Showing 1–20 of 643 results
/ Date/ Name
Jan 31, 2012The Cosmic History of Hot Gas Cooling and Radio AGN Activity in Massive Early-Type GalaxiesJul 14, 2023XMM-Newton Observations of Two Archival X-ray Weak Type 1 Quasars: Obscuration Induced X-ray Weakness and VariabilitySep 10, 2010Weak-Line Quasars at High Redshift: Extremely High Accretion Rates or Anemic Broad-Line Regions?Sep 10, 2010The Extended Chandra Deep Field-South Survey: Optical spectroscopy of faint X-ray sources with the VLT and KeckJun 10, 2010The LABOCA survey of the Extended Chandra Deep Field South: A photometric redshift survey of submillimetre galaxiesJun 23, 2010Radiation pressure, absorption and AGN feedback in the Chandra Deep FieldsNov 11, 2010The SIMPLE survey: observations, reduction, and catalogAug 3, 2010Parsec-Scale Bipolar X-ray Shocks Produced by Powerful Jets from the Neutron Star Circinus X-1Jun 13, 2022Spectral Energy Distributions in Three Deep-Drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time: Source Classification and Galaxy PropertiesDec 17, 2010The XMM Deep survey in the CDFS I. First results on heavily obscured AGNSep 19, 2012The high-redshift (z>3) AGN population in the 4 Ms Chandra Deep Field SouthJul 3, 2012Insights on the X-ray weak quasar phenomenon from XMM-Newton monitoring of PHL 1092Aug 3, 2012Broad Absorption Line Disappearance on Multi-Year Timescales in a Large Quasar SampleJun 21, 2011GOODS-Herschel: The far-infrared view of star formation in AGN host galaxies since z~3Dec 14, 2023The kinematics of massive high-redshift dusty star-forming galaxiesJan 7, 2009Chandra observations of the hybrid morphology radio sources 3C 433 and 4C 65.15: FR IIs with asymmetric environmentsApr 14, 2009High-Redshift SDSS Quasars with Weak Emission LinesNov 2, 2009Optically Selected BL Lacertae Candidates from the Sloan Digital Sky Survey Data Release SevenJan 27, 2010Supermassive Black-Hole Growth Over Cosmic Time: Active Galaxy Demography, Physics, and Ecology from Chandra SurveysFeb 16, 2024Quasar Outflow Deceleration or Acceleration: Predictions and a Search