Globular clusters host a myriad of dynamically-formed objects, some of which may be black hole X-ray binaries. The existence of such systems in globular clusters has yet to be confirmed, but deep radio observations may efficiently find them. The MAVERIC survey was conceived with this goal in mind. In this thesis I present its results, highlighting black hole candidates, contrasting them with neutron star systems, and gauging their nature
This thesis deals with three aspects of modern astrophysical research. We propose a Bayesian data an...
The observed relation between the X-ray and radio properties of low-luminosity accreting black holes...
This article was co-authored by all invited speakers at the Joint Discussion on `Neutron Stars and B...
International audienceWe investigate potential correlations between radio source counts (after backg...
International audienceRadio continuum observations offer a new window on compact objects in globular...
We present the discovery and characterization of a radio-bright binary in the Galactic globular clus...
The Galactic globular cluster (GC) NGC 3201 is the first Galactic GC observed to host dynamically co...
We report the detection of steady radio emission from the known X-ray source X9 in the globular clus...
Radio emission of globular clusters is studied by analyzing the VLA radio survey data of the NVSS an...
International audienceThe MAVERIC survey is the first deep radio continuum imaging survey of Milky W...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2003.Includes bibliographi...
The observed relation between the X-ray and radio properties of low-luminosity accreting black holes...
The population of diffuse, non-thermal radio sources in galaxy clusters presents an ever-increasing ...
International audienceAccreting neutron stars in low-mass X-ray binaries show outflows—and sometimes...
We present the results of a joint Swift-NuSTAR spectroscopy campaign on M31. We focus on the five br...
This thesis deals with three aspects of modern astrophysical research. We propose a Bayesian data an...
The observed relation between the X-ray and radio properties of low-luminosity accreting black holes...
This article was co-authored by all invited speakers at the Joint Discussion on `Neutron Stars and B...
International audienceWe investigate potential correlations between radio source counts (after backg...
International audienceRadio continuum observations offer a new window on compact objects in globular...
We present the discovery and characterization of a radio-bright binary in the Galactic globular clus...
The Galactic globular cluster (GC) NGC 3201 is the first Galactic GC observed to host dynamically co...
We report the detection of steady radio emission from the known X-ray source X9 in the globular clus...
Radio emission of globular clusters is studied by analyzing the VLA radio survey data of the NVSS an...
International audienceThe MAVERIC survey is the first deep radio continuum imaging survey of Milky W...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2003.Includes bibliographi...
The observed relation between the X-ray and radio properties of low-luminosity accreting black holes...
The population of diffuse, non-thermal radio sources in galaxy clusters presents an ever-increasing ...
International audienceAccreting neutron stars in low-mass X-ray binaries show outflows—and sometimes...
We present the results of a joint Swift-NuSTAR spectroscopy campaign on M31. We focus on the five br...
This thesis deals with three aspects of modern astrophysical research. We propose a Bayesian data an...
The observed relation between the X-ray and radio properties of low-luminosity accreting black holes...
This article was co-authored by all invited speakers at the Joint Discussion on `Neutron Stars and B...