## We develop a formalism to model the luminosity functions (LFs) of radio–loud Active Galactic Nuclei (AGN) at GHz frequencies by the cosmological evolution of the supermassive black hole (SMBH) hosted in their nuclei.

Modelling radio luminosity functions of radio-loud AGN by the cosmological evolution of supermassive black holes

## Over the past decade, research has revealed contradictory results on whether mergers of galaxies of similar mass, so-called major mergers, are the dominant or at least an essential mechanism for the formation of active galactic nuclei (AGN) and the growth of supermassive black holes (SMBH) in galaxies.

The Intricate Connection Between Major Mergers and AGN with the Highest Eddington Ratios

## The combination of the linear size from reverberation mapping (RM) and the angular distance of the broad-line region (BLR) from spectroastrometry (SA) in active galactic nuclei can be used as a “standard ruler” to measure the Hubble constant H 0.

The Deviation of the Size of the Broad-line Region between Reverberation Mapping and Spectroastrometry

## Such a recoiling SMBH may be detectable as an active galactic nucleus (AGN) broad-line region offset by up to 10 kpc from a disturbed host galaxy.

AGNs on the Move: A Search for Off-nuclear AGNs from Recoiling Supermassive Black Holes and Ongoing Galaxy Mergers with the Zwicky Transient Facility

## We investigate the physical properties—such as the stellar mass (M∗), star-formation rate (SFR), infrared (IR) luminosity (LIR), X-ray luminosity (LX), and hydrogen column density (NH)—of mid-IR (MIR) galaxies and active galactic nuclei (AGN) at z < 4 in the 140 deg2 field observed by SRG/eROSITA using the Performance-and-Verification-Phase program named the eROSITA Final Equatorial Depth Survey (eFEDS).

The eROSITA Final Equatorial-Depth Survey (eFEDS). A multiwavelength view of WISE mid-infrared galaxies/active galactic nuclei

## Henize 2–10 (He 2–10) is a nearby (D = 9 Mpc) starbursting blue compact dwarf galaxy that boasts a high star formation rate and a low-luminosity active galactic nucleus.

Toward a More Complex Understanding of Natal Super Star Clusters with Multiwavelength Observations

## Both the radio International Celestial Reference Frame (ICRF) and the optical Gaia Celestial Reference Frame (Gaia-CRF2) are derived from observations of jets produced by the Super Massive Black Holes (SMBH) powering active galactic nuclei and quasars.

Anchored in Shadows: Tying the Celestial Reference Frame Directly to Black Hole Event Horizons

## Massive black holes (MBHs) inhabit galaxy centers, power luminous quasars and Active Galactic Nuclei (AGN) and shape their cosmic environment with the energy they produce.

The origins of massive black holes

## Astrometric positions of radio-emitting active galactic nuclei (AGNs) can be determined with sub-milliarcsec accuracy using very long baseline interferometry (VLBI).

Change in the Radio Structure and Position of the Quasar CTA 21

## 45, which was regularly monitored as part of the Interferometric Monitoring of GAmma-ray Bright Active Galactic Nuclei (iMOGABA) program – a key science program of the Korean Very long baseline interferometry Network (KVN).

Interferometric monitoring of gamma-ray bright AGNs: Measuring the magnetic field strength of 4C +29.45

## The star formation activity of the host galaxies of active galactic nuclei provides valuable insights into the complex interconnections between black hole growth and galaxy evolution.

The Infrared Emission and Vigorous Star Formation of Low-redshift Quasars

## There is an ongoing debate on whether feedback from active galactic nuclei (AGNs) can effectively regulate the star formation activities in their host galaxies.

Unraveling the Complex Structure of AGN-driven Outflows. V. Integral-field Spectroscopy of 40 Moderate-luminosity Type-2 AGNs

## Theoretical models show that the power of relativistic jets of active galactic nuclei depends on the spin and mass of the central supermassive black holes, as well as the accretion.

The Powers of Relativistic Jets Depend on the Spin of Accreting Supermassive Black Holes

## Recoiling active galactic nuclei (AGNs) can be formed after the merging of two galaxies and their central supermassive black holes.

4C 18.47: A Recoiling AGN Candidate in the Radio and Infrared

## We also consider electron densities in the accretion disc up to 1020 cm−3, which are found in most of the stellar mass black holes and in some active galactic nuclei.

