Na minha lista:
Detalhes bibliográficos
Principais autores: Chang, Seo-Won, Im, Myungshin, Jeong, Mankeun, Kim, Joonho, Park, Bomi, Lee, Jaewon, Buckley, David A. H., Cooke, Jeff, Jung, Sungho, Kim, Dong-Jin, Kim, Ji Hoon, Kim, Yongjung, Lee, Chung-Uk, Lee, Seong-Kook, Paek, Gregory S. H., Shin, Jiseop
Formato: Preprint
Publicado em: 2026
Assuntos:
Acesso em linha:https://arxiv.org/abs/2603.28089
Tags: Adicionar Tag
Sem tags, seja o primeiro a adicionar uma tag!
_version_ 1866914431533842432
author Chang, Seo-Won
Im, Myungshin
Jeong, Mankeun
Kim, Joonho
Park, Bomi
Lee, Jaewon
Buckley, David A. H.
Cooke, Jeff
Jung, Sungho
Kim, Dong-Jin
Kim, Ji Hoon
Kim, Yongjung
Lee, Chung-Uk
Lee, Seong-Kook
Paek, Gregory S. H.
Shin, Jiseop
author_facet Chang, Seo-Won
Im, Myungshin
Jeong, Mankeun
Kim, Joonho
Park, Bomi
Lee, Jaewon
Buckley, David A. H.
Cooke, Jeff
Jung, Sungho
Kim, Dong-Jin
Kim, Ji Hoon
Kim, Yongjung
Lee, Chung-Uk
Lee, Seong-Kook
Paek, Gregory S. H.
Shin, Jiseop
contents 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$^{\circ}$ < Decl. < -28.8$^{\circ}$ in the $B$, $V$, $R$, and $I$ 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 $\sim$4,000 deg$^{2}$ to enable a broad range of astrophysical research. The release includes deep co-added images reaching median 5$σ$ depths of 22.0-23.5 AB mag. It is accompanied by two source catalogs containing over 200 million sources with SNR $>5$: an $I$-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 $+0.054 \pm 0.129$ arcsec in RA and $-0.015 \pm 0.120$ arcsec in Dec relative to Gaia DR3. {\refbf Photometric uniformity for point sources is maintained within $\pm 0.03$ 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.
format Preprint
id arxiv_https___arxiv_org_abs_2603_28089
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle KMTNet Synoptic Survey of Southern Sky III: The First Data Release
Chang, Seo-Won
Im, Myungshin
Jeong, Mankeun
Kim, Joonho
Park, Bomi
Lee, Jaewon
Buckley, David A. H.
Cooke, Jeff
Jung, Sungho
Kim, Dong-Jin
Kim, Ji Hoon
Kim, Yongjung
Lee, Chung-Uk
Lee, Seong-Kook
Paek, Gregory S. H.
Shin, Jiseop
Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
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$^{\circ}$ < Decl. < -28.8$^{\circ}$ in the $B$, $V$, $R$, and $I$ 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 $\sim$4,000 deg$^{2}$ to enable a broad range of astrophysical research. The release includes deep co-added images reaching median 5$σ$ depths of 22.0-23.5 AB mag. It is accompanied by two source catalogs containing over 200 million sources with SNR $>5$: an $I$-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 $+0.054 \pm 0.129$ arcsec in RA and $-0.015 \pm 0.120$ arcsec in Dec relative to Gaia DR3. {\refbf Photometric uniformity for point sources is maintained within $\pm 0.03$ 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.
title KMTNet Synoptic Survey of Southern Sky III: The First Data Release
topic Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2603.28089