activity
20152026
most citedAn embedded X-ray source shines through the aspherical AT2018cow: revealing the inner workings of the most luminous fast-evolving optical transients

267 citations · 740 across the 37 of their papers we have counts for

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33 papers · 1 filter

astro-ph.HE2026

First X-ray detection of symbiotic nova CN Cha with eROSITA/SRG

Sara Saeedi, Jaroslav Merc, Manami Sasaki +2

Aims. We report on the first X-ray detection of the symbiotic star CN Cha with eROSITA (extended Roentgen Survey with an Imaging Telescope Array) onboard Spektrum-Roentgen Gamma (S…

astro-ph.HE2026

Ultraluminous X-ray sources in the first eROSITA survey I. Candidate catalogs

P. Weber, T. P. Roberts, S. Hämmerich +28

Ultraluminous X-ray sources (ULXs) are luminous non-nuclear X-ray point sources embedded in galaxies. Their luminosities exceeding 10^39 erg/s potentially require sub-Eddington acc…

astro-ph.HE2026

Spectral and timing variability of the transient ultraluminous X-ray source NGC 4631 X-4

Sinan Allak, Wei Yu, Lorenzo Ducci +4

Ultraluminous X-ray sources (ULXs) are among the best laboratories for studying super-Eddington accretion onto compact objects. We present a detailed spectral and timing analysis o…

astro-ph.HE2026

A candidate cyclotron line at 1.89 keV in the ultraluminous X-ray source NGC 4861 X-2

Sinan Allak, Lorenzo Ducci, Valery F. Suleimanov +6

In this Letter, we report the detection of an absorption-like feature at ~1.89 keV in Chandra/ACIS spectra of the ultraluminous X-ray source NGC 4861 X-2, based on the deepest obse…

astro-ph.HE2026

NICER detection of a new candidate cyclotron line in the bursting X-ray pulsar GRO J1744-28

Qi Liu, Lingda Kong, Long Ji +15

We report the detection of cyclotron resonant scattering features (CRSFs) in the spectrum of the unique bursting pulsar GRO J1744-28, observed during its recent outburst in 2021 wi…

astro-ph.HE2026

Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262

Lingda Kong, Xiaohang Dai, Andrea Santangelo +12

Accretion onto strongly magnetized neutron stars is commonly interpreted using quasi-steady models, in which the accretion-column structure adjusts smoothly to the mass inflow rate…

astro-ph.HE2026★ 1 cited

Identification of three new ultraluminous X-ray sources in NGC 4631 and NGC 1097: Evidence for stellar-mass black holes

Sinan Allak, Aysun Akyuz, Yasemin Aladag +2

Recent observations of galaxies continue to reveal new ultraluminous X-ray sources (ULXs), increasing their known population and improving the statistics needed to understand their…

astro-ph.HE2026

Long-term evolution of cyclotron resonant scattering features in the accreting pulsar Vela X-1: A pulse-to-pulse approach

Yu-Jia Du, Peng-Ju Wang, Lorenzo Ducci +5

We investigated the long-term evolution of the cyclotron line energy, as well as the relationship between cyclotron line energy and luminosity in the high-mass X-ray binary Vela X-…

astro-ph.HE2025

Discovery of a 9.67-s pulsar in an ultraluminous X-ray source in NGC 4631 with XMM-Newton

L. Ducci, S. Mereghetti, F. Pintore +4

Thanks to a recent observation with XMM-Newton, we discovered periodic pulsations at P= 9.6652 +/- 0.0002 s in a new ultraluminous X-ray source (ULX) in the galaxy NGC 4631. This s…

astro-ph.HE2025

Probing the emission geometry of the X-ray pulsar 2S 1417624 during a weak outburst with NICER, IXPE, and NuSTAR

Menglei Zhou, Pengju Wang, Honghui Liu +12

We report results from a multi-mission observational campaign of the transient X-ray pulsar 2S~1417624 during its 2025 outburst, using data from NICER, IXPE, and NuSTAR. Phase-a…

astro-ph.HE2025★ 1 cited

Probing the polarized emission from the accretion-powered pulsar 4U 1907+09 with IXPE

Menglei Zhou, Lorenzo Ducci, Honghui Liu +12

We present observations of the accretion-powered X-ray pulsar (XRP) 4U 1907+09, conducted with the Imaging X-ray Polarimetry Explorer (IXPE) that delivers the first high-quality po…

astro-ph.HE2025

Timing and spectral variability in 2S 1417-624 observed with Insight-HXMT

Qi Liu, Lingda Kong, Can Güngör +5

We present the results of the spectral and timing analyses of the accreting X-ray pulsar, 2S 1417-624, during the 2018 and 2021 outbursts with Insight-HXMT. We find that the pulse…

astro-ph.HE2025

Timing and spectral studies of the Be/X-ray binary EXO 2030+375 using Insight-HXMT observations

