Six new supermassive black hole mass determinations from adaptive-optics assisted SINFONI observations
Astronomy and Astrophysics EDP Sciences 625 (2019) A62
Optical integral field spectroscopy of intermediate redshift infrared bright galaxies
Monthly Notices of the Royal Astronomical Societ Oxford University Press 486:4 (2019) 5621-5645
Abstract:
The extreme infrared (IR) luminosity of local luminous and ultraluminous IR galaxies (U/LIRGs; 11 < logLIR/L < 12 and logLIR/L > 12, respectively) is mainly powered by star formation processes triggered by mergers or interactions. While U/LIRGs are rare locally, at z > 1, they become more common, dominate the star formation rate (SFR) density, and a fraction of them are found to be normal disc galaxies. Therefore, there must be an evolution of the mechanism triggering these intense starbursts with redshift. To investigate this evolution, we present new optical SWIFT integral field spectroscopic H α + [N II] observations of a sample of nine intermediate-z (0.2Detecting Earth-like Biosignatures on Rocky Exoplanets around Nearby Stars with Ground-based Extremely Large Telescopes
\baas 51 (2019) 3
Directly Imaging Rocky Planets from the Ground
\baas 51 (2019) 3
The Mid-Infrared Search for Biosignatures on Temperate M-Dwarf Planets
Astro2020: Decadal Survey on Astronomy and Astrophysics 2020 (2019) 462-462