VizieR Online Data Catalog: NGC 330 seen by MUSE (Bodensteiner+, 2020)

NGC 330 was observed with MUSE in wide-field mode (WFM) with adaptive optics (AO) on 19 November 2018 at Yepun, one of the four Unit Telescopes of the VLT in Paranal, Chile. MUSE is an integral-field spectrograph comprising 24 individual spectrographs. The observations were carried out in the extended wavelength mode covering a broad optical range (i.e., 4600Å-9300Å). The spectral resolving power ranges from 2000 at 4600Å to 4000 at 9300Å. Spectra were extracted for all stars brighter than 18.5 in V. Their positions are based on an input list from archival HST data which provides better spatial resolution and thus more accurate stellar positions.

(1 data file).