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We report an analysis of Insight-HXMT observations of the newly discovered accreting millisecond pulsar SRGA J144459.2$-$604207. During the outburst, detected in 2024 February by SRG/ART-XC, the broadband persistent spectrum was well fitted…

We present the discovery, with the Neutron Star Interior Composition Explorer (NICER), that SRGA J144459.2-604207 is a 447.9 Hz accreting millisecond X-ray pulsar (AMXP), which underwent a four-week long outburst starting on 2024 February…

We present the results obtained from the spectral and temporal study of thermonuclear bursts from the millisecond X-ray pulsar SRGA J144459.2-604207 detected with NICER. The dynamic evolution of the spectral parameters in a broad energy…

高能天体物理现象 · 物理学 2025-07-23 Manoj Mandal , Sachindra Naik , Birendra Chhotaray

We present a comprehensive study of the X-ray spectral properties of the accreting millisecond pulsar IGR J17498$-$2921 during its 2023 outburst. Similar to other accreting millisecond pulsars, the broad-band spectral emission observed…

We analyze three NuSTAR observations and two NICER observations of the transient accreting millisecond pulsar SAX J1808.4-3658 in the hard spectral state during its most recent outbursts in 2022 and 2025. The spectral analysis of the…

高能天体物理现象 · 物理学 2026-04-09 Mahasweta Bhattacharya , Aditya S. Mondal , Gulab C. Dewangan

We report the discovery of burst oscillations at the spin frequency in ten thermonuclear bursts from the accreting millisecond X-ray pulsar (AMXP) IGR J17511-3057. The burst oscillation properties are, like those from the persistent AMXPs…

高能天体物理现象 · 物理学 2015-05-19 D. Altamirano , A. Watts , M. Linares , C. B. Markwardt , T. Strohmayer , A. Patruno

The accreting millisecond X-ray pulsar IGR J17498-2921 went into X-ray outburst on April 13-15, 2023, for the first time since its discovery on August 11, 2011. Here, we report on the first follow-up \nustar{} observation of the source,…

高能天体物理现象 · 物理学 2024-09-12 Mahasweta Bhattacharya , Aditya S. Mondal , Mayukh Pahari , Biplab Raychaudhuri , Rohit Ghosh , Gulab C. Dewangan

The twelfth accretion-powered millisecond pulsar, IGR J17511-3057, was discovered in September 2009. In this work we study its spectral and timing properties during the 2009 outburst based on Swift and RXTE data. Our spectral analysis of…

高能天体物理现象 · 物理学 2015-03-18 A. Ibragimov , J. J. E. Kajava , J. Poutanen

Thermonuclear (type-I) bursts exhibit properties that depend both on the local surface conditions of the neutron stars on which they ignite, as well as the physical parameters of the host binary system. However, constraining the system…

高能天体物理现象 · 物理学 2024-10-23 D. K. Galloway , A. J. Goodwin , T. Hilder , L. Waterson , M. Cupák

We present a spectral and timing study of the NuSTAR and Swift observations of the black hole candidate IGR J17091-3624 in the hard state during its outburst in 2016. Disk reflection is detected in each of the NuSTAR spectra taken in three…

We report the spectral analysis of accretion powered millisecond X-ray pulsar SAX J1748.9-2021 from the NuSTAR observation made during its 2015 outburst. The spectra displayed a broad emission line at $\sim 6.5$ keV with line width of $\sim…

高能天体物理现象 · 物理学 2018-10-17 Rahul Sharma , Chetana Jain , Anjan Dutta

SRGA J144459.2$-$604207 is a newly confirmed accreting millisecond X-ray pulsar and type I X-ray burster. We present the broadband X-ray timing and spectral behaviors of SRGA J144459.2$-$604207 during its 2024 outburst. The data were…

The millisecond pulsar MAXI J1816-195 was recently discovered in an outburst by MAXI in 2022 May. We study different properties of the pulsar using data from NuSTAR and NICER observations. The unstable burning of accreted material on the…

高能天体物理现象 · 物理学 2023-02-28 Manoj Mandal , Sabyasachi Pal , Jaiverdhan Chauhan , Anne Lohfink , Priya Bharali

We report the broadband timing and spectral properties of the neutron star low-mass X-ray binary Aql X-1 during the 2024 outburst with NICER, NuSTAR, and Swift observatories. We detected six thermonuclear X-ray bursts during the NICER and…

高能天体物理现象 · 物理学 2025-04-25 Manoj Mandal , Sabyasachi Pal , G. K. Jaisawal , Anne Lohfink , Sachindra Naik , Jaiverdhan Chauhan

In August 2008, the accreting milli-second X-ray pulsar (AMXP), IGR J00291+5934, underwent an outburst lasting ~ 100 days, the first since its discovery in 2004. We present data from the double-peaked outburst from Faulkes Telescope North,…

IGR J17511-3057 is the second X-ray transient accreting millisecond pulsar discovered by INTEGRAL. It was in outburst for about a month from September 13, 2009. The broad-band average spectrum is well described by thermal Comptonization…

高能天体物理现象 · 物理学 2011-07-18 M. Falanga , L. Kuiper , J. Poutanen , D. K. Galloway , E. W. Bonning , E. Bozzo , A. Goldwurm , W. Hermsen , L. Stella

We report on the broadband spectral and timing properties of the accreting millisecond X-ray pulsar IGR J17498$-$2921 during its April 2023 outburst using data from NICER (1$-$10 keV), NuSTAR (3$-$79 keV), Insight-HXMT (2$-$150 keV), and…

高能天体物理现象 · 物理学 2024-11-06 Zhaosheng Li , L. Kuiper , Y. Y. Pan , M. Falanga , J. Poutanen , Y. P. Chen , R. X. Xu , M. Y. Ge , Y. Huang , L. M. Song , S. Zhang , F. J. Lu , S. N. Zhang

We report on the discovery of the new accreting millisecond X-ray pulsar SRGAJ144459.2-604207 using the SRG/ART-XC data. The source was observed twice in February 2024 during the declining phase of the outburst. Timing analysis revealed a…

We report on an XMM-Newton observation of the accreting millisecond pulsar, IGR J17511-3057. Pulsations at 244.8339512(1) Hz are observed with an RMS pulsed fraction of 14.4(3)%. A precise solution for the P_orb=12487.51(2)s binary system…

高能天体物理现象 · 物理学 2015-05-19 A. Papitto , A. Riggio , T. Di Salvo , L. Burderi , A. D'Aì , R. Iaria , E. Bozzo , M. T. Menna

An outburst of the accreting X-ray millisecond pulsar SAX J1808.4-3658 in October-November 2002 was followed by the Rossi X-ray Timing Explorer for more than a month. We demonstrate how the area covered by the hotspot at the neutron star…

太阳与恒星天体物理 · 物理学 2010-02-20 Askar Ibragimov , Juri Poutanen
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