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Related papers: PSR J1838-0655: X-Ray Observations with NICER and …

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We analyzed X-ray data from Chandra, XMM-Newton, NICER, and NuSTAR to characterize the properties of the pulsar PSR J1838$-$0655 and its pulsar wind nebula (PWN) associated with HESS J1837$-$069. Based on 5.5 years of NICER monitoring, we…

High Energy Astrophysical Phenomena · Physics 2025-08-12 Minseo Park , Jaegeun Park , Chanho Kim , Hongjun An

We report on the long-term timing analysis of PSR J2022+3842 using observations from the Neutron Star Interior Composition Explorer (NICER), along with spectral properties derived from joint observations with NICER and the Nuclear…

High Energy Astrophysical Phenomena · Physics 2026-05-26 Jia-Ning Hu , Xiang-Hua Li , Xian-Ao Wang , Han-Long Peng , Shi-Qi Zhou , Wen-Tao Ye , Shi-Jie Zheng , Ze-Jun Jiang , Ming-Yu Ge

We report on a NuSTAR observation of the young, energetic pulsar PSR J1617-5055. Parkes Observatory 3 GHz radio observations of the pulsar (taken about 7 years before the NuSTAR observations) are also reported here. NuSTAR detected…

High Energy Astrophysical Phenomena · Physics 2022-01-05 J. Hare , I. Volkov , G. G. Pavlov , O. Kargaltsev , S. Johnston

We present the results of the broadband timing and spectral analysis of the poorly understood SMC pulsar RX J0032.9-7348 (= SXP 7.02) using NuSTAR and NICER observations during its X-ray brightening in 2024. Our timing analysis revealed a…

High Energy Astrophysical Phenomena · Physics 2025-05-01 Birendra Chhotaray , Gaurava K. Jaisawal , Sachindra Naik , Arghajit Jana

We present a hard X-ray NuSTAR observation of PSR J0437-4715, the nearest millisecond pulsar. The known pulsations at the apparent pulse period ~5.76 ms are detected at energies up to 20 keV. We measure a photon index $\Gamma= 1.65\pm0.24$…

Synchrotron X-ray emission from a pulsar wind nebula (PWN) is a sensitive probe of its magnetic field and high-energy particle population. Here we analyze contemporaneous NuSTAR and XMM-Newton observations of the PWN G54.1+0.3, powered by…

High Energy Astrophysical Phenomena · Physics 2025-06-30 J. A. J. Alford , G. -B. Zhang , J. D. Gelfand

We report on our monitoring of the strong-field magnetar-like pulsar PSR J1846-0258 with the Neutron Star Interior Composition Explorer (NICER) and the timing and spectral evolution during its outburst in August 2020. Phase-coherent timing…

We report on Nuclear Spectroscopic Telescope Array (NuSTAR) hard X-ray observations of the young rotation-powered radio pulsar PSR B1509$-$58 in the supernova remnant MSH 15$-$52. We confirm the previously reported curvature in the hard…

High Energy Astrophysical Phenomena · Physics 2016-02-03 Ge Chen , Hongjun An , Victoria M. Kaspi , Fiona A. Harrison , Kristin K. Madsen , Daniel Stern

We report on the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER) of the accreting millisecond X-ray pulsar IGR J17591-2342, detecting coherent X-ray pulsations…

We present in this paper the hard X-ray view of the pulsar wind nebula in G11.2-0.3 and its central pulsar PSR J1811-1925 as seen by NuSTAR. We complement the data with Chandra for a more complete picture and confirm the existence of a…

High Energy Astrophysical Phenomena · Physics 2020-03-04 K. K. Madsen , C. L. Fryer , B. W. Grefenstette , L. A. Lopez , S. Reynolds , A. Zoglauer

We present broad-band X-ray spectroscopy of the energetic components that make up the supernova remnant (SNR) Kesteven 75 using concurrent 2017 Aug 17-20 XMM-Newton and NuSTAR observations, during which the pulsar PSR J1846-0258 is found to…

