activity
20072023
most citedThe 4th IBIS/ISGRI soft gamma-ray survey catalog

236 citations · 1.3k across the 39 of their papers we have counts for

collaborators

39 papers

astro-ph.HE2023

4U 1210-64: a new member of the rare intermediate-mass X-ray binary subclass

Itumeleng M. Monageng, Vanessa A. McBride, Julia Alfonso-Garzon +5

4U 1210-64 is a peculiar X-ray binary that was first discovered in 1978 by the Uhuru satellite. The analysis of the X-ray data revealed a 6.7-day orbital period and an additional l…

astro-ph.HE2020★ 81 cited

Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions

Peter Kretschmar, Felix Fürst, Lara Sidoli +48

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology,…

astro-ph.SR2020★ 7 cited

Optical and X-ray study of the peculiar high mass X-ray binary XMMU J010331.7-730144

Itumeleng M. Monageng, Malcolm J. Coe, David A. H. Buckley +6

For a long time XMMU J010331.7-730144 was proposed as a high-mass X-ray binary candidate based on its X-ray properties, however, its optical behaviour was unclear - in particular p…

astro-ph.HE2019★ 3 cited

An X-ray and optical study of the outbursting behaviour of the SMC Be X-ray binary SXP 91.1

Itumeleng Monageng, Malcolm Coe, Jamie Kennea +6

In this paper we report on the optical and X-ray behaviour of the Be X-ray binary, SXP 91.1, during a recent type I outburst. We monitored the outburst using the Neil Gehrels Swift…

astro-ph.HE2019★ 8 cited

The SMC X-ray binary SXP4.78 : a new Type II outburst and the identification and study of the optical counterpart

Itumeleng Monageng, Malcolm Coe, Lee Townsend +6

SXP4.78 was originally discovered in 2000 as a pulsar in the Small Magellanic Cloud (SMC) by the Rossi X-ray Timing Explorer (RXTE) but it was not spatially located at that time. A…

astro-ph.GA2018★ 12 cited

NGC 3105: a young open cluster with low metallicity

J. Alonso-Santiago, A. Marco, I. Negueruela +4

NGC 3105 is a young open cluster hosting blue, yellow and red supergiants. This rare combination makes it an excellent laboratory to constrain evolutionary models of high-mass star…