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The AGEL Survey Data Release 2: A Gravitational Lens Sample for Galaxy Evolution and Cosmology

Authors: Tania M. Barone, Keerthi Vasan G.C., Kim-Vy Tran, Glenn G. Kacprzak, Karl Glazebrook, Tucker Jones, Duncan J. Bowden, Faith Dalessandro, Nandini Sahu, Hannah Skobe, Rebecca J. Allen, A. Makai Baker, Daniel J. Ballard, Yuguang Chen, Thomas E. Collett, Giovanni Ferrami, Jimena González, William Gottemoller, Anishya Harshan, Xiaosheng Huang, Leena Iwamoto, Colin Jacobs, Tesla E. Jeltema, Kaustubh Rajesh Gupta, Geraint F. Lewis, Sebastian Lopez, Themiya Nanayakkara, Nikole M. Nielsen, Jackson O'Donnell, Huimin Qu, Sunny Rhoades, Anowar J. Shajib, Sarah M. Sweet, Nicolas Tejos

Tania M. Barone et al 2026 The Astronomical Journal 171 .

Provider: AAS Journals

Caption: Figure 11.

Comparison of the AGEL spectroscopic sample to other lensing samples. Panel (a) shows the deflector redshifts, (b) the source redshifts (all redshifts spectroscopically confirmed). The AGEL sample spans higher source and deflector redshifts than most previous samples. Panel (c) shows the relationship between source and deflector redshifts, with the Spearman rank-order correlation coefficient for each sample annotated in the bottom right corner. All the samples have p-value< < 0.05 except for SL2S (p = 0.16), implying that SL2S is the only sample in which the source redshift has no statistically significant dependence on the deflector redshift. The gray line in panel (c) shows the one-to-one relation.

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