activity
20182022
most citedX-ray Spectroscopy of the gamma-ray Brightest Nova V906 Car (ASASSN-18fv)

27 citations · 52 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph.HE202211 cited

4FGL J1120.0-2204: A Unique Gamma-ray Bright Neutron Star Binary with an Extremely Low Mass Proto-White Dwarf

Samuel J. Swihart, Jay Strader, Elias Aydi +5

We have discovered a new X-ray emitting compact binary that is the likely counterpart to the unassociated Fermi-LAT GeV -ray source 4FGL J1120.0-2204, the second brightest Fermi…

astro-ph.HE2021

Timing observations of three Galactic millisecond pulsars

D. R. Lorimer, A. M. Kawash, P. C. C. Freire +16

We report observed and derived timing parameters for three millisecond pulsars (MSPs) from observations collected with the Parkes 64-m telescope, Murriyang. The pulsars were found…

astro-ph.HE202114 cited

Multiwavelength evidence for a new flare-mode transitional millisecond pulsar

Jay Strader, Samuel J. Swihart, Ryan Urquhart +7

We report the discovery of a new low-mass X-ray binary near the center of the unassociated Fermi GeV gamma-ray source 4FGL J0540.0-7552. The source shows the persistent presence of…

astro-ph.HE2020

Early spectral evolution of classical novae: consistent evidence for multiple distinct outflows

E. Aydi, L. Chomiuk, L. Izzo +18

The physical mechanism driving mass ejection during a nova eruption is still poorly understood. Possibilities include ejection in a single ballistic event, a common envelope intera…

astro-ph.HE2020

A New Candidate Transitional Millisecond Pulsar in the Sub-luminous Disk State: 4FGL J0407.7--5702

Jessie M. Miller, Samuel J. Swihart, Jay Strader +7

We report the discovery of a variable optical and X-ray source within the error ellipse of the previously unassociated Fermi Large Area Telescope -ray source 4FGL J0407.7--5702.…

astro-ph.HE202027 cited

X-ray Spectroscopy of the gamma-ray Brightest Nova V906 Car (ASASSN-18fv)

Kirill V. Sokolovsky, Koji Mukai, Laura Chomiuk +15

Shocks in gamma-ray emitting classical novae are expected to produce bright thermal and non-thermal X-rays. We test this prediction with simultaneous NuSTAR and Fermi/LAT observati…