activity
20072017
most citedThe long-term evolution of the spin, pulse shape, and orbit of the accretion-powered millisecond pulsar SAX J1808.4-3658

200 citations · 392 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2017★ 87 cited

The Radio Sky at Meter Wavelengths: m-Mode Analysis Imaging with the Owens Valley Long Wavelength Array

Michael W. Eastwood, Marin M. Anderson, Ryan M. Monroe +17

A host of new low-frequency radio telescopes seek to measure the 21-cm transition of neutral hydrogen from the early universe. These telescopes have the potential to directly probe…

astro-ph.HE2009★ 90 cited

A decade of timing an accretion-powered millisecond pulsar: The continuing spin down and orbital evolution of SAX J1808.4-3658

J. M. Hartman, A. Patruno, D. Chakrabarty +4

The Rossi X-ray Timing Explorer has observed five outbursts from the transient 2.5 ms accretion-powered pulsar SAX J1808.4-3658 during 1998-2008. We present a pulse timing study of…

astro-ph2008★ 15 cited

The Luminosity and Energy Dependence of Pulse Phase Lags in the Accretion-powered Millisecond Pulsar SAX J1808.4-3658

Jacob M. Hartman, Anna L. Watts, Deepto Chakrabarty

Soft phase lags, in which X-ray pulses in lower energy bands arrive later than pulses in higher energy bands, have been observed in nearly all accretion-powered millisecond pulsars…

astro-ph2007★ 200 cited

The long-term evolution of the spin, pulse shape, and orbit of the accretion-powered millisecond pulsar SAX J1808.4-3658

Jacob M. Hartman, Alessandro Patruno, Deepto Chakrabarty +6

We present a 7 yr timing study of the 2.5 ms X-ray pulsar SAX J1808.4-3658, an X-ray transient with a recurrence time of ~2 yr, using data from the Rossi X-ray Timing Explorer cove…