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The Contribution of the Color Space in LSST-like Photometry for the Selection of Extragalactic Globular Cluster Candidates

  • Authors: Nicholas Schweder-Souza, Ana L. Chies-Santos, Rafael S. de Souza, Kristen C. Dage, Charles J. Bonatto, Juan P. Caso, Michele Cantiello, Pedro dos Santos-Lopes, Pedro Floriano, Thayse A. Pacheco, Katherine L. Rhode, Pauline Barmby, Jennifer Sobeck, Ana I. Ennis, Yasna Ordenes-Briceño, Teymoor Saifollahi, Julia Gschwend, Niranjana P., Rubens E. G. Machado

Nicholas Schweder-Souza et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 9.

ΔmagFDS−DES vs. g, r, iFDS: the difference in magnitude for the same source, in the same band, but in different surveys against the FDS magnitude in the same band. The first row displays the plots where DES MAG_APER_5 (2﹩\mathop{.}\limits^{\unicode{x02033}}﹩92) data were used, the second DES MAG_APER_4 (1﹩\mathop{.}\limits^{\unicode{x02033}}﹩92), and the third DES MAG_AUTO. Black points denote foreground stars selected via Criterion (2), as in Section 2.2. The horizontal black line is y = 0.

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