activity
20072026
most citedAn 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5

1.1k citations · 18.6k across the 293 of their papers we have counts for

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Showing 2012Show all

9 papers · 1 filter

astro-ph.CO2012★ 39 cited

On the cool gaseous haloes of quasars

E. P. Farina, R. Falomo, R. Decarli +2

We present optical spectroscopy of projected QSO pairs to investigate the MgII and the CIV absorption features imprinted on the spectrum of the background object by the gaseous hal…

astro-ph.CO2012★ 35 cited

HST narrow-band search for extended Ly-alpha emission around two z>6 quasars

Roberto Decarli, Fabian Walter, Yujin Yang +8

We search for extended Ly-alpha emission around two z>6 quasars, SDSS J1030+0524 (z=6.309) and SDSS J1148+5251 (z=6.419) using WFC3 narrow-band filters on board the Hubble Space Te…

astro-ph.CO2012★ 30 cited

Search of sub-parsec massive binary black holes through line diagnosis II

C. Montuori, M. Dotti, F. Haardt +2

Massive black hole binaries at sub-parsec separations may display in their spectra anomalously small flux ratios between the MgII and CIV broad emission lines, i.e. F_MgII/F_CIV <~…

astro-ph.CO2012★ 293 cited

The Intense Starburst HDF850.1 in a Galaxy Overdensity at z=5.2 in the Hubble Deep Field

Fabian Walter, R. Decarli, C. Carilli +24

The Hubble Deep Field (HDF) is a region in the sky that provides one of the deepest multi-wavelength views of the distant universe and has led to the detection of thousands of gala…

astro-ph.CO2012★ 21 cited

On the redshift of the bright BL Lac object PKS 0048-097

Marco Landoni, Renato Falomo, Aldo Treves +4

Aims: The determination of elusive redshifts of bright BL Lac objects Methods: We use the capabilities of newly available spectrograph X-Shooter at European Southern Observatory (E…

astro-ph.CO2012★ 25 cited

The optical spectrum of PKS 1222+216 and its black hole mass

E. P. Farina, R. Decarli, R. Falomo +2

We investigate the optical spectral properties of the blazar PKS 1222+216 during a period of 3 years. While the continuum is highly variable the broad line emission is practically…