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A Maximum Likelihood Method to Improve Faint‐Source Flux and Color Estimates

A Maximum Likelihood Method to Improve Faint‐Source Flux and Color Estimates

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_26666042

A Maximum Likelihood Method to Improve Faint‐Source Flux and Color Estimates

About this item

Full title

A Maximum Likelihood Method to Improve Faint‐Source Flux and Color Estimates

Publisher

The University of Chicago Press

Journal title

Publications of the Astronomical Society of the Pacific, 1998-06, Vol.110 (748), p.727-731

Language

English

Formats

Publication information

Publisher

The University of Chicago Press

More information

Scope and Contents

Contents

Flux estimates for faint sources or transients are systematically biased high because there are far more truly faint sources than bright. Corrections that account for this effect are presented as a function of signal‐to‐noise ratio and the (true) slope of the faint‐source number‐flux relation. The corrections depend on the source being originally i...

Alternative Titles

Full title

A Maximum Likelihood Method to Improve Faint‐Source Flux and Color Estimates

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_26666042

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_26666042

Other Identifiers

ISSN

0004-6280

E-ISSN

1538-3873

DOI

10.1086/316173

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