Modelling correlated variability in accreting black holes: the effect of high density and variable ionization on reverberation lags

## Accretion states, which are universally observed in stellar-mass black holes in X-ray binaries, might be expected in active galactic nuclei (AGN).

X-ray binary accretion states in active galactic nuclei? Sensing the accretion disc of supermassive black holes with mid-infrared nebular lines

## Here we consider the perspective to detect sub-pc super-massive binary black-hole (SMBBH) systems using long-term photometric and spectroscopic monitoring campaigns of active galactic nuclei.

Detecting subparsec supermassive binary black holes: Long-term monitoring perspective

## The recent report of an association of the gravitational-wave (GW) binary black hole (BBH) merger GW190521 with a flare in the active galactic nuclei (AGNs) J124942.

Do LIGO/Virgo Black Hole Mergers Produce AGN Flares? The Case of GW190521 and Prospects for Reaching a Confident Association

## Inspired by our serendipitous discovery of six active galactic nuclei (AGNs) with varying broad-Hα fluxes over years from our search for intermediate-mass black holes (IMBHs), we conduct a systematic investigation of changing-look (CL) and large-variability AGNs.

Local Active Galactic Nuclei with Large Broad-Hα Variability Reside in Red Galaxies

## These might be intermediate mass black holes or low luminosity active galactic nuclei near the center of the galaxy in the process of merging.

Resolving the ultraluminous X-ray sources in the Ly α emitting galaxy Haro 11

## Determining the black hole masses in active galactic nuclei (AGN) is of crucial importance to constrain the basic characteristics of their central engines and shed light on their growth and co-evolution with their host galaxies.

Estimating black hole masses in obscured AGN using X-rays

## Six galaxies host active galactic nuclei, three of which have the estimated black hole masses substantially below those expected for their (pseudo-)bulge properties suggesting poor merger histories.

Observational insights on the origin of giant low surface brightness galaxies

## Many X-ray bright active galactic nuclei (AGNs) are predicted to follow an extended stage of obscured black hole growth.

Where Do Obscured AGN Fit in a Galaxy’s Timeline?

## Contrary to expectations from scenarios of black hole growth driven by galaxy interactions and mergers, dual active galactic nuclei (AGN) with kiloparsec separations are rarely observed and are very difficult to identify, in particular at high redshifts (i.

A meeting at z~3: young massive galaxies and an AGN within 30kpc of the luminous QSO LBQS0302-0019

## Blazars are active galactic nuclei with their relativistic jets pointing toward the observer, comprising two major subclasses, flat-spectrum radio quasars (FSRQs) and BL Lac objects.

The Changing-look Blazar B2 1420+32

## BL Lacertae objects (BL Lacs) and flat-spectrum radio quasars (FSRQs), known as blazars, are low- and high-luminosity radio-loud Active Galactic Nuclei (AGNs) with relativistic jets pointed towards Earth (1).

A BL Lacertae object at a cosmic age of 800 Myr

## We demonstrate that a population of active galactic nuclei (AGN) can describe the observed spectrum of ultra-high-energy cosmic rays (UHECRs) at and above the ankle, and that the dominant contribution comes from low-luminosity BL Lacertae objects.

Active Galactic Nuclei Jets as the Origin of Ultrahigh-Energy Cosmic Rays and Perspectives for the Detection of Astrophysical Source Neutrinos at EeV Energies.

## Active Galactic Nuclei are the dominant sources of gamma rays outside our Galaxy and also candidates for being the source of ultra-high energy cosmic rays.

Millimeter-wave Monitoring of Active Galactic Nuclei with the Africa Millimetre Telescope

## Radio-loud active galactic nuclei (RL AGNs) show very powerful jet emission in the radio band, while the radio-quiet (RQ) ones do not.

XMM-Newton spectrum of the radio-loud quasar 3C 215: slim accretion disk or SMBH binary?

## We develop a formalism to model the luminosity functions (LFs) of radio–loud Active Galactic Nuclei (AGN) at GHz frequencies by the cosmological evolution of the supermassive black hole (SMBH) hosted in their nuclei.

Modelling radio luminosity functions of radio-loud AGN by the cosmological evolution of supermassive black holes

## Henize 2–10 (He 2–10) is a nearby (D = 9 Mpc) starbursting blue compact dwarf galaxy that boasts a high star formation rate and a low-luminosity active galactic nucleus.

