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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Veröffentlicht in:	The Astrophysical journal 2025-01, Vol.978 (1), p.14
Hauptverfasser:	Lee, Lilian L., Förster Schreiber, Natascha M., Price, Sedona H., Liu, Daizhong, Genzel, Reinhard, Davies, Ric, Tacconi, Linda J., Shimizu, Taro T., Nestor Shachar, Amit, Espejo Salcedo, Juan M., Pastras, Stavros, Wuyts, Stijn, Lutz, Dieter, Renzini, Alvio, Übler, Hannah, Herrera-Camus, Rodrigo, Sternberg, Amiel
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Astronomy data analysis Astronomy data modeling Dispersion Emission analysis Galactic rotation Galaxies Galaxy dynamics Galaxy kinematics High-redshift galaxies Infrared analysis Infrared imaging Interferometry Kinematics Near infrared radiation Parameter sensitivity Red shift Rotating disks Signal to noise ratio Spectroscopy Star formation Stars & galaxies Velocity
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