• Title/Summary/Keyword: binary program

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The BINSYN Program Package

  • Linnell, Albert P.
    • Journal of Astronomy and Space Sciences
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    • v.29 no.2
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    • pp.123-129
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    • 2012
  • The BINSYN program package, recently expanded to calculate synthetic spectra of cataclysmic variables, is being further extended to include synthetic photometry of ordinary binary stars in addition to binary stars with optically thick accretion disks. The package includes a capability for differentials correction optimization of eclipsing binary systems using synthetic photometry.

GENERAL PROGRAM FOR BINARY STARS RESEARCH AT MAYDANAK

  • ZAKIROV M. M.;HOJAEV A. S.;ARZUMANYANTS G. C.
    • Journal of The Korean Astronomical Society
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    • v.29 no.spc1
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    • pp.245-246
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    • 1996
  • The extensive close binary research program earring out at High Altitude Maydanak Observatory (Uzbekistan) by means of the UBVR photoelectric photometry on 1.0 m and 0.6 m Zeiss telescopes is described. It includes more than 240 close binary systems (CBS) in 89 different stellar aggregates. Lightcurves of CBS as well as their orbital elements derived by us are presented.

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Design and Implementation of a Dynamic Instrumentation Framework based on Light-weight Dynamic Binary Translation (경량 동적 코드 변환 기법을 이용한 동적 인스트루멘테이션 기법 설계 및 구현)

  • Kim, Jeehong;Lee, Dongwoo;Kim, Inhyeok;Eom, Young Ik
    • Journal of KIISE
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    • v.41 no.11
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    • pp.892-899
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    • 2014
  • Dynamic binary instrumentation is a code insertion technique for debugging a program without scattering its execution flow, while the program is running. Most dynamic instrumentations are implemented using dynamic binary translation techniques. Existing studies translated program codes dynamically by parsing the machine code stream to intermediate representation (IR) and then applying compilation techniques for IRs. However, they have high overhead during translation, which is a major cause of difficulty in applying the dynamic binary translation technique to the program which requires high responsiveness. In this paper, we introduce a light-weight dynamic binary instrumentation framework based on a novel dynamic binary translation technique which has low overhead while translating the program code. In order to reduce the translation overhead, our approach adopts a tabular-based address translation and exploits a translation bypassing scheme, which stores the translated address of a frequently called library function in advance. It then accesses the translated address and executes function codes without code translation when calling the function. Our experiment results demonstrated that the proposed approach outperforms the prior dynamic binary translation techniques from 2% up to 65%.

Static Control Flow Analysis of Binary Codes (이진 코드의 정적 제어 흐름 분석)

  • Kim, Ki-Tae;Kim, Je-Min;Yoo, Weon-Hee
    • The Journal of the Korea Contents Association
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    • v.10 no.5
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    • pp.70-79
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    • 2010
  • We perform static program analysis for the binary code. The reason you want to analyze at the level of binary code, installed on your local computer, run the executable file without source code. And the reason we want to perform static analysis, static program analysis is to understand what actions to perform on your local computer. In this paper, execution flow graph representing information such as the execution order among functions and the flow of control is generated. Using graph, User can find execution flow of binary file and calls of insecure functions at the same time, and the graph should facilitate the analysis of binary files. In addition, program to be run is ensured the safety by providing an automated way to search the flow of execution, and program to be downloaded and installed from outside is determined whether safe before running.

A CHARACTERISTIC PLANETARY FEATURE IN CAUSTIC-CROSSING HIGH-MAGNIFICATION MICROLENSING EVENTS

  • Kim, Do-Eon;Han, Cheong-Ho
    • Journal of The Korean Astronomical Society
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    • v.42 no.3
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    • pp.33-37
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    • 2009
  • We propose a diagnostic that can resolve the planet/binary degeneracy of central perturbations in caustic-crossing high-magnification microlensing events. The diagnostic is based on the difference in the morphology of perturbation inside the central caustics induced by a planet and a wide-separation binary companion. We find that the contours of excess exhibit a concentric circular pattern around the caustic center for the binary-lensing case, while the contours are elongated or off-centered for the planetary case. This difference results in the distinctive features of the individual lens populations in the residual of the trough region between the two peaks of the caustic crossings, where the shape of the residual is symmetric for binary lensing while it tends to be asymmetric for planetary lensing. We determine the ranges of the planetary parameters for which the proposed diagnostic can be used. The diagnostic is complementary to previously proposed diagnostics in the sense that it is applicable to caustic-crossing events with small finite-source effect.

