Aims. Fossil record methods based on spectral synthesis techniques have matured during
the past decade, and their application to integrated galaxy spectra has fostered substantial …

I review the spatially resolved spectroscopic properties of low-redshift star-forming galaxies
(and their retired counterparts) using results from the most recent optical integral field …

Context. Over the past decade, 3D optical spectroscopy has become the preferred tool for
understanding the properties of galaxies and is now increasingly used to carry out galaxy …

ABSTRACT We use the Mitchell Spectrograph (formerly VIRUS-P) to observe 12 nearby disk
galaxies. We successfully measure ages in the outer disk in six systems. In three cases …

We measure the radial profile of the 12 CO (1–0) to H 2 conversion factor (X CO) in NGC
628. The Hα emission from the VENGA integral field spectroscopy is used to map the star …

This paper aims to provide aperture corrections for emission lines in a sample of spiral
galaxies from the Calar Alto Legacy Integral Field Area Survey (CALIFA) database. In …

We present optical integral field unit observations of the Taffy system (UGC 12914/15),
named for the radio emission that stretches between the two galaxies. Given that these gas …

The ALFALFA Hα survey utilizes a large sample of HI-selected galaxies from the ALFALFA
survey to study star formation in the local universe. ALFALFA Hα contains 1555 galaxies …

Telescopes with a primary aperture of 8m or more pepper the mountains of both
hemispheres and give us eyes to observe back to the beginnings of the Universe. Bigger is …