activity
20072026
most citedThe spectral energy distribution of the central parsecs of the nearest AGN

112 citations · 1.1k across the 59 of their papers we have counts for

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43 papers · 1 filter

astro-ph.GA2026

ReveaLLAGN 3: Revealing the Infrared Spectral Energy Distributions of Low Luminosity AGN

David Ohlson, Anil C. Seth, Kameron Goold +18

The spectral energy distributions of active galactic nuclei (AGN) provide valuable information on the emission mechanisms taking place in their inner regions. Here we use the James…

astro-ph.GA2026

The black hole-galaxy correlations of the 12 micron local AGN sample: a NuSTAR perspective

M. Gliozzi, L. Spinoglio, J. A. Fernandez-Ontiveros +4

The M-sigma correlation of inactive galaxies plays a crucial role in estimating the black hole mass (MBH) in active galactic nuclei (AGN): 1) it is used to calibrate the reverberat…

astro-ph.GA2025

MIRACLE III. JWST/MIRI expose the hidden role of the AGN outflow in NGC 1068

C. Marconcini, A. Marconi, M. Ceci +27

We present new JWST IFS observations of the active galaxy NGC 1068, combining Mid-IR and optical IFS data from MIRI and MUSE to characterize the multi-phase circumnuclear gas prope…

astro-ph.GA2025★ 1 cited

J-PAS: A Neural Network Approach to Single Stellar Population Characterization

H. Domínguez Sánchez, P. Coelho, G. Bruzual +28

J-PAS (Javalambre Physics of the Accelerating Universe Astrophysical Survey) will present a groundbreaking photometric survey covering 8500 deg of the visible sky from Javalamb…

astro-ph.GA2025★ 2 cited

JWST/MIRI-MRS view of the metal-poor galaxy CGCG 007-025: the spatial location of PAHs and very highly ionized gas

Macarena G. del Valle-Espinosa, Matilde Mingozzi, Bethan James +16

Polycyclic Aromatic Hydrocarbons (PAHs) are key diagnostics of the physical conditions in the interstellar medium and are widely used to trace star formation in the mid-infrared (m…

astro-ph.GA2025★ 1 cited

J-PLUS: The stellar mass function of quiescent and star-forming galaxies at 0.05 <= z <= 0.2

F. D. Arizo-Borillo, C. Lopez-Sanjuan, I. Pintos-Castro +22

Aims. We derive the stellar mass function (SMF) of quiescent and star-forming galaxies at z <= 0.2 using 12-band optical photometry from the third data release (DR3) of the Javalam…

astro-ph.GA2025★ 8 cited

MIRACLE I.: Unveiling the Multi-Phase, Multi-Scale physical properties of the Active Galaxy NGC 424 with MIRI, MUSE, and ALMA

C. Marconcini, A. Feltre, I. Lamperti +26

We present the analysis of the multi-phase gas properties in the Seyfert II galaxy NGC 424, using spatially resolved spectroscopic data from JWST/MIRI, part of the Mid-InfraRed Act…

astro-ph.GA2025★ 2 cited

Spatially-resolved spectro-photometric SED Modeling of NGC 253's Central Molecular Zone I. Studying the star formation in extragalactic giant molecular clouds

Pedro K. Humire, Subhrata Dey, Tommaso Ronconi +29

Studying the interstellar medium in nearby starbursts is essential for understanding the physical mechanisms driving these objects, thought to resemble young star-forming galaxies.…

astro-ph.GA2024

The PARSEC view of star formation in galaxy centres: from protoclusters to star clusters in an early-type spiral

Almudena Prieto, Gladis Magris C., Gustavo Bruzual +2

Understanding star formation in galaxies requires resolving the physical scale on which star formation often occurs: the scale of star clusters. We present a multiwavelength, eight…

astro-ph.GA2024★ 1 cited

A case study of gas impacted by black-hole jets with the JWST: outflows, bow shocks, and high excitation of the gas in the galaxy IC5063

K. M. Dasyra, G. F. Paraschos, F. Combes +8

We present James Webb Space Telescope MIRI data of the inner 3x2kpc^2 of the galaxy IC5063, in which the jets of a supermassive black hole interact with the gaseous disk they are c…

astro-ph.GA2023

The spectral energy distributions and the bolometric luminosities of local AGN: study of the complete 12 micron AGN sample

