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The structure of the X-ray absorber in Mrk 915 revealed bySwiftAGN feedback in action: a new powerful wind in 1SXPS J050819.8+172149?Exploring the active galactic nuclei population with extreme X-ray-to-optical flux ratios (fx/fo > 50)X-ray observation of ULAS J1120+0641, the most distant quasar atz= 7.08The variable ionized absorber in the Seyfert 2 Mrk 348Using the Bright UltrahardXMM-Newtonsurvey to define an IR selection of luminous AGN based onWISEcoloursNGC 454: unveiling a new ‘changing look’ active galactic nucleusSuzaku and SWIFT-BAT observations of a newly discovered Compton-thick AGNThe stellar content of the XMM-Newton bright serendipitous surveyExtremely compact massive galaxies at z 1.4An X-ray bright ERO hosting a type 2 QSODating the stellar population in massive early-type galaxies atz∼ 1.5The First Optical Validation of an X-Ray Line-emitting Object: A Detection in theXMM-NewtonObservation of the Chandra Deep Field-SouthLooking for obscured QSOs in the X-ray emitting ERO populationThe density of very massive evolved galaxies to z = 1.7XMM-Newton spectroscopy of an X-ray selected sample of RL AGNsExploring the X-ray sky with the XMM-Newton bright serendipitous surveyX-Ray Line-emitting Objects inXMM-NewtonObservations: The Tip of the IcebergThe XMM-Newton Bright Serendipitous Survey: First Extragalactic ResultsThe Ultra Luminous Infrared Galaxy Mrk 231: new clues from BeppoSAX and XMM-NewtonThe XMM-Newton and BeppoSAX view of the Ultra Luminous Infrared Galaxy MKN 231The XMM-NewtonHBS28 sample: Studying the obscuration in hard X-ray selected AGNsA hard medium survey with ASCAAn XMM-Newton hard X-ray survey of ultraluminous infrared galaxiesXMM-Newtonobservations reveal AGN in apparently normal galaxiesXMM-Newtonobservations of ULIRGs: A Compton-thick AGN in IRAS 19254–7245The Kormendy relation of massive elliptical galaxies at z 1.5: evidence for size evolutionThe TESIS Project: Are Type 2 QSO Hidden in X-Ray Emitting EROs?The TESIS Project: Revealing Massive Early-Type Galaxies at z > 1Massive $z\sim1.3$ evolved galaxies revealedALMA [C i]3 P 1–3 P 0 Observations of NGC 6240: A Puzzling Molecular Outflow, and the Role of Outflows in the Global α CO Factor of (U)LIRGsAn H$_\alpha$ catalogue of galaxies in Hickson compact groupsThe HELLAS2XMM survey. IX. Spectroscopic identification of super-EROs hosting AGNsThe HELLAS2XMM survey. V. Near-Infrared observations of X-ray sources with extreme X/O ratiosThe HELLAS2XMM survey. III. Multiwavelength observations of hard X-ray selected sources in the PKS 0312-77 fieldThe HELLAS2XMM surveyThe HELLAS2XMMSurvey. II. Multiwavelength Observations of P3: An X‐Ray–bright, Optically Inactive GalaxyThe final data release of ALLSMOG: a survey of CO in typical local low-M∗ star-forming galaxiesThe XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogueThe XMM-Newton serendipitous survey. IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)
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description
forsker
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researcher ORCID ID = 0000-0001-5619-5896
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wetenschapper
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name
P. Severgnini
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P. Severgnini
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Paola Severgnini
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Paola Severgnini
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P. Severgnini
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P. Severgnini
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Paola Severgnini
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Paola Severgnini
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P. Severgnini
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P. Severgnini
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P. Severgnini
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Paola Severgnini
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Paola Severgnini
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P31
P496
0000-0001-5619-5896