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DETECT: A Pipeline to Quantify Detection Thresholds in Rubin for Nearby Targets Embedded in Bright Host Galaxies

  • Authors: Tobias Géron, Maria R. Drout, W. V. Jacobson-Galán, C. D. Kilpatrick

Tobias Géron et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 5.

The blue region in the left panel shows the locations in the host galaxy where the flux in the template is within 5% of the flux in the template at the SN location. The red cross shows the location of SN 2025brs. The right panel shows the distribution of fluxes that are found by performing forced photometry on the difference image at all of these locations. The dashed vertical line indicates the median of this distribution, which is equal to 863 ± 353 nJy.

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