• 천문학회보
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• 제44권2호
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• pp.79.2-79.2
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• 2019

We introduce Maemi Dual Field Telescope System (MDFTS) which is newly installed at Kyung Hee Astronomical Observatory (KHAO). MDFTS consists of two telescope tubes (40cm and 10cm), whose observing fields are aligned with different field of view, 15' x 11' and 83' x 63' respectively. We present the specification of instruments (telescope, mount, camera, and filter system) and the observation environment of KHAO. We expect that MDFTS can be used for transient survey e.g. Intensive Monitoring Survey of Nearby Galaxies (IMSNG). Based on observations conducted so far, the limiting magnitude of 40cm telescope in B-band is B_lim ~ 16 mag at 5-σ detection with 150 seconds total integration time under dark and clear observing condition. Also the integrated observing software for MDFTS, KAOS40 is now under developing.

• 천문학회보
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• 제32권2호
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• pp.73-73
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• 2007

• 천문학회보
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• 제32권2호
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• pp.72.2-72.2
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• 2007

• 천문학회보
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• 제34권1호
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• pp.126.1-126.1
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• 2009

• 천문학회보
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• 제35권2호
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• pp.37.2-37.2
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• 2010

The IMS (Infrared or Intermediate-wide, Medium-deep Survey) program for the search of z~7 quasars has been running since last year. In order to discover enough number of quasars at z~7, a strategy sufficing both survey area (~150 square deg.) and image depth (23 AB mag in J filter), together with using existing multi-wavelength data is chosen. We have been carrying imaging observations with the UKIRT 4m telescope, now covering ~50 square deg. (including UKIDSS survey area) of J-band data. We then used selection in color-color space to choose high-z quasar candidates having the rest-frame Ly-alpha break, and to exclude contamination from stars and galaxies at low-z. We show quasar candidates of redshift z~7 and z~6, out of 25 square deg. data analyzed, and note implications and future plans.

• 천문학회보
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• 제36권1호
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• pp.51.2-51.2
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• 2011

The Spitzer Public Legacy Survey of the UKIDSS Ultra Deep Survey (SpUDS) has been carried out with four IRAC bands and one MIPS band (24um). SpUDS surveys 1 square degree of the UDS field, that has been covered by one of the deepest near IR surveys and by various multiwavelength observations from X-ray to radio (XMM, GALEX, Subaru, SCUBA, VLA). We present a summary of the photometric data including number counts derived at 3.6-24 microns. In conjunction with extensive multiwavelengh data, we are able to show the multiwavelenght color distribution of MIR sources, and how different SED types contribute to the number counts.

• 천문학회보
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• 제32권1호
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• pp.71.2-71.2
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• 2007

• 한국지구과학회지
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• 제28권7호
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• pp.789-802
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• 2007

이 논문에서는 한국과 일본의 초등 예비교사들이 가지고 있는 천문학 기초개념에 대한 이해 정도와 천문학에 대한 태도를 조사하여 비교하였다. 천문학 기초개념 및 지식은 1998년에 천문교육연구협의회(The Collaboration for Astronomy Education Research, CAER)에서 개발한 천문학진단검사지(Astronomy Diagnostic Test, ADT ver.2.0)의 21문항에서 한일 양국의 중등학교 교육과정을 고려하여 선정한 12개 문항을 양국의 언어로 번안하여 투입하였다. 천문학 기초개념 및 지식에 대한 검사문항의 신뢰도는 0.69이었다. 천문학 태도에 대한 검사는 제일릭 등(Zeilik et at., 1999)이 개발한 천문학태도조사지(the Survey of Attitudes Towards Astronomy, SATA)를 그대로 번역하여 사용하였다. 신뢰도는 0.87이었다. 조사 결과 천문학 기초개념에 대한 한국의 예비교사들의 정답률은 38%이었고 일본은 37%이었지만, 통계적으로 유의미한 차이는 없었다. 천문학에 대한 태도에서는 한국의 초등 예비교사가 일본보다 높았다. 특히 천문학에 대한 인지적 능력과 가치의 범주는 통계적으로 유의미한 차이가 있었다(p<.05). 이 연구를 통해 부가적으로, 한국과 일본의 초등 예비교사들의 가진 천문학 기초개념이 지식의 수준이 40%, 미만이었으며, 천문학에 대한 태도 점수가 미국의 대학생들에 비하여 상당히 낮다는 점을 발견할 수 있었다.

• 천문학회보
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• 제46권1호
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• pp.54.2-54.2
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• 2021

Galaxy clusters are the largest structures in the universe located at the top of the cosmological hierarchical model, so the evolution of the universe can be understood by studying clusters of galaxies. Therefore, finding a larger number of galaxy clusters plays an important role in exploring how the universe evolves. A large number of catalogs for galaxy clusters in the northern sky have been published; however, there are few catalogs in the southern sky due to the lack of wide sky survey data. KMTNet Synoptic Survey of Southern Sky(KS4) project, which observes a wide area of the southern sky about 7000 deg² with KMTNet telescopes for two years, is in progress under the SNU Astronomy Research Center. We use the KS4 multi-wavelength optical data and measure photometric redshifts of galaxies for finding galaxy clusters at redshift z<1. Currently, the KS4 project has observed approximately 33% of the target region, and a pipeline that measures photometric redshifts of galaxies has been created. When the project is completed, we expect to find more than a hundred thousand galaxy clusters, and this will improve the study of galaxy clusters in the southern sky.

• 천문학회보
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• 제46권2호
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• pp.68.2-68.2
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• 2021

Galaxy clusters are the largest structures in the universe located at the top of the cosmological hierarchical model, so the evolution of the universe can be understood by studying clusters of galaxies. Therefore, finding a larger number of galaxy clusters plays an important role in exploring how the universe evolves. A large number of catalogs for galaxy clusters in the northern sky have been published; however, there are few catalogs in the southern sky due to the lack of wide sky survey data. KMTNet Synoptic Survey of Southern Sky(KS4) project, which observes a wide area of the southern sky about 7000 deg² with KMTNet telescopes for two years, is in progress under the SNU Astronomy Research Center. We use the KS4 multi-wavelength optical data and measure photometric redshifts of galaxies for finding galaxy clusters at redshift z<1. Currently, the KS4 project has observed approximately 50% of the target region, and a pipeline that measures photometric redshifts of galaxies has been created. When the project is completed, we expect to find more than a hundred thousand galaxy clusters, and this will improve the study of galaxy clusters in the southern sky.