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Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra

Astronomy and astrophysics (Berlin), 2017-12, Vol.608, p.A31

2017

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Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method

Astronomy and astrophysics (Berlin), 2016-07, Vol.591, p.A25

2016

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X-ray dips and a complex UV/X-ray cross-correlation function in the black hole candidate MAXI J1820+070

Monthly notices of the Royal Astronomical Society, 2019-09, Vol.488 (1), p.L18-L23

2019

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Swift observations of V404 Cyg during the 2015 outburst: X-ray outflows from super-Eddington accretion

Monthly notices of the Royal Astronomical Society, 2017-10, Vol.471 (2), p.1797-1818

2017

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Observations of a radio-bright, X-ray obscured GRS 1915+105

Monthly notices of the Royal Astronomical Society, 2021-05, Vol.503 (1), p.152-161

2021

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Hard-state Accretion Disk Winds from Black Holes: The Revealing Case of MAXI J1820+070

Astrophysical journal. Letters, 2019-07, Vol.879 (1), p.L4

2019

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The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608−52

Monthly notices of the Royal Astronomical Society, 2014-08, Vol.442 (4), p.3777-3790

2014

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The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

Monthly notices of the Royal Astronomical Society, 2017-04, Vol.466 (1), p.906-913

2017

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Hard X-ray variability of V404 Cygni during the 2015 outburst

Astronomy and astrophysics (Berlin), 2017-06, Vol.602, p.A40

2017

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Basic parameters of the helium-accreting X-ray bursting neutron star in 4U 1820−30

Monthly notices of the Royal Astronomical Society, 2017-12, Vol.472 (4), p.3905-3913

2017

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Spectral variability of ultraluminous X-ray sources

Monthly notices of the Royal Astronomical Society, 2009-09, Vol.398 (3), p.1450-1460

2009

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The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts

Monthly notices of the Royal Astronomical Society, 2014-12, Vol.445 (4), p.4218-4234

2014

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Detection of burning ashes from thermonuclear X-ray bursts

Monthly notices of the Royal Astronomical Society, 2017-01, Vol.464 (1), p.L6-L10

2017

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Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070

Science (American Association for the Advancement of Science), 2022-02, Vol.375 (6583), p.874-876

2022

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Burst-induced coronal cooling in GS 1826–24

Astronomy and astrophysics (Berlin), 2020-02, Vol.634

2020

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Evolution of the spectral curvature in the ultraluminous X-ray source Holmberg II X-1

Monthly notices of the Royal Astronomical Society, 2012-05, Vol.422 (2), p.990-996

2012

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Expanding hot flow in the black hole binary SWIFT J1753.5−0127: evidence from optical timing

Monthly notices of the Royal Astronomical Society, 2017-09, Vol.470 (1), p.48-59

2017

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The 2009 outburst of accreting millisecond pulsar IGR J17511-3057 as observed by Swift and RXTE

Monthly notices of the Royal Astronomical Society, 2011-08, Vol.415 (2), p.1864-1874

2011

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Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5−0127

Monthly notices of the Royal Astronomical Society, 2014-12, Vol.445 (3), p.2424-2439

2014

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Rapid late-time X-ray brightening of the tidal disruption event OGLE16aaa

Astronomy and astrophysics (Berlin), 2020-07, Vol.639, p.A100

2020

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The black hole binary V404 Cygni: a highly accreting obscured AGN analogue

Monthly notices of the Royal Astronomical Society, 2017-06, Vol.468 (1), p.981-993

2017

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Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5−0127

Monthly notices of the Royal Astronomical Society, 2014-12, Vol.445 (3), p.2424-2439

2014

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X-ray burst-induced spectral variability in 4U 1728–34

Astronomy and astrophysics (Berlin), 2017-03, Vol.599, p.A89

2017

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Searching for X-ray sources in nearby late-type galaxies with low-star formation rates

Monthly notices of the Royal Astronomical Society, 2016-03, Vol.456 (3), p.2966-2973

2016

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Varying disc-magnetosphere coupling as the origin of pulse profile variability in SAX J1808.4−3658

Monthly notices of the Royal Astronomical Society, 2011-10, Vol.417 (2), p.1454-1465

2011

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Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra

Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method

X-ray dips and a complex UV/X-ray cross-correlation function in the black hole candidate MAXI J1820+070

Swift observations of V404 Cyg during the 2015 outburst: X-ray outflows from super-Eddington accretion

Observations of a radio-bright, X-ray obscured GRS 1915+105

Hard-state Accretion Disk Winds from Black Holes: The Revealing Case of MAXI J1820+070

The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608−52

The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii

Hard X-ray variability of V404 Cygni during the 2015 outburst

Basic parameters of the helium-accreting X-ray bursting neutron star in 4U 1820−30

Spectral variability of ultraluminous X-ray sources

The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts

Detection of burning ashes from thermonuclear X-ray bursts

Black hole spin-orbit misalignment in the x-ray binary MAXI J1820+070

Burst-induced coronal cooling in GS 1826–24

Evolution of the spectral curvature in the ultraluminous X-ray source Holmberg II X-1

Expanding hot flow in the black hole binary SWIFT J1753.5−0127: evidence from optical timing

The 2009 outburst of accreting millisecond pulsar IGR J17511-3057 as observed by Swift and RXTE

Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5−0127

Rapid late-time X-ray brightening of the tidal disruption event OGLE16aaa

The black hole binary V404 Cygni: a highly accreting obscured AGN analogue

Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5−0127

X-ray burst-induced spectral variability in 4U 1728–34

Searching for X-ray sources in nearby late-type galaxies with low-star formation rates

Varying disc-magnetosphere coupling as the origin of pulse profile variability in SAX J1808.4−3658

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