output
19922026
most citedAGATA - Advanced Gamma Tracking Array

469 citations

Showing astro-ph.GAShow all

83 papers · 1 filter

astro-ph.GA2026

Dynamical Evolution of The Open Clusters Collinder 110 and NGC 2477

Zahra Al, Yüksel Karataş, Forough Rajaei

Using Gaia DR3 photometric and astrometric data, we identified the likely members of the open clusters Collinder 110 and NGC 2477, and derived their astrophysical and dynamical par…

astro-ph.GA2025★ 1 cited

Photometrically Selected Protocluster Candidates at z~9-10 in the JWST COSMOS-Web field

Cossas K. -W. Wu, Chih-Teng Ling, Tomotsugu Goto +8

High-redshift protoclusters are crucial for understanding the formation of galaxy clusters and the evolution of galaxies in dense environments. The James Webb Space Telescope (JWST…

astro-ph.GA2025★ 1 cited

Constraining Lens Masses in Moderately to Highly Magnified Microlensing Events from Gaia

U. Pylypenko, Ł. Wyrzykowski, P. J. Mikołajczyk +57

Microlensing events provide a unique way to detect and measure the masses of isolated, non-luminous objects, particularly dark stellar remnants. Under certain conditions, it is pos…

astro-ph.GA2025★ 13 cited

Study of Open Star Clusters Using the Gaia DR3: I- Poorly Studied King 2 and King 5

Aly Haroon, Waleed Elsanhoury, Essam Elkholy +2

In this study, we utilize photometric and kinematic data from \textit{Gaia} DR3 and the {\sc ASteCA} package to analyze the sparsely studied open clusters, King 2 and King 5. For K…

astro-ph.GA2023★ 1 cited

Astrophysical Parameters of the Open Cluster Berkeley 6

S. Koc, T. Yontan

In this study, the structural and basic astrophysical parameters of the poorly studied open cluster Berkeley 6 are calculated. Analyses of the cluster are carried out using the thi…

astro-ph.GA2023★ 10 cited

Study of the Open Clusters in Kepler Prime Field

Yüksel Karataş, Hikmet Çakmak, İnci Akkaya Oralhan +3

We present a detailed study of NGC 6791, NGC 6811, NGC 6819 and NGC 6866, the four open clusters that are located in the Kepler prime field. We use new CCD UBV(RI)KC photometry, wh…