Toward a More Complex Understanding of Natal Super Star Clusters with Multiwavelength Observations

## In the accretion flows around low-luminosity active galactic nuclei such as M87, electrons and ions are not in thermal equilibrium.

Comparison of the ion-to-electron temperature ratio prescription: GRMHD simulations with electron thermodynamics

## We present a multi-wavelength study of the gaseous medium surrounding the nearby active galactic nucleus (AGN) Fornax A.

AGN feeding and feedback in Fornax A. Kinematical analysis of the multi-phase ISM

## In the future, it is expected that additional and more sensitive VLBI observations will be pursued for other nearby active galactic nuclei (AGN), and it is therefore important to understand which possible features can be expected in such images.

General relativistic radiation transport: implications for VLBI/EHT observations of AGN discs, winds, and jets

## Most likely this system contains a dual active galactic nucleus (AGN), but we are possibly detecting an AGN plus a parsec-scale X-ray jet, the latter lying in a region at very high magnification.

Resolving Complex Inner X-Ray Structure of the Gravitationally Lensed AGN MG B2016+112

## 03) dual active galactic nuclei (AGNs) Mrk 739, whose projected nuclear separation is ∼3.

The Complex Gaseous and Stellar Environments of the Nearby Dual Active Galactic Nucleus Mrk 739

## Radio active galactic nuclei (RAGNs) are mainly found in dense structures (i.

Implications of the Environments of Radio-detected Active Galactic Nuclei in a Complex Protostructure at z ∼ 3.3

## Remnant radio galaxies represent an important phase in the life-cycle of radio active galactic nuclei.

Multi-frequency characterisation of remnant radio galaxies in the Lockman Hole field

## 45, which was regularly monitored as part of the Interferometric Monitoring of GAmma-ray Bright Active Galactic Nuclei (iMOGABA) program – a key science program of the Korean Very long baseline interferometry Network (KVN).

Interferometric monitoring of gamma-ray bright AGNs: Measuring the magnetic field strength of 4C +29.45

## Many X-ray bright active galactic nuclei (AGNs) are predicted to follow an extended stage of obscured black hole growth.

Where Do Obscured AGN Fit in a Galaxy’s Timeline?

## Even in deep X-ray surveys, Compton-thick active galactic nuclei (CT AGNs, NH ≥ 1.

Multiwavelength Selected Compton-thick AGNs in Chandra Deep Field-South Survey

## The X-ray emission of JO201 is provided by both the Compton-thick active galactic nucleus (L = 2.

GASP XXXIV: Unfolding the Thermal Side of Ram Pressure Stripping in the Jellyfish Galaxy JO201

## We are compiling a new list of gamma-ray jetted active galactic nuclei (AGN), starting from the fourth catalog of point sources of the Fermi Large Area Telescope (LAT).

A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei—Preliminary Results

## Mrk 926 is known to be a highly variable active galactic nucleus.

The Great Slump: Mrk 926 reveals discrete and varying Balmer line satellite components during a drastic phase of decline.

## Variable active galactic nuclei showing periodic light curves have been proposed as massive black hole binary (MBHB) candidates.

Binary black hole signatures in polarized light curves

## Luminous active galactic nuclei and X-ray binaries often contain geometrically thin, radiatively cooled accretion discs.

Disc tearing and Bardeen–Petterson alignment in GRMHD simulations of highly tilted thin accretion discs

## Absorption lines with high blueshifted velocities are frequently found in the ultraviolet (UV) and X-ray spectra of luminous active galactic nuclei (AGNs).

Magnetohydrodynamic Winds Driven by the Line Force from the Standard Thin Disk around Supermassive Black Holes. I. The Case of Weak Magnetic Field

## We present the results of photometric reverberation mapping observations on the changing look active galactic nucleus Mrk 590 at z = 0.

Changing look AGN Mrk 590: Broad line region and black hole mass from photometric reverberation mapping

## The changes of broad emission lines should be a crucial issue in understanding the physical properties of changing-look active galactic nuclei (CL-AGNs).

Reverberation Mapping of Changing-look Active Galactic Nucleus NGC 3516

## UV/optical variation, likely driven by accretion disk turbulence, is a defining characteristic of type 1 active galactic nuclei and quasars.

