• 천문학회보
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• 제40권1호
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• pp.46.2-46.2
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• 2015

Modern methods in determining the value of the Hubble constant are divided into two main ways: the classical distance ladder method and the inverse distance ladder method. The classical distance ladder method is based on Cepheid calibrated Type Ia supernovae (SNe Ia), which are known as powerful distance indicator. The inverse distance ladder method uses cosmic microwave background radiation, which emitted from the high-z universe, and the cosmological model. Recent estimations of the Hubble constant based on these two methods show a $2{\sim}3{\sigma}$ difference, which called the "Hubble tension". It is currently an issue in the modern cosmology. We have been working on the luminosity calibration of SNe Ia based on the Tip of the Red Giant Branch (TRGB), which is a precise population I distance indicator. We present the TRGB distance estimates of 5 SNe Ia host galaxies with the archival Hubble Space Telescope image data. We derive the mean absolute maximum magnitude of 5 SNe Ia and the value of the Hubble constant. Cosmological implications of our estimate will be discussed.

• 한국수학교육학회지시리즈A:수학교육
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• 제56권4호
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• pp.387-405
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• 2017

The purpose of this study is to investigate the change of students 'perception and expression about the motion of object following distance function $={x \atop 3}$ and distance function $y=\frac{x^3}{3}+3$ according to the necessity of research on students' perception and expression about integral constant. In this paper, we present the recognition and the expression of the difference of the constant in the relationship between the distance function and the speed function of the students, while examining the process of constructing the speed function and the inverse process of the distance function. This provides implications for the relationship between the derivative and the indefinite integral corresponding to the inverse process. In particular, in a teaching experiment, a constructive activity was performed to analyze the motion of two distance functions, where the student had a difference of the constant term. At this time, the students used the expression 'starting point' for the constants in the distance function, and the motion was interpreted by using the meaning. This can be seen as a unique 'students' mathematics' in the process of analyzing the motion of objects. These scenes, in introducing the notion of the relation between differential and indefinite integral, it is beyond the comprehension of the integral constant as a computational procedure, so that the learner can understand the meaning of the integral constant in relation to the motion of the object. It is expected that it will be a meaningful basic research on the relationship between differential and integral.

• 대한수학회보
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• 제54권2호
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• pp.507-519
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• 2017

We present an upper bound on the Cheeger constant of a distance-regular graph. Recently, the authors found an upper bound on the Cheeger constant of distance-regular graph under a certain restriction in their previous work. Our new bound in the current paper is much better than the previous bound, and it is a general bound with no restriction. We point out that our bound is explicitly computable by using the valencies and the intersection matrix of a distance-regular graph. As a major tool, we use the discrete Green's function, which is defined as the inverse of ${\beta}$-Laplacian for some positive real number ${\beta}$. We present some examples of distance-regular graphs, where we compute our upper bound on their Cheeger constants.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2006년도 공동학술대회 논문집
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• pp.221-224
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• 2006

소규모 공동 탐지를 위한 시험지역에서 시추공 편차를 고려한 탄성파 토모그래피를 수행하였다. 시추공 편차보정방법은 일정 거리를 더하는 보정과 일정 각을 시추공간 거리에 고려하는 보정을 적용하였다. 시추공 편차를 고려한 토모그래피는 영상의 왜곡을 줄일 수 있어 공동을 명확히 영상화할 수 있었으며, 일정 각을 거리에 고려하는 보정방법이 공동탐지에 가장 효과적이지만 일정 거리 보정도 만족할 만한 결과를 얻을 수 있음을 알 수 있었다.

• 한국산학기술학회논문지
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• 제10권6호
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• pp.1201-1206
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• 2009

음상의 거리정위에 있어서 중요한 물리적 요인으로는 알려진 음압레벨, 반사음, 양 귀간 차, 음원의 종류, 머리전달함수(HRTF) 등의 여러 요인들이 중요한 판단 자료로 이용되어진다고 알려져 있다. 본 논문에서는 거리판단에 사용되어지는 물리적 요인 중 음압레벨의 크기가 거리정위에 미치는 영향을 알아보기 위해 반사음이 존재하지 않은 무향실에서 음원의 출력 음압레벨을 일정한 경우와 귀 입력 음압레벨을 일정하게 한 경우에 대하여 청취실험을 통해 거리판단에 있어서 음압레벨의 영향에 대하여 고찰했다. 그 결과. 음원출력 음압레벨을 일정하게 한 경우와 귀 입력 음압레벨을 일정하게 한 청취실험에 있어서 제시한 음원거리보다 지각한 음상거리를 가깝게 정위하는 경향이 있다는 것이 관찰되었다. 또, 귀 입력 음압레벨이 일정한 경우에는 약 2m 정도까지의 거리에서는 실제 제시한 음원거리의 증가에 따라 지각한 음상의 거리가 음원거리에 대응하여 증가하지만, 그 이상의 거리에서는 음원거리의 증가에 따라 지각한 음상거리가 증가가 거의 없음을 알 수 있었다. 반면 음원출력 음압레벨이 일정한 경우에는 지각한 음상거리가 귀 입력 음압레벨이 일정한 경우보다 보다 더 먼 3m 정도의 거리까지 증가하고 있음을 알 수 있었다. 이와 같은 청취실험 결과로부터 반사음이 존재하지 않은 조건에서의 음상의 거리정위에는 음압레벨이 거리판단의 중요한 요소로 작용하고 있음이 확인되었다.

