We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct
morphological masks of sub-galactic environments based on Spitzer 3.6 μm images. At the …

ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies (S 4 G) is a deep 3.6 and 4.5
μm imaging survey of 2352 nearby (< 40 Mpc) galaxies. We describe the S 4 G data analysis …

The PHANGS collaboration has been building a reference data set for the multiscale,
multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With …

We report on the determination of electron densities, and their impact on the outflow masses
and rates, measured in the central few hundred parsecs of 11 local luminous active …

We present subkiloparsec-scale mapping of the 870 μm ALMA continuum emission in six
luminous (L IR∼ 5× 10 12 L⊙) submillimeter galaxies (SMGs) from the ALESS survey of the …

Spirals in galaxies have long been thought to be caused by gravitational instability in the
stellar component of the disk, but discerning the precise mechanism had proved elusive …

Large-scale bars can fuel galaxy centers with molecular gas, often leading to the
development of dense ringlike structures where intense star formation occurs, forming a very …

THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G): PRECISE STELLAR
MASS DISTRIBUTIONS FROM AUTOMATED DUST CORRECTION AT 3.6 μm - IOPscience …

The central regions of disc galaxies hold clues to the processes that dominate their
formation and evolution. To exploit this, the TIMER project has obtained high signal-to-noise …

I use distance-and mass-limited subsamples of the Spitzer Survey of Stellar Structure in
Galaxies (S4G) to investigate how the presence of bars in spiral galaxies depends on mass …