Showing 1–20 of 66 results
/ Date/ Name
Mar 13, 2020The Evolution of the Star-forming Interstellar Medium across Cosmic TimeApr 26, 2002Studying the Dynamics of Star Forming and IR Luminous Galaxies with Infrared SpectroscopyFeb 10, 2010High molecular gas fractions in normal massive star forming galaxies in the young UniverseFeb 3, 2017PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas FractionsNov 10, 2005High-resolution Millimeter Imaging of Submillimeter GalaxiesNov 25, 2012PHIBSS: molecular gas content and scaling relations in z~1-3 normal star forming galaxiesApr 2, 2013PHIBSS: molecular gas, extinction, star formation and kinematics in the z=1.5 star forming galaxy EGS13011166Jun 2, 2001Ultra-Luminous Infrared Mergers: Elliptical Galaxies in Formation?Jan 23, 2008Submillimeter Galaxies at z~2: Evidence for Major Mergers & Constraints on Lifetimes, IMF and CO-H2 Conversion FactorMar 13, 2017Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years agoOct 14, 2013The SINS/zC-SINF survey of z~2 galaxy kinematics: evidence for gravitational quenchingJul 18, 2002Ultr-Luminous Infrared Galaxies: QSOs in Formation?Feb 14, 2012COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: III. Comparison with semi-analytic models of galaxy formationMar 8, 2011COLD GASS, an IRAM legacy survey of molecular gas in massive galaxies: I. Relations between H2, HI, stellar content and structural propertiesMay 4, 2012Quantifying the role of bars in the build-up of central mass concentrations in disk galaxiesNov 26, 2012The SINS/zC-SINF Survey of z~2 Galaxy Kinematics: The Nature of Dispersion Dominated GalaxiesMay 26, 2014A Consistent Study of Metallicity Evolution at 0.8 < z < 2.6Dec 2, 2019The CO(3-2)/CO(1-0) luminosity line ratio in nearby star-forming galaxies and AGN from xCOLD GASS, BASS and SLUGSAug 12, 2020The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational PerspectiveSep 4, 2020Structural evolution in massive galaxies at z~2