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F. Fuerst

California Institute of Technology

61

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Long-term pulse period evolution of the ultra-luminous X-ray pulsar NGC 7793 P13.

2021 arXiv: High Energy Astrophysical Phenomena
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Quasi-periodic dipping in the ultraluminous X-ray source, NGC 247 ULX-1.

2021 arXiv: High Energy Astrophysical Phenomena
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Brightening of MAXI J0903-531 Seen with Fermi GBM and Swift BAT, and a Candidate Orbital Period

2021 The astronomer's telegram
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XMM-Newton campaign on the ultraluminous X-ray source NGC 247 ULX-1: outflows.

2021 arXiv: High Energy Astrophysical Phenomena
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Long-term pulse period evolution of the ultra-luminous X-ray pulsar NGC 7793 P13

2021 Astronomy and Astrophysics
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Swift monitoring of M51: A 38-day super-orbital period from the ULX7 pulsar and a new transient ULX

2020
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NICER and NuSTAR observations of the Be/X-ray binary pulsar 1A 0535+262 during the 2020 November giant outburst

2020 The astronomer's telegram
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Probing the Black Hole Engine with Measurements of the Relativistic X-ray Reflection Component

2019 arXiv: High Energy Astrophysical Phenomena
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Erratum for the Report “A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni”

2018
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Lense-Thirring precession in ULXs as a possible means to constrain the neutron star equation-of-state.

2018 Monthly Notices of the Royal Astronomical Society
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Citations (36)