activity
19962020
most citedThe XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

489 citations · 3.5k across the 63 of their papers we have counts for

collaborators

63 papers

astro-ph.HE2020★ 67 cited

The XMM-Newton serendipitous survey. X: The second source catalogue from overlapping XMM-Newton observations and its long-term variable content

I. Traulsen, A. D. Schwope, G. Lamer +12

The XMM-Newton Survey Science Centre Consortium (SSC) develops software in close collaboration with the Science Operations Centre to perform a pipeline analysis of all XMM-Newton o…

astro-ph.HE2018★ 34 cited

The XMM-Newton serendipitous survey. VIII: The first XMM-Newton serendipitous source catalogue from overlapping observations

I. Traulsen, A. D. Schwope, G. Lamer +13

XMM-Newton has observed the X-ray sky since early 2000. The XMM-Newton Survey Science Centre Consortium has published catalogues of X-ray and ultraviolet sources found serendipitou…

astro-ph.GA2017★ 5 cited

AGN with discordant optical and X-ray classification are not a physical family: Diverse origin in two AGN

I. Ordovás-Pascual, S. Mateos, F. J. Carrera +7

Approximately 3-17 percent of Active Galactic Nuclei (AGN) without detected rest-frame UV/optical broad emission lines (type-2 AGN) do not show absorption in X-rays. The physical o…

astro-ph.GA2016★ 6 cited

X-ray selected BALQSOs

M. J. Page, F. J. Carrera, M. Ceballos +11

We study a sample of six X-ray selected broad absorption line (BAL) quasi-stellar objects (QSOs) from the XMM-Newton Wide Angle Survey. All six objects are classified as BALQSOs us…

astro-ph.IM2016★ 1 cited

The ARCHES project

C. Motch, F. Carrera, F. Genova +12

ARCHES (Astronomical Resource Cross-matching for High Energy Studies) is a FP7-Space funded project whose aim is to provide the international astronomical community with well-chara…

astro-ph.HE2015★ 11 cited

Infrared identification of hard X-ray sources in the Galaxy

A. Nebot Gómez-Morán, C. Motch, F. -X. Pineau +3

The nature of the low- to intermediate-luminosity (Lx erg s) source population revealed in hard band (2-10 keV) X-ray surveys of the Galactic Plane is poo…