papers

Publications (38)

astro-ph.GA2025

Long Term Reverberation Mapping of Iron Coronal Lines in MKN 110

Charles Yin, Andy Lawrence, Martin Ward +2

We present flux measurements of the coronal lines [Fe VII] and [Fe X] spanning three decades, in the highly variable Active Galactic Nucleus (AGN) MKN 110. These coronal lines are…

astro-ph.GA2023

Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey

Pablo G. Pérez-González, Luca Costantin, Danial Langeroodi +41

We present the ultraviolet luminosity function and an estimate of the cosmic star formation rate density at derived from deep NIRCam observations taken in parallel with th…

astro-ph.HE2011

Intrinsic disc emission and the Soft X-ray Excess in AGN

Chris Done, Shane Davis, Chichuan Jin +2

(Abridged) Narrow Line Seyfert 1 (NLS1) galaxies have low mass black holes and mass accretion rates close to (or exceeding) Eddington, so a standard blackbody accretion disc should…

astro-ph2000

1-5 micron imaging of 3CRR galaxies: The K-z relation and the geometry of the torus

Chris Simpson, Martin Ward, J. V. Wall

It has been claimed by Taylor et al. that the low-redshift end of the K-z relation for radio galaxies is too bright by about half a magnitude due to contributions from the obscured…

astro-ph.HE2017

Super-Eddington QSO RX J0439.6-5311. II. Multi-wavelength Constraints on the Global Structure of the Accretion Flow

Chichuan Jin, Chris Done, Martin Ward +1

We present a detailed multi-wavelength study of an unobscured, highly super-Eddington Type-1 QSO RX J0439.6-5311. We combine the latest XMM-Newton observation with all archival dat…

astro-ph.HE2015

The Best Constraints on A Super-Eddington Accretion Flow: XMM-Newton Observations of An Intermediate-mass Black Hole

Chichuan Jin, Chris Done, Martin Ward

RX J1140.1+0307 (hereafter RX1140) is a Narrow Line Seyfert 1 (NLS1) with one of the lowest black hole masses known in an AGN (M M). We show results from two…

astro-ph.HE2017

Determining the torus covering factors for a sample of type 1 AGN in the local Universe

Savithri H. Ezhikode, Poshak Gandhi, Chris Done +4

In the unified scheme of active galactic nuclei, a dusty torus absorbs and then reprocesses a fraction of the intrinsic luminosity which is emitted at longer wavelengths. Thus, sub…

astro-ph1998

Optical and infrared observations of the luminous quasar PDS 456: a radio-quiet analogue of 3C 273?

Chris Simpson, Martin Ward, Paul O'Brien +1

We present infrared photometry and optical and infrared spectroscopy of the recently-discovered, extremely luminous nearby quasar PDS 456. A number of broad emission features are s…

astro-ph.HE2020

Re-observing the NLS1 Galaxy RE J1034+396. II. New Insights on the Soft X-ray Excess, QPO and the Analogy with GRS 1915+105

Chichuan Jin, Chris Done, Martin Ward

The active galactic nucleus (AGN) RE J1034+396 displays the most significant X-ray Quasi-Periodic Oscillation (QPO) detected so far. We perform a detailed spectral-timing analysis…

astro-ph.HE2022

X-ray Intraday Variability and Power Spectral Density Profiles of the Blazar 3C 273 with XMM-Newton during 2000-2021

G. S. Pavana Gowtami, Haritma Gaur, Alok C. Gupta +3

We present X-ray intraday variability and power spectral density (PSD) analyses of the longest 23 pointed XMM-Newton observations of the blazar 3C 273 that were taken during 2000 -…

astro-ph2003

A Massive X-Ray Outflow from the Quasar PDS 456

James Reeves, Paul O'Brien, Martin Ward

We report on XMM-Newton spectroscopic observations of the luminous, radio-quiet quasar PDS 456. The hard X-ray spectrum of PDS 456 shows a deep absorption trough (constituting 50%…

astro-ph.HE2013

A Long XMM-Newton Observation of An Extreme Narrow Line Seyfert 1: PG 1244+026

Chichuan Jin, Chris Done, Matthew Middleton +1

We explore the origin of the strong soft X-ray excess in Narrow Line Seyfert 1 galaxies using spectral-timing information from a 120ks {\it XMM-Newton} observation of PG 1244+026.…

astro-ph2008

A ~1-hour X-ray periodicity in an active galaxy RE J1034+396

Marek Gierlinski, Matthew Middleton, Martin Ward +1

Active galactic nuclei and quasars are thought to be scaled up versions of Galactic black hole binaries, powered by accretion onto supermassive black holes with masses of 10^6-10^9…

