Measuring the baryonic Tully-Fisher relation below the detection threshold
We present a novel 2D flux density model for observed H i emission lines combined with a Bayesian stacking technique to measure the baryonic Tully-Fisher relation below the nominal detection threshold. We simulate a galaxy catalogue, which includes H i lines described with either Gaussian or busy fu...
Huvudupphovsmän: | Pan, H, Jarvis, MJ, Ponomareva, AA, Santos, MG, Allison, JR, Maddox, N, Frank, BS |
---|---|
Materialtyp: | Journal article |
Språk: | English |
Publicerad: |
Oxford University Press
2021
|
Liknande verk
Liknande verk
-
MIGHTEE-H I: the baryonic Tully–Fisher relation over the last billion years
av: Ponomareva, AA, et al.
Publicerad: (2021) -
From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully–Fisher relation
av: Ponomareva, A, et al.
Publicerad: (2017) -
Measuring the H I mass function below the detection threshold
av: Pan, H, et al.
Publicerad: (2019) -
The Baryonic Tully–Fisher Relation. II. Stellar Mass Models
av: Francis Duey, et al.
Publicerad: (2025-01-01) -
The Baryonic Tully–Fisher Relation. I. WISE/Spitzer Photometry
av: Francis Duey, et al.
Publicerad: (2024-01-01)