Mapping the core of the Tarantula Nebula with VLT-MUSE. III. A template for metal-poor starburst regions in the visual and far-ultraviolet

Cumulative optical (VLT/MUSE) and far-ultraviolet (mix of HST empirical and ULLYSES templates) spectrum of NGC2070 (2x2 arcmin^2) presented in Figures 2 and 4, respectively, of Crowther & Castro (MNRAS in press, https://arxiv.org/abs/2311.07642) which should be cited if either dataset is used. 
Contents:
MUSE.dat (ascii format, column 1 wavelength in Angstrom, column 2 flux in erg/s/cm^2/Ang). Further details of MUSE dataset is described in N. Castro et al. (2018 A&A 614 A147)
ULLYSES.dat (ascii format, column 1 wavelength in Angstrom, column 2 flux in erg/s/cm^2/Ang, some detector gaps). Further details of ULLYSES survey is described in R. Roman-Duval et al. (2020, Research Notes of AAS, 4, 205)