C. J. Walcher

TL;DR: In this paper, the extinction-corrected H$\alpha$ star formation rate (SFR) of the different morphological components that shape galaxies (bulges, bars, and disks) was estimated using a multi-component photometric decomposition based on SDSS imaging to CALIFA Integral Field Spectroscopy data.

TL;DR: In this paper, the authors compare the relation between age and alpha-element abundances for stars in the solar neighborhood to that of local, early-type galaxies and find both relations to be very similar.

TL;DR: In this article, the angular diameter-redshift and Hubble diagrams are applied to the same sample of objects (i.e., velocity selected galactic discs) to derive a characteristic chart, the cosmology-evolution diagram, mapping the relation between global cosmological parameters and local structural parameters of discs such as size and luminosity.

TL;DR: WEAVE as discussed by the authors is a massively multiplexed spectroscopic survey facility for the William Herschel Telescope that will see first light in late 2022, and consists of a 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable integral field units (IFUs), and a single large IFU.

TL;DR: In this paper, a combined analysis of SDSS imaging and CALIFA integral field spectroscopy data was performed to detect star-forming spiral-arm-like features in the periphery of three nearby early-type galaxies.