More Variable Quasars Have Stronger Emission Lines

## The corresponding optical spectrum indicates that this object is a type-1 active galactic nucleus (AGN).

The eROSITA Final Equatorial-Depth Survey (eFEDS)

## We investigate the relation of black hole mass versus host stellar mass and that of mass accretion rate versus star formation rate (SFR) in moderately luminous ( ), X-ray selected broad-line active galactic nuclei (AGNs) at z = 1.

Black Hole and Galaxy Coevolution in Moderately Luminous Active Galactic Nuclei at z ∼ 1.4 in SXDF

## We investigate the use of the [O II] $\lambda3727$ emission line as a star formation rate (SFR) estimator using Sloan Digital Sky Spectra for nearly 100,000 star-forming galaxies and 5,500 galaxies with narrow-line active galactic nuclei.

Recalibration of [O II] $\lambda 3727$ as a Star Formation Rate Estimator for Active and Inactive Galaxies

## Using ultraviolet (UV) nebular line ratio diagnostics, Very Large Telescope (VLT)/X-shooter observations rule out strong active galactic nuclei (AGN) activity, indicating a stellar origin of the hard radiation field instead.

Assessing the sources of reionization: a spectroscopic case study of a 30× lensed galaxy at z ∼ 5 with Lyα, C iv, Mg ii, and [Ne iii]

## The relativistic BAL features, combined with a strongly blueshifted C iv emission line, indicate that there is a strong active galactic nucleus (AGN)-driven outflow in this system.

A Luminous Quasar at Redshift 7.642

## 5 M ⊙ and were selected to host active galactic nuclei (AGNs) based on narrow emission line ratios derived from Sloan Digital Sky Survey spectroscopy.

The Diverse Morphologies and Structures of Dwarf Galaxies Hosting Optically Selected Active Massive Black Holes

## Six galaxies host active galactic nuclei, three of which have the estimated black hole masses substantially below those expected for their (pseudo-)bulge properties suggesting poor merger histories.

Observational insights on the origin of giant low surface brightness galaxies

## Heavily obscured active galactic nuclei (AGNs) are known to show deep silicate absorption features in the mid-infrared (mid-IR) wavelength range of 10–20 μm.

A systematic study of silicate absorption features in heavily obscured AGNs observed by Spitzer/IRS

## Thus, obscured active galactic nuclei (AGN) are very difficult to identify in optical or X-ray bands but shine bright in the IR.

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

## One way to test these theories is to monitor TeV photons time-of-flight emitted by distant, highly energetic and highly variable astrophysical sources such as flaring active galactic nuclei.

Modeling intrinsic time-lags in flaring blazars in the context of Lorentz Invariance Violation searches

## High-energy photons emitted by flaring active galactic nuclei (AGNs) have been used for many years to constrain modified dispersion relations in vacuum encountered in the context of quantum gravity phenomenology.

Modeling spectral lags in active galactic nucleus flares in the context of Lorentz invariance violation searches

## Here we present the first results of our optical follow-up of these radio-selected active galactic nuclei (AGNs) in dwarf galaxies using integral field unit (IFU) data from Gemini-North.

Outflows, Shocks, and Coronal Line Emission in a Radio-selected AGN in a Dwarf Galaxy

## Based on the spectroscopic and shear catalogs for SDSS galaxies in the local Universe, we compare optically-selected active galactic nuclei (AGNs) with control star-forming and quiescent galaxies on galactic, inter-halo and larger scales.

Hosts and triggers of AGNs in the Local Universe

## We use X-ray Active Galactic Nuclei (AGN) observed by the Chandra X-ray Observatory within the 9.

The role of AGN and its obscuration on the position of the host galaxy relative to Main Sequence

## GSN 069 is an ultra-soft X-ray active galactic nucleus that previously exhibited a huge X-ray outburst and a subsequent long-term decay.

Evidence of a Tidal-disruption Event in GSN 069 from the Abnormal Carbon and Nitrogen Abundance Ratio

## Studies based on published IceCube alerts and radio observations report a possible radio-neutrino correlation in both gamma-ray bright and gamma-ray dim active galactic nuclei (AGN).