Luigi Spinoglio, Juan Antonio Fernandez-Ontiveros, Matthew A. Malkan

We measure the bolometric luminosity of a complete and unbiased 12 micron-selected sample of active galactic nuclei (AGN) in the local Universe. For each galaxy we used a 10-band r…

astro-ph.GA2023

ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052

K. Goold, A. Seth, M. Molina +28

We present the first results from the Revealing Low-Luminosity Active Galactic Nuclei (ReveaLLAGN) survey, a JWST survey of seven nearby LLAGN. We focus on two observations with th…

astro-ph.GA2022★ 10 cited

J-PLUS DR3: Galaxy-Star-Quasar classification

R. von Marttens, V. Marra, M. Quartin +20

The Javalambre Photometric Local Universe Survey (J-PLUS) is a 12-band photometric survey using the 83-cm JAST telescope. Data Release 3 includes 47.4 million sources. J-PLUS DR3 o…

astro-ph.GA2022★ 19 cited

The high-ionization IR fine-structure lines as bolometric indicators of the AGN power: study of the complete 12 micron AGN sample

Luigi Spinoglio, Juan Antonio Fernandez-Ontiveros, Matthew A. Malkan

The high-ionization mid-IR lines, excited in the Narrow Line Regions (NLR) of Active Galactic Nuclei (AGN), barely affected by stellar excitation and dust extinction, trace the AGN…

astro-ph.GA2022

Linking pressure gradients with the stability of molecular clouds in galactic outflows

K. M. Dasyra, G. F. Paraschos, T. Bisbas +2

The jets launched by actively accreting black holes are capable of launching several of the massive (million or billion solar mass) molecular outflows observed in galaxies. These o…

astro-ph.GA2021★ 1 cited

Galaxy evolution through infrared and submillimeter spectroscopy: Measuring star formation and black hole accretion with JWST and ALMA

Sabrina Mordini, Luigi Spinoglio, Juan Antonio Fernández-Ontiveros

Rest-frame mid- to far-infrared spectroscopy is a powerful tool to study how galaxies formed and evolved, because a major part of their evolution occurs in heavily dust enshrouded…

astro-ph.GA2021★ 2 cited

Simulating infrared spectro-photometric surveys with a SPRITZ

L. Bisigello, C. Gruppioni, F. Calura +19

Mid- and far-infrared (IR) photometric and spectroscopic observations are fundamental to a full understanding of the dust-obscured Universe and the evolution of both star formation…

astro-ph.GA2021★ 20 cited

SOFIA observations of far-IR fine-structure lines in galaxies to measure metallicity

Luigi Spinoglio, Juan Antonio Fernandez-Ontiveros, Matthew A. Malkan +8

We present new and archival SOFIA FIFI-LS far-IR spectroscopic observations of 25 local galaxies of either the [OIII]52um and/or the [NIII]57um lines. Including other 31 galaxies f…

astro-ph.GA2021★ 3 cited

CO kinematics unveil outflows plausibly driven by a young jet in the Gigahertz Peaked Radio Core of NGC6328

Michalis Papachristou, Kalliopi Maria Dasyra, Juan Antonio Fernández-Ontiveros +3

We report the detection of outflowing molecular gas in the center of the nearby (z=0.014) massive radio galaxy NGC6328. The radio core of the galaxy, PKS B1718-649, is identified a…

astro-ph.GA2021★ 9 cited

The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena

L. Barchiesi, F. Pozzi, C. Vignali +21

In the BH-galaxy co-evolution framework, most of the star-formation (SF) and the black hole (BH) accretion is expected to take place in highly obscured conditions. Thus, obscured A…

astro-ph.GA2021★ 7 cited

Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission

Luigi Spinoglio, Sabrina Mordini, Juan Antonio Fernandez-Ontiveros +31

We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering large cosmological volu…

astro-ph.GA2020★ 9 cited

/PACS OH Spectroscopy of Seyfert, LINER, and Starburst Galaxies

Jordan N. Runco, Matthew A. Malkan, Juan Antonio Fernández-Ontiveros +2

We investigated the 65m, 71m, 79m, 84m, 119m, and 163m OH doublets of 178 local (0 < < 0.35) galaxies. They were observed using the /PACS spectromet…

astro-ph.GA2020★ 4 cited

Low optical polarisation at the core of the optically-thin jet of M87

A. Y. Fresco, J. A. Fernández-Ontiveros, M. A. Prieto +2

We study the optical linear and circular polarisation in the optically-thin regime of the core and jet of M87. Observations were acquired two days before the Event Horizon Telescop…

astro-ph.GA2020

The physics of Galaxy Evolution with SPICA observations

Luigi Spinoglio, Juan A. Fernandez-Ontiveros, Sabrina Mordini

The evolution of galaxies at Cosmic Noon (redshift 1<z<3) passed through a dust-obscured phase, during which most stars formed and black holes in galactic nuclei started to shine,…