activity
20082026
most citedUbiquitous equatorial accretion disc winds in black hole soft states

426 citations · 3.7k across the 64 of their papers we have counts for

collaborators

63 papers

astro-ph.HE2026

Supermassive Black Hole Winds in X-rays -- SUBWAYS. VI. Interplay between the soft X-ray excess and ultra-fast outflows

V. E. Gianolli, P-O. Petrucci, S. Bianchi +42

We present a broadband, multiwavelength study of the interplay between the soft X-ray excess (SE), ultra-fast outflows (UFOs), and warm absorbers (WAs) in 21 active galactic nuclei…

astro-ph.HE2026★ 5 cited

Accretion disc winds in X-ray binaries

Teo Muñoz-Darias, María Díaz Trigo, Chris Done +2

Despite early theoretical expectations that large-scale, massive outflows would be triggered by accretion onto black holes and neutron stars, their presence was not firmly establis…

astro-ph.HE2025

State-dependent signatures of jets and winds in the optical and infrared spectrum of the black hole transient GX 3394

A. Ambrifi, D. Mata Sánchez, T. Muñoz-Darias +14

GX 3394 is one of the prototypical black hole X-ray transients, exhibiting recurrent outbursts that allow detailed studies of black hole accretion and ejection phenomena. In thi…

astro-ph.HE2024★ 3 cited

The more the merrier: SRG/eROSITA discovers two further galaxies showing X-ray quasi-periodic eruptions

R. Arcodia, Z. Liu, A. Merloni +20

X-ray quasi-periodic eruptions (QPEs) are a novel addition to the group of extragalactic transients. In this work, we report the discovery of two further galaxies showing QPEs, eRO…

astro-ph.GA2023

O Corona, where art thou? eROSITA's view of UV-optical-IR variability-selected massive black holes in low-mass galaxies

R. Arcodia, A. Merloni, J. Comparat +16

Finding massive black holes (MBHs, ) in the nuclei of low-mass galaxies () is crucial to constrain seeding and…

astro-ph.GA2023★ 29 cited

The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA

N. Locatelli, G. Ponti, X. Zheng +7

The first all-sky maps of the diffuse emission of high ionization lines observed in X-rays by SRG/eROSITA, provide an excellent probe for the study of the warm-hot phase (T~10^6 K)…

astro-ph.HE2023

Searching for X-Ray Counterparts of Degree Wide TeV Halos Around Middle-Aged Pulsars with SRG/eROSITA

A. Khokhriakova, W. Becker, G. Ponti +3

Context. Extended gamma-ray TeV emission (TeV halos) around middle-aged pulsars has been detected. A proposed model to explain these TeV halos is that electrons from a degree-wide…

astro-ph.GA2023★ 6 cited

The JWST Galactic Center Survey -- A White Paper

Rainer Schoedel, Steve Longmore, Jonny Henshaw +111

The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post ma…

astro-ph.HE2023★ 24 cited

The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band

M. Parra, P. -O. Petrucci, S. Bianchi +3

The presence of blueshifted absorption lines in the X-ray spectra of Black Hole Low Mass X-ray Binaries is the telltale of massive outflows called winds. These signatures are found…

astro-ph.GA2023★ 19 cited

Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission

Joel Bregman, Renyue Cen, Yang Chen +51

The Hot Universe Baryon Surveyor (HUBS) is a proposed space-based X-ray telescope for detecting X-ray emissions from the hot gas content in our universe. With its unprecedented spa…

astro-ph.HE2023

An XMM-Newton View of the ANdromeda Galaxy as Explored in a Legacy Survey (New-ANGELS) I: the X-ray Source Catalogue

Rui Huang, Jiang-Tao Li, Wei Cui +6

We introduce the New-ANGELS program, an XMM-Newton survey of area around M 31, which aims to study the X-ray populations in M 31 disk and the X-ray emitting hot…

astro-ph.HE2023★ 6 cited

Coordinated X-ray and UV absorption within the accretion disk wind of the active galactic nucleus PG 1126-041

M. Giustini, P. Rodríguez Hidalgo, J. N. Reeves +14

Accretion disk winds launched close to supermassive black holes (SMBHs) are a viable mechanism to provide feedback between the SMBH and the host galaxy. We aim to characterize the…

astro-ph.HE2023★ 12 cited

Optical and near-infrared spectroscopy of the black hole transient 4U 1543-47 during its 2021 ultra-luminous state

