• 제목/요약/키워드: light curve

검색결과 567건 처리시간 0.024초

DETECTION LEVEL ENHANCEMENTS OF GRAVITATIONAL MICROLENSING EVENTS FROM LIGHT CURVES: THE SIMULATIONS

  • IBRAHIM, ICHSAN;MALASAN, HAKIM L.;DJAMAL, MITRA;KUNJAYA, CHATIEF;JELANI, ANTON TIMUR;PUTRI, GERHANA PUANNANDRA
    • 천문학논총
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    • 제30권2호
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    • pp.235-236
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    • 2015
  • Microlensing can be seen as a version of strong gravitation lensing where the separation angle of the image formed by light deflection by a massive object is too small to be seen by a ground based optical telescope. As a result, what can be observed is the change in light intensity as function of time; the light curve. Conventionally, the intensity of the source is expressed in magnitudes, which uses a logarithmic function of the apparent flux, known as the Pogson formulae. In this work, we compare the magnitudes from the Pogson formulae with magnitudes from the Asinh formulae (Lupton et al. 1999). We found for small fluxes, Asinh magnitudes give smaller deviations, about 0.01 magnitudes smalller than Pogson magnitudes. This result is expected to give significant improvement in detection level of microlensing light curves.

접촉쌍성 V523 CAS의 광도곡선 분석 (LIGHT CURVE ANALYSIS OF CONTACT BINARY SYSTEM V523 CASSIOPEIAE)

  • 김진희;정장해
    • Journal of Astronomy and Space Sciences
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    • 제19권4호
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    • pp.263-272
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    • 2002
  • 보현산 천문대의 1.8m 망원경을 이용하여 1999년 10월 19일부터 21일까지 총 3일간 W UMa형 접촉쌍성 V523 Cas를 CCD 측광관측하여 총 616 (308의 ${\Delta}$b점, 308의 ${\Delta}$v점) 개의 관측점을 얻었다. 우리의 관측점으로부터 4개의 새로운 극심시각(주극심 2개, 부극심 2개)을 산출하였다. 우리가 얻은 BV 광도곡선과 Milone et al.(1985)의 시선속도곡선을 Wilson-Devinney(WD) 방법으로 흑점이 있는 경우와 없는 경우로 나누어 광도곡선의 해를 산출하였다.

LIGHT CURVE VARIATIONS OF AR LACERTAE

  • Nha, Il-Seong
    • Journal of Astronomy and Space Sciences
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    • 제8권2호
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    • pp.149-158
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    • 1991
  • Sixteen unitary Light curves of AR Lac in B and V are made at Yonsei University Observatory in the period of 1980-1988. Some overview findings of light variations are made. (1) The light variation outside eclipse follow none of the wave migration patterns reported by previous investigators. (2) Complicated shapes outside eclipse are apparently much reduced in the light curves of 1983-1984. This suggests than, in the future, AR Lac has a chance to attain a normal state with no complicated interactions. (3) The depths of the primary and the secondary mid-eclipses are changing year-to-year. (4) The K0 star, the larger component, has brightened by $0.^m$ 14 in V, while the G2 star has shown a fluctuation of about $0.^m$05 in V. (5) The B-V values at primary mid-eclipse have no correlation with the depth variations. (6) Independently of the increase of maximum brightness, the B-V colors in the non-eclipsed phases changed slightly over the years.

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Contact and Near-Contact Binaries with co-relation of Mass transfer and Asymmetric Light Curve

  • Rittipruk, Pakakaew;Kang, Young-Woon
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
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    • 한국우주과학회 2010년도 한국우주과학회보 제19권1호
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    • pp.32.3-32.3
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    • 2010
  • We have analyzed times of minima for six eclipsing binary systems which show asymmetric light curves. We found that five binary systems show period decrease and one system shows cyclic period variation. Three asymmetric light curves (SV Cen, RT Scl and VW Boo) are due to hot spot caused by mass transfer. Other three asymmetric light curves (AD Phe,, EZ Hya and TY Boo) are due to cool spot on the cooler component caused by magnetic activities. We also obtain absolute dimensions from photometric solution and spectroscopic solution by analyzing their light curves and radial velocity curves, collected from literatures, using 2007 version Wilson and Devinney computer code.

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맥동 식쌍성 Y Cam의 ROCHE 모형과 절대 물리량 (ROCHE MODEL AND ABSOLUTE DIMENSIONS OF THE ECLIPSING BINARY Y CAM WITH A PULSATING COMPONENT)

  • 이재우;김천휘;김승리;윤재혁;권순길
    • Journal of Astronomy and Space Sciences
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    • 제19권3호
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    • pp.187-196
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    • 2002
  • 2000년 11월부터 2001년 5월까지 총 16일간 맥동 식쌍성 Y Carn을 소백산천문대의 61cm 망원경에 부착된 단일 V 필터로 CCD 측광을 수행하였다. 새롭게 얻은 V 광도곡선과 Broglia & Marin(1974)의 BV 광도곡선을 Wilson-Devinney 방법의 Mode 2(분리형)와 Mode 5(준분리형)으로 분석하였다. 분석 결과는 다음과 같다. 1) 광도곡선 분석만으로는 분리헝과 준분리형의 Roche 모형 중 어느 것이 Y Cam의 진실한 Roche 모형인가를 가려낼 수가 없다. 2) Y Cam의 B광도곡선에는 삼체의 광도가 약 2%, V광도곡선에는 약 3% 존재한다. 3) Y Cam의 주성에서 발생하는 맥동에 의한 밝기 변화는 광도곡선 해에 거의 영향을 주지 않으나, 맥동을 고려하였을 경우 분리형 모델이 준분리형 모델보다 약간 더 관측치를 잘 맞춘다. 4) 분리형과 준분리형 각각에 대해 Y Cam의 절대물리량을 계산하였다.

