activity
20242026
collaborators

5 papers

astro-ph.IM2026

Thermal background reduction for mid-infrared imaging by low-rank background and sparse point-source modelling

R. A. R. Moens, A. G. M. Pietrow, B. Brandl +1

Mid-infrared astronomy from the ground faces critical challenges in accurately detecting and quantifying sources due to the dominant spatially and time-variable background noise. M…

astro-ph.GA2025

First detection of ices in intermediate-mass young stellar objects beyond the Milky Way

Guido De Marchi, Nolan Habel, Margaret Meixner +15

Using NIRSpec on JWST, we studied a sample of 15 intermediate-mass (1.8-4.1 Msun) young stellar objects (YSOs) previously identified with MIRI photometry in the low-metallicity NGC…

astro-ph.SR2025

Kinematic evidence of magnetospheric accretion for Herbig Ae stars with JWST NIRSpec

Ciarán Rogers, Bernhard Brandl, Guido de Marchi

Hydrogen emission lines have been used to estimate the mass accretion rate of pre-main-sequence stars for over years, although the physical origin of these lines is still uncl…

astro-ph.SR2025

Externally irradiated young stars in NGC 3603. A JWST NIRSpec catalogue of pre-main-sequence stars in a massive star formation region

Ciarán Rogers, Guido de Marchi, Bernhard Brandl

NGC 3603 is the optically brightest massive star forming region (SFR) in the Milky Way, representing a small scale starburst region. Studying young stars in regions like this allow…

astro-ph.SR2024

Protoplanetary discs around sun-like stars appear to live longer when the metallicity is low

Guido De Marchi, Giovanna Giardino, Katia Biazzo +17

Previous Hubble Space Telescope (HST) observations of the star-forming cluster NGC 346 in the Small Magellanic Cloud (SMC) had revealed a large population of pre-main sequence (PMS…