Showing 1–20 of 94 results
/ Date/ Name
Dec 21, 2009The X-ray to optical-UV luminosity ratio of X-ray selected Type 1 AGN in XMM-COSMOSFeb 21, 2011The redshift and nature of AzTEC/COSMOS 1: A starburst galaxy at z=4.6Oct 3, 2018The molecular gas content and fuel efficiency of starbursts at z ~ 1.6 with ALMAMay 8, 2019The Main Sequence at $z \sim 1.3$ contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts?Dec 15, 2020COLDz: Deep 34 GHz Continuum Observations and Free-free Emission in High-redshift Star-forming GalaxiesMar 4, 2014Gas reservoir of a hyper-luminous QSO at z=2.6Mar 7, 2017The unexpectedly large dust and gas content of quiescent galaxies at z>1.4Jan 5, 2016The Chandra COSMOS Legacy survey: overview and point source catalogMar 28, 2017VLA-COSMOS 3GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to $z\lesssim6$Oct 3, 2012The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy DistributionsSep 18, 2020Observations of [OI]63micron line emission in main-sequence galaxies at z~1.5Mar 28, 2019Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25Mar 28, 2017The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5Mar 1, 2018GOODS-ALMA: 1.1 mm galaxy survey - I. Source catalogue and optically dark galaxiesSep 29, 2014CO excitation of normal star forming galaxies out to z=1.5 as regulated by the properties of their interstellar mediumJun 18, 2016HELP: XID+, The Probabilistic De-blender for Herschel SPIRE mapsFeb 21, 2013The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4Dec 18, 2014Enabling the next generation of cm-wavelength studies of high-redshift molecular gas with the SKAAug 30, 2011Dissecting Photometric redshift for Active Galactic Nuclei using XMM- and Chandra-COSMOS samplesDec 3, 2014COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS