Disk Kinematics at High Redshift: DysmalPy’s Extension to 3D Modeling and Comparison with Different Approaches

Disk Kinematics at High Redshift: DysmalPy’s Extension to 3D Modeling and Comparison with Different Approaches

Spatially resolved emission-line kinematics are invaluable for investigating fundamental galaxy properties and have become increasingly accessible for galaxies at z ≳0.5 through sensitive near-infrared imaging spectroscopy and millimeter interferometry. Kinematic modeling is at the core of the analy...

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Bibliographic Details
Main Authors: Lilian L. Lee, Natascha M. Förster Schreiber, Sedona H. Price, Daizhong Liu, Reinhard Genzel, Ric Davies, Linda J. Tacconi, Taro T. Shimizu, Amit Nestor Shachar, Juan M. Espejo Salcedo, Stavros Pastras, Stijn Wuyts, Dieter Lutz, Alvio Renzini, Hannah Übler, Rodrigo Herrera-Camus, Amiel Sternberg
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
High-redshift galaxies
Galaxy kinematics
Galaxy dynamics
Astronomy data analysis
Astronomy data modeling
Online Access:https://doi.org/10.3847/1538-4357/ad90b5
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https://doi.org/10.3847/1538-4357/ad90b5

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