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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

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astro-ph2008★ 103 cited

The XMM-Newton Serendipitous Survey. VI. The X-ray Luminosity Function

J. Ebrero, F. J. Carrera, M. J. Page +6

We present the X-ray luminosity function of AGN in three energy bands (Soft: 0.5-2 keV, Hard: 2-10 keV and Ultrahard: 4.5-7.5 keV). We have used the XMS survey along with other hig…

astro-ph2008★ 11 cited

An extreme EXO: a type 2 QSO at z=1.87

A. Del Moro, M. G. Watson, S. Mateos +6

We aim to understand the multi-wavelength properties of 2XMM J123204+215255, the source with the most extreme X-ray-to-optical flux ratio amongst a sample of bright X-ray selected…

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★ 99 cited

High precision X-ray logN-logS distributions: implications for the obscured AGN population

S. Mateos, R. S. Warwick, F. J. Carrera +13

We have constrained the extragalactic source count distributions over a broad range of X-ray fluxes and in various energy bands to test whether the predictions from X-ray backgroun…

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-ph2007★ 56 cited

The XMM-Newton bright serendipitous survey. Identification and optical spectral properties

A. Caccianiga, P. Severgnini, R. Della Ceca +12

AIMS: We present the optical classification and redshift of 348 X-ray selected sources from the XMM-Newton Bright Serendipitous Survey (XBS) which contains a total of 400 objects (…

astro-ph2007★ 89 cited

The XMM-Newton Serendipitous Survey V. Optical identification of the XMM-Newton Medium sensitivity Survey (XMS)

X. Barcons, F. J. Carrera, M. T. Ceballos +53

We present the XMM-Newton Medium sensitivity Survey (XMS), including a total of 318 X-ray sources found among the serendipitous content of 25 XMM-Newton target fields. The XMS comp…

astro-ph2007★ 43 cited

The XMM large scale structure survey: optical vs. X-ray classifications of active galactic nuclei and the unified scheme

O. Garcet, P. Gandhi, E. Gosset +25

Our goal is to characterize AGN populations by comparing their X-ray and optical classifications. We present a sample of 99 spectroscopically identified X-ray point sources in the…

astro-ph2007★ 21 cited

An XMM-Newton study of Hyper-Luminous Infrared Galaxies

A. Ruiz, F. J. Carrera, F. Panessa

Hyper-Luminous Infrared Galaxies (HLIRGs) are the most luminous persistent objects in the Universe. They exhibit extremely high star formation rates, and most of them seem to harbo…

astro-ph2007★ 73 cited

Elusive AGN in the XMM-Newton bright serendipitous survey

A. Caccianiga, P. Severgnini, R. Della Ceca +3

AIMS: We investigate here the nature of all the sources (35 in total) in the XBS survey (which is 86% optically identified) showing an optical spectrum dominated by the light from…

astro-ph2007★ 46 cited

The XMM-Newton serendipitous survey IV. The AXIS X-ray source counts and angular clustering

F. J. Carrera, J. Ebrero, S. Mateos +14

AXIS (An XMM-Newton International Survey) is a survey of 36 high Galactic latitude XMM-Newton observations covering 4.8 deg2 and containing 1433 serendipitous X-ray sources detecte…

astro-ph2007★ 153 cited

The X-ray and Radio Connection in Low-luminosity Active Nuclei

F. Panessa, X. Barcons, L. Bassani +4

We present the results of the correlation between the nuclear 2-10 keV X-ray and radio (at 2cm, 6cm and 20cm) luminosities for a well defined sample of local Seyfert galaxies. We u…

astro-ph2006

Multi-wavelength and black hole mass properties of Low Luminosity Active Nuclei

F. Panessa, L. Bassani, M. Cappi +6

We investigate the relation between the X-ray nuclear emission, optical emission line, radio luminosity and black hole mass for a sample of nearby Seyfert galaxies. Strong linear c…

astro-ph2006

Biased galaxy formation in the fields of high-redshift AGN

J. A. Stevens, M. J. Page, F. J. Carrera +2

We discuss preliminary results from our programme to map the fields of high-redshift AGN. In the context of the hierarchical models such fields are predicted to contain an over-den…

astro-ph2006

X-ray absorbed QSOs and the QSO evolutionary sequence

M. J. Page, F. J. Carrera, J. Ebrero +2

Unexpected in the AGN unified scheme, there exists a population of broad-line z~2 QSOs which have heavily absorbed X-ray spectra. These objects constitute 10% of the population at…

astro-ph2006★ 352 cited

On the X-ray, optical emission line and black hole mass properties of local Seyfert galaxies

F. Panessa, L. Bassani, M. Cappi +5

We investigate the relation between X-ray nuclear emission, optical emission line luminosities and black hole masses for a sample of 47 Seyfert galaxies. The sample, which has been…

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…

astro-ph2005★ 74 cited

Submillimetre photometry of X-ray absorbed QSOs: their formation and evolutionary status

J. A. Stevens, M. J. Page, R. J. Ivison +4

We present an analysis of the submillimetre/X-ray properties of 19 X-ray absorbed, Compton-thin quasi-stellar objects (QSOs) selected to have luminosities and redshifts which repre…

astro-ph2005★ 3 cited

Tentative detection of warm intervening gas towards PKS 0548-322 with XMM-Newton

X. Barcons, F. B. S. Paerels, F. J. Carrera +2

We present the results of a long (~93 ksec) XMM-Newton observation of the bright BL-Lac object PKS 0548-322 (z=0.069). Our Reflection Grating Spectrometer (RGS) spectrum shows a si…

astro-ph2004★ 59 cited

X-ray spectra of XMM-Newton serendipitous medium flux sources

S. Mateos, X. Barcons, F. J. Carrera +7

We report on the results of a detailed analysis of the X-ray spectral properties of a large sample of sources detected serendipitously with the XMM-Newton observatory in 25 selecte…

astro-ph2004★ 20 cited

Simultaneous X-Ray and optical spectroscopy of the Seyfert galaxy Mrk 993

A. Corral, X. Barcons, F. J. Carrera +2

We present the results of simultaneous XMM-Newton X-ray and 3.5m/CAHA optical spectroscopic observations of the Seyfert galaxy Mrk 993. This galaxy exhibited in the past significan…

astro-ph2004★ 117 cited

Exploring the X-ray Sky with the XMM-Newton Bright Serendipitous Survey

R. Della Ceca, T. Maccacaro, A. Caccianiga +11

ABRIDGED. We present "The XMM-Newton Bright Serendipitous Survey", two flux-limited samples with flux limit fx ~7E-14 cgs in the 0.5-4.5 keV (BSS) and 4.5-7.5 keV (HBSS) energy ban…

astro-ph2004★ 131 cited

The evolutionary sequence of active galactic nuclei and galaxy formation revealed

M. J. Page, J. A. Stevens, R. J. Ivison +1

Today, almost every galaxy spheroid contains a massive black hole: a remnant of, and testament to, a period in its evolution when it contained an active galactic nucleus (AGN). How…

astro-ph2003★ 93 cited

The XMM-Newton HBS28 sample: studying the obscuration in hard X-ray selected AGNs

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

This paper presents the analysis of a statistically complete sample of 28 serendipitous X-ray sources selected in 82 pointed XMM-Newton fields down to a count-rate of 0.002 counts…