astro-ph.CO2013

Nuclear Infrared Spectral Energy Distribution of Type II Active Galactic Nuclei

Liza Videla, Paulina Lira, Heather Andrews +3

We present near and mid--IR observations of a sample of Seyfert II galaxies drawn from the m Galaxy Sample. The sample was observed in the J, H, K, L, M and N bands. Galaxy S…

astro-ph.GA2024

MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field

Göran Östlin, Pablo G. Pérez-González, Jens Melinder +41

The recently launched James Webb Space Telescope (JWST) is opening new observing windows on the distant universe. Among JWST's instruments, the Mid Infrared Instrument (MIRI) offer…

astro-ph.GA2024

The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20-214 m imaging atlas of active galactic nuclei using SOFIA

Lindsay Fuller, Enrique Lopez-Rodriguez, Ismael Garcia-Bernete +24

We present a 19.7 - 214 m imaging atlas of local (4 - 181 Mpc; median 43 Mpc) active galactic nuclei (AGN) observed with FORCAST and HAWC+ on board the SOFIA telescope with ang…

astro-ph.GA2025

A close look at the black hole masses and hot dusty toruses of the first quasars with MIRI-MRS

Sarah E. I. Bosman, Javier Álvarez-Márquez, Frederick B. Davies +29

The presence of supermassive black holes (SMBHs, ) at remains a puzzle. While their existence appears to require exotic formation or growth proce…

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-ph2008

RE J1034+396: The origin of the soft X-ray excess and QPO

Matthew Middleton, Chris Done, Martin Ward +2

The X-ray quasi-periodic oscillation (QPO) seen in RE J1034+396 is so far unique amongst AGN. Here we look at the another unique feature of RE J1034+396, namely its huge soft X-ray…

astro-ph.CO2016

The habitability of the Universe through 13 billion years of cosmic time

Pratika Dayal, Martin Ward, Charles Cockell

The field of astrobiology has made tremendous progress in modelling galactic-scale habitable zones which offer a stable environment for life to form and evolve in complexity. Recen…

astro-ph.HE2012

A combined Optical and X-ray Spectra Study for Type 1 AGN. III. Broadband SED Properties

Chichuan Jin, Martin Ward, Chris Done

In this third paper in a series of three, we present a detailed study of the AGN broadband SED based on a nearby unobscured Type 1 AGN sample. We perform a systematic cross-correla…

astro-ph.HE2022

Multi-wavelength Campaign on the Super-Eddington NLS1 RX J0134.2-4258 -- I. Peculiar X-ray Spectra and Variability

Chichuan Jin, Chris Done, Martin Ward +3

We have conducted a new long-term multi-wavelength campaign on one of the most super- Eddington narrow-line Seyfert 1s (NLS1s) known, namely RX J0134.2-4258. In this first paper, w…

astro-ph.CO2010

Searching for Compton-thick active galactic nuclei at z~0.1

Andy Goulding, David Alexander, James Mullaney +4

Using a suite of X-ray, mid-IR and optical active galactic nuclei (AGN) luminosity indicators, we search for Compton-thick (CT) AGNs with intrinsic L_X>10^42erg/s at z~0.03-0.2, a…

astro-ph.GA2025

The Rich JWST Spectrum of the Western Nucleus of Arp 220: Shocked Hot Core Chemistry Dominates the Inner Disk

Victorine Buiten, Paul van der Werf, Serena Viti +20

We present full 3-28 JWST MIRI/MRS and NIRSpec/IFU spectra of the western nucleus of Arp 220, the nearest ultraluminous infrared galaxy. This nucleus has long been s…

astro-ph.HE2020

State-of-the-art AGN SEDs for Photoionization Models: BLR Predictions Confront the Observations

Gary Ferland, Chris Done, Chichuan Jin +2

The great power offered by photoionization models of Active Galactic Nuclei (AGN) emission-line regions has long been mitigated by the fact that very little is known about the spec…

astro-ph.HE2022

The Extreme Super-Eddington NLS1 RX J0134.2-4258 -- II. A Weak-Line Seyfert Linking to the Weak-Line Quasar

Chichuan Jin, Chris Done, Martin Ward +3

RX J0134.2-4258 is one of the most super-Eddington narrow-line Seyfert 1 (NLS1) galaxies, on which we conducted a monitoring campaign from radio to X-rays. In this paper, we presen…

astro-ph.GA2024

Dust beyond the torus: Revealing the mid-infrared heart of local Seyfert ESO 428-G14 with JWST/MIRI