Yu-Jia Du, Lorenzo Ducci, Long Ji +5

We report the X-ray spectral and timing analysis of the high mass X-ray binary EXO 2030+375 during the 2021 type-II outburst based on the Insight-HXMT observations. Pulsations can…

astro-ph.HE2024

Searching for orbital period modulation in X-ray observations of the symbiotic X-ray binary GX 1+4

Moritz Klawin, Lorenzo Ducci, M. Mirac Serim +3

The symbiotic X-ray binary GX 1+4 possesses a number of peculiar properties that have been studied since the early 1970s. In particular, the orbital period has been a point of deba…

astro-ph.HE2024★ 3 cited

The high-energy cyclotron line in 2S 1417-624 discovered with Insight-HXMT during the 2018 outburst

Q. Liu, A. Santangelo, L. D. Kong +7

We report a detailed timing and spectral analysis of the X-ray pulsar 2S~1417-624 using the data from Insight-HXMT during the 2018 outburst. The pulse profiles are highly variable…

astro-ph.HE2024★ 3 cited

Temporal and spectral variations of the X-ray pulsar Cen X-3 observed by NuSTAR

Qi Liu, Wei Wang, Andrea Santangelo +3

We report a time-resolved analysis of the accreting X-ray pulsar Cen X-3 using observations carried out by NuSTAR, which cover approximately two binary orbits in different intensit…

astro-ph.HE2024

XMM-Newton observations of the peculiar Be X-ray binary A0538-66

Michela Rigoselli, Caterina Tresoldi, Lorenzo Ducci +1

A0538-66 is a neutron star/Be X-ray binary located in the Large Magellanic Cloud and, since its discovery in the seventies, it showed a peculiar behavior which makes it a unique ob…

astro-ph.HE2024★ 2 cited

Soft X-ray emission from the classical nova AT 2018bej

A. Tavleev, L. Ducci, V. F. Suleimanov +4

Classical novae are known to demonstrate a supersoft X-ray source (SSS) state following outbursts, which is associated with residual thermonuclear burning on the white dwarf (WD) s…

astro-ph.HE2024★ 17 cited

Discovery of the first anti-glitch event in the rotation-powered pulsar PSR B0540-69

Youli Tuo, M. M. Serim, Marco Antonelli +5

Using data from the Neutron star Interior Composition ExploreR (NICER) observatory, we identified a permanent spin frequency decrease of $Δν=-(1.04\pm0.07)\times 10^{-7}\,\mathrm{H…

astro-ph.HE2024

Timing analysis of the newly discovered black hole candidate Swift J1727.8-1613 with Insight-HXMT

Wei Yu, Qing-Cui Bu, Shuang-Nan Zhang +9

We present the results obtained from an X-ray timing study of the new black hole candidate (BHC) Swift J1727.8-1613. The work is based on Hard X-ray Modulation Telescope (Insight-H…

astro-ph.HE2024

The polarization of the boundary layer around weakly magnetized neutron stars in X-ray binaries

R. Farinelli, A. Waghmare, L. Ducci +1

X-ray binaries hosting a compact object have been among the main targets of the Imaging X-ray Polarimetry Explorer (IXPE) since its launch, due to their high brightness in the 2-8…

astro-ph.HE2024★ 6 cited

Correlated spectro-polarimetric study along the Z track in XTE J1701-462 puts constraints on its coronal geometry

Wei Yu, Qingcui Bu, Victor Doroshenko +13

Context. In September 2022, the transient neutron star low-mass X-ray binary XTE J1701-462 went into a new outburst. Aims. The objective of this work is to examine the evolution of…

astro-ph.HE2023

Timing and Spectral Analysis of HMXB 4U 1700-37 Observed with Insight-HXMT

Hua Xiao, Long Ji, Peng Zhang +5

We report timing and spectral studies of the high mass X-ray binary 4U 1700-37 using Insight-HXMT observations carried out in 2020 during its out-of-eclipse state. We found signifi…

astro-ph.HE2023★ 1 cited

Discovery of spin-phase dependent QPOs in the super-critical accretion regime from the X-ray pulsar RX J0440.9+4431

Christian Malacaria, Daniela Huppenkothen, Oliver J. Roberts +5

RX J0440.9+4431 is an accreting X-ray pulsar (XRP) that remained relatively unexplored until recently, when major X-ray outburst activity enabled more in-depth studies. Here, we re…