activity
20222026
most citedNLTE abundances of Eu for a sample of metal-poor stars in the Galactic Halo and Metal-poor Disk with 1D and <3D> models

7 citations · 19 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

The -Process Alliance: On J00101735, an Accreted, Chemically Unusual, Metal-poor Star with -process Enhancement

Zoe Hackshaw, Rana Ezzeddine, Shivani P. Shah +11

We present a detailed chemo-dynamical analysis of the chemically peculiar very metal-poor ([Fe/H]) Milky Way (MW) halo star, 2MASS J001017581735387 (hereafter J0…

astro-ph.GA2026

Enhancing Photometric Redshift Estimation for LSST with a Hybrid LSTM-Mixture Density Network

Zhijian Luo, Yangyang Li, Xinyu Luo +4

Accurate photometric redshift (photo-) estimation and robust uncertainty quantification are essential for the LSST to achieve its precision cosmology goals. Traditional machine…

astro-ph.GA2026

Beyond Colors: Probing Redshifts from Galaxy Morphology in Single-band Images with ViT-MDNz

Zhijian Luo, Yangyang Li, Jianzhen Chen +5

To address the challenge of estimating redshifts when only single-band images are available, this study introduces a deep learning model named ViT-MDNz. Leveraging robust statistic…

astro-ph.GA2025

BALNet: Deep Learning-Based Detection and Measurement of Broad Absorption Lines in Quasar Spectra

Yangyang Li, Zhijian Luo, Shaohua Zhang +5

Broad absorption line (BAL) quasars serve as critical probes for understanding active galactic nucleus (AGN) outflows, black hole accretion, and cosmic evolution. To address the li…

astro-ph.SR2025

Investigating non-LTE abundances of Neodymium (Nd) in metal-poor FGK stars

John D. Dixon, Rana Ezzeddine, Yangyang Li +3

The dominant site(s) of the -process are a subject of current debate. Ejecta from -process enrichment events like kilonovae are difficult to directly measure, so we must inst…

astro-ph.SR2024★ 7 cited

NLTE abundances of Eu for a sample of metal-poor stars in the Galactic Halo and Metal-poor Disk with 1D and <3D> models

Yanjun Guo, Nicholas Storm, Maria Bergemann +6

Accurate measurements of europium abundances in cool stars are essential for an enhanced understanding of the r-process mechanisms. We measure the abundance of Eu in solar spectra…

astro-ph.SR2022★ 5 cited

Discovery of a Metal-Poor Red Giant Star with the Highest Ultra-Lithium Enhancement

Jeremy Kowkabany, Rana Ezzeddine, Corinne Charbonnel +10

We present the discovery of 2MASS J05241392-0336543 (hereafter J0524-0336), a very metal-poor ([Fe/H]=-2.43 +- 0.16), highly r-process-enhanced ([Eu/Fe]= +1.34 +- 0.10) Milky Way h…

astro-ph.SR2022★ 7 cited

LOTUS: A (non-)LTE Optimization Tool for Uniform derivation of Stellar atmospheric parameters

Yangyang Li, Rana Ezzeddine

Precise fundamental atmospheric stellar parameters and abundance determination of individual elements in stars are important for all stellar population studies. Non-Local Thermodyn…