal antibody was labeled by reacting $$^{188}$$Re(I) tricarbonyl precursor with A7 directly. $$^{188}$$Re labeled A7 was prepared with radiochemical yield of 23%. After purification, $$^{188}$$Re labeled A7 showed radiochemical purity over 98%. After 24 hours of incubation, about 93% of $$^{188}$$Re-A7 remained intact, which indicates $$^{188}$$Re-A7 is stable in vitro. In biodistribution experiment, 11.2% of the injected dose/g of $$^{188}$$Re-A7 accumulated in the tumor at 24 hours postinjection, and tumor to blood ratio was over 1.0 at the same time.

Oral presentation

Synthesis and evaluation of $$^{186}$$Re-labeled biotin as a labeling agent for antibodies

Hirasawa, Makoto*; Kawashima, Hidekazu*; Ogawa, Kazuma*; Kimura, Hiroyuki*; Ono, Masahiro*; Hashimoto, Kazuyuki; Saji, Hideo*

no journal, , 

no abstracts in English

Oral presentation

Pretargeted radioimmunotherapy of tumor using a novel radiorhenium-labeled biotin derivative and streptavidin conjugated anti-cytokeratin 19 monoclonal antibody

Kawashima, Hidekazu*; Hirasawa, Makoto*; Kimura, Hiroyuki*; Ono, Masahiro*; Hashimoto, Kazuyuki; Saji, Hideo*

no journal, , 

no abstracts in English

10 (Records 1-10 displayed on this page)
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