Search Publications

Discovery of pulsations from NGC 300 ULX1 and its fast period evolution
DOI: 10.1093/mnrasl/sly030 Bibcode: 2018MNRAS.476L..45C

Haberl, F.; Vasilopoulos, G.; Maitra, C. +1 more

The supernova impostor SN 2010da located in the nearby galaxy NGC 300, later identified as a likely supergiant B[e] high-mass X-ray binary, was simultaneously observed by NuSTAR and XMM-Newton between 2016 December 16 and 20, over a total time span of ∼310 ks. We report the discovery of a strong periodic modulation in the X-ray flux with a pulse p…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 250
Explaining changing-look AGN with state transition triggered by rapid mass accretion rate drop
DOI: 10.1093/mnras/sty2032 Bibcode: 2018MNRAS.480.3898N

Done, Chris; Noda, Hirofumi

We model the broad-band (optical/UV and X-ray) continuum spectrum of the `changing-look' active galactic nucleus (AGN) Mrk 1018, as it fades from Seyfert 1 to 1.9 in ∼ 8 years. The brightest spectrum, with Eddington ratio L/LEdd ∼ 0.08 has a typical type 1 AGN continuum, with a strong `soft X-ray excess' spanning between the UV and soft…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 192
A physical model of the broad-band continuum of AGN and its implications for the UV/X relation and optical variability
DOI: 10.1093/mnras/sty1890 Bibcode: 2018MNRAS.480.1247K

Done, Chris; Kubota, Aya

We develop a new spectral model for the broad-band spectral energy distribution (SED) of active galactic nuclei (AGN). This includes an outer standard disc, an inner warm Comptonizing region to produce the soft X-ray excess and a hot corona. We tie these together energetically by assuming Novikov-Thorne emissivity, and use this to define a size sc…

2018 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 192
Finding counterparts for all-sky X-ray surveys with NWAY: a Bayesian algorithm for cross-matching multiple catalogues
DOI: 10.1093/mnras/stx2651 Bibcode: 2018MNRAS.473.4937S

Salvato, M.; Buchner, J.; Nandra, K. +6 more

We release the AllWISE counterparts and Gaia matches to 106 573 and 17 665 X-ray sources detected in the ROSAT 2RXS and XMMSL2 surveys with |b| > 15°. These are the brightest X-ray sources in the sky, but their position uncertainties and the sparse multi-wavelength coverage until now rendered the identification of their counterparts a demanding…

2018 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 151
Constraining the mass and radius of neutron stars in globular clusters
DOI: 10.1093/mnras/sty215 Bibcode: 2018MNRAS.476..421S

Heinke, C. O.; Ho, W. C. G.; Bogdanov, S. +4 more

We analyse observations of eight quiescent low-mass X-ray binaries in globular clusters and combine them to determine the neutron star mass-radius curve and the equation of state of dense matter. We determine the effect that several uncertainties may have on our results, including uncertainties in the distance, the atmosphere composition, the neut…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 148
Systematic study of magnetar outbursts
DOI: 10.1093/mnras/stx2679 Bibcode: 2018MNRAS.474..961C

Esposito, Paolo; Rea, Nanda; Coti Zelati, Francesco +2 more

We present the results of the systematic study of all magnetar outbursts observed to date, through a reanalysis of data acquired in about 1100 X-ray observations. We track the temporal evolution of the outbursts' soft X-ray spectral properties and the luminosities of the single spectral components as well as of the total emission. We model empiric…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 141
BAT AGN Spectroscopic Survey - XII. The relation between coronal properties of active galactic nuclei and the Eddington ratio
DOI: 10.1093/mnras/sty1879 Bibcode: 2018MNRAS.480.1819R

Treister, E.; Bauer, F. E.; Paltani, S. +12 more

The bulk of the X-ray emission in active galactic nuclei (AGNs) is produced very close to the accreting supermassive black hole (SMBH), in a corona of hot electrons which up scatters optical and ultraviolet photons from the accretion flow. The cut-off energy (EC) of the primary X-ray continuum emission carries important information on t…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 118
Evidence for a variable Ultrafast Outflow in the newly discovered Ultraluminous Pulsar NGC 300 ULX-1
DOI: 10.1093/mnras/sty1626 Bibcode: 2018MNRAS.479.3978K

Fabian, A. C.; Pinto, C.; Bachetti, M. +5 more

Ultraluminous pulsars are a definite proof that persistent super-Eddington accretion occurs in nature. They support the scenario according to which most Ultraluminous X-ray Sources (ULXs) are super-Eddington accretors of stellar mass rather than sub-Eddington intermediate mass black holes. An important prediction of theories of supercritical accre…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 109
The SUrvey for Pulsars and Extragalactic Radio Bursts - I. Survey description and overview
DOI: 10.1093/mnras/stx2126 Bibcode: 2018MNRAS.473..116K

Possenti, A.; Kramer, M.; Burgay, M. +19 more

We describe the Survey for Pulsars and Extragalactic Radio Bursts (SUPERB), an ongoing pulsar and fast transient survey using the Parkes radio telescope. SUPERB involves real-time acceleration searches for pulsars and single-pulse searches for pulsars and fast radio bursts. We report on the observational set-up, data analysis, multiwavelength/mess…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 100
The 1.5 Ms observing campaign on IRAS 13224-3809 - I. X-ray spectral analysis
DOI: 10.1093/mnras/sty836 Bibcode: 2018MNRAS.477.3711J

Harrison, F. A.; Fabian, A. C.; Miller, J. M. +16 more

We present a detailed spectral analysis of the recent 1.5 Ms XMM-Newton observing campaign on the narrow-line Seyfert 1 galaxy IRAS 13224-3809, taken simultaneously with 500 ks of NuSTAR data. The X-ray light curve shows three flux peaks, registering at about 100 times the minimum flux seen during the campaign, and rapid variability with a time-sc…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 91