activity
19982024
most citedMetis: the Solar Orbiter visible light and ultraviolet coronal imager

190 citations · 1.6k across the 56 of their papers we have counts for

collaborators

56 papers

astro-ph.SR2024★ 4 cited

Multiwavelength Study of on-disk Coronal Hole Jets with IRIS and SDO observations

Myrto Koletti, Costis Gontikakis, Spiros Patsourakos +1

Solar jets are an important field of study, as they may contribute to the mass and energy transfer from the lower to the upper atmosphere. We use the Interface Region Imaging Spect…

astro-ph.HE2022★ 5 cited

Double flows anchored in a Kerr black hole horizon. I. Meridionally self-similar MHD models with loading terms

L. Chantry, V. Cayatte, C. Sauty +2

Recent observations of supermassive black holes have brought us new information on their magnetospheres. In this study we attempt a theoretical modelling of the coupling of black h…

astro-ph.SR2021★ 50 cited

First light observations of the solar wind in the outer corona with the Metis coronagraph

M. Romoli, E. Antonucci, V. Andretta +65

The investigation of the wind in the solar corona initiated with the observations of the resonantly scattered UV emission of the coronal plasma obtained with UVCS-SOHO, designed to…

astro-ph.SR2019★ 190 cited

Metis: the Solar Orbiter visible light and ultraviolet coronal imager

Ester Antonucci, Marco Romoli, Vincenzo Andretta +100

Metis is the first solar coronagraph designed for a space mission capable of performing simultaneous imaging of the off-limb solar corona in both visible and UV light. The observat…

astro-ph.SR2019★ 9 cited

The Hubble Catalog of Variables (HCV)

A. Z. Bonanos, M. Yang, K. V. Sokolovsky +33

The Hubble Space Telescope (HST) has obtained multi-epoch observations providing the opportunity for a comprehensive variability search aiming to uncover new variables. We have the…

astro-ph.GA2019★ 30 cited

Robust Identification of Active Galactic Nuclei through HST Optical Variability in GOODS-S: Comparison with the X-ray and mid-IR Selected Samples

E. Pouliasis, I. Georgantopoulos, A. Z. Bonanos +9

Identifying Active Galactic Nuclei (AGNs) through their X-ray emission is efficient, but necessarily biased against X-ray-faint objects. We aim to characterize this bias by compari…