Economic Cooperation Organization (ECO), based on regional and multicultural cooperation, has focused on the improvement of living standards, collective as well as individual prosperity of people and economic development of member’s states. Since February 1992 ECO has been expanded to ten as the result of collapse of the Soviet Union. Of course, gas and oil are very important factors in this re...

economic cooperation organization (eco) is one of the institutions that have been established to help identify and resolve the problems faced by the region. in order to celebrate the eco day, a meeting was held at the center for graduate international studies, faculty of law and political science, university of tehran as attended by yahya maroufi, eco secretary-general, mr. taherian, eco under-...

Ryotaro Inoue, 2, ∗ Kenta Muranaga, Hideaki Takayanagi, 3 Eiichi Hanamura, Masafumi Jo, Tatsushi Akazaki, 2 and Ikuo Suemune 2 Dept. of Applied Physics, Tokyo Univ. of Science, Tokyo 162-8601, Japan. CREST, Japan Science and Technology Agency, Kawaguchi 332-0012, Japan. MANA, National Inst. for Materials Science, Tsukuba 305-0044, Japan. Japan Science and Technology Agency, Kawaguchi 332-0012, ...

an investigation was conducted to study the larvicidal activity of teknar (san-402-i-bacillus thuringiensis, serotype h-14, sandoz, 600 itu/mg) on mosquitolarvaein kazeroun, fars province, southern iran. five experimental plots were selected randomly in a rice field and three concentrations of teknar: .0003, .0006 and .0012 cc/1 was used. maximum larval mortality usually occurred during the fir...

Engineering Change Order or ECO phase is always challenging for any family of chip design. High Performance Microprocessors are largest and most complex overall design within Semiconductor Industry as a whole. To add further, there are additional design and methodology challenge related to bleeding edge of process nodes. Hence, current and future microprocessor design requires a set of well pla...

Yuma Kinoshita, 2, ∗ Ryo Namiki, 2 Takashi Yamamoto, 2 Masato Koashi, 2, 3 and Nobuyuki Imoto 2, 3 Division of Materials Physics, Department of Materials Engineering Science, Graduate school of Engineering Science, Osaka University, 1-3 Machikaneyama, Toyonaka, Osaka 560-8531, Japan CREST Reserch Team for Photonic Quantum Information, 4-1-8 Honmachi, Kawaguchi, Saitama 331-0012, Japan SORST Res...

Abstract We previously reported a putative detection of radio galaxy at $z=10.15$ , selected from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. The redshift this source, GLEAM J0917–0012, was based on three weakly detected molecular emission lines observed with Atacama Large Millimetre (ALMA). In order to confirm result, we conducted deep spectroscopic follow-...