activity
20142017
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 1.6k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE201776 cited

A Hard Look at the Neutron Stars and Accretion Disks in 4U 1636-53, GX 17+2, and 4U 1705-44 with

R. M. Ludlam, J. M. Miller, M. Bachetti +9

We present observations of neutron star (NS) low-mass X-ray binaries: 4U 1636-53, GX 17+2, and 4U 1705-44. We observed 4U 1636-53 in the hard state, with an Eddingt…

astro-ph.HE201681 cited

Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-Orbital Phase

F. Fuerst, D. J. Walton, D. Stern +5

We present broad-band, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best des…

astro-ph.HE201620 cited

Detection of Very Low-Frequency Quasi-Periodic Oscillations in the 2015 Outburst of V404 Cygni

D. Huppenkothen, G. Younes, A. Ingram +12

In June 2015, the black hole X-ray binary (BHXRB) V404 Cygni went into outburst for the first time since 1989. Here, we present a comprehensive search for quasi-periodic oscillatio…

astro-ph.HE2016

Observations of Supernova Remnants with the Sardinia Radio Telescope

E. Egron, A. Pellizzoni, S. Loru +11

In the frame of the Astronomical Validation activities for the 64m Sardinia Radio Telescope, we performed 5-22 GHz imaging observations of the complex-morphology supernova remnants…

astro-ph.HE2016

Modelling high-resolution spatially-resolved Supernova Remnant spectra with the Sardinia Radio Telescope

Sara Loru, Alberto Pellizzoni, Elise Egron +12

Supernova Remnants (SNRs) exhibit spectra featured by synchrotron radio emission arising from the relativistic electrons, and high-energy emission from both leptonic (Bremsstrahlun…

astro-ph.HE201698 cited

Magnetar-like activity from the central compact object in the SNR RCW103

Nanda Rea, Alice Borghese, Paolo Esposito +4

The 6.67 hr periodicity and the variable X-ray flux of the central compact object (CCO) at the center of the SNR RCW 103, named 1E 161348-5055, have been always difficult to interp…