Accounting for Source Uncertainties in Analyses of Astronomical Survey Data
Explore this paper's citation graph
Summary
An issue arising in analyzing data from astronomical surveys: accounting for measurement uncertainties in the properties of individual sources detected in a survey when making inferences about the entire population of sources is discussed.
- Type
- article
- Published
- 2004-09-15
- Cited by
- 117
- References
- 6
- Access
- Open access
- OpenAlex
- https://openalex.org/W1580764193
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:3229314
Keywords
Sample (material), Bayesian probability, Point estimation, Population, Point (geometry)
References
Cited by
- Short versus long gamma-ray bursts: a comprehensive study of energetics and prompt gamma-ray correlations
- OBSCURATION-DEPENDENT EVOLUTION OF ACTIVE GALACTIC NUCLEI
- THE ABSOLUTE MAGNITUDE DISTRIBUTION OF KUIPER BELT OBJECTS
- HIGH ECLIPTIC LATITUDE SURVEY FOR SMALL MAIN-BELT ASTEROIDS
- A derivation of the luminosity function of the Kuiper belt from a broken power-law size distribution
- INFERRING THE ECCENTRICITY DISTRIBUTION
- The Kuiper belt luminosity function from mR = 21 to 26
- A 3D extinction map of the northern Galactic plane based on IPHAS photometry
- Binary Black Hole Mergers in the First Advanced LIGO Observing Run
- Galaxy gas as obscurer: I. GRBs x-ray galaxies and find a N_H ~ M* relation
- Accounting for sample selection in Bayesian analyses
- Hierarchical analysis of gravitational-wave measurements of binary black hole spin–orbit misalignments
- Statistical Methods in Astronomy
- Insights into binary black hole formation from gravtitational waves
- Explaining LIGO's observations via isolated binary evolution with natal kicks
- Linking black hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution
- A gravitational-wave standard siren measurement of the Hubble constant
- Inferences about the distribution, merger rate, and evolutionary processes of compact binaries from gravitational wave observations
- Limits on the number of spacetime dimensions from GW170817
- Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
Related papers
No related papers recorded.