most citedSDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula

3 citations · 3 across the 2 of their papers we have counts for

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astro-ph.GA2025

Danger Zone: Establishing Buffers for Enhanced Classification in BPT Diagrams

Changhyun Cho, Ahmad Nemer, Ivan Yu. Katkov +1

This study utilizes unsupervised machine learning, specifically the uniform manifold approximation and projection (UMAP) algorithm, to classify optical spectra originating from sta…

astro-ph.GA20253 cited

SDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula

Natascha Sattler, J. Eduardo Méndez-Delgado, Kathryn Kreckel +18

The chemical abundance of the interstellar medium sets the initial conditions for star formation and provides a probe of chemical galaxy evolution models. However, unresolved inhom…

astro-ph.GA2024

Analyzing the Abundance Discrepancy Problem in HII Regions with Photoionization Modeling

Ahmad Nemer, J. E. Mendez-Delgado, Natascha Sattler +5

Understanding the complex ionization structure and chemical composition of \hii\ regions poses a significant challenge in astrophysics. The abundance discrepancy problem, character…

astro-ph.GA2024

A closer look at the origin of LINER emission and its connection to evolved stars with a machine learning classification scheme

Ahmad Nemer, Ivan Katkov, Jospeh Gelfand +1

Identifying the dominant ionizing sources in galaxies is essential for understanding their formation and evolution. Traditionally, spectra are classified based on their dominant io…

astro-ph.GA2024

Excitation mechanisms of C II optical permitted lines in ionized nebulae

E. Reyes-Rodríguez, J. E. Méndez-Delgado, J. García-Rojas +4

Context. Carbon is the fourth most abundant element in the universe and its distribution is critical to understanding stellar evolution and nucleosynthesis. In optical studies of i…