Hysteretic performance of a novel composite wall panel consisted of a light-steel frame and aerated concrete blocks

  • Wang, Xiaoping;Li, Fan;Wan, Liangdong;Li, Tao
    • Steel and Composite Structures
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    • 제41권6호
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    • pp.861-871
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    • 2021
  • This study aims at investigating the hysteretic performance of a novel composite wall panel fabricated by infilling aerated concrete blocks into a novel light-steel frame used for low-rise residential buildings. The novel light-steel frame is consisted of two thin-wall rectangular hollow section columns and a truss-beam assembled using patented U-shape connectors. Two bare light-steel frames and two composite wall panels have been tested to failure under horizontal cyclic loading. Hysteretic curves, lateral resistance and stiffness of four specimens have been investigated and analyzed. Based on the testing results, it is found that the masonry infill can significantly increase the lateral resistance and stiffness of the novel light-steel frame, about 2.3~3 and 21.2~31.5 times, respectively. Failure mode of the light-steel frame is local yielding of the column. For the composite wall panel, firstly, masonry infill is crushed, subsequently, local yielding may occur at the column if loading continues. Hysteretic curve of the composite wall panel obtained is not plump, implying a poor energy dissipation capacity. However, the light-steel frame of the composite wall panel can dissipate more energy after the masonry infill is crushed. Therefore, the composite wall panel has a much higher energy dissipation capacity compared to the bare light-steel frame.

MAGNETOSPHERIC STRUCTURE OF THE INTERMEDIATE POLAR

  • Kim, Yong-Gi
    • Journal of Astronomy and Space Sciences
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    • 제11권1호
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    • pp.1-12
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    • 1994
  • The structure of the magnetic funnel element in the intermediate polar is considered in terms of an important site for the X-ray absorption and the reemission of the X-ray as the optical light. In this paper the column density and the optical depth vary with the filling factor, which is introduced to characterize the structure of matter in the magnetic funnel element. The results of the energy dependence of the X-ray spectrum and the modulation depth of the X-ray light curve are discussed.

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A Study on the healing factors of Forest Sound

  • Yi, Eun-Young;Bae, Myung-Jin
    • International Journal of Internet, Broadcasting and Communication
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    • 제9권2호
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    • pp.70-77
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    • 2017
  • Where there are all the flowers, the songs of all kinds of insects and birds are put in, the sunshine and shadows flicker The forest through which the water sound flows is an optimum resting space. All living creatures in these spaces will awaken the five senses of humans and perhaps turn the sensibility index (EQ). The forest meditation in the forest, which can be an optimal shelter for the people who need it, needs to feel the reverence of nature, to refine emotions, to be a self-reflection, to have a mind to respect, Have an important meaning. In this paper, we tried to consider the cause of the influence of forest sounds on human hearing from the acoustical aspect. The type of sound source of forest was divided into four seasons of spring, summer, autumn, winter. And the change in the duration of the sound during the four seasons, so that the general characteristics of the sounds of the four seasons are as follows: It can be seen that the change in the ratio of sub-band energy is almost equal to the change in dB in frequency of the equal-light curve. To compare this phenomenon, the criterion for changing the sound duration of each forest is natural The main forms of the luminance curve, such as the change in the duration of the white signal in the sound, are determined by the minimum, maximum audible frequency and the most sensitive frequency band, and the auditory characteristics of the other three inflection points Determines the overall shape of the equal-light curve.

경량전철에 대한 차체 및 대차틀의 피로강도평가 (Fatigue Strength Evaluation of Carbody and Bogie Frame for the Light Rail Transit System)

  • 이은철;이준성;최윤종;이정환;서명원;이호용;이양창
    • 한국정밀공학회지
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    • 제25권10호
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    • pp.77-83
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    • 2008
  • In terms of saving costs, energy and materials, the weight of cars has been gradually reduced by optimizing design of structure, which also gives us good performance. In compliance with this, it should satisfy the lifetime of cars for 25 years under the operation. The purpose of this study is to evaluate the strength of fatigue using date from strain gauges attached carbody and bogie frame. This dynamic stress can be evaluated using S-N curve based on stress amplitude. Modified S-N curve by CORTON-DOLAN is used for more conservative and substantial evaluation. In addition, !he loadings itself of carbody and bogie frame are considered by calculating the rate of the differences which are occurred between empty car and fuiiy occupied car with passengers. Rainflow cycle counting method is applied to arrange the stress data for the modified S-N curve to predict lifetime of the materials. Conclusively the cumulative damages are not only calculated by Miner's Rule, but the safety factors are also determined by Goodman diagram.