Broadband SED of Mrk 501 during the two VHE high states observed within the campaign (upper panel: MJD 54 952, lower panel: MJD 54 973). See text for details regarding the included spectral measurements. The data points have been corrected for EBL absorption according to the model by Franceschini et al. (2008). The emission of the host galaxy parameterized according to Silva et al. (1998) is shown with a gray dashed line, while the one-zone SSC model describing the average broadband SED over the entire campaign (see Abdo et al. 2011a) is depicted with a gray solid line.