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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 2.

Magnitude errors plotted vs. magnitudes for the bands in common between DES and FDS, gri. Black dots represent confirmed GCs. The first row of plots refers to FDS PSF photometry data, the second to DES circular aperture photometry, and the third to DES automatic aperture (based on the Kron radius) photometry. For visualization purposes, the magnitude error axes were truncated at a value of 0.6 mag. Errors in FDS data do not exceed 0.6 mag: All FDS data points are visible in these plots.

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