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Anna L Watts

Has grant

University of Amsterdam

Netherlands

Research Interests

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Professors in Netherlands

Recent Grants

Grant: Open

Probing the phase diagram of quantum chromodynamics

Open Date: 2022-11-01

Close Date: 2027-10-31

Grant: Close

Advancing the Equation of state of Neutron Stars

Open Date: 2020-06-01

Close Date: 2025-05-31

Grant: Close

The physics and forensics of neutron star explosions

Open Date: 2015-06-01

Close Date: 2020-05-31

Articles (16)

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2026

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2022

Collaborators (7)

Valery Suleimanov

GERMANY

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Oliver Porth

Associate Prof

University of Amsterdam

NETHERLANDS

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Vladislav Loktev

University of Turku

FINLAND

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David Ballantyne

Associate Professor

Georgia Institute of Technology

UNITED STATES

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John Rankin

University of Ferrara

ITALY

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Juri Poutanen

professor of astronomy, director

Turun Yliopisto

FINLAND

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Jörn Wilms

Professor

Friedrich-Alexander Universität Erlangen-Nürnberg

GERMANY

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Anna L Watts

Research Interests

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Recent Grants

Articles (16)

Pulse profile modelling of the accretion-powered millisecond pulsar SAX J1808.4−3658 using NICER data from its 2019 and 2022 outbursts

Astrophysics Equation of State Inference with Bayesian Chiral Effective Field Theory Uncertainties

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2−604207

A NICER View of PSR J0030+0451: Updated Constraints from 6 yr of NICER Observations

Equation-of-state-informed pulse profile modeling

Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes

Parameter constraints for accreting millisecond pulsars with synthetic NICER data

Impact of accretion assumptions on pulse profile modelling of superburst oscillations in 4U 1636−536

Neutron stars and the dense matter equation of state

Cross-comparison of sampling algorithms for pulse profile modeling of PSR J0740+6620

Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

Probing fermionic asymmetric dark matter cores using global neutron star properties

Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate

NEoST: A Python package for nested sampling of the neutron star equation of state

Constraining a relativistic mean field model using neutron star mass–radius measurements II: hyperonic models

GRMHD simulations of accreting neutron stars with non-dipole fields

Collaborators (7)

Valery Suleimanov

Oliver Porth

Vladislav Loktev

David Ballantyne

John Rankin

Juri Poutanen

Jörn Wilms

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