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Fig. 4

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Examples of best-fit solutions assuming a SMC extinction law for 6 sources covering a wide range of magnitudes (~20  ≤ m678 ≤  ~ 23.5) and spectroscopic redshifts (0.7 ≤ z ≤ 2.3). Each panel includes the observed photometry, associated errors, and FWHM for each of the 23 ALHAMBRA filter set (black dots, vertical and horizontal error bar respectively). Photometric upper limits are indicated by arrows. The continuous line shows the best-fit solution, while the open circles give the expected magnitude from the model corrected from systematic offsets. Additional info for each source includes: model name, reduced χ2, amount of extinction, the normalized probability distribution as a function of z (Pdz), the spectro-z (and its source catalog), and the best-fit photo-z solution. The title of each panel is labeled with the source ID in the ALHAMBRA catalog and the measured magnitude in the m678 filter (green dot).

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