• Journal of the Optical Society of Korea
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• 제16권4호
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• pp.343-348
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• 2012

This paper described an off-axis five-mirror-anastigmatic telescope. It is composed of three aspheric surfaces and one spherical surface while the third mirror and fifth mirror have the same parameters at the same place. This configuration is useful for having wide field of view. The strip full field of view for the near infrared telescope is $20^{\circ}{\times}0.2^{\circ}$. The entrance pupil is located in front of the first mirror. There is an intermediate image between the second mirror and the third mirror. The entrance pupil diameter is 100 mm and the effective focal length is 250 mm. The spectral range is $0.85-1.75{\mu}m$. The pixel pitch is $15{\mu}m$. The image quality is near the diffraction limit. Some methods were used to restrain the stray light such as a field stop near the intermediate image, the baffle, the narrow-band pass filter and a stop in front of the focal plane.

• 천문학회보
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• 제44권1호
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• pp.46.3-46.3
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• 2019

We present our observational and theoretical investigation of Raman-scattered features in symbiotic stars (SySts). SySts are long interacting binaries, consisting of a hot compact star and an evolved giant, whose interaction via accretion process is at the origin of a tangled network of gas and dust nebulae. These systems are ideal objects to study a variety of important astrophysical problems, and have also been proposed as possible progenitors of type Ia supernova. In this talk, we emphasize that Raman-scattered features are exclusive spectroscopic tools to probe the stellar wind accretion processes in SySts. We studied mass transfer and mass loss processes in SySts using high resolution spectra obtained with 1.8m telescope at Mt. Bohyun and the 6.5m Magellan-Clay telescope combining with the theoretical modeling of radiative transfer of Raman-scattered features. We also note that there are a much smaller number of SySts known in our Galaxy, implying the necessity of systematic search programs. In view of the fact that Raman O VI features at $6830{\AA}$ are found in only bona fide SySts, we will carry out a photometric search of objects with Raman O VI features using a narrow band filter centered at $6830{\AA}$ in Local group galaxies.

• 천문학회보
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• 제44권1호
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• pp.44.4-44.4
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• 2019

The supernova remnant Cassiopeia A (Cas A) provides a unique opportunity to observe the fine details of the explosion of core-collapse supernova (SN). Previous optical and near-infrared (NIR) observations of Cas A have shown that the spatial distribution of the metal-enriched SN ejecta is very complicated, indicating that the SN explosion should have been asymmetric and turbulent, especially near the core. Recently, we obtained a long-exposure (~10 hr) image of Cas A by using the UKIRT 3.6-m telescope with a narrow-band filter centered at [Fe II] 1.644 um emission. This 'deep [Fe II] image' provides an unprecedented panoramic view of Cas A, revealing the distribution of dense SN ejecta over the entire remnant. We have carried out NIR multi-object spectroscopic observations of the dense ejecta knots in the northeastern (NE) and eastern (E) outer regions of the remnant using the MMIRS attached on the MMT 6.5-m telescope. A total of 67 ejecta knots are detected. By analyzing their spectra, we have found that the knots in the NE area show strong [S II]/[S III] and [Fe II] lines but little or no [P II] line, while those in the E outer region show strong [Fe II] lines but weak [S II]/[S III] lines. In this talk, we present the preliminary results of our NIR spectroscopic observations and discuss the implications.

• 천문학회보
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• 제45권1호
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• pp.66.4-67
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• 2020

Gyeonggi science high school for the gifted (GSHS) installed 60cm telescope, which is waiting for student observers. It is essential to understand the characteristics of the photometric system, consisting of telescope, filter, and CCD, to get reliable data. CCD images of SA98 Landolt standard field and M67 were obtained on 19th March 2020. The images of each field were combined by filters, i.e., we ignored the monochromatic atmospheric extinction since the photometric objects themselves are standard stars. 24 standard stars in SA98 field and 12 standard stars in M67 were used to derive the tentative transformation equation between our bv photometric system and Johnson BV photometric system. In this poster, we present the preliminary standardization result for Johnson BV photometric system in GSHS 60cm telescope. The reproductivity is discussed by comparing color coefficients of two fields. We plan to extend this process to Johnsons-Cousins BVRI photometric system and narrow-band filters for flux calibration.

