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Related papers: Simultaneous NICER and NuSTAR Observations of the …

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We report on X-ray and radio observations of the ultra-compact X-ray binary 4U 1543-624 taken in August 2017 during an enhanced accretion episode. We obtained NICER monitoring of the source over a $\sim10$ day period during which…

We report on the first simultaneous $NICER$ and $NuSTAR$ observations of the neutron star (NS) low-mass X-ray binary 4U 1735$-$44, obtained in 2018 August. The source was at a luminosity of $\sim1.8~(D/5.6\ \mathrm{kpc})^{2}\times10^{37}$…

We present the first joint NuSTAR and NICER observations of the ultra-compact X-ray binary (UCXB) 4U 0614+091. This source shows quasi-periodic flux variations on the timescale of ~days. We use reflection modeling techniques to study…

In this study, we examine 51 archival NICER observations and 6 archival NuSTAR observations of the neutron star (NS) ultra-compact X-ray binary (UCXB) 4U 0614+091, which span over 5 years. The source displays persistent reflection features,…

High Energy Astrophysical Phenomena · Physics 2024-09-17 David L. Moutard , Renee M. Ludlam , Edward M. Cackett , Javier A. García , Jon M. Miller , Dan R. Wilkins

We report on a simultaneous NuSTAR and Swift observation of the neutron star low-mass X-ray binary 4U 1728-34. We identified and removed four Type I X-ray bursts during the observation in order to study the persistent emission. The…

Studying the reflection of X-rays off the inner edge of the accretion disk in a neutron star low-mass X-ray binary, allows us to investigate the accretion geometry and to constrain the radius of the neutron star. We report on a NuSTAR…

High Energy Astrophysical Phenomena · Physics 2016-02-10 N. Degenaar , J. M. Miller , D. Chakrabarty , F. Harrison , E. Kara , A. C. Fabian

We present a spectral analysis of NuSTAR and NICER observations of the luminous, persistently accreting neutron star (NS) low-mass X-ray binary Cygnus X-2. The data were divided into different branches that the source traces out on the…

High Energy Astrophysical Phenomena · Physics 2022-03-14 R. M. Ludlam , E. M. Cackett , J. A. García , J. M. Miller , A. L. Stevens , A. C. Fabian , J. Homan , M. NG , S. Guillot , D. J. K. Buisson , D. Chakrabarty

We report the discovery of a broad emission feature at ~0.7 keV in the spectra of the ultra-compact X-ray binary 4U 1543-624, obtained with the high-resolution spectrographs of the XMM-Newton and Chandra satellites. We confirm the presence…

High Energy Astrophysical Phenomena · Physics 2015-05-20 O. K. Madej , P. G. Jonker

We report on observations of the neutron star (NS) residing in the low-mass X-ray binary 1RXS J180408.9-34205 taken 2015 March by $\emph{NuSTAR}$ and $\emph{XMM-Newton}$ while the source was in the hard spectral state. We find multiple…

High Energy Astrophysical Phenomena · Physics 2016-06-15 R. M. Ludlam , J. M. Miller , E. M. Cackett , A. C. Fabian , M. Bachetti , M. L. Parker , J. A. Tomsick , D. Barret , L. Natalucci , V. Rana , F. A. Harrison

Spitzer observations of the neutron star (ultra-compact) X-ray binary (XRB) 4U 0614+091 with the Infrared Array Camera reveal emission of non-thermal origin in the range 3.5-8 um. The mid-infrared spectrum is well fit by a power law with…

We present two simultaneous NICER and NuSTAR observations of the ultra-compact X-ray binary (UCXB) candidate SLX 1735-269 while the source was in two different spectral states. Using various reflection modeling techniques, we find that…

4U 1820-30 is a ultracompact X-ray binary located in the globular cluster NGC 6624, consisting of a neutron star accreting material from a helium white dwarf companion characterized by the shortest known orbital period for this type of star…

High Energy Astrophysical Phenomena · Physics 2025-04-04 A. Anitra , A. Gnarini , T. Di Salvo , R. Iaria , A. Sanna , L. Burderi , A. Marino , M. Del Santo , G. Matt , F. Ursini , S. Bianchi , F. Capitanio , S. Fabiani , A. Tarana , A. Di Marco

We present spectroscopic X-ray data of two candidate ultra-compact X-ray binaries: 4U~0614+091 and 4U~1543$-$624. We confirm the presence of a broad O VIII Ly$\alpha$ reflection line (at $\approx18\ \AA$) using {\it XMM-Newton} and {\it…

High Energy Astrophysical Phenomena · Physics 2015-06-19 O. K. Madej , J. Garcia , P. G. Jonker , M. L. Parker , R. Ross , A. C. Fabian , J. Chenevez

We present $\emph{NuSTAR}$ observations of neutron star (NS) low-mass X-ray binaries: 4U 1636-53, GX 17+2, and 4U 1705-44. We observed 4U 1636-53 in the hard state, with an Eddington fraction, $F_{\mathrm{Edd}}$, of 0.01; GX 17+2 and 4U…

High Energy Astrophysical Phenomena · Physics 2017-02-22 R. M. Ludlam , J. M. Miller , M. Bachetti , D. Barret , A. C. Bostrom , E. M. Cackett , N. Degenaar , T. Di Salvo , L. Natalucci , J. A. Tomsick , F. Paerels , M. L. Parker

We present a broadband spectral analysis of the atoll source 4U~1636-536 observed for $\sim92$ ks with \nustar{}. The source was found to be in a low-luminosity state during this observation with $3-79 \kev{}$ X-ray luminosity of $L_{3-79…

High Energy Astrophysical Phenomena · Physics 2021-04-21 Aditya S. Mondal , B. Raychaudhuri , G. C. Dewangan

We present 3-79 keV NuSTAR observations of the neutron star low-mass X-ray binary 4U 1636-53 in the soft, transitional and hard state. The spectra display a broad emission line at 5-10 keV. We applied several models to fit this line: A…

High Energy Astrophysical Phenomena · Physics 2017-03-17 Yanan Wang , Mariano Mendez , Andrea Sanna , Diego Altamirano , T. M. Belloni

We report on the results of NuSTAR and XMM-Newton observations of the persistent X-ray source 1E1743.1-2843, located in the Galactic Center region. The source was observed between September and October 2012 by NuSTAR and XMM-Newton,…

We analysed a dedicated NuSTAR observation of the neutron-star low-mass X-ray binary Z-source GX 13+1 to study the timing and spectral properties of the source. From the colour-colour diagram, we conclude that during that observation the…

We report on an observation of the neutron star low-mass X-ray binary Serpens X-1, made with NuSTAR. The extraordinary sensitivity afforded by NuSTAR facilitated the detection of a clear, robust, relativistic Fe K emission line from the…

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…

High Energy Astrophysical Phenomena · Physics 2017-04-05 R. M. Ludlam , J. M. Miller , E. C. Cackett , N. Degenaar , A. C. Bostrom
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