activity
20012014
most citedGas-regulation of galaxies: the evolution of the cosmic sSFR, the metallicity-mass-SFR relation and the stellar content of haloes

875 citations · 2.8k across the 50 of their papers we have counts for

collaborators

52 papers

astro-ph.GA2014★ 18 cited

The Zurich Environmental Study (ZENS) of Galaxies in Groups along the Cosmic Web. V. Properties and Frequency of Merging Satellites and Centrals in Different Environments

A. Pipino, A. Cibinel, S. Tacchella +6

We use the Zurich ENvironmental Study (ZENS) database to investigate the environmental dependence of the merger fraction and merging galaxy properties in a sample of ~1300 grou…

astro-ph.GA2014★ 36 cited

The hunt for the Milky Way's accreted disc

Gregory R. Ruchti, Justin I. Read, Sofia Feltzing +2

The Milky Way is expected to host an accreted disc of stars and dark matter. This forms as massive >1:10 mergers are preferentially dragged towards the disc plane by dynamical fric…

astro-ph.GA2014★ 30 cited

On the relation between sSFR and metallicity

A. Pipino, S. J. Lilly, C. M. Carollo

In this paper we present an exact general analytic expression linking the gas metallicity Z to the specific star formation rate (sSFR), that validates a…

astro-ph.CO2014★ 55 cited

ZENS IV. Similar Morphological Changes associated with Mass- and Environment-Quenching, and the Relative importance of Bulge Growth versus the Fading of Disks

C. M. Carollo, A. Cibinel, S. J. Lilly +6

We use ZENS data at low redshift to study the dependence of the quenched satellite fraction and of the morphological mix of these quenched satellites, on three different environmen…

astro-ph.GA2013★ 62 cited

The dust content of QSO hosts at high redshift

F. Calura, R. Gilli, C. Vignali +3

Infrared observations of high-z quasar (QSO) hosts indicate the presence of large masses of dust in the early universe. When combined with other observables, such as neutral gas ma…

astro-ph.CO2013★ 29 cited

Galactic and Cosmic Type Ia SN rates: is it possible to impose constraints on SNIa progenitors?

I. Bonaparte, F. Matteucci, S. Recchi +3

We compute the Type Ia supernova rates in typical elliptical galaxies by varying the progenitor models for Type Ia supernovae. To do that a formalism which takes into account the d…