Stars on the ascending helium giant branch - I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948

Open Access

Fig. A.2.

SED fitting performed using photometry from the following surveys covering the UV to infrared range: the HST/STIS spectrum, Gaia XP spectra, and G/G_BP/G_RP photometry (Gaia Collboration 2022); VISTA (Cioni et al. 2011; McMahon et al. 2013); VST (Shanks et al. 2015); Skymapper (Onken et al. 2024); DENIS (DENIS Consortium 2005); 2MASS (Cutri et al. 2003); and WISE (Cutri et al. 2021; Schlafly et al. 2019; Marocco et al. 2020).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.