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相关论文: Study of the reflection spectra of SAX J1748.9-202…

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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

SAX J1748.9-2021 is a transient accretion powered millisecond X-ray pulsar located in the Globular cluster NGC 6440. We report on the spectral and timing analysis of SAX J1748.9-2021 performed on AstroSat data taken during its faint and…

高能天体物理现象 · 物理学 2020-01-22 Rahul Sharma , Aru Beri , Andrea Sanna , Anjan Dutta

We analyzed a 115 ks XMM-Newton observation and the stacking of 8 days of INTEGRAL observations, taken during the raise of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021. The source showed numerous type-I burst…

The first discovered accreting millisecond pulsar, SAX J1808.4-3658, went into X-ray outburst in April 2015. We triggered a 100 ks XMM-Newton ToO, taken at the peak of the outburst, and a 55 ks NuSTAR ToO, performed four days apart. We…

高能天体物理现象 · 物理学 2018-11-14 T. Di Salvo , A. Sanna , L. Burderi , A. Papitto , R. Iaria , A. F. Gambino , A. Riggio

SAX J1748.9-2021 is an accreting X-ray millisecond pulsar observed in outburst five times since its discovery in 1998. In early October 2017, the source started its sixth outburst, which lasted only ~13 days, significantly shorter than the…

高能天体物理现象 · 物理学 2018-07-18 F. Pintore , A. Sanna , A. Riggio , T. Di Salvo , S. Mereghetti , E. Bozzo , C. Sánchez-Fernández , L. Burderi , R. Iaria

We performed a comprehensive study of thermonuclear bursts from the millisecond X-ray pulsar SAX J1808.4$-$3658 with XMM-Newton and NICER. We report the results from the analysis of an intense burst with NICER using a self-consistent and…

高能天体物理现象 · 物理学 2026-03-31 Manoj Mandal , Sachindra Naik , Birendra Chhotaray

We report on our investigation of the NuSTAR and AstroSat observations along with simultaneous NICER observations of the accreting millisecond X-ray pulsar SAX J1808.4$-$3658, obtained during its tenth outburst from 2022. The NuSTAR…

高能天体物理现象 · 物理学 2026-02-16 Rahul Sharma , Andrea Sanna , Prince Sharma

The accreting millisecond pulsar SAX J1808.4-3658 went into outburst from July to November in 2019 and August to October in 2022, which were observed by \textit{NICER} and \textit{NuSTAR}. In this paper, we first present the light curve for…

高能天体物理现象 · 物理学 2026-01-06 Katherine Bruce , Sachiko Tsuruta , Andrew C. Liebmann , Marcus Teter

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

Accreting millisecond pulsars (AMSPs) are excellent laboratories to study reflection spectra and their features from an accretion disk truncated by a rapidly rotating magnetosphere near the neutron star surface. These systems also exhibit…

We present an analysis of the NuSTAR and Swift spectra of the black hole candidate MAXI J1813-095 in a failed-transition outburst in 2018. The NuSTAR observations show evidence of reflected emission from the inner region of the accretion…

We report on a NuSTAR observation of the recently discovered bright black hole candidate MAXI J1535-571. NuSTAR observed the source on MJD 58003 (five days after the outburst was reported). The spectrum is characteristic of a black hole…

1RXS J180408.9-342058 is a transient neutron star low-mass X-ray binary that exhibited a bright accretion outburst in 2015. We present Nustar, Swift, and Chandra observations obtained around the peak of this outburst. The source was in a…

Ever since the launch of the NuSTAR mission, the hard X-ray range is being covered to an unprecedented sensitivity. This range encodes the reflection features arising from active galactic nuclei (AGN). Especially, the reflection of the…

高能天体物理现象 · 物理学 2022-08-03 Eugenio Bottacini

We report on the \nustar{} observation of the atoll type neutron star (NS) low-mass X-ray binary GX~3+1 performed on 17 October 2017. The source was found in a soft X-ray spectral state with $3-70$keV luminosity of $L_\text{X}\sim3\times…

高能天体物理现象 · 物理学 2019-06-17 Aditya S. Mondal , G. C. Dewangan , B. Raychaudhuri

SAX J1748.9-2021 is a transiently accreting X-ray millisecond pulsar. It is also known as an X-ray burster source discovered by Beppo-SAX. We analysed the persistent emission and type-I X-ray burst properties during its 2015 outburst. The…

高能天体物理现象 · 物理学 2018-12-12 Zhaosheng Li , V. De Falco , M. Falanga , E. Bozzo , L. Kuiper , J. Poutanen , A. Cumming , D. K. Galloway , Shu Zhang

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

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 report on a \textit{NuSTAR} and \textit{Swift}/XRT observation of the newly discovered X-ray transient MAXI J1820+070. \textit{Swift}/XRT and \textit{NuSTAR} have concurrently observed the newly detected source on 14 March 2018. We have…

高能天体物理现象 · 物理学 2019-07-03 Priya Bharali , Jaiverdhan Chauhan , Kalyanee Boruah

We perform the first reflection study of the soft X-ray transient and Type 1 burst source XTE J1709-267 using NuSTAR observations during its 2016 June outburst. There was an increase in flux near the end of the observations, which…

高能天体物理现象 · 物理学 2017-04-05 R. M. Ludlam , J. M. Miller , E. C. Cackett , N. Degenaar , A. C. Bostrom
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