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Related papers: NICER Magnetar Burst Catalog

200 papers

Soft gamma repeaters and anomalous X-ray pulsars are thought to be magnetars, neutron stars with strong magnetic fields of order $\mathord{\sim} 10^{13}$--$10^{15} \, \mathrm{gauss}$. These objects emit intermittent bursts of hard X-rays…

Instrumentation and Methods for Astrophysics · Physics 2017-08-02 Ryan Quitzow-James , James Brau , James Clark , Michael W. Coughlin , Scott B. Coughlin , Raymond Frey , Paul Schale , Dipongkar Talukder , Eric Thrane

We present here a detailed spectral study of the X-ray emission of the persistent source and the low-fluence bursts of SGR J0501+4516 observed during a deep XMM-Newton observation near the peak of its 2008 outburst. For the persistent…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Lin Lin , Ersin Gogus , Tolga Guver , Chryssa Kouveliotou

During 2020 April and May, SGR J1935+2154 emitted hundreds of short bursts and became one of the most prolific transient magnetars. At the onset of the active bursting period, a 130 s burst "forest," which included some bursts with peculiar…

We present a long-term study of the 2011 outburst of the magnetar Swift J1834.9-0846 carried out using new Chandra observations, as well as all the available Swift, RXTE, and XMM-Newton data. The last observation was performed on 2011…

High Energy Astrophysical Phenomena · Physics 2013-02-14 P. Esposito , A. Tiengo , N. Rea , R. Turolla , A. Fenzi , A. Giuliani , G. L. Israel , S. Zane , S. Mereghetti , A. Possenti , M. Burgay , L. Stella , D. Götz , R. Perna , R. P. Mignani , P. Romano

This paper describes an analysis of the NuSTAR data of the fastest-rotating magnetar 1E 1547$-$5408, acquired in 2016 April for a time lapse of 151 ks. The source was detected with a 1-60 keV flux of $1.7 \times 10^{-11}$ ergs s$^{-1}$…

High Energy Astrophysical Phenomena · Physics 2021-02-17 Kazuo Makishima , Teruaki Enoto , Hiroki Yoneda , Hirokazu Odaka

Highly magnetized neutron stars are a source of extreme transients observed in different bands, like the fast radio burst (FRB) and associated hard X-ray burst from the Galactic magnetar SGR 1935+2154. The origin of such outbursts, hard…

High Energy Astrophysical Phenomena · Physics 2024-05-07 J. F. Mahlmann

We present the results obtained from the spectral and temporal study of thermonuclear bursts from the millisecond X-ray pulsar SRGA J144459.2-604207 detected with NICER. The dynamic evolution of the spectral parameters in a broad energy…

High Energy Astrophysical Phenomena · Physics 2025-07-23 Manoj Mandal , Sachindra Naik , Birendra Chhotaray

We report nine long X-ray bursts from neutron stars, detected with Monitor of All-sky X-ray Image (MAXI). Some of these bursts lasted for hours, and hence are qualified as superbursts, which are prolonged thermonuclear flashes on neutron…

High Energy Astrophysical Phenomena · Physics 2016-09-28 Motoko Serino , Wataru Iwakiri , Toru Tamagawa , Takanori Sakamoto , Satoshi Nakahira , Masaru Matsuoka , Kazutaka Yamaoka , Hitoshi Negoro

To identify extragalactic magnetar flares, we have searched for their periodic tails by generating Lomb periodograms of the emission following short bursts detected by the Burst and Transient Source Experiment (BATSE). Out of 358 short…

Astrophysics · Physics 2009-11-11 A. Crider

Long-lived massive magnetars are expected to be remnants of some binary neutron star (BNS) mergers. In this paper, we argue that the magnetic powered flaring activities of these merged magnetars would occur dominantly in their early…

High Energy Astrophysical Phenomena · Physics 2023-08-14 Shu-Xu Yi , Zhen Zhang , Xilu Wang

The Neutron Star Interior Composition Explorer (NICER) has observed seven thermonuclear X-ray bursts from the Low Mass X-ray Binary (LMXB) neutron star 4U 1728-34 from the start of the mission's operations until February of 2019. Three of…

The source GS~1826-24 is a neutron star low mass X-ray binary known as the 'clocked burster' because of its extremely regular bursting behavior. We report on the detection of a long type-I X-ray burst from this source. We perform a detailed…

High Energy Astrophysical Phenomena · Physics 2025-08-21 Aditya S. Mondal , Mayukh Pahari , Gulab C. Dewangan

Spectral lag of the low-energy photons with respect to the high-energy ones is a common astrophysical phenomenon (such as Gamma-ray bursts and the Crab pulsar) and may serve as a key probe to the underlying radiation mechanism. However,…

Burst oscillations during thermonuclear X-ray bursts are powered by thermonuclear energy on the neutron star (NS) surface and typically occur close to the spin frequency of the NS. We performed a comprehensive timing analysis of all…

High Energy Astrophysical Phenomena · Physics 2026-03-16 Manoj Mandal , Sachindra Naik

Giant flares, short explosive events releasing up to 10$^{47}$ erg of energy in the gamma-ray band in less than one second, are the most spectacular manifestation of magnetars, young neutron stars powered by a very strong magnetic field,…

The INTEGRAL satellite has collected a large amount of data on magnetars in our Galaxy, spanning more than 20 years starting from 2003. The large data set obtained with the IBIS/ISGRI instrument at energies above 20 keV allows us to study…

High Energy Astrophysical Phenomena · Physics 2024-11-01 Dominik P. Pacholski , Lorenzo Ducci , Martin Topinka , Sandro Mereghetti

We present the semi-analytical light curve modelling of 13 supernovae associated with gamma-ray bursts (GRB-SNe) along with two relativistic broad-lined (Ic-BL) SNe without GRBs association (SNe 2009bb and 2012ap), considering millisecond…

Fast radio bursts (FRB) are enigmatic powerful single radio pulses with durations of several milliseconds and high brightness temperatures suggesting coherent emission mechanism. For the time being a number of extragalactic FRBs have been…

High Energy Astrophysical Phenomena · Physics 2021-08-23 D. Kostunin , H. Ashkar , F. Schüssler , G. Rowell

We present the detection of 51 thermonuclear X-ray bursts observed from 4U 1636-536 by the Neutron Star Interior Composition Explorer (NICER) over the course of a three year monitoring campaign. We performed time resolved spectroscopy for…

We report on the long term X-ray monitoring with Swift, RXTE, Suzaku, Chandra, and XMM-Newton of the outburst of the newly discovered magnetar Swift J1822.3-1606 (SGR 182-1606), from the first observations soon after the detection of the…