• 천문학논총
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• 제30권2호
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• pp.371-374
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• 2015

Classical Cepheids (hereafter Cepheids) belong to a class of important variable stars that can be used to determine distances to nearby galaxies via the famous period-luminosity (PL) relations, i.e. the Leavitt Law. In turn, these distances can then be used to calibrate a host of secondary distance indicators located well within the Hubble flow, and ultimately determine the Hubble constant in a manner independent of the Cosmic Microwave Background (CMB) measurements. Some recent progress in determining the Hubble constant to within ~ 3% level via the Cepheid-based distance scale ladder (the SH0ES and the Carnegie Hubble Program) were first summarized in this Proceeding, followed by a brief discussion on the prospect of using ultra-long period Cepheids (ULPC) in future distance scale work. ULPC are those Cepheids with periods longer than 80 days, which seem to follow a different PL relation than their shorter period Cepheids. It has been suggested that ULPC can be used to determine the Hubble constant in "one-step". However, based on the two ULPCs found in M31, it was found that the large dispersion in derived distance moduli leads to a less accurate distance modulus to M31 compared to the classical Cepheids. This finding might raise an alert regarding the use of ULPCs in future distance scale work.

• 전자공학회논문지B
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• 제32B권5호
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• pp.693-701
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• 1995

In most application programs, loops usually comprise most of the computation in a program and are the most important source of parallelism. When loops are executed on multiprocessors, the cross iteration data dependences need to be enforced by synchronization between processors. Existing synchronization schemes have been studied mainly on the loop with constant dependence distance. When these schemes are applied to the loop with variable dependence distance, there exists lots of overhead by the use of unnecessary synchronization variables and execution of unuseful synchronization instructions. Even though there exist various variable synchronization schemes, they have a lot of run-time overhead to compute synchronization information. In this paper, we present a new synchronization scheme, Synch-Free/Synch-Hold for managing synchronization efficiently on the loop with constant and variable dependence distance.

• 한국안전학회지
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• 제25권6호
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• pp.40-46
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• 2010

To protect press operator from the after-reach hazard, current Ministry of Labor Notification(MOLN) requires the use of a formula for calculating the safe distance away from the point of operation for locating press protective devices, Two Hand Control Devices(THCD) and Active Opto-Electronic Protective Devices(AOPD), on a power press. This formula is based on a same hand speed constant of 160cm/s. While EN standards use different hand speed constant for THCD and AOPD respectively. The objective of this study is to compare two guidelines on the hand speed constant published by MOLN and EN 692, also to propose a proper hand speed constant and validate it experimentally. As a experimental result, it could be known that hand speed constant of Ministry of Labor Notification should be improved as that of EN standards.

• 융합신호처리학회논문지
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• 제3권4호
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• pp.57-61
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• 2002

We design Collision Avoidance System using model vehicle. The purpose of this system(Collision Avoidance System) is to maintain continuously constant distance between a forward running vehicle and a following automatic guided vehicle(AGV). For this system, we design modeling of vehicle and observe this through simulation. By sing super sonic sensors to measure the distance between vehicles and controller using 80c196kc for changing velocity of motor, we design Collision Avoidance System as maintaining continuously constant distance between vehicles.

• 인터넷정보학회논문지
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• 제10권6호
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• pp.19-26
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• 2009

이 논문에서는 오차 확률 밀도와 델타 함수 사이의 유클리드 거리를 최소화하는 기준을 소개하고 이 기준에 근거한 새로운 CMA 형태의 블라인드 등화 알고리듬을 제안하고 있다. 제안한 기준에 나타나는 오차 항 대신에 constant modulus error를 대치하여 블라인드 알고리듬을 완성하였고 이 알고리듬은 블라인드 등화 환경에서 탁월한 수렴성능과 정상상태의 자승평균오차 성능 특성을 보였으며, 오차 신호 값이 0 값에 보다 집중된 밀도함수 형태를 나타냈다. 시뮬레이션 결과로부터, 이 제안된 방식은 멀티 포인트 통신에서 블라인드 등화를 위한 신뢰성 있는 알고리듬으로 사용될 수 있음을 보이고 있다.