71 citations · 121 across the 4 of their papers we have counts for
7 papers
Is the Bremer Deep Field ionised, at z~7?
José Miguel Rodriguez Espinosa, J. Miguel Mas-Hesse, Rosa Calvi
We show herein that the population of star forming galaxies in the Bremer Deep Field (BDF) have enough ionising power to form two large ionised bubbles which could be in the proces…
Probing the existence of a rich galaxy overdensity at z=5.2
R. Calvi, H. Dannerbauer, P. Arrabal Haro +4
We report the results of a pilot spectroscopic program of a region at z=5.2 in the GOODS-N field containing an overdensity of galaxies around the well-known submillimeter galaxy HD…
An ionised bubble powered by a proto-cluster at z = 6.5
J. M. Rodriguez Espinosa, J. M. Mas-Hesse, E. Salvador Sole +7
We show herein that a proto-cluster of Ly emitting galaxies, spectroscopically confirmed at redshift 6.5, produces a remarkable number of ionising continuum photons. We start fr…
MOS spectroscopy of protocluster candidate galaxies at z=6.5
Rosa Calvi, José Miguel Rodríguez Espinosa, José Miguel Mas-Hesse +7
The epoch corresponding to a redshift of z is close to full re-ionisation of the Universe, and early enough to provide an intriguing environment to observe the early sta…
Morphology rather than environment drives the SFR-Mass relation in the local universe
R. Calvi, B. Vulcani, B. M. Poggianti +3
Exploiting a sample of 680 star-forming galaxies from the Padova-Millennium GalaxyGroup Catalog (PM2GC) (Calvi et al. 2011) in the range 0.038<z<0.104, we present a detailed analys…
The star formation history of galaxies: the role of galaxy mass, morphology and environment
Valentina Guglielmo, Bianca M. Poggianti, Alessia Moretti +5
We analyze the star formation history (SFH) of galaxies as a function of present-day environment, galaxy stellar mass and morphology. The SFH is derived by means of a non-parametri…