110 citations · 271 across the 6 of their papers we have counts for
6 papers
Erratum: "Determining neutron star masses and radii using energy-resolved waveforms of X-ray burst oscillations" (ApJ, 776, 19 [2013])
Ka Ho Lo, M. Coleman Miller, Sudip Bhattacharyya +1
This erratum addresses an error in the text of Lo et al. (2013) and more importantly corrects a computational error that was made in all previously published relativistic computati…
Determining neutron star masses and radii using energy-resolved waveforms of X-ray burst oscillations
Ka-Ho Lo, M. Coleman Miller, Sudip Bhattacharyya +1
Simultaneous, precise measurements of the mass and radius of neutron stars can yield uniquely valuable information about the still uncertain properties of cold matter at se…
Testing the rotating hot spot model using X-ray burst oscillations from 4U 1636-536
Romain Artigue, Didier Barret, Frederick K. Lamb +2
Precise and accurate measurements of neutron star masses and radii would provide valuable information about the still uncertain properties of cold matter at supranuclear densities.…
Implications of high-precision spectra of thermonuclear X-ray bursts for determining neutron star masses and radii
M. Coleman Miller, Stratos Boutloukos, Ka Ho Lo +1
X-ray burst spectra have long been used to estimate neutron star masses and radii. These estimates assumed that burst spectra are accurately described by the model atmosphere spect…
Origin of intermittent accretion-powered X-ray oscillations in neutron stars with millisecond spin periods
Frederick K. Lamb, Stratos Boutloukos, Sandor Van Wassenhove +3
We have shown previously that many of the properties of persistent accretion-powered millisecond pulsars can be understood if their X-ray emitting areas are near their spin axes an…
A model for the waveform behavior of accreting millisecond pulsars: Nearly aligned magnetic fields and moving emission regions
Frederick K. Lamb, Stratos Boutloukos, Sandor Van Wassenhove +5
We investigate further a model of the accreting millisecond X-ray pulsars we proposed earlier. In this model, the X-ray-emitting regions of these pulsars are near their spin axes b…