• 천문학회보
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• 제40권1호
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• pp.54.2-54.2
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• 2015

Phase referencing is an important tool to study weak radio sources, especially in mm-VLBI (Very Long Baseline Interferometry) which are usually too faint to be observed using conventional VLBI. VLBI astrometry is a unique method to measure the position and to identify radio emitting regions of a radio source with unprecedented angular resolution. In order to evaluate the phase referencing and astrometric capabilities of KVN and KaVA, several observations have been conducted and analyzed. I will present the observational results and discuss constraints and requirements for high precision VLBI astrometry.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2004년도 Asia Display / IMID 04
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• pp.568-570
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• 2004

A shielding effectiveness of mesh screen filter of plasma display panel (PDP) has been calculated in this paper. Since the screen filter is located near the radiation source, the near field wave impedance of the radiation source, i.e., the PDP electrodes, has been considered to calculate the shielding effectiveness. The near field shielding effectiveness of screen filter at 30${\sim}$300 MHz has been estimated to be more than 65${\sim}$80 dB. The measured shielding effectiveness of screen filter is 10${\sim}$50 dB at 30${\sim}$300 MHz[1]. The resulting discrepancy indicates that there are other EMI emission sources such as emission from PCB and cable besides the PDP electrodes.

• 천문학회보
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• 제40권2호
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• pp.49.1-49.1
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• 2015

Star formation in galaxies that lie in dense environment tends to increase as the redshift of the cluster increases. At z~1.4, the situation turns to be complex; some clusters still harbor galaxies with vigorous star formation, and others are populated with relatively old, massive galaxies. We present the result from narrow-band photometric study of the fields around the radio galaxy 6CE 1100+3505 at z=1.44. Deep H- and H-narrow band data have been obtained using CFHT/WIRCAM which cover the corresponding wavelengths for redshifted $H{\alpha}$. While the number of IRAC 3.6, and $4.5{\mu}m$ selected sources show clear excess within the central ~1Mpc area from the radio galaxy, number of galaxies identified to show excess in H-narrow band is very small. We discuss the possible integrated star formation rate in this overdense structure, and the implication to the evolution of cosmic star formation rate as a function of environment.

• Journal of Astronomy and Space Sciences
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• 제33권2호
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• pp.101-104
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• 2016

More than 100 γ−ray pulsars have been discovered by the Fermi Gamma-ray Space Telescope. With a significantly enlarged sample size, it is possible to compare the properties of different classes. Radio-quiet (RQ) γ−ray pulsars form a distinct population, and various studies have shown that the properties of the RQ population can be intrinsically different from those of radio-loud (RL) pulsars. Utilizing these differences, it is possible to further classify the pulsar-like unidentified γ−ray sources into sub-groups. In this study, we suggest the possibility of distinguishing RQ/RL pulsars by their spectral shape. We compute the probabilities of a pulsar to be RQ or RL for a given spectral curvature. This can provide a key to the estimation of the intrinsic fraction of radio-quietness in the γ−ray pulsar population, which can place a tight constraint on the emission geometry.

• 한국표면공학회지
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• 제29권5호
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• pp.357-362
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• 1996

Several applications of radio-frequency (RF) thermal plasma to film formation are reviewed. Three types of injection plasma processing (IPP) technique are first introduced for the deposition of materials. Those are thermal plasma chemical vapor deposition (CVD), plasma flash evaporation, and plasma spraying. Radio-frequency (RF) plasma and hybrid (combination of RF and direct current(DC)) plasma are next introduced as promising thermal plasma sources in the IPP technique. Experimental data for three kinds of processing are demonstrated mainly based on our recent researches of depositions of functional materials, such as high temperature semiconductor SiC and diamond, ionic conductor $ZrO_2-Y_2O_3$ and high critical temperature superconductor $YBa_2Cu_3O_7-x$. Special emphasis is given to thermal plasma flash evaporation, in which nanometer-scaled clusters generated in plasma flame play important roles as nanometer-scaled clusters as deposition species. A novel epitaxial growth mechanism from the "hot" clusters namely "hot cluster epitaxy (HCE)" is proposed.)" is proposed.osed.

