Search Publications

Quasi-periodic eruptions as Lense-Thirring precession of super-Eddington flows
DOI: 10.1093/mnras/staf052 Bibcode: 2025MNRAS.537.1688M

Pinto, C.; Miniutti, G.; Dauser, T. +9 more

Quasi-periodic eruptions (QPEs) are a recently identified class of X-ray transient associated with tidal disruption events by supermassive black holes, and for which there are multiple possible explanations. In this paper, we present a simple model which requires the black hole be spinning, be misaligned with the accretion flow (both conditions of…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
Testing disc reprocessing models for AGN optical variability by comparison of X-ray and optical power spectra of NGC 4395
DOI: 10.1093/mnras/staf014 Bibcode: 2025MNRAS.537..293B

Dhillon, V. S.; Knapen, J. H.; Breedt, E. +11 more

It is generally thought that active galactic nucleus (AGN) optical variability is produced, at least in part, by reprocessing of central X-rays by a surrounding accretion disc, resulting in wavelength-dependent lags between bands. Any good model of AGN optical variability should explain not only these lags, but also the overall pattern of variabil…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 2
The XMM Cluster Survey: automating the estimation of hydrostatic mass for large samples of galaxy clusters – I. Methodology, validation, and application to the SDSSRM-XCS sample
DOI: 10.1093/mnras/staf007 Bibcode: 2025MNRAS.537.1404T

Nichol, R. C.; Romer, A. K.; Bhargava, S. +18 more

We describe features of the X-ray: Generate and Analyse (XGA) open-source software package that have been developed to facilitate automated hydrostatic mass ($M_{\rm hydro}$) measurements from XMM X-ray observations of clusters of galaxies. This includes describing …

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
The VMC Survey - LI. Classifying extragalactic sources using a probabilistic random forest supervised machine learning algorithm
DOI: 10.1093/mnras/staf080 Bibcode: 2025MNRAS.537.1028P

Maitra, Chandreyee; Aird, James; de Grijs, Richard +10 more

We used a supervised machine learning algorithm (probabilistic random forest) to classify $\sim$130 million sources in the VISTA Survey of the Magellanic Clouds (VMC). We used multiwavelength photometry from optical to far-infrared as features to be trained on, and …

2025 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 1
Simultaneous optical and X-ray detection of a thermonuclear burst in the 2024 outburst of EXO 0748-676
DOI: 10.1093/mnrasl/slae103 Bibcode: 2025MNRAS.536L..26K

Ingram, Adam; Roberts, Timothy P.; Middleton, Matthew +5 more

The neutron star low-mass X-ray binary, EXO 0748-676, recently returned to outburst after a $\sim\!\! 16$ yr-long quiescence. Since its return, there has been a global effort to capture the previously unseen rise of the source and to understand its somewhat early re…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
Reflection-dominated Compton-thick AGN candidates in the SRG/eROSITA Lockman Hole survey
DOI: 10.1093/mnras/staf082 Bibcode: 2025MNRAS.537.1444B

Gilfanov, M. R.; Medvedev, P. S.; Sunyaev, R. A. +2 more

We search for reflection-dominated Compton-thick active galactic nuclei (CT AGN) candidates in the Lockman Hole (LH) region using the data of SRG/eROSITA LH survey. We selected sources with anomalously hard photon indices in the 0.3-8.0 keV band, untypical for Type I AGN. In particular, we required that the upper end of the 90 per cent error inter…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Mind the gaps: improved methods for the detection of periodicities in unevenly sampled data
DOI: 10.1093/mnras/staf196 Bibcode: 2025MNRAS.537.3210G

Gúrpide, Andrés; Middleton, Matthew

The detection of periodic signals in irregularly sampled time series is a problem commonly encountered in astronomy. Traditional tools used for periodic searches, such as the periodogram, have poorly defined statistical properties under irregular sampling, which complicate inferring the underlying aperiodic variability used for hypothesis testing.…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
X-ray timing and spectral characteristics of compact symmetric objects
DOI: 10.1093/mnras/stae2817 Bibcode: 2025MNRAS.537...97S

Stalin, C. S.; Saikia, D. J.; Paliya, Vaidehi S. +1 more

Compact Symmetric Objects (CSOs) are a distinct category of jetted active galactic nuclei whose high-energy emission is not well understood. We examined the X-ray characteristics of 17 bona fide CSOs using observations from Chandra, XMM-Newton, and NuSTAR. Among the sources with XMM-Newton observations, we found two sources, J0713+4349 and J1326+3…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Accretion onto WD 2226-210, the central star of the Helix Nebula
DOI: 10.1093/mnras/stae2733 Bibcode: 2025MNRAS.536.2477E

Chu, Y. -H.; Estrada-Dorado, S.; Guerrero, M. A. +4 more

The central star of the Helix Nebula, WD 2226$-$210 presents enigmatic hard X-ray emission and mid-IR excess. The latter has been attributed to a dusty disc or a cloud-like structure around WD 2226$-$

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0
Accretion disc dynamics in extragalactic black hole X-ray binaries: a comprehensive study of M33 X-7, NGC 300 X-1, and IC 10 X-1
DOI: 10.1093/mnras/stae2651 Bibcode: 2025MNRAS.536..827B

Nandi, Anuj; Bhuvana, G. R.

Extragalactic black hole X-ray binaries (BH-XRBs) are the most intriguing X-ray sources as some of them are 'home' to the most massive stellar-mass BHs ever found. In this work, we conduct a comprehensive study of three massive, eclipsing extragalactic BH-XRBs i.e. M33X-7, NGC300X-1, and IC10X-1 and using entire X-ray observations available from X…

2025 Monthly Notices of the Royal Astronomical Society
XMM-Newton 0