Houda Haidar, David J. Rosario, Almudena Alonso-Herrero +34

Polar dust has been discovered in a number of local Active Galactic Nuclei (AGN), with radiation-driven torus models predicting a wind to be its main driver. However, little is kno…

astro-ph.CO2011

The X-ray emission of local luminous infrared galaxies

Miguel Pereira-Santaella, Almudena Alonso-Herrero, Maria Santos-Lleo +6

We study the X-ray emission of a representative sample of 27 local luminous infrared galaxies (LIRGs). The median IR luminosity of our sample is log L_IR/L_sun = 11.2, thus the low…

astro-ph.HE2022

Detection of an Unidentified Soft X-ray Emission Feature in NGC 5548

Liyi Gu, Junjie Mao, Jelle S. Kaastra +17

NGC~5548 is an X-ray bright Seyfert 1 active galaxy. It exhibits a variety of spectroscopic features in the soft X-ray band, including in particular the absorption by the AGN outfl…

astro-ph.GA2026

GATOS XI : Excess dust heating in the Narrow Line Regions of nearby AGN revealed with JWST/MIRI

Houda Haidar, David J. Rosario, Ismael García-Bernete +38

We present JWST/MIRI imaging of eight nearby Active Galactic Nuclei (AGN) from the GATOS survey to investigate the physical conditions of extended dust in their narrow line regions…

astro-ph.GA2023

Wavelength Dependences of the Optical/UV and X-ray Luminosity Correlations of Quasars

Chichuan Jin, Elisabeta Lusso, Martin Ward +2

The inter-band correlations between optical/UV and X-ray luminosities of active galactic nuclei (AGN) are important for understanding the disc-coronal connection, as well as using…

astro-ph.CO2013

Modeling the Nuclear Infrared Spectral Energy Distribution of Type II Active Galactic Nuclei

Paulina Lira, Liza Videla, Yanling Wu +3

We present results from model fitting to the Spectral Energy Distribution (SED) of a homogeneous sample of Seyfert II galaxies drawn from the m Galaxy Sample. Imaging and nuc…

astro-ph.HE2020

Re-observing the NLS1 Galaxy RE J1034+396. I. the Long-term, Recurrent X-ray QPO with a High Significance

Chichuan Jin, Chris Done, Martin Ward

RE J1034+396 is a narrow-line Seyfert 1 galaxy (NLS1) in which the first significant X-ray quasi-periodic oscillation (QPO) in an active galactic nuclei (AGN) was observed in 2007.…

astro-ph.GA2026

The Galaxy Activity, Torus, and outflow Survey (GATOS) XIII: Coupling Driven H2 Excitation in Seyferts

Daniel E. Delaney, Erin K. S. Hicks, Lulu Zhang +31

We utilize JWST/MIRI IFU observations from the Galaxy Activity, Torus and Outflow Survey (GATOS) to investigate the diverse range of ionized outflow rates of obscured AGN with simi…

astro-ph.HE2024

Chasing Gravitational Waves with the Cherenkov Telescope Array

Jarred Gershon Green, Alessandro Carosi, Lara Nava +563

The detection of gravitational waves from a binary neutron star merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts…

astro-ph.HE2017

Super-Eddington QSO RX J0439.6-5311. I. Origin of the Soft X-ray Excess and Structure of the Inner Accretion Flow

Chichuan Jin, Chris Done, Martin Ward

We report the results from a recent 133 ks XMM-Newton observation of a highly super-Eddington narrow-line Type-1 QSO RX J0439.6-5311. This source has one of the steepest AGN hard X…

astro-ph.GA2010

An X-ray Study of Local Infrared Bright Galaxies

Miguel Pereira-Santaella, Almudena Alonso-Herrero, Elena Jiménez-Bailón +3

We are carrying out detailed study of the X-ray and infrared (IR) properties of a sample of local (d < 70 Mpc) luminous infrared galaxies (LIRGs) using XMM-Newton and Spitzer (imag…

astro-ph.GA2025

GATOS. VIII. On the physical origin of the extended MIR emission in AGN

Enrique Lopez-Rodriguez, Cristina Ramos Almeida, Miguel Pereira-Santaella +31

The polar mid-infrared (MIR) emission detected within 10-100s pcs in some active galactic nuclei (AGN) has been associated with dusty winds driven away by radiation pressure. The p…