This work focuses on active galactic nuclei (AGNs) and on the relation between the sizes of the hot dust continuum and the broad-line region (BLR). We find that...
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PublicationToward measuring supermassive black hole masses with interferometric observations of the dust continuum
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PublicationTowards a new classification of galaxies: principal component analysis of CALIFA circular velocity curves
We present a galaxy classification system for 238 (E1-Sdm) CALIFA (Calar Alto Legacy Integral Field Area) galaxies based on the shapes and amplitudes of their...
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PublicationTowards universal hybrid star formation rate estimators
Context. To compute the star formation rate (SFR) of galaxies from the rest-frame ultraviolet (UV), it is essential to take the obscuration by dust into account...
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PublicationTracing kinematic (mis)alignments in CALIFA merging galaxies. Stellar and ionized gas kinematic orientations at every merger stage
We present spatially resolved stellar and/or ionized gas kinematic properties for a sample of 103 interacting galaxies, tracing all merger stages: close...
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PublicationTracing Out the Northern Tidal Stream of the Sagittarius Dwarf Spheroidal Galaxy
The main aim of this paper is to report two new detections of tidal debris in the northern stream of the Sagittarius dwarf galaxy located at 45° and 55° from...
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PublicationTracing satellite planes in the Sculptor group. I. Discovery of three faint dwarf galaxies around NGC 253
Context. In recent years, a new generation of large-scale imaging surveys have probed wide field regions for the first time around some nearby galaxies in an...
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PublicationTracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA
Our current knowledge of star formation and accretion luminosity at high redshift (z > 3-4), as well as the possible connections between them, relies mostly on...
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PublicationTracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
We analyse the physical properties of 121 SNR ≥ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450 μm survey. We model their UV-to-radio spectral energy...
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PublicationTracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
We analyse the physical properties of 121 SNR ≥ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450 μm survey. We model their UV-to-radio spectral energy...