Showing 1–20 of 101 results
/ Date/ Name
Jul 3, 2020Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formationJan 25, 2013Submm/mm Galaxy Counterpart Identification Using a Characteristic Density DistributionApr 1, 2026Calibrating Photometric Mid-Infrared Star Formation Rates for JWSTAug 25, 2020Completing the Census of AGN in GOODS-S/HUDF: New Ultra-Deep Radio Imaging and Predictions for JWSTFeb 14, 2011The Evolution of Stellar Populations in the Outer Disks of Spiral GalaxiesOct 22, 2013The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion yearsApr 12, 2016Star Formation and AGN Activity in Galaxy Clusters from $z=1-2$: a Multi-wavelength Analysis Featuring $Herschel$/PACSJan 4, 2022Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at $z\sim1.4$Jan 22, 2026JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: MIRI Coordinated Parallels in GOODS-S and GOODS-NDec 19, 2023To high redshift and low mass: exploring the emergence of quenched galaxies and their environments at $3<z<6$ in the ultra-deep JADES MIRI F770W parallelSep 6, 2022From Clusters to Proto-clusters: the Infrared Perspective on Environmental Galaxy EvolutionMay 24, 2024SMILES Initial Data Release: Unveiling the Obscured Universe with MIRI Multi-band ImagingJan 24, 2023JEMS: A deep medium-band imaging survey in the Hubble Ultra-Deep Field with JWST NIRCam & NIRISSFeb 14, 2023JADES NIRSpec Spectroscopy of GN-z11: Lyman-$α$ emission and possible enhanced nitrogen abundance in a $z=10.60$ luminous galaxyJul 13, 2023The UV Continuum Slopes of Early Star-Forming Galaxies in JADESJan 16, 2024What is the nature of Little Red Dots and what is not, MIRI SMILES editionMar 9, 2020Simulating JWST/NIRCam Color Selection of High-Redshift GalaxiesMar 14, 2012The Spectral Energy Distributions and Infrared Luminosities of z \approx 2 Dust Obscured Galaxies from Herschel and SpitzerDec 21, 2014Star Formation in High-Redshift Cluster EllipticalsMay 28, 20245-25 $μ$m Galaxy Number Counts from Deep JWST Data