1.1k citations · 5k across the 100 of their papers we have counts for
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On the Lack of Correlation Between [OIII]/[OII] and Lyman-Continuum Escape Fraction
R. Bassett, E. V. Ryan-Weber, J. Cooke +9
We present the first results of our pilot study of 8 photometrically selected Lyman continuum (LyC) emitting galaxy candidates from the COSMOS field and focus on their optical emis…
On the slow quenching of M* galaxies: heavily-obscured AGNs clarify the picture
Thibaud Moutard, Nicola Malavasi, Marcin Sawicki +2
We investigate the connection between X-ray and radio-loud AGNs and the physical properties of their evolved and massive host galaxies, focussing on the mass-related quenching chan…
Gemini Infrared Multi-Object Spectrograph: Instrument Overview
Suresh Sivanandam, Scott Chapman, Luc Simard +27
The Gemini Infrared Multi-Object Spectrograph (GIRMOS) is a powerful new instrument being built to facility-class standards for the Gemini telescope. It takes advantage of the late…
On the fast quenching of young low-mass galaxies up to z 0.6: new spotlight on the lead role of environment
Thibaud Moutard, Marcin Sawicki, Stéphane Arnouts +5
We investigate the connection between environment and the different quenching channels that galaxies are prone to follow in the rest-frame NUVrK colour diagram, as identified by Mo…
Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common
Christopher C. Hayward, Scott C. Chapman, Charles C. Steidel +19
Interferometric observations have demonstrated that a significant fraction of single-dish submillimetre (submm) sources are blends of multiple submm galaxies (SMGs), but the nature…
Spatially-unresolved SED fitting can underestimate galaxy masses: a solution to the missing mass problem
Robert Sorba, Marcin Sawicki
We perform spatially-resolved, pixel-by-pixel SED fitting on galaxies up to in the Hubble Extreme Deep Field (XDF). Comparing stellar mass estimates from spatially resol…