We present the first public data release (DR1) of the KMTNet Synoptic Survey of Southern Sky (KS4). This deep, wide-field imaging survey covers a southern footprint of −85<sup>◦</sup> < Decl. < −28.8<sup>◦</sup> i...

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https://www.riss.kr/link?id=A110254247
장서원 (서울대학교 기초과학연구원) ; 임명신 (서울대학교) ; 정만근 (서울대학교) ; 김준호 (Daegu National Science Museum) ; 박보미 (서울대학교) ; 이재원 (서울대학교) ; David A. H. Buckley (University of Cape Town) ; Cooke Jeff (Swinburne University of Technology) ; 정성호 (서울대학교) ; 김동진 (한국천문연구원) ; 김지훈 (서울대학교) ; 김용정 (세종대학교) ; 이충욱 (한국천문연구원) ; 이성국 (서울대학교) ; 백승학 (서울대학교) ; 신지섭 (서울대학교)
2026
English
KCI등재,SCIE,SCOPUS
학술저널
179-198(20쪽)
0
상세조회0
다운로드다국어 초록 (Multilingual Abstract)
We present the first public data release (DR1) of the KMTNet Synoptic Survey of Southern Sky (KS4). This deep, wide-field imaging survey covers a southern footprint of −85<sup>◦</sup> < Decl. < −28.8<sup>◦</sup> i...
We present the first public data release (DR1) of the KMTNet Synoptic Survey of Southern Sky (KS4). This deep, wide-field imaging survey covers a southern footprint of −85<sup>◦</sup> < Decl. < −28.8<sup>◦</sup> in the <i>B</I>, <i>V</i> , <i>R</i>, and <I>I</I> bands using a network of three 1.6-m telescopes. Although primarily designed to secure reference imaging for gravitational wave counterpart identification, DR1 delivers science-ready data for ∼4,000 deg<sup>2</sup> to enable a broad range of astrophysical research. The release includes deep co-added images reaching median 5σ depths of 22.0–23.5 AB mag. It is accompanied by two source catalogs containing over 200 million sources with SNR > 5: an <i>I</I>-band-selected forced-photometry catalog optimized for consistent colors, and a band-merged catalog offering enhanced completeness. Validation demonstrates robust data quality, characterized by mean astrometric offsets of +0.054 ± 0.129 arcsec in RA and −0.015 ± 0.120 arcsec in Dec relative to Gaia DR3. Photometric uniformity for point sources is maintained within ±0.03 mag relative to Gaia XP for 97.5–99.8% of the footprint across all four bands. A key advantage of KS4 is its uniform and contiguous spatial coverage. It extends to fainter magnitudes than other uniform surveys while filling irregular gaps in existing deep datasets. All data products are publicly available via the CDS and NOIRLab’s Astro Data Lab.
KMTNet Synoptic Survey of Southern Sky II: Data Reduction and Real-Time Transient Detection Pipeline
Weak Lensing Spectrotomography: A1767 and A2065
SOLO: Wide-Field Asteroid Light Curve Monitoring System for SPHEREx
SQUIDPOL: Seoul National University QUadruple Imaging Device for POLarimetry