activity
19972022
most citedDust in the polar region as a major contributor to the IR emission of AGN

216 citations · 2.1k across the 55 of their papers we have counts for

collaborators

54 papers

astro-ph.IM2022★ 28 cited

EMIR, the near-infrared camera and multi-object spectrograph for the GTC

F. Garzón, M. Balcells, J. Gallego +18

We present EMIR, a powerful near-infrared (NIR) camera and multi-object spectrograph (MOS) installed at the Nasmyth focus of the 10.4 m GTC. EMIR was commissioned in mid-2016 and i…

astro-ph.GA2021★ 25 cited

A novel black-hole mass scaling relation based on coronal gas, and its dependence with the accretion disc

M. Almudena Prieto, Alberto Rodríguez-Ardila, Swayamtrupta Panda +1

Using bona-fide black hole (BH) mass estimates from reverberation mapping and the line ratio [SiVI] 1.963m/Br as tracer of the AGN ionising continuum, a novel BH-…

astro-ph.GA2021

A geometric distance to the supermassive black Hole of NGC 3783

GRAVITY Collaboration, A. Amorim, M. Bauböck +45

The angular size of the broad line region (BLR) of the nearby active galactic nucleus (AGN) NGC 3783 has been spatially resolved by recent observations with VLTI/GRAVITY. A reverbe…

astro-ph.GA2021★ 55 cited

The Milky Way's nuclear stellar disc: A dynamically cool and metal-rich component formed from the Central Molecular Zone?

M. Schultheis, T. K. Fritz, G. Nandakumar +10

The nuclear stellar disc (NSD) is, together with the nuclear star cluster (NSC) and the central massive black hole, one of the main components in the central parts of our Milky Way…

astro-ph.GA2021★ 5 cited

Raining in MKW 3s: a Chandra-MUSE analysis of X-ray cold filaments around 3CR 318.1

A. Jimenez-Gallardo, F. Massaro, B. Balmaverde +23

We present the analysis of X-ray and optical observations of gas filaments observed in the radio source 3CR 318.1, associated with NGC 5920, the Brightest Cluster Galaxy (BCG) of M…

astro-ph.GA2021★ 83 cited

The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region

GRAVITY Collaboration, A. Amorim, M. Bauböck +47

Using VLTI/GRAVITY and SINFONI data, we investigate the sub-pc gas and dust structure around the nearby type 1 AGN hosted by NGC 3783. The K-band coverage of GRAVITY uniquely allow…