464 citations
- California Institute of TechnologyUS47 papers
- Goddard Space Flight CenterUS31 papers
- University of CambridgeGB27 papers
- University of California, BerkeleyUS22 papers
- Center for Astrophysics Harvard & SmithsonianUS19 papers
- European Space Astronomy CentreES18 papers
- Max Planck Institute for Extraterrestrial PhysicsDE16 papers
- Centre National de la Recherche ScientifiqueFR11 papers
- Jet Propulsion LaboratoryUS11 papers
- Max Planck Institute for Solar System ResearchDE11 papers
- National Institute for AstrophysicsIT11 papers
- University of SouthamptonGB11 papers
119 papers
eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge
Tathagata Saha, Chandreyee Maitra, Philip Charles +9
The Magellanic Bridge stellar population is a relic of the tidal interaction between the Large and Small Magellanic Clouds. A comprehensive view of the evolution of the Bridge stel…
Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES
Juliana Ehrhardt, Luis Thomas, Hanna Kellermann +57
We report the confirmation and characterization of four hot Jupiter-type exoplanets initially detected by TESS: TOI-1295 b, TOI-2580 b, TOI-6016 b, and TOI-6130 b. Using observatio…
About the accuracy of the relxill/relxill_nk models in view of the next generation of X-ray missions
Honghui Liu, Askar B. Abdikamalov, Temurbek Mirzaev +4
X-ray reflection spectroscopy is a powerful tool to study the strong gravity region of black holes. The next generation of astrophysical X-ray missions promises to provide unpreced…
Proof of principle X-ray reflection mass measurement of the black hole in H1743-322
Edward Nathan, Adam Ingram, James F. Steiner +9
The black hole X-ray binary H1743-322 lies in a region of the Galaxy with high extinction, and therefore it has not been possible to make a dynamical mass measurement. In this pape…
Large Exomoons unlikely around Kepler-1625 b and Kepler-1708 b
René Heller, Michael Hippke
There are more than 200 moons in our Solar System, but their relatively small radii make similarly sized extrasolar moons very hard to detect with current instruments. The best exo…
Measuring Black Hole Spins through X-ray Reflection Spectroscopy and the Relativistic Precession Model: the case of XTE J1859+226
Gitika Mall, Honghui Liu, Cosimo Bambi +2
The development of techniques to measure accurately black hole spins is crucial to study the physics and astrophysics of these objects. X-ray reflection spectroscopy is currently t…