activity
20152026
most citedIonized outflows in local luminous AGN: what are the real densities and outflow rates?

150 citations · 1.9k across the 45 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2026

XRISM Resolves the Circum-nuclear Environment of NGC 4945

Peter G. Boorman, Poshak Gandhi, Yoshihiro Ueda +31

Compton-thick Active Galactic Nuclei (AGN) represent one of the most elusive phases of massive black hole growth, yet are expected to contribute substantially to the Cosmic X-ray B…

astro-ph.GA2026

SDSS-V: Revealing a weak accretion state in X-ray selected red quasars

Paloma Guetzoyan, James Aird, Amy L. Rankine +17

Red quasars (rQSOs) have been recognized as a short-lived, early stage in the evolutionary cycle of Active Galactic Nuclei (AGN), with fundamental differences in their intrinsic pr…

astro-ph.GA2026★ 2 cited

Decoupling the AGN outflow and star-forming disk kinematics in the nuclear region of NGC 7582 with JWST NIRSpec and MIRI/MRS

Oscar Veenema, Niranjan Thatte, Dimitra Rigopoulou +24

We present a detailed study of the inner regions of NGC~7582, a nearby Seyfert~2 galaxy, from the Galaxy Activity, Torus and Outflow Survey (GATOS). The galaxy hosts a circumnuclea…

astro-ph.HE2024

The NuSTAR Serendipitous Survey: the 80-month catalog and source properties of the high-energy emitting AGN and quasar population

Claire L. Greenwell, Lizelke Klindt, George B. Lansbury +32

We present a catalog of hard X-ray serendipitous sources detected in the first 80 months of observations by the Nuclear Spectroscopic Telescope Array (NuSTAR). The NuSTAR serendipi…

astro-ph.HE2023★ 5 cited

XMM-Newton --NuSTAR monitoring campaign of the Seyfert 1 galaxy IC 4329A

A. Tortosa, C. Ricci, E. Shablovinskaia +13

We present the results of a joint {\it XMM-Newton} and {\it NuSTAR} campaign on the active galactic nucleus (AGN) IC 4329A, consisting of 9 20 ks {\it XMM-Newton} observat…

astro-ph.HE2023★ 1 cited

Prospects for Time-Domain and Multi-Messenger Science with AXIS

The AXIS Time-Domain, Multi-Messenger Science Working Group, : +19

The Advanced X-ray Imaging Satellite (AXIS) promises revolutionary science in the X-ray and multi-messenger time domain. AXIS will leverage excellent spatial resolution (<1.5 arcse…

astro-ph.HE2021★ 19 cited

Extreme Relativistic Reflection in the Active Galaxy ESO 033-G002

D. J. Walton, M. Balokovic, A. C. Fabian +13

We present the first high signal-to-noise broadband X-ray spectrum of the radio-quiet type-2 Seyfert ESO 033-G002, combining data from - and . The nuclear X-ra…

astro-ph.HE2020★ 25 cited

A Full Characterisation of the Supermassive Black Hole in IRAS 09149-6206

D. J. Walton, W. N. Alston, P. Kosec +11

We present new broadband X-ray observations of the type-I Seyfert galaxy IRAS 09149-6206, taken in 2018 with -, and . The source is highly complex, sho…

astro-ph.HE2020★ 26 cited

Observations of Four Nearby X-ray Faint AGN: Low Luminosity or Heavy Obscuration?

A. Annuar, D. M. Alexander, P. Gandhi +20

We present observations of four active galactic nuclei (AGN) located within 15 Mpc. These AGN, namely ESO 121-G6, NGC 660, NGC 3486 and NGC 5195, have observed X-ray lumin…

astro-ph.HE2020★ 11 cited

Constraining X-ray reflection in the low-luminosity AGN NGC 3718 using NuSTAR and XMM--Newton

Y. Diaz, P. Arévalo, L. Hernández-García +9

One distinctive feature of low-luminosity active galactic nuclei (LLAGN) is the relatively weak reflection features they may display in the X-ray spectrum, which can result from th…

astro-ph.GA2020★ 32 cited

Local AGN Survey (LASr): I. Galaxy sample, infrared colour selection and predictions for AGN within 100 Mpc

D. Asmus, C. L. Greenwell, P. Gandhi +12

In order to answer some of the major open questions in the fields of supermassive black hole (SMBH) and galaxy evolution, a complete census of SMBH growth, i.e., active galactic nu…

astro-ph.GA2020★ 150 cited

Ionized outflows in local luminous AGN: what are the real densities and outflow rates?

