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We have performed a comprehensive spectral and timing analysis of the first NuSTAR observation of the high-mass X-ray binary 4U 1538-522. The observation covers the X-ray eclipse of the source, plus the eclipse ingress and egress. We use…

We present a comprehensive timing and spectral analysis of the HMXB 4U 1538-522 by using the Nuclear Spectroscopic Telescope Array (NuSTAR) observatory data. Using three archived observations made between 2019 and 2021, we have detected…

High Energy Astrophysical Phenomena · Physics 2023-05-10 Prince Sharma , Chetana Jain , Anjan Dutta

We present a spectral and timing analysis of INTEGRAL observations of two high mass X-ray binaries, 4U 1538-522 and 4U 1907+09. Our timing measurements for 4U 1538-522 find the pulse period to have exhibited a spin-up trend until…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Paul Hemphill , Richard Rothschild , Isabel Caballero , Katja Pottschmidt , Matthias Kuehnel , Felix Fuerst , Joern Wilms

We report the first report on cyclotron line studies with the LAXPC instrument onboard AstroSat of the High mass X-ray Binary pulsar 4U 1538-52. During the observation of source which spanned about one day with a net exposure of 50 ks,the…

High Energy Astrophysical Phenomena · Physics 2018-12-26 Varun , Chandreyee Maitra , Pragati Pradhan , Harsha Raichur , Biswajit Paul

We report X-ray observations of the High Mass X-ray Binary (HMXB) pulsar 4U 1907+09. Spectral and Timing analysis of the source has been performed using NuSTAR observation. Timing analysis of the photon events revealed the coherent X-ray…

High Energy Astrophysical Phenomena · Physics 2022-11-14 Mohammed Tobrej , Binay Rai , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We present the broadband X-ray study of the BeXRB pulsar IGR J06074+2205 using NuSTAR observations. The temporal and spectral characteristics of the source are investigated. We detect coherent X-ray pulsations of the source and determine…

High Energy Astrophysical Phenomena · Physics 2024-04-24 Mohammed Tobrej , Binay Rai , Manoj Ghising , Bikash Chandra Paul

An overview of the results of observations for the transient X-ray pulsar 4U 0115+63, a member of a binary system with a Be star, since its discovery to the present day (~40 years) based on data from more than dozen observatories and…

High Energy Astrophysical Phenomena · Physics 2015-06-16 P. A. Boldin , S. S. Tsygankov , A. A. Lutovinov

We report comprehensive spectral and temporal properties of the Be/X-ray binary pulsar SMC X-2 using X-ray observations during the 2015 and 2022 outbursts. The pulse profile of the pulsar is unique and strongly luminosity dependent. It…

High Energy Astrophysical Phenomena · Physics 2023-03-21 G. K. Jaisawal , G. Vasilopoulos , S. Naik , C. Maitra , C. Malacaria , B. Chhotaray , K. C. Gendreau , S. Guillot , M. Ng , A. Sanna

We report the results of temporal and spectral analysis performed on the X-ray pulsar 4U 1538-52 observed by BeppoSAX. We obtained a new estimate of the spin period of the neutron star P=528.24 \pm 0.01 s (corrected for the orbital motion…

Astrophysics · Physics 2009-11-07 N. R. Robba , L. Burderi , T. Di Salvo , R. Iaria , G. Cusumano

We present both timing and spectral analysis of the outburst of 4U 0115+63 in April -- May 2008 with INTEGRAL and RXTE observations. We have determined the spin period of the neutron star at $\sim 3.61430 \pm 0.00003$ s, and a spin up rate…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Jun Li , Wei Wang , Yongheng Zhao

The cyclotron line feature in the X-ray spectrum of the accretion powered pulsar Her X-1 has been observed and monitored for over three decades. The line energy exhibited a slow secular decline over the period 1995-2014, with a possible…

High Energy Astrophysical Phenomena · Physics 2020-07-15 S. Bala , D. Bhattacharya , R. Staubert , C. Maitra

We present the results of the pulse-amplitude-resolved spectroscopy of the accreting pulsar V 0332+53 using the NuSTAR observations of the source in 2015 and 2016. We investigate the dependence of the energy of the cyclotron resonant…

High Energy Astrophysical Phenomena · Physics 2018-03-14 Vadim Vybornov , Viktor Doroshenko , Rürdiger Staubert , Andrea Santangelo

We have performed a full time- and luminosity-resolved spectral analysis of the high-mass X-ray binary 4U 1538-522 using the available RXTE, INTEGRAL, and Suzaku data, examining both phase-averaged and pulse-phase-constrained datasets and…

We report the X-ray characteristics of the persistent X-ray pulsar 4U 1626-67 using simultaneous NuSTAR and NICER observations. The X-ray pulsar 4U 1626-67 has just encountered a torque reversal in 2023 and is presently in the spin-down…

High Energy Astrophysical Phenomena · Physics 2024-01-26 Mohammed Tobrej , Ruchi Tamang , Binay Rai , Manoj Ghising , Bikash Chandra Paul

We have monitored a Type II outburst of the Be/X-ray binary MXB 0656-072 in a series of pointed RXTE observations during October through December 2003. The source spectrum shows a cyclotron resonance scattering feature at 32.8 +/- 0.5 keV,…

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…

High Energy Astrophysical Phenomena · Physics 2023-02-24 Manoj Ghising , Binay Rai , Mohammed Tobrej , Ruchi Tamang , Bikash Chandra Paul

We report results of a spectral and timing analysis of the poorly studied transient X-ray pulsar 2S 1553-542 using data collected with the NuSTAR and Chandra observatories and the Fermi/GBM instrument during an outburst in 2015. Properties…

High Energy Astrophysical Phenomena · Physics 2016-01-27 Sergey S. Tsygankov , Alexander A. Lutovinov , Roman A. Krivonos , Sergey V. Molkov , Peter J. Jenke , Mark H. Finger , Juri Poutanen

We report on a timing and spectral analysis of a 50-ks NuSTAR observation of IGR J16320-4751 (= AX J1631.9-4752); a high-mass X-ray binary hosting a slowly-rotating neutron star. In this observation from 2015, the spin period was…

We present broadband X-ray observations of the High Mass X-ray Binary (HMXB) pulsar SMC X-2, using concurrent NuSTAR and NICER observations during its 2022 outburst. The source is found to be spinning with a period of 2.37281(3) s. We…

High Energy Astrophysical Phenomena · Physics 2025-01-08 Mohammed Tobrej , Binay Rai , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

OAO 1657-415 is an accreting X-ray pulsar with a high mass companion that has been observed by several telescopes over the years, in different orbital phases. Back in 1999, observations performed with Beppo-SAX lead to the detection of a…

High Energy Astrophysical Phenomena · Physics 2022-03-08 Enzo A. Saavedra , Federico A. Fogantini , Jorge A. Combi , Federico García , Sylvain Chaty
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