Showing 1–13 of 13 results
/ Date/ Name
Oct 1, 2025Serendipitous Discovery of an Optically-Dark Ultra-Luminous Infrared Galaxy at $z$ = 3.4May 12, 2025Why is the Star Formation Rate Proportional to Dense Gas Mass?Apr 29, 2025Multi-Component Ionized Gas Outflows in a Hot Dust-Obscured Galaxy W2026+0716 with Keck/OSIRISApr 24, 2025Hot Diggity Dog: Simultaneous CO and Dust Modeling of the Most Luminous WISE Hot Dust-Obscured Galaxy Unveils Extreme Molecular Gas ExcitationApr 18, 2025Resolving the black hole sphere of influence in a hyper-luminous obscured quasar at redshift 4.6Mar 3, 2025The Host Galaxy of FRB 20190520B and Its Unique Ionized Gas DistributionFeb 14, 2025Spatially resolved dust properties over 50 kpc in a hyperluminous galaxy merger at $z = 4.6$Dec 5, 2024Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured GalaxiesDec 6, 2023The Initial Mass Function Based on the Full-sky 20-pc Census of $\sim$3,600 Stars and Brown DwarfsOct 3, 2023H I content of selected mid-infrared bright, starburst blue compact dwarf galaxiesMar 28, 2023Global dynamic scaling relations of HI-rich ultra-diffuse galaxiesDec 14, 2022Discovery of a radio jet in the Cloverleaf Quasar at z = 2.56May 8, 2015Results from the Wide-field Infrared Survey Explorer (WISE) Future Uses Session at the WISE at 5 Meeting