Interferometric evidence for quantum heated particles in the inner region of protoplanetary disks around Herbig stars

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Table B.1

Stellar and extended fluxes from Fig. 2

Object	f_h	σ_{f_h}	f_s	σ_{f_s}	Field of view [au]

HD 31648	0.01	0.008	0.37	0.050	26
HD 34282	0.07	0.041	0.33	0.050	80
HD 95881	0.04	0.005	0.27	0.022	24
HD 97048	0.05	0.001	0.43	0.031	36
HD 100453	0.11	0.005	0.58	0.002	23
HD 100546	0.10	0.013	0.47	0.010	21
HD 139614	0.06	0.009	0.54	0.018	28
HD 141569	0.01	0.005	0.84	0.069	20
HD 142527	0.03	0.008	0.42	0.011	29
HD 144432	0.00	0.003	0.43	0.017	29
HD 163296	0.01	0.005	0.25	0.009	24
HD 169142	0.08	0.005	0.72	0.027	29
MWC297	0.01	0.008	0.11	0.001	50
HD 179218	0.03	0.021	0.58	0.003	48

Notes. For each object shown in Fig. 2, we list the stellar flux f_s, the extended flux, f_h and their 1σ errors as calculated by Lazareff et al. (2017) using a geometric model. We also give the size of the PIONIER field of view in au. The distances for each object are from Acke & van den Ancker (2004).

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