SIMBAD references

1998PASP..110..727H - Publ. Astron. Soc. Pac., 110, 727-731 (1998/June-0)

A maximum likelihood method to improve faint-source flux and color estimates.

HOGG D.W. and TURNER E.L.

Abstract (from CDS):

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 identified in the image in which it is being photometered. If a source has been identified in other data, the corrections are different; a prescription for calculating the corrections is presented. Implications of these corrections for analyses of surveys are discussed; the most important is that sources identified at signal-to-noise ratios of 4 or less are practically useless.

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