The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …

The Gemini Planet Imager (GPI) has as its science instrument an infrared integral field
spectrograph/polarimeter (IFS). Integral field spectrographs are scientificially powerful but …

The near-infrared spectrograph (NIRSpec) on the James Webb Space Telescope (JWST)
offers the first opportunity to use integral-field spectroscopy from space at near-infrared …

We report on the design and performance of the Keck Cosmic Web Imager (KCWI), a
general purpose optical integral field spectrograph that has been installed at the Nasmyth …

We present new, more precise measurements of the mass and distance of our Galaxy's
central supermassive black hole, Sgr A*. These results stem from a new analysis that more …

We report new precision measurements of the properties of our Galaxy's supermassive
black hole. Based on astrometric (1995-2007) and radial velocity (RV; 2000-2007) …

Determining the atmospheric structure and chemical composition of an exoplanet remains a
formidable goal. Fortunately, advancements in the study of exoplanets and their …

We study the link between galaxies and H i-selected absorption systems at z∼ 3–4 in the
MUSE Analysis of Gas around Galaxies (MAGG) survey, an ESO large programme …

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Observational work conducted over the past few decades indicates that all massive galaxies
have supermassive black holes at their centres. Although the luminosities and brightness …