J. Sánchez-Sierras, T. Muñoz-Darias, J. Casares +10

We present simultaneous optical and near-infrared spectra obtained during the 2021 outburst of the black hole transient 4U 1543-47. The X-ray hardness-intensity diagram and the com…

astro-ph.GA2023★ 7 cited

Transient obscuration event captured in NGC 3227 IV. Origin of the obscuring cloud variability

S. Grafton-Waters, J. Mao, M. Mehdipour +13

Obscuration events in type I active galactic nuclei (AGN) have been detected more frequently in recent years. The strong flux decrease in the soft X-ray band between observations h…

astro-ph.HE2023★ 9 cited

Discovery of periodicities in two highly variable intermediate polars towards the Galactic Center

Samaresh Mondal, Gabriele Ponti, Frank Haberl +5

We discovered Fe complex emission and pulsation in two highly variable sources (4XMM J174917.7--283329, 4XMM J174954.6--294336). The equivalent widths of 6.4 and 6.7 keV line…

astro-ph.HE2023★ 5 cited

Capturing the lowest luminosity state of the Supergiant Fast X-ray Transient XTE J1739-302

Lara Sidoli, Gabriele Ponti, Vito Sguera +1

We report here on the results of the analysis of Chandra, XMM-Newton and NuSTAR recent observations of the Supergiant Fast X-ray Transient XTEJ1739-302. The source was caught in a…

astro-ph.HE2023★ 19 cited

Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data

K. Anastasopoulou, G. Ponti, M. C. Sormani +14

The diffuse Fe XXV (6.7 keV) line emission observed in the Galactic ridge is widely accepted to be produced by a superposition of a large number of unresolved X-ray point sources.…

astro-ph.HE2022★ 12 cited

Supermassive Black Hole Winds in X-rays: SUBWAYS. II. HST UV spectroscopy of winds at intermediate redshifts

M. Mehdipour, G. A. Kriss, M. Brusa +35

We present a UV spectroscopic study of ionized outflows in 21 active galactic nuclei (AGN), observed with the HST. The targets of the SUBWAYS sample were selected with the aim to p…

astro-ph.HE2022★ 55 cited

Supermassive Black Hole Winds in X-rays -- SUBWAYS. I. Ultra-fast outflows in QSOs beyond the local Universe

G. A. Matzeu, M. Brusa, G. Lanzuisi +48

We present a new X-ray spectroscopic study of luminous () active galactic nuclei (AGNs) at intermed…

astro-ph.HE2022★ 8 cited

On the patchy appearance of the circum-Galactic medium and the influence of foreground absorption

G. Ponti, J. S. Sanders, N. Locatelli +10

Recent studies have demonstrated that the emission from the circumgalactic medium of the Milky Way displays a relatively high degree of patchiness on angular scales of $\sim10^\cir…

astro-ph.HE2022★ 57 cited

Abundance and temperature of the outer hot circum-Galactic medium: The SRG/eROSITA view of the soft X-ray background in the eFEDS field

G. Ponti, X. Zheng, N. Locatelli +14

Despite their vital importance to understand galaxy evolution and our own Galactic ecosystem, our knowledge of the physical properties of the hot phase of the Milky Way is still in…

astro-ph.HE2022

Diffuse Hot Plasma in the Interstellar Medium and Galactic Outflows

Manami Sasaki, Gabriele Ponti, Jonathan Mackey

We summarise observations and our current understanding of the interstellar medium (ISM) in galaxies, which mainly consists of three phases: cold atomic or molecular gas and clouds…

astro-ph.HE2022★ 25 cited

Discovery of optical and infrared accretion disc wind signatures in the black hole candidate MAXI J1348-630

G. Panizo-Espinar, M. Armas Padilla, T. Muñoz-Darias +11

MAXI J1348-630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this event, the system sampled both hard and soft states following the standard evolut…

astro-ph.HE2022★ 24 cited

Simultaneous X-ray and optical spectroscopy of V404 Cygni supports the multi-phase nature of X-ray binary accretion disc winds

Teo Muñoz-Darias, Gabriele Ponti

Observational signatures of accretion disc winds have been found in a significant number of low-mass X-ray binaries at either X-ray or optical wavelengths. The 2015 outburst of the…