most citedEvolution of the reverberation lag in GX 339-4 at the end of an outburst

64 citations · 169 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE201736 cited

An X-ray survey of the central molecular zone: variability of the Fe Ka emission line

R. Terrier, M. Clavel, S. Soldi +4

There is now abundant evidence that the luminosity of the Galactic super-massive black hole (SMBH) has not always been as low as it is nowadays. The observation of varying non-ther…

astro-ph.HE201727 cited

NuSTAR + XMM-Newton monitoring of the neutron star transient AX J1745.6-2901

G. Ponti, S. Bianchi, T. Munos-Darias +12

AX J1745.6-2901 is a high-inclination (eclipsing) transient neutron star (NS) Low Mass X-ray Binary (LMXB) showcasing intense ionised Fe K absorption. We present here the analysis…

astro-ph.HE201764 cited

Evolution of the reverberation lag in GX 339-4 at the end of an outburst

B. De Marco, G. Ponti, P. O. Petrucci +13

We studied X-ray reverberation lags in the BHXRB GX 339-4 at the end of the 2014-2015 outburst. We analysed data from a XMM-Newton campaign covering the end of the transition from…

astro-ph.HE201712 cited

Galactic Sources Detected in the NuSTAR Serendipitous Survey

John A. Tomsick, George B. Lansbury, Farid Rahoui +13

The Nuclear Spectroscopic Telescope Array (NuSTAR) provides an improvement in sensitivity at energies above 10 keV by two orders of magnitude over non-focusing satellites, making i…

astro-ph.HE201730 cited

Sagittarius A* High Energy X-ray Flare Properties During NuSTAR Monitoring of the Galactic Center from 2012 to 2015

Shuo Zhang, Frederick K. Baganoff, Gabriele Ponti +17

Understanding the origin of the flaring activity from the Galactic center supermassive black hole, Sagittarius A*, is a major scientific goal of the NuSTAR Galactic plane survey ca…

astro-ph.HE2016

Identifying IGR J14091-6108 as a magnetic CV with a massive white dwarf using X-ray and optical observations

John A. Tomsick, Farid Rahoui, Roman Krivonos +3

IGR J14091-6108 is a Galactic X-ray source known to have an iron emission line, a hard X-ray spectrum, and an optical counterpart. Here, we report on X-ray observations of the sour…