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相关论文: Evolution of MAXI J1631-479 during the January 201…

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In this paper we report on the observations performed with INTEGRAL and Swift of the first outburst detected from the hard X-ray transient MAXI J1828-249. During the first about two days of the outburst, the source was observed by MAXI to…

高能天体物理现象 · 物理学 2015-06-19 E. Filippova , E. Bozzo , C. Ferrigno

The X-ray transient MAXI J1631-479 went into outburst on 2018 December 21 and remained active for about seven months. Owing to various constraints it was monitored by NICER only during the decay phase of the outburst for about four months.…

高能天体物理现象 · 物理学 2021-05-19 Sandeep K. Rout , Mariano Méndez , Tomaso M. Belloni , Santosh Vadawale

MAXI J1813-095 is an X-ray transient discovered during an outburst in 2018. We report on X-ray and optical observations obtained during this event, which indicate that the source is a new low-mass X-ray binary. The outburst lasted ~70 d and…

We report the energy-resolved broadband timing analysis of the black hole X-ray transient MAXI J1631-479 during its 2019 outburst from February 11 to April 9, using data from the Insight-Hard X-ray Modulation Telescope (Insight-HXMT), which…

We report the results from the broad-band X-ray monitoring of the new Galactic black hole candidate MAXI J1803$-$298 with the MAXI/GSC and Swift/BAT during its outburst. After the discovery on 2021 May 1, the soft X-ray flux below 10 keV…

We report X-ray, optical, and near-infrared monitoring of the new X-ray transient MAXI J1820$+$070 discovered with MAXI on 2018 March 11. Its X-ray intensity reached $\sim 2$ Crab in 2--20 keV at the end of March, and then gradually…

MAXI J1834-021 is a new X-ray transient that was discovered in February 2023. We analysed the spectral and timing properties of MAXI J1834-021 using NICER, NuStar and Swift data collected between March and October 2023. The light curve…

The well known black-hole X-ray binary transient XTE J1550-564 underwent an outburst during the spring of 2003 which was substantially underluminous in comparison to previous periods of peak activity in that source. In addition, our…

天体物理学 · 物理学 2009-11-10 S. J. Sturner , C. R. Shrader

On 2 September 2017 MAXI J1535-571 went into outburst and peaked at ~5 Crab in the 2-20 keV energy range. Early in the flare INTEGRAL performed Target of Opportunity pointings and monitored the source as it transitioned from the hard state…

高能天体物理现象 · 物理学 2023-02-13 James Rodi , E. Jourdain , J. P. Roques

The black hole binary GS 2023+338 exhibited an unprecedently bright outburst on June 2015. Since June 17th, the high energy instruments on board INTEGRAL detected an extremely variable emission during both bright and low luminosity phases,…

We present a detailed X-ray spectral and variability study of the full 2018 outburst of MAXI J1727-203 using NICER observations. The outburst lasted approximately four months. Spectral modelling in the 0.3-10 keV band shows the presence of…

We present a type-I outburst of the high-mass X-ray binary EXO 2030+375, detected during INTEGRAL's Performance and Verification Phase in December 2002 (on-source time about 10e+06 seconds). In addition, six more outbursts have been…

天体物理学 · 物理学 2009-11-11 A. Camero Arranz , C. A. Wilson , P. Connell , S. Martínez Núñez , P. Blay , V. Beckmann , V. Reglero

On March 2003, IBIS, the gamma-ray imager on board the INTEGRAL satellite, detected an outburst from a new source, IGR J17464-3213, that turned out to be a HEAO-1 transient, H1743-322. In this paper we report on the high energy behaviour of…

We present a detailed timing analysis of the bright black hole X-ray binary MAXI J1820+070 (ASASSN-18ey), during its first detected outburst lasting from March 2018 until October 2019 based on Swift/XRT window timing mode observations,…

高能天体物理现象 · 物理学 2020-02-12 H. Stiele , A. K. H. Kong

We study the spectral and temporal properties of the black hole X-ray transient binary MAXI J1820+070 during the 2018 outburst with Insight-HXMT observations. The outburst of MAXI J1820+070 can be divided into three intervals. For the two…

高能天体物理现象 · 物理学 2025-02-21 J. Q. Peng , S. Zhang , Y. P. Chen , L. D. Kong , P. J. Wang , S. N. Zhang , L. Ji , L. Tao , J. L. Qu , M. Y. Ge , Q. C. Shui , J. Li , Z. Chang , Z. S. Li , Y. X. Xiao

We present results from quasi-simultaneous multiwavelength observations of the Galactic black hole X-ray transient MAXI J1820$+$070 during the decay of the 2018 outburst and its entire subsequent mini-outburst in March 2019. We fit the…

高能天体物理现象 · 物理学 2022-07-06 M. Özbey Arabacı , E. Kalemci , T. Dinçer , C. Bailyn , D. Altamirano , T. Ak

We report on the detection and subsequent X-ray monitoring of the new Galactic black hole candidate MAXI J1535-571 with the MAXI/GSC. Afterthe discovery on 2017 September 2 made independently with MAXI and the Swift/BAT, the source…

We studied the transient Galactic black hole candidate MAXI J0637-430 with data from Insight-HXMT, Swift and XMM-Newton. The broad-band X-ray observations from Insight-HXMT help us constrain the power-law component. MAXI J0637-430 is…

高能天体物理现象 · 物理学 2022-06-22 R. C. Ma , R. Soria , L. Tao , W. Zhang , J. L. Qu , S. N. Zhang , L. Zhang , E. L. Qiao , S. J. Zhao , M. Y. Ge , X. B. Li , Y. Huang , L. M. Song , S. Zhang , Q. C. Bu , Y. N. Wang , X. Ma , S. M. Jia

Soft X-ray transients are systems that are detected when they go into an outburst, wherein their X-ray luminosity increases several orders of magnitude. These outbursts are markers of the poorly understood change in the spectral state of…

高能天体物理现象 · 物理学 2022-02-21 Neal Titus Thomas , Shivappa B. Gudennavar , Ranjeev Misra , Bubbly S. G

MAXI J1803-298 is a transient black hole candidate discovered in May of 2021 during an outburst that lasted several months. Multiple X-ray observations reveal recurring "dipping" intervals in several of its light curves, particularly during…

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