Showing 1–20 of 122 results
/ Date/ Name
Aug 22, 2022GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096Mar 28, 2022The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5Sep 22, 2020The ALMA Spectroscopic Survey in the HUDF: Constraining the Molecular Content at $\log{(M_*/M_\odot)} \sim 9.5$ with CO stacking of MUSE detected $z\sim1.5$ GalaxiesApr 20, 2010The Buried Starburst in the Interacting Galaxy II Zw 096 as Revealed by the Spitzer Space TelescopeJun 13, 2018The AKARI 2.5-5 Micron Spectra of Luminous Infrared Galaxies in the Local UniverseSep 18, 2013Mid-Infrared Atomic Fine-Structure Emission Line Spectra of Luminous Infrared Galaxies: Spitzer/IRS Spectra of the GOALS SampleOct 10, 2017The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxiesFeb 16, 2011Infrared Luminosity Functions of AKARI-SDSS GalaxiesApr 17, 2023JWST/NIRSpec Measurements of Extremely Low Metallicities in High Equivalent Width Lyman-$α$ EmittersOct 2, 2008Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep fieldJul 27, 2023GOALS-JWST: Small neutral grains and enhanced 3.3 micron PAH emission in the Seyfert galaxy NGC 7469Sep 7, 2012Spectral Energy Distributions of Local Luminous And Ultraluminous Infrared GalaxiesAug 21, 2018A census of galaxy constituents in a Coma Progenitor observed at z>3Sep 17, 2018ALMA Observation of NGC5135: The Circumnuclear CO(6-5) and Dust Continuum Emission at 45 Parsec Resolution[$\star$]Mar 20, 2019The evolution of the cosmic molecular gas densityFeb 20, 2020The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to $z\sim3$Feb 25, 2020Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emittersMar 21, 2019The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopyMay 26, 2021Measuring the average molecular gas content of star-forming galaxies at $z=3-4$Apr 28, 2016Spectroscopic Confirmation of a Protocluster at z=3.786