• 천문학회보
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• 제42권1호
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• pp.54.1-54.1
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• 2017

The UKIRT Wide-field Infrared survey for Fe+(UWIFE) is an unbiased survey of the first Galactic quadrant, with narrow-band filter centered on $1.644{\mu}m$. This survey covers $7^{\circ}$ < l < $62^{\circ}$ and |b| < $1.5^{\circ}$, where active interaction of stars and interstellar medium is expected. With median seeing of 0.8 arcsec, 5 - sigma detection limit of 18.7 mag and surface brightness limit of $8.1{\times}10^{-20}W\;m^{-2}arcsec^{-2}$, this survey gives an opportunity to statistically study Galactic [Fe II] - emitting sources for the first time. In order to identify Ionized Fe Objects (IFOs) in survey area systematically, we conducted visual inspection and automatic detection simultaneously. Total of ~300 extended IFOs are identified, most of them are found out to be part of supernova remnants (SNRs), young stellar objects, HII regions and planetary nebulae. The majority of IFOs are new discoveries which reveal shocked structures in high-extinction region. Spatial distribution of IFOs suggest that they trace Galactic structure. As a part of spectroscopic follow-up, we observed SNR candidate IFO J183740.829-061452.41 with IGRINS (Immersion Grating Infrared Spectrograph, Yuk+2010), mounted on 2.7m Harlan Smith telescope. This unknown arc-like, 6'-long IFO is coincident with inner part of radio continuum loop G25.8+0.2, which has been known as HII region. However, interior of this radio shell is filled with diffuse soft X-ray emission, and possible association of hard X-ray pulsar / pulsar wind nebula makes the nature of the IFO unclear. The H and K-band 2D spectrum shows shock-ionized [Fe II] filaments, which is apart from photoionized HII filaments. In this presentation we present basic statistics of newly identified IFOs, as well as the follow-up study of IFO J183740.829-061452.41.

• 한국전자파학회논문지
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• 제15권2호
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• pp.134-139
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• 2004

40 Gb/s 광 수신기용 클락 복원회로를 설계 및 제작하였다. 클락 복원회로는 전치 증폭기, 다이오드를 이용한 비선형 회로, 대역통과 필터, 클락 증폭기로 구성되어 있다. 40 Gb/s 클락 복원회로를 제작하기에 앞서 10 Gb/s 클락 복원회로를 제작, 측정하였다. 40 Gb/s 클락 복원회로에 -10 dBm의 40 Gb/s NRZ 신호를 입력하였을 때, 비선형 회로를 통과한 후에 40 GHz의 클락이 출력 전력 -20 dBm으로 복원되었다. 비선형 회로를 통과하여 복원된 클락은 협대역 필터를 통과하고, 증폭되게 된다. 제작된 클락 복원회로는 클락의 지터를 감소시키고, 더욱 안정화 시키기 위하여 위상 동기 회로의 입력으로 사용되게 된다.

• 한국정보통신학회:학술대회논문집
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• 한국해양정보통신학회 2002년도 추계종합학술대회
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• pp.148-150
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• 2002

본 논문에서는 테프론을 이용하여 커플링 수가 5개인 대역통과필터를 제안한다. BPF의 경우, 1 GHz 이내의 낮은 주파수에서는 좁은 대역폭과 저지대역에서 우수한 특성을 갖는 필터를 집중소자를 이용하여 만들 수 있지만 그 이상의 주파수에서는 유전체를 이용한 마이크로 스트립과 같은 분포소자를 이용하여 설계하여야 한다. 한편 분포 소자를 이용하는 방법으로서 2 GHz 이하에서는 저 비용이면서도 우수한 특성을 보이는 FR4를 사용하지만, 2 GHz ~ 10 GHz에서 FR4구조는 설계치와 측정치의 차이가 크므로 FR4 대신, 테프론을 이용한다. 제안한 필터의 중심 주파수는 2.3 GHz, 삽입 손실이 1.2 dB, 반사 손실이 30 dB, 대역폭이 100 MHz, 크기는 8.3 cm $\times$ 4.9 cm 이다.

