Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Astrophysics and Star Formation Studies, and Stellar, planetary, and galactic studies.
MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
Metallicity calibrations based on auroral lines from PHANGS–MUSE data
<i>Euclid</i> preparation
Feeding and feedback processes in the Spiderweb proto-intracluster medium <i>(Corrigendum)</i>
Star-formation-driven outflows in local dwarf galaxies as revealed from [CII] observations by<i>Herschel</i>
A solar metallicity galaxy at <i>z</i> &gt; 7? Possible detection of the [N <scp>ii</scp>] 122 μm and [O <scp>iii</scp>] 52 μm lines
A dusty compact object bridging galaxies and quasars at cosmic dawn
The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4
The ALPINE-ALMA [C II] survey. Dust attenuation curves at <i>z</i> = 4.4–5.5
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [C <scp>ii</scp>] Survey: kinematic diversity and rotation in massive star-forming galaxies at <i>z</i> ~ 4.4–5.9
The ALPINE-ALMA [C II] survey: Luminosity function of serendipitous [C II] line emitters at z ∼5
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [C II] survey
The ALPINE-ALMA [CII] survey
The ALPINE-ALMA [C II] survey
The ALPINE-ALMA [CII] survey
The ALPINE–ALMA [C ii] Survey: Size of Individual Star-forming Galaxies at z = 4–6 and Their Extended Halo Structure