R. Davies, D. Baron, T. Shimizu +23

We report on the determination of electron densities, and their impact on the outflow masses and rates, measured in the central few hundred parsecs of 11 local luminous active gala…

astro-ph.GA2020★ 47 cited

BAT AGN Spectroscopic Survey -- XV: The High Frequency Radio Cores of Ultra-hard X-ray Selected AGN

Krista Lynne Smith, Richard F. Mushotzky, Michael Koss +14

We have conducted 22 GHz radio imaging at 1" resolution of 100 low-redshift AGN selected at 14-195 keV by the Swift-BAT. We find a radio core detection fraction of 96%, much higher…

astro-ph.HE2019★ 35 cited

A Low-Flux State in IRAS 00521-7054 seen with NuSTAR and XMM-Newton: Relativistic Reflection and an Ultrafast Outflow

D. J. Walton, E. Nardini, L. C. Gallo +8

We present results from a deep, coordinated -+ observation of the Seyfert 2 galaxy IRAS 00521-7054. The data provide the first detection of this sourc…

astro-ph.HE2018★ 148 cited

BAT AGN Spectroscopic Survey -- XII. The relation between coronal properties of Active Galactic Nuclei and the Eddington ratio

C. Ricci, L. C. Ho, A. C. Fabian +12

The bulk of the X-ray emission in Active Galactic Nuclei (AGN) is produced very close to the accreting supermassive black hole (SMBH), in a corona of hot electrons which up scatter…

astro-ph.GA2018★ 42 cited

Revisiting the "forbidden" region: AGN radiative feedback with radiation trapping

W. Ishibashi, A. C. Fabian, C. Ricci +1

Active galactic nucleus (AGN) feedback, driven by radiation pressure on dust, is an important mechanism for efficiently coupling the accreting black hole to the surrounding environ…

astro-ph.GA2017★ 19 cited

Joint NuSTAR and Chandra analysis of the obscured quasar in IC 2497 - Hanny's Voorwerp system

Lia F. Sartori, Kevin Schawinski, Michael J. Koss +9

We present new Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the core of IC 2497, the galaxy associated with Hanny's Voorwerp. The combined fits of the Chandra (0.…

astro-ph.HE2017★ 54 cited

The NuSTAR Serendipitous Survey: Hunting for The Most Extreme Obscured AGN at >10 keV

G. B. Lansbury, D. M. Alexander, J. Aird +27

We identify sources with extremely hard X-ray spectra (i.e., with photon indices of Gamma<0.6 in the 13 sq. deg. NuSTAR serendipitous survey, to search for the most highly obscured…

astro-ph.HE2017★ 38 cited

X-ray bolometric corrections for Compton-thick active galactic nuclei

M. Brightman, M. Baloković, D. R. Ballantyne +16

We present X-ray bolometric correction factors, (), for Compton-thick (CT) active galactic nuclei (AGN) with the aim of testing AGN torus models, prob…

astro-ph.GA2017★ 35 cited

Hard X-ray selected AGNs in low-mass galaxies from the NuSTAR serendipitous survey

C. -T. J. Chen, W. N. Brandt, A. E. Reines +14

We present a sample of 10 low-mass active galactic nuclei (AGNs) selected from the 40-month NuSTAR serendipitous survey. The sample is selected to have robust NuSTAR detections at…

astro-ph.HE2016★ 41 cited

Broadband X-ray spectral analysis of the Seyfert 1 galaxy GRS 1734-292

A. Tortosa, A. Marinucci, G. Matt +14

We discuss the broadband X-ray spectrum of GRS 1734-292 obtained from non-simultaneous XMM-Newton and NuSTAR observations, performed in 2009 and 2014, respectively. GRS1734-292 is…

astro-ph.HE2016★ 27 cited

The nature of the torus in the heavily obscured AGN Markarian 3: an X-ray study

M. Guainazzi, G. Risaliti, H. Awaki +22

In this paper we report the results of an X-ray monitoring campaign on the heavily obscured Seyfert galaxy Markarian 3 carried out between the fall of 2014 and the spring of 2015 w…

astro-ph.HE2016★ 39 cited

The weak neutral Fe fluorescence line and long-term X-ray evolution of the Compton-thick AGN in NGC 7674

P. Gandhi, A. Annuar, G. B. Lansbury +26

We present X-ray observations of the active galactic nucleus (AGN) in NGC 7674. The source shows a flat X-ray spectrum, suggesting that it is obscured by Compton-thick gas…

astro-ph.HE2016★ 36 cited

NuSTAR reveals the extreme properties of the super-Eddington accreting SMBH in PG 1247+267

G. Lanzuisi, M. Perna, A. Comastri +26

PG1247+267 is one of the most luminous known quasars at and is a strongly super-Eddington accreting SMBH candidate. We obtained NuSTAR data of this intriguing source in De…