Testing the AGN Radio and Neutrino correlation using the MOJAVE catalog and 10 years of IceCube Data

## Studies based on published IceCube alerts and radio observations report a possible radio-neutrino correlation in both gamma-ray bright and gamma-ray dim active galactic nuclei (AGN).

Testing the AGN Radio and Neutrino correlation using the MOJAVE catalog and 10 years of IceCube Data

## We studied the absorption features of CO lines against the continuum originating from the heated dust in the obscuring tori around active galactic nuclei (AGNs).

Circumnuclear Multi-phase Gas in Circinus Galaxy IV: Absorption Owing to High-J CO Rotational Transitions

## Information on the structure around active galactic nuclei (AGN) has long been derived from measuring lags in their varying light output at different wavelengths.

Infrared lags in the light curves of AGNs measured using a deep survey

## The absorbed soft X-ray (<1 keV) emission from Compton thin type-II active galactic nuclei (AGNs) with neutral absorption columns in the range N H = 1021−23 cm−2 may contain emission from star formation or scattered photons from the primary X-ray emission in Compton-thin circumnuclear gas extending out to ∼1  kpc, or leaky-absorbers along the line of sight allowing a part of the primary AGN emission to manifest in the soft X-rays.

The Nature of the Absorbed Soft X-Ray Variations in Compton-thin Type-II Active Galactic Nuclei

## I have studied the variability of the FeKα emission line flux in response to changes in the 2–10 keV unabsorbed flux in a sample of Compton thin type-II active galactic nuclei.

The Distance of the Narrow FeKalpha Emitting Region for a Sample of Compton-thin Type-II Active Galactic Nuclei

## Many low-redshift active galactic nuclei harbor a supermassive black hole accreting matter at low or medium rates.

Nonthermal processes in hot accretion flows onto supermassive black holes: An inhomogeneous model

## From spectral index mapping our large frequency coverage reveals that the curvature of the different ring spectra increases with distance away from the central active galactic nucleus.

Origin of the ring structures in Hercules A. Sub-arcsecond 144 MHz to 7 GHz observations

## However, theoretical studies indicate that ram pressure from a hot wind, driven either by the central active galactic nucleus (AGN) or a starburst, cannot accelerate existing cold gas to such high speeds without destroying it.

Dynamics and Morphology of Cold Gas in Fast, Radiatively Cooling Outflows: Constraining AGN Energetics with Horseshoes

## However, dipoles from number counts, sky brightness or redshift distributions in large samples of distant active galactic Nuclei (AGNs) have yielded values of the peculiar velocity many times larger than that from the CMBR, though in all cases the directions agreed with the CMBR dipole.

Solar System Peculiar Motion from Mid Infra Red AGNs and Its Cosmological Implications

## However, some other dipoles, for instance, from the number counts, sky brightness or redshift distributions in large samples of distant Active Galactic Nuclei (AGNs), have yielded values of the peculiar velocity many times larger than that from the CMBR, though surprisingly, in all cases the directions agreed with the CMBR dipole.

Our Peculiar Motion Inferred from Number Counts of Mid Infra Red AGNs and the Discordance Seen with the Cosmological Principle

## Of the 750 sources of known or suspected origin in the catalog, 56% are extragalactic (mostly active galactic nuclei, AGN; and clusters of galaxies) and the rest are Galactic (mostly cataclysmic variables, CVs; and lowand high-mass X-ray binaries).

SRG/ART-XC all-sky X-ray survey: catalog of sources detected during the first year

## The link between the two fundamental frames is realized through two samples of distant extragalactic sources, mostly active galactic nuclei and quasars, but only the smaller sample of radio-loud ICRF sources with optical counterparts is available to determine the mutual orientation.

Functional Principal Component Analysis of Radio–Optical Reference Frame Tie

## 35) colors suggest that Mrk 1239 is more similar to type-2 active galactic nuclei like NGC 1068.

Mrk 1239: a Type-2 Counterpart of Narrow-line Seyfert-1?

## This object is a local radio-quiet type 2 active galactic nucleus (AGN) previously selected as a double AGN candidate on the basis of the double-peaked [OIII] emission line.

A possible sub-kiloparsec dual AGN buried behind the galaxy curtain

## Spatially resolved spectroscopy from the Sloan Digital Sky Survey IV Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey has revealed a class of quiescent, relatively common early-type galaxies termed “red geysers” that possibly host large-scale active galactic nuclei–driven winds.

