output
20072024
most citedFirst M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

4.3k citations

Showing 2024Show all

8 papers · 1 filter

astro-ph.HE202411 cited

Contemporaneous X-ray Observations of 30 Bright Radio Bursts from the Prolific Fast Radio Burst Source FRB 20220912A

Amanda M. Cook, Paul Scholz, Aaron B. Pearlman +22

We present an extensive contemporaneous X-ray and radio campaign performed on the repeating fast radio burst (FRB) source FRB 20220912A for eight weeks immediately following the so…

astro-ph.GA20245 cited

MeerKAT reveals a ghostly thermal radio ring towards the Galactic Centre

C. Bordiu, M. D. Filipovic, G. Umana +26

We present the serendipitous discovery of a new radio-continuum ring-like object nicknamed Kyklos (J1802-3353), with MeerKAT UHF and L-band observations. The radio ring, which rese…

astro-ph.IM20249 cited

GRAVITY for MATISSE -- Improving the MATISSE performance with the GRAVITY fringe tracker

J. Woillez, R. Petrov, R. Abuter +23

Context: MATISSE, the mid-infrared spectro-imaging instrument of VLTI, was designed to deliver its advertised performance when paired with an external second generation fringe trac…

astro-ph.EP20243 cited

Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)

S. de Regt, C. Ginski, M. A. Kenworthy +9

The observed diversity of exoplanets can possibly be traced back to the planet formation processes. Planet-disk interactions induce sub-structures in the circumstellar disk that ca…

astro-ph.GA20245 cited

A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030

M. D. Gorski, S. Aalto, S. König +23

How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution. One potential way to re…

astro-ph.EP2024

Molecular Gas Tracers in Young and Old Protoplanetary Disks

Dana E. Anderson, L. Ilsedore Cleeves, Geoffrey A. Blake +6

Molecular emission is used to investigate both the physical and chemical properties of protoplanetary disks. Therefore, to accurately derive disk properties, we need a thorough und…