Measuring Scaling Relations: Fitting Technique Matters
Scaling relationships, both integrated and spatially resolved, arise owing to the physical processes that govern galaxy evolution and are frequently measured in both observed and simulated data. However, the accuracy and comparability of these measurements are hindered by various differences between...
Saved in:
| Main Authors: | Bryanne McDonough, Olivia Curtis, Tereasa G. Brainerd |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/ade13c |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
by: Bryanne McDonough, et al.
Published: (2024-01-01) -
Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
by: Yanzhe Zhang, et al.
Published: (2025-01-01) -
Effects of Galactic Environment on Size and Dark Matter Content in Low-mass Galaxies
by: Francisco J. Mercado, et al.
Published: (2025-01-01) -
MSA-3D: Dissecting Galaxies at z ∼ 1 with High Spatial and Spectral Resolution
by: Ivana Barišić, et al.
Published: (2025-01-01) -
Spatial Variations of Stellar Elemental Abundances in FIRE Simulations of Milky Way-mass Galaxies: Patterns Today Mostly Reflect Those at Formation
by: Russell L. Graf, et al.
Published: (2025-01-01)