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After spending almost a decade in a radio-quiet state, the Anomalous X-ray Pulsar XTE J1810-197 turned back on in early December 2018. We have observed this radio magnetar at 1.5 GHz with ~daily cadence since the first detection of radio…

高能天体物理现象 · 物理学 2019-08-07 L. Levin , A. G. Lyne , G. Desvignes , R. P. Eatough , R. Karuppusamy , M. Kramer , M. Mickaliger , B. W. Stappers , P. Weltevrede

In addition to being the most magnetic objects in the known universe, magnetars are the only objects observed to generate fast-radio-burst-like emissions. The formation mechanism of magnetars is still highly debated, and may potentially be…

高能天体物理现象 · 物理学 2024-06-10 Hao Ding , Marcus E. Lower , Adam T. Deller , Ryan M. Shannon , Fernando Camilo , John Sarkissian

We study the timing and spectral properties of the low-magnetic field, transient magnetar SWIFT J1822.3-1606 as it approached quiescence. We coherently phase-connect the observations over a time-span of ~500 days since the discovery of…

We analyze the slow periodicities identified in burst sequences from FRB 121102 and FRB 180916 with periods of about 16 and 160 d, respectively, while also addressing the absence of any fast periodicity that might be associated with the…

高能天体物理现象 · 物理学 2022-04-21 J. M. Cordes , I. Wasserman , Shami Chatterjee , Gauri Batra

We have analyzed XMM-Newton and Chandra observations of the transient magnetar XTE J1810-197, spanning more than 11 years, from the initial phases of the 2003 outburst to the current quiescent level. We investigated the evolution of the…

高能天体物理现象 · 物理学 2016-04-20 F. Pintore , F. Bernardini , S. Mereghetti , P. Esposito , R. Turolla , N. Rea , F. Coti Zelati , G. L. Israel , A. Tiengo , S. Zane

Providing a link between magnetars and radio pulsars, high magnetic field neutron stars are ideal targets to investigate how bursting/magnetospheric activity and braking torque variations are connected to rotational glitches. The last…

高能天体物理现象 · 物理学 2015-06-23 D. Antonopoulou , P. Weltevrede , C. M. Espinoza , A. L. Watts , S. Johnston , R. M. Shannon , M. Kerr

We demonstrate that the high-magnetic field pulsar J1119-6127 exhibits three different types of behaviour in the radio band. Trailing the "normal" profile peak there is an "intermittent" peak and these components are flanked by two…

太阳与恒星天体物理 · 物理学 2015-05-20 Patrick Weltevrede , Simon Johnston , Cristobal M. Espinoza

The magnetar Swift J1834.9-0846 presents a significant challenge to neutron star spin-down models. It exhibits two key anomalies: an insufficient rotational energy loss rate to power its observed X-ray luminosity, and a braking index of $ =…

高能天体物理现象 · 物理学 2026-02-09 Biaopeng Li , Zhifu Gao , Wenqi Ma , Weifeng Zhang , Quan Cheng , L. C. Garcia de Andrade

We report the radio and high-energy properties of a new outburst from the radio-loud magnetar 1E 1547.0$-$5408. Following the detection of a short burst from the source with Swift-BAT on 2022 April 7, observations by NICER detected an…

After 15 years, in late 2018, the magnetar XTE J1810-197 underwent a second recorded X-ray outburst event and reactivated as a radio pulsar. We initiated an X-ray monitoring campaign to follow the timing and spectral evolution of the…

4U 0142+61 is one of a small class of persistently bright magnetars. Here we report on a monitoring campaign of 4U 0142+61 from 2011 July 26 - 2016 June 12 using the Swift X-ray Telescope, continuing a 16 year timing campaign with the Rossi…

高能天体物理现象 · 物理学 2017-01-18 R. F. Archibald , V. M. Kaspi , P. Scholz , A. P. Beardmore , N. Gehrels , J. A. Kennea

Boasting supreme magnetic strengths, magnetars are among the prime candidates to generate fast radio bursts. Several theories have been proposed for the formation mechanism of magnetars, but have not yet been fully tested. As different…

高能天体物理现象 · 物理学 2023-03-07 Hao Ding , Adam Deller , Marcus Lower , Ryan Shannon

The magnetar Swift J1822.3$-$1606 entered an outburst phase in 2011 July. Previous X-ray studies of its post-outburst rotational evolution yielded inconsistent measurements of the spin-inferred magnetic field. Here we present the timing…

高能天体物理现象 · 物理学 2015-06-18 P. Scholz , V. M. Kaspi , A. Cumming

XTE J1810-197 (PSR J1809-1943) was the first ever magnetar which was found to emit transient radio emission. It has recently undergone another radio and high-energy outburst. This is only the second radio outburst that has been observed…

高能天体物理现象 · 物理学 2019-09-10 Yogesh Maan , Bhal Chandra Joshi , Mayuresh P. Surnis , Manjari Bagchi , P. K. Manoharan

We report on the multi-frequency multi-epoch radio observations of the magnetar, XTE J1810-197, which exhibited a radio outburst from December 2018 after its 10-year quiescent period. We performed quasi-simultaneous observations with VERA…

Magnetars are slowly rotating, highly magnetized young neutron stars that can show transient radio phenomena for radio pulses and fast radio bursts. We conducted radio observations of from two magnetars SGR$~$J1935+2154 and…

高能天体物理现象 · 物理学 2025-02-03 Lang Xie , J. L. Han , Z. L. Yang , W. C. Jing , D. J. Zhou , W. Q. Su , Yi Yan , Tao Wang , N. N. Cai , P. F. Wang , Chen Wang

We present the X-ray timing and spectral evolution of the Galactic Center magnetar SGR J1745-2900 for the first ~4 months post-discovery using data obtained with the Nuclear Spectroscopic Telescope Array (NuSTAR)} and Swift observatories.…

We report on the aftermath of a magnetar outburst from the young, high-magnetic-field radio pulsar PSR J1119-6127 that occurred on 2016 July 27. We present the results of a monitoring campaign using the Neil Gehrels Swift X-ray Telescope,…

高能天体物理现象 · 物理学 2019-01-09 R. F. Archibald , V. M. Kaspi , S. P. Tendulkar , P. Scholz

Swift J1858.6-0814 is a transient neutron star X-ray binary discovered in October 2018. Multi-wavelength follow-up observations across the electromagnetic spectrum revealed many interesting properties, such as erratic flaring on minute…

XTE J1810-197 (J1810) was the first magnetar identified to emit radio pulses, and has been extensively studied during a radio-bright phase in 2003$-$2008. It is estimated to be relatively nearby compared to other Galactic magnetars, and…

天体物理仪器与方法 · 物理学 2020-09-02 H. Ding , A. T. Deller , M. E. Lower , C. Flynn , S. Chatterjee , W. Brisken , N. Hurley-Walker , F. Camilo , J. Sarkissian , V. Gupta