101 citations · 197 across the 4 of their papers we have counts for
10 papers
An analysis of satellite planar configurations around the MW and M31: singling out new high quality planes
Isabel M. Santos-Santos, Rosa Domínguez-Tenreiro, Marcel S. Pawlowski
We present a detailed characterization of planes of satellites in the Milky Way (MW) and M31 systems. To this end we introduce an extension to the '4-galaxy-normal density plot' me…
The host galaxies of luminous type 2 AGN at 0.3-0.4
J. J. Urbano-Mayorgas, M. Villar Martín, F. Buitrago +7
We study the morphological and structural properties of the host galaxies associated with 57 optically-selected luminous type 2 AGN at 0.3-0.4: 16 high-luminosity Seyfert 2…
NIHAO XIV: Reproducing the observed diversity of dwarf galaxy rotation curve shapes in LCDM
Isabel M. Santos-Santos, Arianna Di Cintio, Chris B. Brook +3
The significant diversity of rotation curve (RC) shapes in dwarf galaxies has recently emerged as a challenge to LCDM: in dark matter (DM) only simulations, DM halos have a univers…
Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
Isabel M. E. Santos-Santos, Rosa Domínguez-Tenreiro, Gian Luigi Granato +2
The spectral energy distributions (SEDs) of low-mass low-metallicity (dwarf) galaxies are a challenging piece of the puzzle of galaxy formation in the near Universe. These SEDs sho…
NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
Tobias Buck, Andrea V. Macciò, Aura Obreja +3
Many massive star forming disc galaxies in the redshift range 3 to 0.5 are observed to have a clumpy morphology showing giant clumps of size 1 kpc and masses of about $10^7M_…
Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift
David Goz, Pierluigi Monaco, Gian Luigi Granato +5
We present predictions of Spectral Energy Distributions (SEDs), from the UV to the FIR, of simulated galaxies at . These were obtained by post-processing the results of an N-b…