• Journal of the Optical Society of Korea
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• 제18권3호
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• pp.261-273
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• 2014

In this paper, metal insulator metal (MIM) plasmonic slot cavity narrow band-pass filters (NBPFs) are studied. The metal and dielectric of the structures are silver (Ag) and air, respectively. To improve the quality factor and attenuation range, two novel NBPFs based on tapered structures and double cavity systems are proposed and numerically analyzed by using the two-dimensional (2-D) finite difference time domain (FDTD) method. The impact of different parameters on the transmission spectrum is scrutinized. We have shown that increasing the cavities' lengths increases the resonance wavelength in a linear relationship, and also increases the quality factor, and simultaneously the attenuation of the wave transmitted through the cavities. Furthermore, increasing the slope of tapers of the input and output waveguides decreases attenuation of the wave transmitted through the waveguide, but simultaneously decreases the quality factor, hence there should be a trade-off between loss and quality factor. However, the idea of adding tapers to the waveguides' discontinuities of the simple structure helps us to improve the device total performance, such as quality factor for the single cavity and attenuation range for the double cavity. According to the proposed NBPFs, two, three, and four-port power splitters functioning at 1320 nm and novel ultra-compact two-wavelength and triple-wavelength demultiplexers in the range of 1300-1550 nm are proposed and the impacts of different parameters on their performances are numerically investigated. The idea of using tapered waveguides at the structure discontinuities facilitates the design of ultra-compact demultiplexers and splitters.

• 대한전자공학회논문지SP
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• 제45권2호
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• pp.81-89
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• 2008

광대역 신호는 16 kHz로 표본화되어 50-7000 Hz로 밴드 제한된 신호를 말하며, 전화대역 음성 신호에 비해서 높은 자연성(naturalness)과 명료성(intelligibility)을 가진다. 이런 특징으로 광대역 부호화기는 화상회의, 디지털 AM 방송 및 고음질 음성통신 등에 사용될 수 있다. 본 논문에서는 가변대역 특징을 갖는 광대역 음성 오디오 부호화기를 제안하였다. 제안된 부호화기는 대역분한 구조를 가진다. 저주파 대역은 전화대역 음성 부호화기로 많이 사용되고 있는 8 kbit/s ITU-T G.729나 보다 높은 전송률로 오디오 신호까지 처리할 수 있는 11.8 kbit/s ITU-T G.729 Annex E로 부호화한다. 고주파 대역은 청각 모델을 기반으로 한 파라미터 부호화 방법으로 부호화한다. 제안된 고주파 대역 부호화는 감마톤 필터뱅크(gammatone filterbank)를 이용하여 입력신호를 임계대역으로 분할한 후, 각각의 임계대역 신호를 양자화한다. 저주파 대역 부호화기와 고주파 대역 부호화기는 서로 독립되어 있으므로, 복호화기에서는 채널 조건에 따라 전화대역 합성신호와 광대역 합성신호를 선택할 수 있는 특징이 있다. 성능 평가 결과, 제안된 부호화기는 낮은 전송률과 짧은 지연 시간으로 음성과 오디오 신호 모두에 대해 ITU-T G.722.1 24 kbit/s와 동등한 음질을 제공한다는 것을 확인하였다.

• 한국통신학회논문지
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• 제34권11C호
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• pp.1085-1097
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• 2009

본 논문에서는 VDL 모드-2 규격을 따르는 송신기와 수신기의 구조 및 설계방법 그리고 개발한 모뎀의 성능시험 결과에 대해 기술한다. VDL 모드-2에서 송신기 필터는 올림 코사인 필터를 사용하고 수신기에서는 일반 저역 통과 필터(LPF)를 사용(비 정합필터)하기 때문에 ISI 경감 효과는 없으나 스펙트럼 특성은 더 좋다. 이는 정합필터를 적용했을 경우보다 1~2 dB 정도의 BER 성능은 저하되나 협 대역 통신에서 이웃 채널에 간섭을 최소화하는 것이 더 중요하기 때문이다. 송신기에서 변조신호 생성 시 발생되는 아날로그 방식의 단점(I/Q 이득 불균형, DC 오프셋 등)을 최소화하기 위해 디지털 방식으로 생성하였으며 수신기도 디지털 IF 샘플링 기법을 통하여 디지털 하향변환기를 적용하였다. 본 논문은 기 제안된 일부 구조 및 알고리듬을 포함하며 모뎀 구성에 필요한 전반적인 구조와 설계 방법 그리고 모의실험 결과가 추가되었다. 개발된 모뎀은 VDR 장비에 통합되어 각종 기능 실험과 환경시험을 거친 후 지상통신시험을 실시하였고 비행통신시험결과 시속 870 km/h로 310 km까지 메시지 송수신이 정상적으로 이루어짐을 확인하였다.