Quasar-driven galactic outflows are a major driver of the evolution of massive galaxies. We
report observations of a powerful galactic-scale outflow in az= 3 extremely red and …

Massive galaxies formed most actively at redshifts z= 1–3 during the period known as"
cosmic noon." Here we present an emission-line study of the extremely red quasar …

Dual quasars—two active supermassive black holes at galactic scales—represent crucial
objects for studying the impact of galaxy mergers and quasar activity on the star formation …

The [O iii] 5007 Å emission line is the most common tracer of warm, ionized outflows in
active galactic nuclei across cosmic time. JWST newly allows us to use mid-IR spectral …

Fast accreting, extremely luminous quasars contribute heavily to the feedback process
within galaxies. While these systems are most common at cosmic noon (z∼ 2), here we …

The evolution of galaxies depends on their masses and local environments; understanding
when and how environmental quenching starts to operate remains a challenge …

Solar flare forecasting research using machine learning (ML) has focused on high-resolution
magnetogram data from the SDO/HMI era covering solar cycle 24 and the start of solar cycle …

Abstract We present Swift Ultraviolet Optical Telescope (UVOT) observations of the deep
field GOODS-N in four near-UV filters. A catalog of detected galaxies is reported, which will …

We report integral field spectroscopy observations with the Near-Infrared Spectrograph on
board JWST targeting the 60 kpc environment surrounding the most luminous quasar known …