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Lens Model Accuracy in the Expected LSST Lensed AGN Sample

  • Authors: Padmavathi Venkatraman, Sydney Erickson, Phil Marshall, Martin Millon, Philip Holloway, Simon Birrer, Steven Dillmann, Xiangyu Huang, Sreevani Jaragula, Ralf Kaehler, Narayan Khadka, Grzegorz Madejski, Ayan Mitra, Kevil Reil, Aaron Roodman

Padmavathi Venkatraman et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

OM10-cosmoDC2 mapping. We “paint on” host galaxies from the cosmoDC2 catalog (outlined in Section 2.1.3) to systems in the OM10 catalog (outlined in Section 2.1). Nearest neighbor mapping: to obtain a mapping between the two catalogs, we map AGN in OM10 to AGN in cosmoDC2 using their redshift and absolute magnitude and use their corresponding host galaxy. Left panel: the red OM10 systems are mapped to the blue cosmoDC2 systems. The blue points are a subset of the gray points. Middle panel: we demonstrate the scatter of the OM10-cosmoDC2 system mapping along the AGN redshift axis. Right panel: we demonstrate the scatter of the OM10-cosmoDC2 system mapping along the AGN i-band absolute brightness (AB mag) axis.

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