Duncan K. Galloway

2000-2003 Massachusetts Institute of Technology, Cambridge, MA, United States 
"Duncan Galloway"
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Levan A, Gompertz BP, Salafia OS, et al. (2023) Heavy element production in a compact object merger observed by JWST. Nature
Galloway DK, in ’t Zand J, Chenevez J, et al. (2020) The Multi-INstrument Burst ARchive (MINBAR) The Astrophysical Journal Supplement Series. 249: 32
Tse K, Galloway DK, Chou Y, et al. (2020) Detection of millihertz quasi-periodic oscillations in the X-Ray binary 1RXS J180408.9−342058 Monthly Notices of the Royal Astronomical Society. 500: 34-39
Cavecchi Y, Galloway DK, Goodwin AJ, et al. (2020) The efficiency of nuclear burning during thermonuclear (Type I) bursts as a function of accretion rate Monthly Notices of the Royal Astronomical Society. 499: 2148-2156
Goodwin AJ, Russell DM, Galloway DK, et al. (2020) Enhanced optical activity 12 d before X-ray activity, and a 4 d X-ray delay during outburst rise, in a low-mass X-ray binary Monthly Notices of the Royal Astronomical Society. 498: 3429-3439
Gompertz BP, Cutter RJ, Steeghs D, et al. (2020) Searching for electromagnetic counterparts to gravitational-wave merger events with the prototype Gravitational-Wave Optical Transient Observer (GOTO-4) Monthly Notices of the Royal Astronomical Society. 497: 726-738
Johnston Z, Heger A, Galloway DK. (2020) Multi-epoch X-ray burst modelling: MCMC with large grids of 1D simulations Monthly Notices of the Royal Astronomical Society. 494: 4576-4589
Kuiper L, Tsygankov SS, Falanga M, et al. (2020) High-energy characteristics of the accretion-powered millisecond pulsar IGR J17591−2342 during its 2018 outburst Astronomy & Astrophysics. 641: A37
Ackley K, Amati L, Barbieri C, et al. (2020) Observational constraints on the optical and near-infrared emission from the neutron star–black hole binary merger candidate S190814bv Astronomy & Astrophysics. 643: A113
Jaisawal GK, Chenevez J, Bult P, et al. (2019) NICER Observes a Secondary Peak in the Decay of a Thermonuclear Burst from 4U 1608–52 The Astrophysical Journal. 883: 61
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