Results 81 to 90 of about 443 (134)
AstroM3: A Self-supervised Multimodal Model for Astronomy
While machine-learned models are now routinely employed to facilitate astronomical inquiry, model inputs tend to be limited to a primary data source (namely images or time series) and, in the more advanced approaches, some metadata.
M. Rizhko, J. S. Bloom
doaj +1 more source
Squeezing Full-shape Dynamical Dark Energy Constraints with Galaxy Alignments
Recent 2 σ –4 σ deviations from the cosmological constant ${\rm{\Lambda }}$ suggest that dark energy (DE) may be dynamical, based on baryon acoustic oscillations and full-shape galaxy clustering (FS GC) analyses.
Junsup Shim +2 more
doaj +1 more source
Formation of the first three gravitational-wave observations through isolated binary evolution. [PDF]
Stevenson S +6 more
europepmc +1 more source
Proceedings of the First Astrostatistics School: Bayesian Methods in Cosmology
Proceedings (in Spanish), supplemental electronic material accessible via links within the PDF. Appears in Cuadernos en Estadistica aplicada, Edicion especial, (2014)
openaire +2 more sources
This new SAS ® tool is two-dimensional color chart for visualizing changes in a population or system over time. Data for one point in time appear as a thin horizontal band of color.
David J Corliss
core
Developments in Approximate Bayesian Computation and Statistical Applications in Astrostatistics [PDF]
The title of this Thesis embraces two topics that have been investigated. Most of the present work is dedicated to develops and extensions for Approximate Bayesian Computation (ABC).
Simola, Umberto
core
Inference for the physical sciences. [PDF]
Jones NS, Maccarone TJ.
europepmc +1 more source
We present a statistical analysis of the extremely bright, apparently nonrepeating fast radio burst FRB 20250316A, detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME), to assess its rarity. Using a model-agnostic framework based on the
Wen-Long Zhang, Jun-Jie Wei
doaj +1 more source
Wide binary stars are important for testing alternative models of gravitation in the weak-field regime and understanding the statistical outcomes of dynamical interactions in the general Galactic field. The Gaia mission’s collection of weakly bound pairs
Valeri V. Makarov
doaj +1 more source

