activity
20112025
most citedTesting warm Comptonization models for the origin of the soft X-ray excess in AGN

192 citations · 765 across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.HE2025

Fe XVIII-XXIV K beta Inner-shell Absorption Lines in the X-ray Spectra of Neutron Star and Black Hole Binaries with XRISM

Masahiro Tsujimoto, Daiki Miura, Hiroya Yamaguchi +8

The advent of the X-ray microcalorimeter spectrometer Resolve onboard the XRISM space telescope opened a new era for high-resolution X-ray spectroscopy of astrophysical plasmas. Ma…

astro-ph.GA2025

The 2025 Release of Cloudy

Chamani M. Gunasekera, Peter A. M. van Hoof, Maryam Dehghanian +6

We present the 2025 release of the spectral synthesis code Cloudy, highlighting significant enhancements to the scope and accuracy of the physics which have been made since the pre…

astro-ph.IM2025

Observatory Science with eXTP

Ping Zhou, Jirong Mao, Liang Zhang +97

Scheduled for launch in 2030, the enhanced X-ray Timing and Polarization (eXTP) telescope is a Chinese space-based mission aimed at studying extreme conditions and phenomena in ast…

astro-ph.HE2023

The Polarized Cosmic Hand: IXPE Observations of PSR B1509-58/MSH 15-52

Roger W. Romani, Josephine Wong, Niccolo Di Lalla +99

We describe IXPE polarization observations of the Pulsar Wind Nebula (PWN) MSH15-52, the `Cosmic Hand'. We find X-ray polarization across the PWN, with B field vectors generally al…

astro-ph.GA2021★ 16 cited

Photoionisation Modelling of the X-ray Emission Line Regions within the Seyfert 2 AGN NGC 1068

S. Grafton-Waters, G. Branduardi-Raymont, M. Mehdipour +4

We investigate the photoionised X-ray emission line regions (ELRs) within the Seyfert 2 galaxy NGC 1068, to determine if there are any characteristic changes between observations t…

astro-ph.HE2020★ 38 cited

The soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-NuSTAR monitoring campaign

R. Middei, P. -O. Petrucci, S. Bianchi +7

XMM-Newton and NuSTAR multiple exposures allow us to disentangle the different emission components of active galactic nuclei (AGNs) and to study the evolution of their different sp…

astro-ph.HE2019★ 52 cited

NuSTAR/XMM-Newton monitoring of the Seyfert 1 galaxy HE 1143-1810. Testing the two-corona scenario

F. Ursini, P. -O. Petrucci, S. Bianchi +11

We test the two-corona accretion scenario for active galactic nuclei in the case of the `bare' Seyfert 1 galaxy HE 1143-1810. We perform a detailed study of the broad-band UV--X-ra…

astro-ph.HE2019★ 6 cited

Evolution of the disc atmosphere in the X-ray binary MXB 1659-298, during its 2015-2017 outburst

G. Ponti, S. Bianchi, B. De Marco +3

We report on the evolution of the X-ray emission of the accreting neutron star (NS) low mass X-ray binary (LMXB), MXB 1659-298, during its most recent outburst in 2015-2017. We det…

astro-ph.GA2019★ 5 cited

Multiwavelength campaign on Mrk 509. XVI. Continued HST/COS monitoring of the far-ultraviolet spectrum

G. A. Kriss, N. Arav, D. Edmonds +10

To elucidate the location, physical conditions, mass outflow rate, and kinetic luminosity of the outflow from the active nucleus of the Seyfert 1 galaxy Mrk 509 we used coordinated…

astro-ph.HE2018★ 24 cited

Radio/X-ray monitoring of the broad-line radio galaxy 3C 382. High-energy view with XMM-Newton and NuSTAR

F. Ursini, P. -O. Petrucci, G. Matt +14

We present the analysis of five joint XMM-Newton/NuSTAR observations, 20 ks each and separated by 12 days, of the broad-line radio galaxy 3C 382. The data were obtained as part of…

astro-ph.HE2017★ 27 cited

Anatomy of the AGN in NGC 5548 IX. Photoionized emission features in the soft X-ray spectra

Junjie Mao, J. S. Kaastra, M. Mehdipour +10

The X-ray narrow emission line region (NELR) of the archetypal Seyfert 1 galaxy NGC\,5548 has been interpreted as a single-phase photoionized plasma that is absorbed by some of the…

astro-ph.HE2017★ 192 cited

Testing warm Comptonization models for the origin of the soft X-ray excess in AGN

