Showing 1–20 of 37 results
/ Date/ Name
Feb 18, 2013Herschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting proto-ellipticalsOct 14, 2019The fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removalAug 23, 2017Can planet formation resolve the dust budget crisis in high redshift galaxies?Jul 25, 2017Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at $z<1$Jun 29, 2016The Herschel-ATLAS Data Release 1 Paper II: Multi-wavelength counterparts to submillimetre sourcesMay 3, 2024The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5Dec 18, 2014The evolution of the cold interstellar medium in galaxies following a starburstMar 15, 2026All-sky Searches for Continuous Gravitational Waves from Isolated Neutron Stars in the Data from the First Part of the Fourth LIGO-Virgo-KAGRA Observing RunApr 18, 2023The role of mass and environment in the build up of the quenched galaxy population since cosmic noonAug 15, 2012Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z < 0.5Sep 28, 2011H-ATLAS/GAMA: Dusty early-type galaxies and passive spiralsOct 4, 2016Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relationsJul 30, 2013A Herschel-ATLAS study of dusty spheroids: probing the minor-merger process in the local UniverseFeb 18, 2013GAMA/H-ATLAS: Linking the Properties of Sub-mm Detected and Undetected Early-Type Galaxies: I. z$\le$0.06 SampleOct 6, 2024Measuring the ISM Content of Nearby, Luminous, Type 1 and Type 2 QSOs through CO and [C II]Jan 9, 2024The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formationOct 10, 2019The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)May 26, 2015H-ATLAS/GAMA and HeViCS - Dusty Early-Type Galaxies in Different EnvironmentsNov 18, 2016Host galaxies of luminous z$\sim$0.6 quasars: Major mergers are not prevalent at the highest AGN luminositiesJun 4, 2024Quasi-periodic X-ray eruptions and tidal disruption events prefer similar host galaxies