VizieR Online Data Catalog: Spectroscopy & HST photometry of galaxy Leo V (Mutlu-Pakdil+, 2019)

We have obtained deep optical observations of the candidate debris stream of Leo V, which was identified in ground-based (Magellan/Megacam) data, using the F606W and F814W filters on the Hubble Space Telescope / Advanced Camera for Surveys (HST/ACS; PI:D.Sand).

Spectroscopic data were obtained with the Hectochelle multiobject fiber spectrograph at the Multi Mirror Telescope (MMT). Hectochelle has a 1deg diameter field of view and can achieve ~1km/s velocity precision for high S/N data; the effective resolution for our setup was R~32000. Both data sets were taken with the "RV31" filter in place, giving a spectral range of 5150-5300Å, which contains the prominent Mg-b triplet.

(5 data files).