Astrophysical: Galaxies

  • Publication
    Mid-IR galaxy morphology from S4G (Buta+,
    The goals of the S4G project are described by Sheth et al. (2010, submitted). (1 data file).
  • Publication
    MIGHTEE-H I: H I galaxy properties in the large-scale structure environment at z 0.37 from a stacking experiment
    We present the first measurement of H I mass of star-forming galaxies in different large scale structure environments from a blind survey at z ~ 0.37. In...
  • Publication
    MIGHTEE-H I: possible interactions with the galaxy NGC 895
    The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (H I) is an excellent way to trace...
  • Publication
    Mild radial variations of the stellar IMF in the bulge of M31
    Using new, homogeneous, long-slit spectroscopy in the wavelength range from ~0.35 to $\sim 1 \, \mu$m, we study radial gradients of optical and near-infrared...
  • Publication
    Mild Velocity Dispersion Evolution of massive galaxies since z~2
    Making use of public spectra from Cimatti et al. (2008), we measure for the first time the velocity dispersion of spheroid-like massive (M* ~ 1011M&sun;)...
  • Publication
    Mild Velocity Dispersion Evolution of Spheroid-Like Massive Galaxies Since z ~ 2
    Making use of public spectra from Cimatti et al., we measure for the first time the velocity dispersion of spheroid-like massive (M sstarf ~ 1011 M sun)...
  • Publication
    MILES base models & new line index system (Vazdekis+, 2010)
    We present synthetic spectral energy distributions (SEDs) for single-age, single-metallicity stellar populations (SSPs) covering the full optical spectral range...
  • Publication
    MILES extended: Stellar population synthesis models from the optical to the infrared
    We present the first single-burst stellar population models, which covers the optical and the infrared wavelength range between 3500 and 50 000 Å and which are...
  • Publication
    MILES SSP Models
    We present SEDs for single-age, single-metallicity stellar populations (SSPs) covering the full optical spectral range at resolution (FWHM = 2.3Å). These SEDs...