From these data, Trinity infers the average SMBH mass, SMBH accretion rate, merger rate, and Eddington ratio distribution as functions of halo mass, galaxy stellar mass, and redshift.
Astrophysics of Galaxies
Gaussian processes (GPs) are commonly used as a model of stochastic variability in astrophysical time series.
Instrumentation and Methods for Astrophysics Earth and Planetary Astrophysics Solar and Stellar Astrophysics Data Analysis, Statistics and Probability
The HI T-RECS model is based on the most recent HI mass function estimates, combined with prescriptions to convert HI mass to total integrated HI flux.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
As a proof of concept, the proposed methodology is applied to twelve single-line spectroscopic binaries with astrometric data that lacked a joint astrometric-spectroscopic solution, for which we provide full orbital elements.
Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics Computational Physics Data Analysis, Statistics and Probability
We discuss the approach used for this dataset, the choice for a suitable architecture, particularly the use of a network with two branches to work with images in different resolutions, and its optimization.
Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
We present an auto-differentiable spectral modeling of exoplanets and brown dwarfs.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics
In Very Long Baseline Interferometry (VLBI), signals from multiple antennas combine to create a sparsely sampled virtual aperture, its effective diameter determined by the largest antenna separation.
Instrumentation and Methods for Astrophysics Astrophysics of Galaxies Optimization and Control
By modeling the misalignment between galaxies and their host halo, we show that the 3-dimensional two-point position and orientation correlation functions of simulated (sub)halos and galaxies can be accurately reproduced from quasi-linear scales down to $0. 1~h^{-1}{\rm Mpc}$.
Cosmology and Nongalactic Astrophysics
In this work, we explore the usage of Vision Transformer (ViT) for galaxy morphology classification for the first time.
Astrophysics of Galaxies
However, subcritically spinning configurations with mean density of less than a few times nuclear saturation density yield a significantly thermally enhanced mass.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology