Showing 1–20 of 29 results
/ Date/ Name
Oct 28, 2025PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-domain Field IIIApr 27, 2024Spin-dependent $π$$π^{\ast}$ gap in graphene on a magnetic substrateJan 10, 2024TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time Domain FieldSep 28, 2021The NuSTAR Extragalactic Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain FieldMar 30, 2020The deep Chandra survey in the SDSS J1030+0524 fieldSep 2, 2019Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at z=1.7: star formation promoted by large-scale AGN feedback?Aug 6, 2019Spectral Properties Of Populations Behind The Coherence In Spitzer Near-Infrared And Chandra X-Ray BackgroundsMar 26, 2019Cosmic evolution of supermassive black holes: A view into the next two decadesMar 11, 2019Populations behind the source-subtracted cosmic infrared background anisotropiesSep 21, 2018X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey FieldFeb 15, 2018The 500 ks Chandra observation of the z = 6.31 QSO SDSS J1030+0524Sep 8, 2016The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution FunctionsApr 25, 2016Discovery of a galaxy cluster with a violently starbursting core at z=2.506Jul 14, 2015Satellite content and quenching of star formation in galaxy groups at z~1.8Feb 28, 2015Detailed Shape and Evolutionary Behavior of the X-ray Luminosity Function of Active Galactic NucleiSep 5, 2014Compton Thick AGN in the XMM-COSMOS surveyJul 2, 2013The lack of star formation gradients in galaxy groups up to z~1.6Jun 10, 2013The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ missionApr 21, 2013The XMM-Newton deep survey in the Chandra Deep Field South. III. Point source catalogue and number counts in the hard X-raysAug 30, 2011Dissecting Photometric redshift for Active Galactic Nuclei using XMM- and Chandra-COSMOS samples