activity
20162024
most citedModeling the gravitational potential of a cosmological dark matter halo with stellar streams

38 citations · 118 across the 7 of their papers we have counts for

collaborators

5 papers

astro-ph.IM20245 cited

The MICADO first light imager for the ELT: overview and current Status

E. Sturm, R. Davies, J. Alves +151

MICADO is a first light instrument for the Extremely Large Telescope (ELT), set to start operating later this decade. It will provide diffraction limited imaging, astrometry, high…

astro-ph.GA202318 cited

INSPIRE: INvestigating Stellar Population In RElics IV. The Initial Mass Function slope in relics

I. Martin-Navarro, C. Spiniello, C. Tortora +10

In the last decade, growing evidence has emerged supporting a non-universal stellar Initial Mass Function (IMF) in massive galaxies, with a larger number of dwarf stars with respec…

astro-ph.GA202321 cited

INSPIRE: INvestigating Stellar Population In RElics III. Second data release (DR2): testing the systematics on the stellar velocity dispersion

G. D'Ago, C. Spiniello, L. Coccato +15

This is the second data release (DR2) of the INvestigating Stellar Population In RElics (INSPIRE) project, comprising 21 new systems with observations completed before March 2022.…

astro-ph.GA202229 cited

The survey of planetary nebulae in Andromeda (M 31) V. Chemical enrichment of the thin and thicker discs of Andromeda. Oxygen to argon abundance ratios for planetary nebulae and H II regions

Magda Arnaboldi, Souradeep Bhattacharya, Ortwin Gerhard +6

We use oxygen and argon abundances for planetary nebulae (PNe) with low internal extinction (progenitor ages of (>4.5 Gyr) and high extinction (progenitor ages <2.5 Gyr), as well a…

astro-ph.GA201638 cited

Modeling the gravitational potential of a cosmological dark matter halo with stellar streams

Robyn E. Sanderson, Johanna Hartke, Amina Helmi

Stellar streams result from the tidal disruption of satellites and star clusters as they orbit a host galaxy, and can be very sensitive probes of the gravitational potential of the…