• 전자공학회논문지SC
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• 제41권2호
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• pp.37-44
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• 2004

본 논문에서는 전파천문 분야에서 특이한 전파원의 서베이 연구나, 외부은하의 스펙트럴 선 관측연구에 필요한 자기상관분광기 형태의 광-대역 전파분광기 제작에 있어서 가장 핵심적인 역할을 하는 상관기 보드를 설계, 제작하였다. 본 연구에서는 미국 국립천문대(NRAO)에서 개발된 QUAINT 상관기 칩을 사용하여 최대 100 ㎒의 동작 속도로 최대 400 ㎒ 대역폭을 갖는 중간주파수 신호를 분광할 수 있는 상관기 보드를 설계, 제작하였다. 제작된 상관기 보드의 성능시험을 위해 1.67 ㎒와 0.5 ㎒의 구형파를 인가하여 자기상관계수를 구하고, FFT를 취한 결과 이론적인 상관결과와 거의 같은 결과를 얻었다.

• 천문학회지
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• 제1권1호
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• pp.29-36
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• 1968

1. 28 candidates of novae and supernovae were selected from ancient Korean observational records. 2. 4 Supernovae were confirmed. 3. 1 guest star was suspected as the original explosion of Cas A. 4. 9 asterisked positions were suggested for further study in the hope of finding additional supernovae-radio sources.

• 천문학회보
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• 제31권2호
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• pp.48.1-48.1
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• 2006

• 한국전자통신학회논문지
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• 제16권6호
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• pp.1175-1182
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• 2021

한국우주전파관측망(KVN: Korea VLBI Network)을 이루는 각 망원경의 수신기에는 우주에서 오는 전파 신호를 디지털 신호로 바꾸는 샘플러가 있다. 이 샘플러의 성능(특히, 대역폭과 샘플링 주파수 그리고 샘플링 비트수)은, 대역폭을 n배 증가시키면 관측감도는 sqrt(n) 만큼 향상되고, 연속전파원의 경우 관측 가능한 천체의 수가 기하급수학적으로 증가하게 된다. 대역폭이 넓어지면, 전파원에서 동시에 모니터링 할 수 있는 스펙트럼의 선들도 많아진다. 이는 전파 관측에서 연구영역을 대폭 확장시킬 수 있게 된다. 이러한 이유로 고속 샘플러의 기술과 성능 향상을 독자적으로 확보하려하는 것이다. 이에, 지금까지의 연구 경험과 기술 축적을 바탕으로, 샘플링 주파수를 가변할 수 있으며, 보다 광대역으로 관측을 할 수 있는 최대 3.5GHz 샘플링을 할 수 있는 장치를, 초기 시험용으로 설계·제작하였다. 본 연구에서는 개발된 가변 샘플링 시스템의 내용과 시험 측정 결과를 발표하고자 한다.

• KSII Transactions on Internet and Information Systems (TIIS)
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• 제11권3호
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• pp.1279-1300
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• 2017

In the interweave cognitive networks, the interference from the primary user degrades the performance of the cognitive user transmissions. In this paper, we propose an adaptive cooperation scheme in the interweave cognitive networks to improve the performance of the cognitive user transmissions. In the proposed scheme for the bidirectional communication of two end-source cognitive users, the bidirectional communication is completed through the non-relay direct transmission, the one-way relaying cooperation transmission, and the two-way relaying cooperation transmission depending on the limited feedback from the end-sources. For the performance analysis of the proposed scheme, we derive the outage probability and the finite-SNR diversity multiplexing tradeoff (f-DMT) in a closed form, considering the imperfect spectrum sensing, the interference from the primary user, and the power allocation between the relay and the end-sources. The results show that compared with the direct transmissions (DT), the pure one-way relaying transmissions (POWRT), and the pure two-way relaying transmissions (PTWRT), the proposed scheme has better outage performance. In terms of the f-DMT, the proposed scheme outperforms the full cooperation transmissions of the POWRT and PTWRT.