activity
20042026
most citedThe Milky Way: An Exceptionally Quiet Galaxy; Implications for the formation of spiral galaxies

263 citations · 3.1k across the 88 of their papers we have counts for

collaborators

89 papers

astro-ph.GA2026

Direct Abundance Maps and Radial Metallicity Gradients of two Galaxies at z~4-5 in the GARDEN Survey

L. Stanghellini, S. A. Kassin, C. Pacifici +26

We investigate galaxies in the GARDEN (Galaxies at All Redshifts Deciphered and Explained with the NIRSpec MSA) survey that exhibit auroral emission lines, enabling spatially resol…

astro-ph.IM2023

The ESO's Extremely Large Telescope Working Groups

Paolo Padovani, Michele Cirasuolo, Remco van der Burg +82

Since 2005 ESO has been working with its community and industry to develop an extremely large optical/infrared telescope. ESO's Extremely Large Telescope, or ELT for short, is a re…

astro-ph.IM2020

MOSAIC: the high-multiplex and multi-IFU spectrograph for the ELT

Rubén Sánchez-Janssen, Francois Hammer, Simon Morris +40

MOSAIC is the planned multi-object spectrograph for the 39m Extremely Large Telescope (ELT). Conceived as a multi-purpose instrument, it offers both high multiplex and multi-IFU ca…

astro-ph.GA2019★ 22 cited

Simulating MOS science on the ELT: Ly forest tomography

J. Japelj, C. Laigle, M. Puech +14

Mapping of the large-scale structure through cosmic time has numerous applications in the studies of cosmology and galaxy evolution. At , the structure can be traced by the…

astro-ph.GA2019

Are Milky-Way dwarf-spheroidal galaxies dark-matter free?

F. Hammer, Y. B. Yang, J. L. Wang +4

We have found that the high velocity dispersions of dwarf spheroidal galaxies (dSphs) can be well explained by Milky Way (MW) tidal shocks, which reproduce precisely the gravitatio…

astro-ph.GA2019★ 3 cited

Time-average properties of major mergers: mergers significantly scatter high-z scaling relations

Mathieu Puech, Hector Flores, Myriam Rodrigues +2

Interpreting the scaling relations measured by recent large kinematic surveys of galaxies has remained hampered by large observational scatter. We show that the observed IS…