Optimum Condition of Mobile Phase Composition for Purine Compounds by HCI Program (HCI프로그램을 이용한 퓨린 유도체의 이동상 조성의 최적화 조건)

  • Jin, Chun Hua;Lee, Ju Weon;Row, Kyung Ho
    • Applied Chemistry for Engineering
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    • v.17 no.3
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    • pp.317-320
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    • 2006
  • The optimum mobile phase condition for analysis of the six purine derivatives (caffeine, guanine, hypoxanthine, purine, theobromine, and theophylline) were determined by a HCI program. Reversed-phase HPLC system was used with the binary mobile phase, water and methanol. Three retention models (Snyder, Langmuir, and Binary polynomial) were considered to predict the retention factors. The elution profiles were calculated by the plate theory based on the binary polynomial retention model. From the final calculated results, the binary polynomial retention model showed the best agreements between the calculated and experimental data. In the isocratic mode, the optimum mobile phase composition of water/methanol is 93/7(v/v). However, we used step-gradient mode to decrease the run-time ($1^{st}$ mobile phase : water/methanol = 93/7 (v/v), gradient time : 5 min, $2^{nd}$ mobile phase : water/methanol = 75/25 (v/v)). The experimental and simulated profiles of above the two conditions show a good agreement.

The Development of Programmable Controller Using Binary-Decision Method (Binary-Decision 방식을 이용한 프로그래머블 콘트롤러의 개발에 관한 연구)

  • 전병실;이준환;엄경배
    • The Journal of Korean Institute of Communications and Information Sciences
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    • v.12 no.5
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    • pp.492-504
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    • 1987
  • The Binary Decision method can evaluate any switching function in the number of steps not exceeding the number of input variables. A Binary Decision Programmable Controller module is designed using this method so as to improve scan speed. A compiler system is also developed to relieve the memory problem which the Binary Decision method entails. A communication channel between MDS and BD-PC modules is also constructed to load the compiled BD-PC object program into the memory of BD machine.

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SMALL MASS RATIO CONTACT BINARY GR Vir AND HV Aqr (질량비가 작은 접촉쌍성 GR Vir과 HV Aqr)

  • 오규동;김천휘;강영운;김호일;이우백
    • Journal of Astronomy and Space Sciences
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    • v.21 no.2
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    • pp.83-92
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    • 2004
  • The absolute dimensions of low mass contact binary, GR Vir and HV Aqr were obtained using WD program from the published spectroscopic and photometric observational data. The evolutionary status of this type of system including GR Vir and HV Aqr has been considered. The primary stars of low mass contact binary system were located on the Terminal Age Main-sequence and secondary stars were located under the Zero Age Main-sequence in H-R diagram.

THE BIMA PROJECT: O-C DIAGRAMS OF ECLIPSING BINARY SYSTEMS

  • HAANS, G.K.;RAMADHAN, D.G.;AKHYAR, S.;AZALIAH, R.;SUHERLI, J.;IRAWATI, P.;SAROTSAKULCHAI, T.;ARIFIN, Z.M.;RICHICHI, A.;MALASAN, H.L.;SOONTHORNTHUM, B.
    • Publications of The Korean Astronomical Society
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    • v.30 no.2
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    • pp.205-209
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    • 2015
  • The Eclipsing Binaries Minima (BIMA) Monitoring Project is a CCD-based photometric observational program initiated by Bosscha Observatory - Lembang, Indonesia in June 2012. Since December 2012 the National Astronomical Research Institute of Thailand (NARIT) has joined the BIMA Project as the main partner. This project aims to build an open-database of eclipsing binary minima and to establish the orbital period of each system and its variations. The project is conducted on the basis of multisite monitoring observations of eclipsing binaries with magnitudes less than 19 mag. Differential photometry methods have been applied throughout the observations. Data reduction was performed using IRAF. The observations were carried out in BVRI bands using three different small telescopes situated in Indonesia, Thailand, and Chile. Computer programs have been developed for calculating the time of minima. To date, more than 140 eclipsing binaries have been observed. From them 71 minima have been determined. We present and discuss the O-C diagrams for some eclipsing binary systems.

Optimum Design of Diameters of Marine Propulsion Shafting by Binary-Coded Genetic Algorithm and Modal Analysis Method (이진코딩 유전알고리즘과 모드해석법을 이용한 선박 추진축계의 직경 최적설계)

  • Choi, Myung-Soo;Moon, Deok-Hong;Seol, Jong-Ku
    • Journal of Power System Engineering
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    • v.7 no.3
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    • pp.29-34
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    • 2003
  • Genetic algorithm is a optimization technique based on the mechanics of natural selection and natural genetics. Global optimum solution can be obtained efficiently by operations of reproduction, crossover and mutation in genetic algorithm. The authors developed a computer program which can optimize marine propulsion shafting by using binary-coded genetic algorithm and modal analysis method. In order to confirm the effectiveness of the developed computer program, we apply the program to a optimum design problem which is to obtain optimum diameters of intermediate shaft and propeller shaft in marine propulsion shafting. Objective function is to minimize total mass of shafts and constraints are that torsional vibration stresses of shafts in marine propulsion shafting can not exceed the permissible torsional vibration stresses of the ship classification society. The computational results by the program were compared with those of conventional design technique.

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