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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…

高能天体物理现象 · 物理学 2022-10-12 Manoj Ghising , Mohammed Tobrej , Binay Rai , Ruchi Tamang , Bikash Chandra Paul

We report timing and spectral properties of the transient Be X-ray pulsar EXO 053109--6609.2 studied using observations made with the ASCA and BeppoSAX observatories. Though there must have been at least one spin-down episode of the pulsar…

天体物理学 · 物理学 2009-11-10 B. Paul , S. N. A. Jaaffery , S. Naik , P. C. Agrawal

We report the results obtained from a detailed timing and spectral studies of Be/X-ray binary pulsar 2S 1417-624 using data from Swift and NuSTAR observatories. The observations were carried out at the peak of a giant outburst of the pulsar…

高能天体物理现象 · 物理学 2019-10-16 Shivangi Gupta , Sachindra Naik , Gaurava K. Jaisawal

We have studied the temporal and spectral properties of SXP 15.3 observed by \textit{NuSTAR} in hard energy range 3-79 keV during late 2018. The timing analysis of \textit{NuSTAR} observation predicts coherent pulsation at…

高能天体物理现象 · 物理学 2023-02-24 Manoj Ghising , Binay Rai , Mohammed Tobrej , Ruchi Tamang , Bikash Chandra Paul

We report on the discovery of X-ray pulsations in the Be/X-ray binary IGR J21343+4738 during an XMM-Newton observation. We obtained a barycentric corrected pulse period of 320.35+-0.06 seconds. The pulse profile displays a peak at low…

高能天体物理现象 · 物理学 2015-06-19 P. Reig , A. Zezas

We present the results of the observations of the giant bursts from the X-ray pu lsar A0535+26 made by HEXE onboard Mir-Kvant in April 1989, November 1993 and February 1994. The pulse periods were measured, pulse profiles in different…

We report the detection of pulsed X-ray emission ($4.9\sigma$) from the binary millisecond pulsar PSR J0218+4232 in a 100 ks ROSAT HRI observation. The pulse profile shows a sharp main pulse and an indication for a second weaker pulse at…

天体物理学 · 物理学 2007-05-23 L. Kuiper , W. Hermsen , F. Verbunt , T. Belloni , A. Lyne

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…

高能天体物理现象 · 物理学 2023-07-12 Binay Rai , Mohammed Tobrej , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We have detected pulsed X-ray emission from the fastest millisecond pulsar known, PSR B1937+21 (P=1.558 msec), with ASCA. The pulsar is detected as a point source above $\sim 1.7$ keV, with no indication of nebulosity. The source flux in…

天体物理学 · 物理学 2009-11-06 M. Takahashi

We present the timing and spectral properties of the transient Be/X-ray binary pulsar 3A 0535+262 during quiescence using three observations with the narrow field imaging instruments (NFI) of BeppoSAX. Assuming a distance of 2 kpc for this…

数据分析、统计与概率 · 物理学 2009-11-10 U. Mukherjee , B. Paul

We present a comprehensive timing and spectral studies of Be/X-ray binary pulsar EXO 2030+375 using extensive Rossi X-ray Timing Explorer observations from 1995 till 2011, covering numerous Type I and 2006 Type II outbursts. Pulse profiles…

高能天体物理现象 · 物理学 2017-11-08 Prahlad Epili , Sachindra Naik , Gaurava K. Jaisawal , Shivangi Gupta

We study the timing and spectral properties of the Be/X-ray binary pulsar SXP 138 using four NuSTAR observations spanning 2016 to 2017. Analysis of the light curves using the Lomb-Scargle periodogram shows an increase in the spin period of…

高能天体物理现象 · 物理学 2025-04-11 Soham Pravin Sanyashiv , Sayantan Bhattacharya , Sudip Bhattacharyya

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…

高能天体物理现象 · 物理学 2017-08-30 E. V. Gotthelf , S. Bogdanov

The results from three ASCA observations of AX J0051.6-7311 = RX J0051.9-7311 are reported. Coherent pulsations with a barycentric period of 172.40 +/- 0.03 s were discovered in the third observation, with an exceptionally long exposure…

天体物理学 · 物理学 2015-06-24 Jun Yokogawa , Ken'ichi Torii , Kensuke Imanishi , Katsuji Koyama

We are reporting a discovery of X-ray pulsations from the source AX J1749.1-2733 with the period of ~132 s based on the XMM-Newton data obtained in March 2007. The observed pulse profile has a double-peaked structure with the pulse fraction…

天体物理学 · 物理学 2009-11-13 D. I. Karasev , S. S. Tsygankov , A. A. Lutovinov

We have studied the timing and spectral properties of the BeXB 4U 1901+03 during the 2019 outburst using \textit{NuSTAR}, \textit{Swift}, and \textit{NICER} observations. Flares are in all observations and were of tens to hundreds of…

高能天体物理现象 · 物理学 2021-09-08 Binay Rai , Bikash Chandra Paul

We investigated the optical, X-ray, and gamma-ray variability of the pulsar SAX J2103.5+4545. Our timing and spectral analyses of the X-ray and gamma-ray emissions from the source using RXTE and INTEGRAL data show that the shape of its…

We present timing and broad-band spectral studies of the high mass X-ray binary pulsar 4U 1909+07 using data from Suzaku observation during 2010 November 2-3. The pulse period of the pulsar is estimated to be 604.11+/-0.14 s. Pulsations are…

高能天体物理现象 · 物理学 2016-02-16 Gaurava K. Jaisawal , Sachindra Naik , Biswajit Paul

During normal Type I outbursts, the pulse profiles of Be/X-ray binary pulsars are found to be complex in soft X-ray energy ranges. The profiles in soft X-ray energy ranges are characterized by the presence of narrow absorption dips or…

太阳与恒星天体物理 · 物理学 2013-11-22 Sachindra Naik

We present the results of a BeppoSAX observation of the fastest rotating pulsar known: PSR B1937+21. The ~200 ks observation (78.5 ks MECS/34 ks LECS on-source time) allowed us to investigate with high statistical significance both the…

天体物理学 · 物理学 2008-11-26 L. Nicastro , G. Cusumano , O. Loehmer , M. Kramer , L. Kuiper , W. Hermsen , T. Mineo , W. Becker