Evidence of Wind Signatures in the Gas Velocity Profiles of Red Geysers

## These galaxies show unique signatures in spatially resolved strong line emission maps that have been interpreted as large-scale active galactic nucleus–driven ionized winds.

Signatures of Inflowing Gas in Red Geyser Galaxies Hosting Radio Active Galactic Nuclei

## The Langmuir–Landau-Centrifugal Drive (LLCD), which can effectively “convert” gravitational energy into particles, is explored as a driving mechanism responsible for the extreme thermal luminosity acquired by some active galactic nuclei (AGN).

On the Heating of AGN Magnetospheres

## 06 K sky brightness produced by active galactic nuclei and ≈96% of the ΔT b ∼ 0.

Source Counts Spanning Eight Decades of Flux Density at 1.4 GHz

## ULIRGs can also host an active galactic nucleus (AGN).

IceCube Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies

## We present a multi-wavelength study of the gaseous medium surrounding the nearby active galactic nucleus (AGN) Fornax A.

AGN feeding and feedback in Fornax A. Kinematical analysis of the multi-phase ISM

10.3390/UNIVERSE7040083

## The Langmuir–Landau-Centrifugal Drive (LLCD), which can effectively “convert” gravitational energy into particles, is explored as a driving mechanism responsible for the extreme thermal luminosity acquired by some active galactic nuclei (AGN).

On the Heating of AGN Magnetospheres

10.3847/1538-4357/abdd37

## 06 K sky brightness produced by active galactic nuclei and ≈96% of the ΔT b ∼ 0.

Source Counts Spanning Eight Decades of Flux Density at 1.4 GHz

10.3847/2515-5172/ac2eef

## We showcase a tool suite that enables the fitting of soft X-ray spectra in active galactic nuclei (AGNs), without the need for specialist software, allowing access to AGN physics for school students.

A Study of the Soft X-Ray Emission Lines in NGC 4151. II. The Internal Plasma Properties

## ULIRGs can also host an active galactic nucleus (AGN).

IceCube Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies

## UltraFast Outflows (UFO) are observed in some active galactic nuclei (AGN), with blueshifted and highly ionised Fe-K absorption features.

UV line-driven disc wind as the origin of UltraFast Outflows in AGN

10.3847/1538-4357/abfb67

## Stars can either be formed in or captured by the accretion disks in active galactic nuclei (AGNs).

Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars

10.3847/1538-4357/abdfd3

## 3) active galactic nuclei (AGNs).

Subarcsecond Mid-infrared View of Local Active Galactic Nuclei. IV. The L- and M-band Imaging Atlas* * This atlas makes use of European Southern Observatory (ESO) observing programs 65.P-0519, 67.B-0332, 70.B-0393, 71.B-0379, 71.B-0404, 072.B-0397, 074.B-0166, 085.B-0639, and 290.B-5133.

10.20944/PREPRINTS202106.0302.V1

## Astrophysical accretion processes near the black hole candidates, such as active galactic nuclei (AGN), X-ray binary (XRB), and other astrophysical sources, are associated with high-energetic emission of radiation of relativistic particles and outflows (winds and/or jets).

Magnetized black hole as an accelerator of charged particle

10.1051/0004-6361/202039770

## 5 × 109 yrs), and, following mid-infrared criteria, two galaxies may contain an active galactic nucleus.

Jellyfish galaxy candidates in MACS J0717.5+3745 and 39 other clusters of the DAFT/FADA and CLASH surveys

## Based on Te determinations through the [O iii](λ4959+λ5007)/λ4363 emission line ratio of each spaxel, temperature variations are quantified by computing the integrated value of the temperature fluctuation parameter (t) projected in the plane of the sky tA, for the first time in Active Galactic Nuclei.

Electron temperature fluctuations in Seyfert galaxies

10.20944/preprints202106.0521.v1

## We then implement a blast-wave model, which explains the genesis of UV photons escape fraction in the context of feedback and co-evolution between galaxies and Active Galactic Nuclei.

The Epoch of Reionization in Warm Dark Matter Scenarios

10.1051/0004-6361/202039976

## This work aims at studying the impact of the energetic feedback due to active galactic nuclei (AGN) on the formation and evolution of ETGs.

The role of AGN feedback in the structure, kinematics, and evolution of ETGs in Horizon simulations