UB Paderborn / Katalog / Suche / in CDI

Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 2019-10, Vol.942, p.162389, Article 162389

2019

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Repetitive patterns in rapid optical variations in the nearby black-hole binary V404 Cygni

Nature (London), 2016-01, Vol.529 (7584), p.54-58

2016

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The long-term enhanced brightness of the magnetar 1E 1547.0–5408

Astronomy and astrophysics (Berlin), 2020-01, Vol.633, p.A31

2020

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Discovery and Long-term Broadband X-Ray Monitoring of Galactic Black Hole Candidate MAXI J1803–298

The Astrophysical journal, 2022-03, Vol.927 (2), p.151

2022

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Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data

The Astrophysical journal, 2024-02, Vol.961 (2), p.189

2024

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A NICER View on the 2020 Magnetar-like Outburst of PSR J1846−0258

The Astrophysical journal, 2023-08, Vol.952 (2), p.120

2023

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Pulse Peak Migration during the Outburst Decay of the Magnetar SGR 1830-0645: Crustal Motion and Magnetospheric Untwisting

Astrophysical journal. Letters, 2022-01, Vol.924 (2), p.L27

2022

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The 2022 High-energy Outburst and Radio Disappearing Act of the Magnetar 1E 1547.0–5408

The Astrophysical journal, 2023-03, Vol.945 (2), p.153

2023

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Constraints on pulsed emission model for repeating FRB 121102

Publications of the Astronomical Society of Japan, 2017-12, Vol.69 (6)

2017

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The RS CVn Type star GT Mus Shows Most Energetic X-ray Flares Throughout the 2010s

The Astrophysical journal, 2021-03, Vol.910 (1), p.25

2021

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A NuSTAR confirmation of the 36 ks hard X-ray pulse-phase modulation in the magnetar 1E 1547.0 − 5408

An Empirical Background Model for the NICER X-Ray Timing Instrument

Further Evidence for the ∼9 s Pulsation in LS 5039 from NuSTAR and ASCA

X-Ray Spectral Variations of Circinus X-1 Observed with NICER throughout an Entire Orbital Cycle

Possible Periodic Dips in the Pulsating Ultraluminous X-Ray Source M51 ULX-7

Relativistic fireball reprise: radio suppression at the onset of short magnetar bursts

MASTER OT J030227.28+191754.5: A Dwarf Nova at a Massive Oxygen–Neon White Dwarf System?

Monitoring the Superorbital Period Variation and Spin Period Evolution of SMC X-1

Broadband High-energy Emission of the Gamma-Ray Binary System LS 5039: Spectral and Temporal Features Using NuSTAR and Fermi Observations

NICER View of the 2020 Burst Storm and Persistent Emission of SGR 1935+2154

Decomposing the Spectrum of Ultraluminous X-Ray Pulsar NGC 300 ULX-1

Unveiling Properties of the Nonthermal X-Ray Production in the Gamma-Ray Binary LS 5039 Using the Long-term Pattern of Its Fast X-Ray Variability

Return of the Big Glitcher: NICER Timing and Glitches of PSR J0537-6910

NICER Observation of the Temporal and Spectral Evolution of Swift J1818.0−1607: A Missing Link between Magnetars and Rotation-powered Pulsars

Anisotropic neutrino effect on magnetar spin: constraint on inner toroidal field

A convolutional neural network approach for reconstructing polarization information of photoelectric X-ray polarimeters

Repetitive patterns in rapid optical variations in the nearby black-hole binary V404 Cygni

The long-term enhanced brightness of the magnetar 1E 1547.0–5408

Discovery and Long-term Broadband X-Ray Monitoring of Galactic Black Hole Candidate MAXI J1803–298

Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data

A NICER View on the 2020 Magnetar-like Outburst of PSR J1846−0258

Pulse Peak Migration during the Outburst Decay of the Magnetar SGR 1830-0645: Crustal Motion and Magnetospheric Untwisting

The 2022 High-energy Outburst and Radio Disappearing Act of the Magnetar 1E 1547.0–5408

Constraints on pulsed emission model for repeating FRB 121102

The RS CVn Type star GT Mus Shows Most Energetic X-ray Flares Throughout the 2010s

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