Results 81 to 90 of about 1,066 (128)
Glitches and Glitching Clusters in Rotation-powered Pulsars
The study of pulsar glitch phenomena serves as a valuable probe into the dynamic properties of matter under extreme high-density conditions, offering insights into the physics within neutron stars.
Pei-Xin Zhu, Xiao-Ping Zheng
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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)
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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
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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
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The next decade of astroinformatics and astrostatistics
Over the past century, major advances in astronomy and astrophysics have been largely driven by improvements in instrumentation and data collection. With the amassing of high quality data from new telescopes, and especially with the advent of deep and large astronomical surveys, it is becoming clear that future advances will also rely heavily on how ...
Siemiginowska, Aneta +51 more
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Formation of the first three gravitational-wave observations through isolated binary evolution. [PDF]
Stevenson S +6 more
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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
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Inference for the physical sciences. [PDF]
Jones NS, Maccarone TJ.
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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
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