High Energy Astrophysical Phenomena · Physics 2021-03-03 E. V. Gotthelf , S. Safi-Harb , S. M. Straal , J. D. Gelfand

We report the results of a deep XMM-Newton observation of the radio-faint $\gamma$-ray pulsar J1741-2054 and its nebula together with the analysis of 5 years of Fermi LAT data. The X-ray spectrum of the pulsar is consistent with an absorbed…

High Energy Astrophysical Phenomena · Physics 2015-06-19 M. Marelli , A. Belfiore , P. Saz Parkinson , P. Caraveo , A. De Luca , C. Sarazin , D. Salvetti , G. R. Sivakoff , F. Camilo

We present Nuclear Spectroscopic Telescope Array (NuSTAR) hard X-ray timing and spectroscopy of the three exceptionally energetic rotation-powered millisecond pulsars PSRs B1821-24, B1937+21, and J0218+4232. By correcting the NuSTAR onboard…

High Energy Astrophysical Phenomena · Physics 2017-08-30 E. V. Gotthelf , S. Bogdanov

We study the timing and spectral properties of the X-ray pulsar 2S 1417--624 during the recent outburst in January 2021 based on the Neutron Star Interior Composition Explorer (NICER) observation. We also used some early data from the 2018…

High Energy Astrophysical Phenomena · Physics 2022-11-28 Manoj Mandal , Sabyasachi Pal

We present and interpret several new X-ray features of the X-ray pulsar PSR J1838-0655. The X-ray data are obtained from the archival data of CHANDRA, RXTE}, and SUZAKU. We combine all these X-ray data and fit the spectra with different…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Lupin Chun-Che Lin , Jumpei Takata , Chorng-Yuan Hwang , Jau-Shian Liang

We report on the results of a NuSTAR observation of the Supergiant Fast X-ray Transient pulsar IGRJ11215-5952 during the peak of its outburst in June 2017. IGRJ11215-5952 is the only SFXT undergoing strictly periodic outbursts, every 165…

High Energy Astrophysical Phenomena · Physics 2020-07-01 L. Sidoli , K. Postnov , A. Tiengo , P. Esposito , V. Sguera , A. Paizis , G. A. Rodrıguez Castillo

The Be X-ray binary GRO J2058+42 recently went through a Type-II outburst during March-April 2019 lasting for about 50 days. This outburst was detected with the operating all sky X-ray monitors like the Fermi-GBM, Swift-BAT and MAXI-GSC.…

High Energy Astrophysical Phenomena · Physics 2020-07-22 Sanhita Kabiraj , Biswajit Paul

We study the recently discovered Be/X-ray pulsar MAXI J0655--013 using the 2022 \emph{NuSTAR} observations. The paper is the first detailed study of the timing and spectral properties of the source. The pulse profiles of the pulsar vary…

High Energy Astrophysical Phenomena · Physics 2023-07-12 Binay Rai , Mohammed Tobrej , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We report on the first focused hard X-ray view of the absorbed supergiant system IGRJ18027-2016 performed with the NuSTAR observatory. The pulsations are clearly detected with a period of $P_{spin}=139.866(1)$ s and a pulse fraction of…

High Energy Astrophysical Phenomena · Physics 2016-12-28 A. Lutovinov , S. Tsygankov , K. Postnov , R. Krivonos , S. Molkov , J. Tomsick

In this paper, we report on the hard X-ray observation of the X-ray pulsar 1E 1145.1-6141 performed with the Nuclear Spectroscopic Telescope Array mission (NuSTAR). The coherent pulsation of the source with a period of…

High Energy Astrophysical Phenomena · Physics 2022-10-12 Manoj Ghising , Mohammed Tobrej , Binay Rai , Ruchi Tamang , Bikash Chandra Paul
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