activity
20092026
most citedBolometric luminosities and Eddington ratios of X-ray selected Active Galactic Nuclei in the XMM-COSMOS survey

417 citations · 8.4k across the 123 of their papers we have counts for

collaborators
Showing 2023 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2023★ 11 cited

Wavelength Dependences of the Optical/UV and X-ray Luminosity Correlations of Quasars

Chichuan Jin, Elisabeta Lusso, Martin Ward +2

The inter-band correlations between optical/UV and X-ray luminosities of active galactic nuclei (AGN) are important for understanding the disc-coronal connection, as well as using…

astro-ph.GA2023

The MUSE Ultra Deep Field (MUDF). IV. A pair of X-ray weak quasars at the heart of two extended Lyα nebulae

Elisabeta Lusso, Emanuele Nardini, Michele Fumagalli +10

We present the results obtained from follow-up observations of the MUSE Ultra Deep Field (MUDF) at X-ray energies with XMM-Newton. The MUDF is centred on a unique field with two br…

astro-ph.GA2023★ 4 cited

On the Metallicities and Kinematics of the Circumgalactic Media of Damped Ly Systems at

Stephanie M. Urbano Stawinski, Kate H. R. Rubin, J. Xavier Prochaska +7

We use medium- and high-resolution spectroscopy of close pairs of quasars to analyze the circumgalactic medium (CGM) surrounding 32 damped Ly absorption systems (DLAs). The prim…

astro-ph.GA2023★ 3 cited

The most luminous blue quasars at 3.0<z<3.3 -- III. LBT spectra and accretion parameters

Bartolomeo Trefoloni, Elisabeta Lusso, Emanuele Nardini +13

We present the analysis of the rest frame ultraviolet and optical spectra of 30 bright blue quasars at , selected to examine the suitability of AGN as cosmological probes.…

astro-ph.GA2023★ 21 cited

MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation

M. Scialpi, F. Mannucci, C. Marconcini +21

The novel Gaia Multi Peak (GMP) technique has proven to be able to successfully select dual and lensed AGN candidates at sub-arcsec separations. Both populations are important beca…

astro-ph.GA2023★ 19 cited

The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging

Mitchell Revalski, Marc Rafelski, Michele Fumagalli +18

We present extremely deep Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) observations of the MUSE Ultra Deep Field (MUDF). This unique region of the sky contains two quasa…

astro-ph.GA2023★ 12 cited

The SOUX AGN Sample: SDSS-XMM-Newton Optical, Ultraviolet and X-ray selected active galactic nuclei spanning a wide range of parameter space -- Sample definition

Daniel Kynoch, Jake A. J. Mitchell, Martin J. Ward +3

We assemble a sample of 696 type 1 AGN up to a redshift of , all of which have an SDSS spectrum containing at least one broad emission line (H , H or Mg II) and an XM…

astro-ph.GA2023★ 31 cited

New multiple AGN systems with sub-arcsec separation: confirmation of candidates selected via the novel GMP method

A. Ciurlo, F. Mannucci, S. Yeh +18

The existence of multiple active galactic nuclei (AGN) at small projected distances on the sky is due to either the presence of multiple, in-spiraling SMBHs, or to gravitational le…