English
Related papers

Related papers: A possible phase dependent absorption feature in t…

200 papers

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

In the beginning of 2023 the Be transient X-ray pulsar RX J0440.9+4431 underwent a fist-ever giant outburst observed from the source peaking in the beginning of February and reaching peak luminosity of $\sim 4.3\times10^{37}$ erg s$^{-1}$.…

The NuSTAR hard X-ray telescope observed the transient Be/X-ray binary GS 0834-430 during its 2012 outburst - the first active state of this system observed in the past 19 years. We performed timing and spectral analysis, and measured the…

We present the results obtained from timing and spectral studies of the newly discovered accreting X-ray binary pulsar Swift J0243.6+6124 using a NuSTAR observation in 2017 October at a flux level of ~280 mCrab. Pulsations at 9.85423(5) s…

High Energy Astrophysical Phenomena · Physics 2017-11-30 Gaurava K. Jaisawal , Sachindra Naik , J. Chenevez

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…

The results of the broadband spectral and timing study of the recently discovered transient X-ray pulsar MAXI J0903-531 in a wide range of luminosities differing by a factor of ~30 are reported. The observed X-ray spectrum in both states…

We report the discovery of the X-ray transient SAX J2103.5+4545 which was active from February to September 1997. The observed peak intensity of 20 mCrab (2 to 25 keV) occurred on April 11. An analysis of data obtained around the time of…

Astrophysics · Physics 2007-05-23 F. Hulleman , J. J. M. in 't Zand , J. Heise

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 present the results of our spectral and timing analysis of the emission from the transient X-ray pulsar XTE J1946+274 based on the simultaneous NuSTAR and Swift/XRT observations in the broad energy range 0.3-79 keV carried out in June…

High Energy Astrophysical Phenomena · Physics 2021-10-12 A. S. Gorban , S. V. Molkov , S. S. Tsygankov , A. A. Lutovinov

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…

High Energy Astrophysical Phenomena · Physics 2026-02-16 Rahul Sharma , Andrea Sanna , Prince Sharma

Aims. We present the first long-term pulse profile study of the X-ray pulsar SAX J2103.5+4545. Our main goal is to study the pulse shape correlation either with luminosity, time or energy. Methods. This Be/X-ray binary system was observed…

Astrophysics · Physics 2009-11-13 A. Camero Arranz , C. A. Wilson , M. H. Finger , V. Reglero

We report on the energy-resolved timing and phase-resolved spectral analysis of X-ray emission from PSR J0659+1414 observed with XMM-Newton and NuSTAR. We find that the new data rule out the previously suggested model of the phase-dependent…

High Energy Astrophysical Phenomena · Physics 2018-12-26 Prakash Arumugasamy , Oleg Kargaltsev , Bettina Posselt , George G. Pavlov , Jeremy Hare

We analyze the properties of the pulsed emission from the accreting millisecond pulsar SAX J1808.4-3658 in observations of its April 1998 outburst by the Rossi X-Ray Timing Explorer. Pulse phase spectroscopy shows that the emission evolves…

Astrophysics · Physics 2009-10-31 Eric C. Ford

We report the timing and spectral properties of Be/X-ray binary pulsar GX 304-1 by using two Suzaku observations during its 2010 August and 2012 January X-ray outbursts. Pulsations at ~275 s were clearly detected in the light curves from…

Solar and Stellar Astrophysics · Physics 2016-02-16 Gaurava K. Jaisawal , Sachindra Naik , Prahlad Epili

We present an X-ray and UV high-time-resolution monitoring of the final flaring phase of the 2022 outburst of the AMSP SAX J1808.4-3658, based on simultaneous XMM-Newton and HST observations. The uninterrupted coverage provided by…

The results of the broadband spectral and timing study of the transient X-ray pulsar GRO J2058+42 in a wide energy range at a low luminosity $L_{x} \simeq 2.5\times 10^{36}$ erg s$^{-1}$ are reported. The data revealed that the pulse…

High Energy Astrophysical Phenomena · Physics 2022-03-08 A. S. Gorban , S. V. Molkov , S. S. Tsygankov , A. A. Mushtukov , A. A. Lutovinov

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 report results of a spectral and timing analysis of the X-ray pulsar XTE J1829-098 using data obtained with the NuSTAR observatory during an outburst in August 2018. A strong absorption feature was detected at the energy of…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Andrey E. Shtykovsky , Alexander A. Lutovinov , Sergey S. Tsygankov , Sergey V. Molkov

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

In two recent INTEGRAL papers, Lutovinov et al. (2003) and Blay et al. (2004) report a timing and spectral analysis of the transient Be/X-ray pulsar SAX J2103.5+4545 at high energies (5--200 keV). In this work we present for the first time…

‹ Prev 1 2 3 10 Next ›