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20172026
most citedThe Kinematics of Quasar Broad Emission Line Regions Using a Disk-wind Model

20 citations · 29 across the 12 of their papers we have counts for

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Showing astro-ph.GAShow all

7 papers · 1 filter

astro-ph.GA2026

The Actinide-Boost Star LAMOST J122216.85-063345.2: A Detailed R-process Abundance Study with Gemini-S/GHOST

Miji Jeong, Young Sun Lee, Vinicius M. Placco +15

We present a detailed chemical-abundance analysis of an actinide-boost ((Th/Dy) = -0.74) star, LAMOST J122216.85-063345.2 (J1222), a very metal-poor ([Fe/H] = -2.45) halo st…

astro-ph.GA2025

Near-Infrared Spectroscopy with IGRINS-2 for Studying Multiple Stellar Populations in Globular Clusters

Dongwook Lim, Young-Wook Lee, Sol Yun +53

Recent advancements in near-infrared (NIR) spectroscopy have opened new opportunities for studying multiple stellar populations in globular clusters (GCs), particularly for newly d…

astro-ph.GA20197 cited

Determining Quasar Orientation

Suk Yee Yong, Rachel L. Webster, Anthea L. King +3

Since the discovery of active galactic nuclei (AGN) and their subclasses, a unification scheme of AGN has been long sought. Orientation-based unified models predict that some of th…

astro-ph.GA20192 cited

Astro2020 Science White Paper - Quasar Microlensing: Revolutionizing our Understanding of Quasar Structure and Dynamics

Leonidas Moustakas, Matthew O'Dowd, Timo Anguita +20

Microlensing by stars within distant galaxies acting as strong gravitational lenses of multiply-imaged quasars, provides a unique and direct measurement of the internal structure o…

astro-ph.GA2018

HST imaging of four gravitationally lensed quasars

Nicholas F. Bate, Georgios Vernardos, Matthew J. O'Dowd +7

We present new HST WFPC3 imaging of four gravitationally lensed quasars: MG 0414+0534; RXJ 0911+0551; B 1422+231; WFI J2026-4536. In three of these systems we detect wavelength-dep…

astro-ph.GA2018

Using the Properties of Broad Absorption Line Quasars to Illuminate Quasar Structure

Suk Yee Yong, Anthea L. King, Rachel L. Webster +3

A key to understanding quasar unification paradigms is the emission properties of broad absorption line quasars (BALQs). The fact that only a small fraction of quasar spectra exhib…