The Impact of Applying Black Hole–Host Galaxy Scaling Relations to Large Galaxy Populations
Supermassive black holes (SMBHs) with dynamically measured masses have shown empirical correlations with host galaxy properties. These correlations are often the only method available to estimate SMBH masses and gather statistics for large galaxy populations across a range of redshifts, even though...
Saved in:
| Main Authors: | Maggie C. Huber, Joseph Simon, Julia M. Comerford |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ade30a |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The ∞ Galaxy: A Candidate Direct-collapse Supermassive Black Hole between Two Massive, Ringed Nuclei
by: Pieter van Dokkum, et al.
Published: (2025-01-01) -
The MASSIVE Survey. XX. A Triaxial Stellar Dynamical Measurement of the Supermassive Black Hole Mass and Intrinsic Galaxy Shape of Giant Radio Galaxy NGC 315
by: Jacob Pilawa, et al.
Published: (2025-01-01) -
Combining Direct Black Hole Mass Measurements and Spatially Resolved Stellar Kinematics to Calibrate the M BH–σ ⋆ Relation of Active Galaxies
by: Nico Winkel, et al.
Published: (2024-01-01) -
Multiwavelength Observations of a Jet Launch in Real Time from the Post-changing-look Active Galaxy 1ES 1927+654
by: Sibasish Laha, et al.
Published: (2025-01-01) -
A JWST View of the Overmassive Black Hole in NGC 4486B
by: Behzad Tahmasebzadeh, et al.
Published: (2025-01-01)