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The S-PLUS Fornax Project (S+FP): Mapping Globular Clusters Systems within 5 Virial Radii around NGC 1399

  • Authors: Luis Lomelí-Núñez, A. Cortesi, A. V. Smith Castelli, M. L. Buzzo, Y. D. Mayya, Vasiliki Fragkou, J. A. Alzate-Trujillo, R. F. Haack, J. P. Calderón, A. R. Lopes, Michael Hilker, M. Grossi, Karín Menéndez-Delmestre, Thiago S. Gonçalves, Ana L. Chies-Santos, L. A. Gutiérrez-Soto, Ciria Lima-Dias, S. V. Werner, Pedro K. Humire, R. C. Thom de Souza, A. Alvarez-Candal, Swayamtrupta Panda, Avinash Chaturvedi, E. Telles, C. Mendes de Oliveira, A. Kanaan, T. Ribeiro, W. Schoenell

Luis Lomelí-Núñez et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 5.

Left panel: example of one completeness curve in the i band for the s27s34 field. The horizontal blue dashed line represents the completeness at the 50% and 90% levels. Center panel: distribution of i﹩{}_{{\mathrm{mag}}_{50}}﹩ magnitudes recovered for all of the Fornax pointings. The vertical black dashed line represents the mean value of the distribution. Right panel: completeness tests for mock sources with different Gaussian profile sizes: ﹩0\mathop{.}\limits^{^{\prime\prime} }55﹩ (black curve), ﹩1\mathop{.}\limits^{^{\prime\prime} }65﹩ (red curve), ﹩2\mathop{.}\limits^{^{\prime\prime} }75﹩ (green), and ﹩5\mathop{.}\limits^{^{\prime\prime} }5﹩ (yellow curve).

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