activity
20032025
most citedMolecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments

762 citations · 3.2k across the 31 of their papers we have counts for

collaborators

30 papers

astro-ph.CO2025

The cosmic web's Lyman- glow at ; hydrodynamic models, dust, and wide-field, narrow-band detection

Oleksii Sokoliuk, John K. Webb, Kenneth M. Lanzetta +12

The diffuse Lyman- glow of the cosmic web has long been predicted but has so far eluded direct detection over cosmologically significant volumes. We construct synthetic Lyman-$α…

astro-ph.SR2025★ 1 cited

PoET: the Paranal solar ESPRESSO Telescope

Nuno C. Santos, Alexandre Cabral, Inês Leite +42

The detection and characterisation of other "Earths", orbiting other suns, is a bold objective of present-day astrophysics. However, this quest is severely challenged by astrophysi…

astro-ph.IM2025

VSTPOL: making the VST a large survey telescope for optical polarimetry

P. Schipani, S. Covino, F. Snik +30

Since the start of operations in 2011, the VLT Survey Telescope (VST) has been one of the most efficient wide-field imagers in the optical bands. However, in the next years the Ver…

astro-ph.EP2024

Assessing methods for telluric removal on atmospheric retrievals of high-resolution optical exoplanetary transmission spectra

Cathal Maguire, Elyar Sedaghati, Neale P. Gibson +2

Recent advancements in ultra-stable ground-based high-resolution spectrographs have propelled ground-based astronomy to the forefront of exoplanet detection and characterisation. R…

astro-ph.IM2022★ 1 cited

Connecting SPHERE and CRIRES+ for the characterisation of young exoplanets at high spectral resolution: status update of VLT/HiRISE

A. Vigan, M. Lopez, M. El Morsy +32

New generation exoplanet imagers on large ground-based telescopes are highly optimised for the detection of young giant exoplanets in the near-infrared, but they are intrinsically…

astro-ph.GA2017★ 70 cited

PAH features within few hundred parsecs of active galactic nuclei

J. J. Jensen, S. F. Hönig, S. Rakshit +6

Spectral features from PAH molecules observed in the mid-IR range are typically used to infer the amount of recent and ongoing star formation (SF) on kpc scales around AGN where mo…