activity
20062025
most citedThe age structure of stellar populations in the solar vicinity. Clues of a two-phase formation history of the Milky Way disk

535 citations · 3.2k across the 27 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

10 papers · 1 filter

astro-ph.CO2014★ 19 cited

The Galaxy Population In Voids: Are All Voids The Same?

Saeed Tavasoli, Hadi Rahmani, Habib G. Khosroshahi +2

The influence of under-dense environments on the formation and evolution of galaxies is studied by analysing the photometric properties of ~200 galaxies residing in voids, taken fr…

astro-ph.CO2013★ 18 cited

The detection of FIR emission from high redshift star-forming galaxies in the ECDF-S

L. J. M. Davies, M. N. Bremer, E. R. Stanway +1

ABRIDGED: We have used the LABOCA Survey of the ECDF-S (LESS) to investigate rest-frame FIR emission from typical SF systems (LBGs) at redshift 3, 4, and 5. We initially concentrat…

astro-ph.CO2012★ 251 cited

CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release

CALIFA collaboration, B. Husemann, K. Jahnke +74

We present the first public data release of the CALIFA survey. It consists of science-grade optical datacubes for the first 100 of eventually 600 nearby (0.005<z<0.03) galaxies, ob…

astro-ph.CO2012★ 113 cited

The ionized gas in the CALIFA early-type galaxies I. Mapping two representative cases: NGC 6762 and NGC 5966

C. Kehrig, A. Monreal-Ibero, P. Papaderos +18

As part of the CALIFA survey, we conducted a thorough 2D analysis of the ionized gas in two E/S0 galaxies, NGC6762 and NGC5966, aiming to shed light on the nature of their warm ion…

astro-ph.CO2011★ 44 cited

Minor mergers and their impact on the kinematics of old and young stellar populations in disk galaxies

Y. Qu, P. Di Matteo, M. D. Lehnert +2

By means of N-body simulations we investigate the impact of minor mergers on the angular momentum and dynamical properties of the merger remnant. Our simulations cover a range of i…

astro-ph.CO2011★ 9 cited

Can Cosmological Accretion be Observed in H-alpha at z~2?

Loïc Le Tiran, Matthew D. Lehnert, Paola Di Matteo +2

In previous studies, it has been shown that the large line widths observed in high surface brightness H-alpha emitters at low and high redshifts are likely due to the mechanical en…