Supplementary material for Shivaei, Alberts, Florian et al. (2024): A new census of dust and polycyclic aromatic hydrocarbons at z=0.7-2 with JWST MIRI

Supplementary data and figure for the paper Shivaei, Alberts, Florian, et al. (2024).

The table includes the properties of the robust PAH fraction (qpah) sample in Shivaei et al. (2024), as described in Section 2.2. The table contains:
# ID: source ID from the SMILES internal v0.3 version catalog
# z_red: redshift
# qpah and qpah_err: PAH fraction and its uncertainty 
# mass and mass_err: stellar mass and its error in solar mass units
# logoh_fmr and logoh_fmr_err: metallicity or 12+log(O/H) calculated from the fundamental metalllicity relation of Sanders et al. (2021) and its error (as plotted in Figures 8 and 9 in Shivaei et al. (2024)) 
# logoh_mzr and logoh_mzr_err: metallicity or 12+log(O/H) calculated from the mass-metallicity relation (MZR) of Topping et al. (2021) and its error (as plotted in Figure 7 in Shivaei et al. (2024))

The figure shows a few examples of the SED fits to the HST, JWST/NIRCam, and JWST/MIRI photometry at z=0.7-2.0, described in Section 2.3 of the paper. The symbols are the same as in Figure 6 of the paper. The 14 objects shown here are randomly selected from the robust-qpah sample and sorted based on their redshift from top-left to bottom-right.