1.3k citations · 4.9k across the 37 of their papers we have counts for
37 papers
Constraining the stellar populations of ultra-diffuse galaxies in the MATLAS survey using spectral energy distribution fitting
Maria Luisa Buzzo, Duncan A. Forbes, Thomas H. Jarrett +12
We use spectral energy distribution (SED) fitting to place constraints on the stellar populations of 59 ultra-diffuse galaxies (UDGs) in the low-to-moderate density fields of the M…
NGC 3314a/b and NGC 3312: Ram pressure stripping in Hydra I Cluster substructure
Kelley M. Hess, Ralf Kotulla, Hao Chen +4
Cluster substructure and ram pressure stripping in individual galaxies are among the primary evidence for the ongoing growth of galaxy clusters as they accrete galaxies and groups…
A near-infrared study of the obscured 3C129 galaxy cluster
M. Ramatsoku, M. A. W Verheijen, R. C. Kraan-Korteweg +3
We present a catalogue of 261 new infrared selected members of the 3C129 galaxy cluster. The cluster, located at 0.02, forms part of the Perseus-Pisces filament and is…
The Herschel Exploitation of Local Galaxy Andromeda (HELGA): IV. Dust scaling relations at sub-kpc resolution
S. Viaene, J. Fritz, M. Baes +18
The imprints of dust-starlight interactions are visible in scaling relations between stellar characteristics, star formation parameters and dust properties. We aim to examine dust…
The Star Formation in Radio Survey: GBT 33 GHz Observations of Nearby Galaxy Nuclei and Extranuclear Star-Forming Regions
E. J. Murphy, J. Bremseth, B. S. Mason +7
We present 33\,GHz photometry of 103 galaxy nuclei and extranuclear star-forming complexes taken with the Green Bank Telescope (GBT) as part of the Star Formation in Radio Survey (…
Mid-Infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. II. Properties of WISE-Selected Active Galactic Nuclei in the NDWFS Boötes Field
Roberto J. Assef, Daniel Stern, Christopher S. Kochanek +11
Stern et al.(2012) presented a study of WISE selection of AGN in the 2 deg^2 COSMOS field, finding that a simple criterion W1-W2>=0.8 provides a highly reliable and complete AGN sa…