34 citations · 144 across the 6 of their papers we have counts for
6 papers
The QSO proximity effect at redshift <z>=2.6 with the FLO approach
V. D'Odorico, M. Bruscoli, F. Saitta +4
We revisit the proximity effect produced by QSOs at redshifts 2.1-3.3 applying the FLO approach (Saitta et al. 2008) to a sample of ~6300 Ly-alpha lines fitted in 21 high resolutio…
Tracing the gas at redshift 1.7-3.5 with the Lyman-alpha forest: the FLO approach
F. Saitta, V. D'Odorico, M. Bruscoli +3
[Abridged] We present FLO (From Lines to Over-densities), a new technique to reconstruct the hydrogen density field for the Lya forest lines observed in high resolution QSO spectra…
The Proximity Effect Around High Redshift Galaxies
A. Maselli, A. Ferrara, M. Bruscoli +2
Recent observations have shown that the intergalactic medium (IGM) is more transparent to Lyalpha photons close to Lyman Break Galaxies (LBGs) than at large distance from them, ie…
The Lyalpha Forest Around High Redshift Galaxies
M. Bruscoli, A. Ferrara, S. Marri +4
Motivated by the relative lack of neutral hydrogen around Lyman Break Galaxies deduced from recent observations, we investigate the properties of the Lyalpha forest around high red…
The power-law behaviours of angular spectra of polarized Galactic synchrotron
M. Bruscoli, M. Tucci, V. Natale +4
We study the angular power spectra of polarized Galactic synchrotron in the range 10<l<800, at several frequencies between 0.4 and 2.7 GHz and at several Galactic latitudes up to n…
How is the Reionization Epoch Defined?
Marialuce Bruscoli, Andrea Ferrara, Evan Scannapieco
We study the effect of a prolonged epoch of reionization on the angular power spectrum of the Cosmic Microwave Background. Typically reionization studies assume a sudden phase tran…