We present the deep homogeneous 𝑈𝐵𝑉𝑅𝐼 photometric data of 135,071 stars down to 𝑉 ∼ 23 mag and 𝐼 ∼ 22 mag toward the Carina Nebula. These stars are cross-matched with those from the previous surveys in the X-ray, near-infrared, and mid-infrared wavelengths as well as the Gaia Early Data Release 3 (EDR3). This master catalog allows us to select reliable members and determine the fundamental parameters distance, size, stellar density of stellar clusters in this star-forming region. We revisit the reddening toward the nebula using the optical and the near-infrared colors of early-type stars. The foreground reddening [𝐸(𝐵 −𝑉) 𝑓 𝑔] is determined to be 0.35 ± 0.02, and it seems to follow the standard reddening law. On the other hand, the total-toselective extinction ratio of the intracluster medium (𝑅𝑉,𝑐𝑙) decreases from the central region (Trumpler 14 and 16, 𝑅𝑉,𝑐𝑙 ∼ 4.5) to the northern region (Trumpler 15, 𝑅𝑉,𝑐𝑙 ∼ 3.4). It implies that the central region is more dusty than the northern region. We find that the distance modulus of the Carina Nebula to be 11.9 ± 0.3 mag (𝑑 = 2.4 ± 0.35 kpc) using a zero-age main-sequence fitting method, which is in good agreement with that derived from the Gaia EDR3 parallaxes. We also present the catalog of 3,331 pre-main-sequence (PMS) members and 14,974 PMS candidates down to 𝑉 ∼ 22 mag based on spectrophotometric properties of young stars at infrared, optical, and X-ray wavelengths. From the spatial distribution of PMS members and PMS candidates, we confirm that the member selection is very reliable down to faint stars. Our data will have a legacy value for follow-up studies with different scientific purposes.

In this study, optical emission spectroscopy was used to monitor the plasma produced during the RF magnetron sputtering of a BaTiO3 target. The intensities of chemical species were measured by real time monitoring with various discharge parameters such as RF power, pressure, and discharge gas. The emission lines of elemental and ionized species from BaTiO3 and Ti targets were analyzed to evaluate the film composition and the optimized growth conditions for BaTiO3 films. The emissions from Ar(I, II), Ba(I, II) and Ti(I) were found during sputtering of the BaTiO3 target in Ar atmosphere. With increasing RF power, all the line intensities increased because the electron density increased with increasing RF power. When the Ar pressure increased, the Ba(II) and Ti(I) line intensity increased, but the Ar+ line intensity decreased with increasing pressure. This result shows that high pressure is of greater benefit for the ionization of Ba than for that of Ar. Oxygen depressed the intensity of the plasma more than Ar did. When the Ar/O2 ratio decreased, the intensity of Ba decreased more sharply than that of Ti. This result indicates that the plasma composition strongly depends on the discharge gas atmosphere. When the oxygen increased, the Ba/Ti ratio and the thickness of the films decreased. The emission spectra showed consistent variation with applied power to the Ti target during co-sputtering of the BaTiO3 and Ti targets. The co-sputtered films showed a Ba/Ti ratio of 1.05 to 0.73 with applied power to the Ti target. The films with different Ba/Ti ratios showed changes in grain size. Ti excess films annealed at 600˚C did not show the second phase such as BaTi2O5 and TiO2.

The study of wave propagation and scattering in biological media has become increasingly important in recent years. The propagation of light within tissues is an important problem that confronts the dosimetry of therapeutic laser delivery and the development of diagnostic spectroscopy. In the clinical application of photodynamic therapy(PDT) and in photobiology, the photon deposition within a tissue determines the spatial distribution of photochemical reactions. Scattered light is measured as a function of the distance (r) between the axis of the incident beam and the detection spot. Consequently, knowledge of the photosensitizer(Chlorophyll-a) function that characterizes a phantom is measured. To obtain the results of scattering coefficients(μs) of a turbid material from diffusion described by experimental approach. It was measured the energy fluency of photon radiation at the position of penetration depth. From fluorescence experimental method obtained the analytical expression for the scattered light as the values of (I/Io)wavelength vs the distance between the center of the incident beam and optical fiber in terms of the condition of "in situ spectroscopy(optically thick)" and real time by fluorometric measurements. The result was compromised with transport of intensities though a random distribution of scatters.

Taguchi methodology has been applied to get an idea about the parameters related to the chemical vapour deposition technique, which influences the formation of semiconducting carbon thin film of a desired band gap. L9 orthogonal array was used for this purpose. The analysis based on Taguchi methodology suggests that amongst the parameters selected, the temperature of pyrolysis significantly controls the magnitude of band gap (46%). Sintering time has a small influence (30%) on the band gap formation and other factors have almost no influence on the band gap formation. Moreover this analysis suggests that lower temperature of pyrolysis (≤ 750℃) and lower time of sintering (≤ 1 h) should be preferred to get carbon thin film with the desired band gap of 1.2eV.

TiO2/Ag 계 적층형 투명 열절연 박막의 최적 제작조건 설정을 위한 기초 연구로써, 스퍼터조건에 따른 결정구조 및 광학특성 변화거동을 관찰하였다. 반응성 스퍼터링에 의한 TiO2박막 제작조건에 따른 결정구조 및 광학특성 변화거동을 관찰하였다. 반응성 스퍼터링에 의한 TiO2 박막 제작시 Po2/PAr≤0.2에서는 α-TiO2 의 결정구조였으나, Po2/PAr≤0.2에서는 기판 온도(RT-370˚C) 및 열처리 온도(100-800˚C)에 관계없이 non-stoichiometric 화합물로 판명되어, 산소 분압비가 TiO2 의 조성제어에 가장 중요한 변수로 나타났다. TiO2 박막은 열처리 온도의 증가(100-800˚C)에 따라 굴절률이 증가(2.19-2.37)하는 경향이었는데, 이는 박막의 밀도증가에서 기인하는 것으로 판단된다. Ag 박막은(111)면과 (200)면이 우세한 결정립으로, 기판 온도(RT-370˚C) 및 열처리(100-800˚C)에 따라 등축상의 결정립 성장을 관찰할 수 있었다.

silica의 precursor로 TMOS를 사용하여 autoclave 내에서 supersritical drying으로 투명한 TiO2-SiO2 이성분계 aerogle을 얻을 수 있었다. 반응성이 뛰어난 titanium alkoxide의 중축합반응을 억제할 수 있는 강한 산성 영역에서 투명한 Aerogel을 얻을 수 있었으며, 물을 직접 첨가하지 않고 silicon alkoxide의 축합반응의 부산물인 물을 이용하여 titanium alkoxide의 반응성을 제어했을 때 투명성이 더욱 증진되었다.

The influences of fluorophor, scatterer, absorber in turbid material by light scattering were interpreted for the scattered fluorescence intensity and wavelength, it has been studied the molecular properties by laser induced fluorescence spectroscopy. It has been found that the effects of optical properties in scattering media by the optical parameters(μs, μa, μt). The value of scattering coefficient μs is large by means of the increasing particles of scatterer, it has been found that the slope decays exponentially as a function of distance from laser source to detector. It may also aid in designing the best model for oil chemistry, laser medicine and application of medical engineering.