P. O. Petrucci, F. Ursini, A. De Rosa +5

The X-ray spectra of many active galactic nuclei (AGN) show a soft X-ray excess below 1-2 keV on top of the extrapolated high- energy power law. The origin of this component is unc…

astro-ph.HE2017★ 17 cited

Multi-wavelength campaign on NGC7469 II. Column densities and variability in the X-ray spectrum

U. Peretz, E. Behar, G. A. Kriss +16

We investigate the ionic column density variability of the ionized outflows associated with NGC7469, to estimate their location and power. This could allow a better understan…

astro-ph.HE2017★ 27 cited

NuSTAR + XMM-Newton monitoring of the neutron star transient AX J1745.6-2901

G. Ponti, S. Bianchi, T. Munos-Darias +12

AX J1745.6-2901 is a high-inclination (eclipsing) transient neutron star (NS) Low Mass X-ray Binary (LMXB) showcasing intense ionised Fe K absorption. We present here the analysis…

astro-ph.HE2017★ 93 cited

Chasing obscuration in type-I AGN: discovery of an eclipsing clumpy wind at the outer broad-line region of NGC 3783

M. Mehdipour, J. S. Kaastra, G. A. Kriss +21

In 2016 we carried out a Swift monitoring program to track the X-ray hardness variability of eight type-I AGN over a year. The purpose of this monitoring was to find intense obscur…

astro-ph.HE2016★ 46 cited

High-energy monitoring of NGC 4593 with XMM-Newton and NuSTAR. X-ray spectral analysis

F. Ursini, P. -O. Petrucci, G. Matt +8

We present results from a joint Xmm-Newton/NuSTAR monitoring of the Seyfert 1 NGC 4593, consisting of 5x20 ks simultaneous observations spaced by two days, performed in January 201…

astro-ph.HE2016★ 58 cited

Anatomy of the AGN in NGC 5548 VIII. XMM-Newton's EPIC detailed view of an unexpected variable multilayer absorber

M. Cappi, B. De Marco, G. Ponti +21

In 2013 we conducted a large multi-wavelength campaign on the archetypical Seyfert 1 galaxy NGC 5548. Unexpectedly, this usually unobscured source appeared strongly absorbed in the…

astro-ph.HE2016★ 43 cited

Anatomy of the AGN in NGC 5548: VII. Swift study of obscuration and broadband continuum variability

M. Mehdipour, J. S. Kaastra, G. A. Kriss +16

We present our investigation into the long-term variability of the X-ray obscuration and optical-UV-X-ray continuum in the Seyfert 1 galaxy NGC 5548. In 2013 and 2014, the Swift ob…

astro-ph.HE2015★ 48 cited

High ionisation absorption in low mass X-ray binaries

G. Ponti, S. Bianchi, T. Munoz-Darias +3

The advent of the new generation of X-ray telescopes yielded a significant step forward in our understanding of ionised absorption generated in the accretion discs of X-ray binarie…

astro-ph.HE2015★ 2 cited

High-energy monitoring of Seyfert galaxies: the case of NGC 4593

F. Ursini, P. -O. Petrucci, G. Matt +6

We discuss preliminary results from a joint XMM-Newton and NuSTAR monitoring program on the active galactic nucleus NGC 4593, consisting of 5x20 ks observations, spaced by two days…

astro-ph.HE2015

Anatomy of the AGN in NGC 5548 IV. The short-term variability of the outflows

L. Di Gesu, E. Costantini, J. Ebrero +16

During an extensive multiwavelength campaign that we performed in 2013-14 the prototypical Seyfert 1 galaxy NGC 5548 has been found in an unusual condition of heavy and persistent…

astro-ph.HE2015★ 1 cited

The physics of accretion-ejection with LOFT

P. Casella, R. Fender, M. Coriat +29

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT f…

astro-ph.CO2012★ 16 cited

Multiwavelength Campaign on Mrk 509 X. Lower limit on the distance of the absorber from HST COS and STIS spectroscopy

N. Arav, D. Edmonds, B. Borguet +15

Active Galactic Nuclei often show evidence of photoionized outflows. A major uncertainty in models for these outflows is the distance () to the gas from the central black hole.…

astro-ph.GA2012★ 16 cited

Multiwavelength campaign on Mrk 509 IX. The Galactic foreground

C. Pinto, G. A. Kriss, J. S. Kaastra +5

The diffuse gas in and nearby the Milky Way plays an important role in the evolution of the entire Galaxy. It has a complex structure characterized by neutral, weakly and highly io…