activity
20172024
most citedHigh-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare

23 citations · 52 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2024★ 2 cited

Combined search in dwarf spheroidal galaxies for branon dark matter annihilation signatures with the MAGIC telescopes

MAGIC Collaboration

Massive brane fluctuations, called branons, behave as weakly interacting massive particles, which is one of the most favored class of candidates to fulfill the role of the dark mat…

astro-ph.HE2024★ 3 cited

Constraints on VHE gamma-ray emission of Flat Spectrum Radio Quasars with the MAGIC telescopes

MAGIC Collaboration

Flat spectrum radio quasars (FSRQs) constitute a class of jetted active galaxies characterized by a very luminous accretion disk, prominent and rapidly moving line-emitting cloud s…

hep-ph2022

Combined search in dwarf spheroidal galaxies for branon dark matter annihilation signatures with the MAGIC Telescopes

T. Miener, D. Nieto, V. Gammaldi +2

One of the most pressing questions for modern physics is the nature of dark matter (DM). Several efforts have been made to model this elusive kind of matter. The largest fraction o…

astro-ph.HE2020★ 23 cited

High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare

M. Lomaeva, V. Grinberg, M. Guainazzi +8

We present a 130 ks observation of the prototypical wind-accreting, high-mass X-ray binary Vela X-1 collected with XMM-Newton at orbital phases between 0.12 and 0.28. A stron…

astro-ph.HE2018★ 15 cited

NuSTAR rules out a cyclotron line in the accreting magnetar candidate 4U2206+54

J. M. Torrejón, P. Reig, F. Fürst +3

Based on our new NuSTAR X-ray telescope data, we rule out any cyclotron line up to 60 keV in the spectra of the high mass X-ray binary 4U2206+54. In particular, we do not find any…

astro-ph.HE2017★ 9 cited

Evidence of Compton cooling during an X-ray flare supports a neutron star nature of the compact object in 4U1700-37

M. Martinez-Chicharro, J. M. Torrejón, L. Oskinova +5

Based on new Chandra X-ray telescope data, we present empirical evidence of plasma Compton cooling during a flare in the non pulsating massive X-ray binary 4U1700-37. This behaviou…