Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …

UV radiation feedback from young massive stars plays a key role in the evolution of giant
molecular clouds (GMCs) by photoevaporating and ejecting the surrounding gas. We …

We present two large catalogs of active galactic nucleus (AGN) candidates identified across
30,093 deg 2 of extragalactic sky from the Wide-field Infrared Survey Explorer's AllWISE …

Their ubiquity and extreme densities make star clusters probes of prime importance of
galaxy evolution. Old globular clusters keep imprints of the physical conditions of their …

We use 3D hydrodynamical models to investigate the effects of massive star feedback from
winds and supernovae on inhomogeneous molecular material left over from the formation of …

We present an assessment of the performance of WISE and the AllWISE data release for a
section of the Galactic Plane. We lay out an approach to increasing the reliability of point …

Aims. A comprehensive and homogeneous determination of stellar parameters for the stars
observed by the Kepler space telescope is necessary for statistical studies of their …

We explored the AllWISE catalogue of the Wide-field Infrared Survey Explorer (WISE)
mission and identified Young Stellar Object (YSO) candidates. Reliable 2MASS and WISE …

We extend our previous smoothed particle hydrodynamics parameter study of the effects of
photoionization from O-stars on star-forming clouds to include initially unbound clouds. We …

Forward modeling of the full galaxy SED is a powerful technique, providing self-consistent
constraints on stellar ages, dust properties, and metallicities. However, the accuracy of these …