arXiv (All)
open access
Combining Multiple Incomplete Astronomical Surveys to Estimate Galaxy Flux Distributions
In astrophysics, the distributions of fluxes or intensities of populations of sources provide insight into the structure and evolution of the universe. We propose a science-driven hierarchical Bayesian framework to estimate the X-ray flux distribution of a population of galaxies. The distribution is
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- The constrainability of galaxy positions in the $M_*$ -- SFR plane from SED fitting#1000412
- The Role of the Cosmic Web in Galaxy Evolution Across 0.4<z<4#1217085
- Identification of low redshift groups and clusters of galaxies in the X-CLASS survey and the X-ray luminosity-temperature relation#398732
- Markov Chain Monte Carlo for Bayesian Parametric Galaxy Modeling in LSST#1155009
- Investigating the Young Stellar Populations and Hierarchies in Nearby Galaxies with the UVIT. III. Evidence for a Largest Scale of Correlated Stellar Structures and a Non-universal Fractal Dimension#821050
Record · ID 1488647
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive