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Bayesian SED-matched source detection with a si...
The benefit of constructing a detection map vs....
The effect of the flux prior in Bayesian SED-ma...
Bayesian SED-matched source detection with a th...
Decision boundaries in signal-to-noise space fo...
Detection rates for the χ2-based and SED-matche...
Relative strengths of the different SED-matched...
Bayesian SED-matched detection method compared ...
Sources detected by the different methods. On t...
Left: a 600 × 600 pixel zoom-in of a tiny fract...
The colors of false-positive detections for eac...
The effect of the flux prior on the decision bo...
Sources that are most strongly detected by each...
Sources detected by the various methods. On the...
Sources detected by each method. On the diagona...
Galaxy detection. Left: detections from an exte...
The 3D magnetic field projections of AR 11158 a...
Schematic of the GC-UNO architecture and the U-...
Comparison of observations of the SDO/AIA 131 Å...
Comparison of magnetic energy between GC-UNO an...
Comparison of results from GC-UNO with observat...
(a) The distributions of SN–host angular separa...
The SPLASH pipeline architecture. When an SN al...
The real vs. predicted values of the stellar ma...
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