Highly structured models for spectral analysis in high-energy astrophysics
From MaRDI portal
Publication:2503928
DOI10.1214/088342304000000314zbMath1100.62637OpenAlexW2102600093MaRDI QIDQ2503928
Publication date: 22 September 2006
Published in: Statistical Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1214/088342304000000314
EM algorithmMarkov chain Monte Carlospectral analysismissing datadata augmentationPoisson modelBayesian methodsposterior predictive checksnonignorable missing dataAstrostatisticspileupthe Chandra X-Ray Observatory
Bayesian inference (62F15) Applications of statistics to physics (62P35) Statistical astronomy (85A35)
Related Items (2)
Detecting abrupt changes in the spectra of high-energy astrophysical sources ⋮ Cross-fertilizing strategies for better EM mountain climbing and DA field exploration: a graphical guide book
Cites Work
- Bayesianly justifiable and relevant frequency calculations for the applied statistician
- Posterior predictive \(p\)-values
- Sampling-Based Approaches to Calculating Marginal Densities
- The Calculation of Posterior Distributions by Data Augmentation
- Statistical analysis of finite mixture distributions
- Deconvolution in high-energy astrophysics: science, instrumentation, and methods
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
This page was built for publication: Highly structured models for spectral analysis in high-energy astrophysics