activity
20062025
most citedThe XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

489 citations · 564 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

Identification of high-redshift X-ray active galactic nuclei in the 4XMM-DR11 serendipitous catalogue using DES data: Comparative analysis with optically-selected QSOs

E. Pouliasis, A. Ruiz, I. Georgantopoulos +8

X-rays provide a robust method in identifying AGN. However, in the high-redshift Universe, their space density is relatively low, and, in combination with the small areas covered b…

astro-ph.SR2014★ 6 cited

X-ray and UV observations of V751 Cyg in an optical high state

K. L. Page, J. P. Osborne, A. P. Beardmore +3

Aims: The VY Scl system (anti-dwarf nova) V751 Cyg is examined following a claim of a super-soft spectrum in the optical low state. Methods: A serendipitous XMM-Newton X-ray observ…

astro-ph.HE2012★ 5 cited

On the nature of high X-ray luminosities in SDSS galaxies

F. E. Jackson, T. P. Roberts, D. M. Alexander +5

Surveys have revealed a class of object displaying both high X-ray luminosities (Lx > 10^42 erg/s), and a lack of a discernible active galactic nucleus (AGN) in the optical band. I…

astro-ph2008★ 46 cited

Average Fe K-alpha emission from distant AGN

A. Corral, M. J. Page, F. J. Carrera +7

One of the most important parameters in the XRB (X-ray background) synthesis models is the average efficiency of accretion onto SMBH (super-massive black holes). This can be inferr…

astro-ph2008★ 489 cited

The XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

M. G. Watson, A. C. Schröder, D. Fyfe +47

Aims: Pointed observations with XMM-Newton provide the basis for creating catalogues of X-ray sources detected serendipitously in each field. This paper describes the creation and…

astro-ph2006★ 18 cited

An X-ray bright ERO hosting a type 2 QSO

P. Severgnini, A. Caccianiga, V. Braito +8

We present the XMM-Newton and the optical-VLT spectra along with the optical and the near-infrared photometric data of one of the brightest X-ray (F(2-10 keV)~1e-13 erg/s cm^2) ext…