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Principled Point-source Detection in Collections of Astronomical Images

  • Authors: Dustin Lang, David W. Hogg

Dustin Lang and David W. Hogg 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

The colors of false-positive detections for each method. We generated 100 million samples of Gaussian noise with equal variance for the g and r fluxes. The thresholds for each method were set to produce approximately equal numbers of false positives. Detections in the quadrants with negative fluxes are shown in separate bins, and “stars” with extreme flux ratios are clipped to the color range shown, −1 to +3. The χ2 method generates false positives in all quadrants equally. The ﹩{\chi }_{+}^{2}﹩ method does not generate any both-negative false positives and generates fewer false positives with one negative flux. The SED-matched methods do not generate any false positives with negative r flux and generally produce false positives in accordance with the SEDs they expect to find.

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