-
181
Applications of X-ray Instrumentation for Dark Matter Searches with Cosmic-ray Antiparticles
Published 2023“…Using X-ray observations of the giant molecular cloud Sagittarius B2, new upper limits are set on low-energy cosmic ray populations near the Galactic center. The limits are comparable to predictions from hydrogen ionization measurements, supporting the observation of elevated Galactic Center cosmic ray populations.…”
Get full text
Thesis -
182
Seeing Black Holes: From the Computer to the Telescope
Published 2018-08-01“…Astronomical observations are about to deliver the very first telescopic image of the massive black hole lurking at the Galactic Center. The mass of data collected in one night by the Event Horizon Telescope network, exceeding everything that has ever been done in any scientific field, should provide a recomposed image in 2018. …”
Get full text
Article -
183
Have Atmospheric Cerenkov Telescopes Observed Dark Matter?
Published 2004“…Two ground-based experiments have recently independently detected TeV $\gamma$-rays from the direction of the Galactic center. The observations made by the VERITAS and CANGAROO collaborations are unexpected, although not impossible to interpret in terms of astrophysical sources. …”
Journal article -
184
Hunting for Cold Exoplanets via Microlensing
Published 2023-08-01“…Microlensing can detect planets at distances ranging from a few hundred parsecs all the way to the Galactic center. The maximum sensitivity is reached for systems that are located half way to the galactic center, with planets orbiting the lens star at a separation of few AUs. …”
Get full text
Article -
185
Indirect detection of Dark Matter with the ANTARES Neutrino Telescope
Published 2016-01-01“…The analysis for different sources of DM (Sun, Galactic Center, Earth, …) or DM models (SUSY, Secluded) will be described and the results presented. …”
Get full text
Article -
186
Gamma-ray signatures of Dark Matter
Published 2017-01-01“…I review the ways in which Dark Matter can produce gamma-rays (and lower energy photons) and I apply the considerations to three specific examples: the tests of multi-TeV pure-WIMP candidates based on high energy gamma-rays from the Galactic Center or dwarfs, the importance of bremsstrahlung emission for light DM, the updated constraints on DM from all-sky radio surveys of the Milky Way.…”
Get full text
Article -
187
Highlights on gamma rays, neutrinos and antiprotons from TeV Dark Matter
Published 2016-01-01“…It has been shown that the gamma-ray flux observed by HESS from the J1745-290 Galactic Center source is well fitted as the secondary gamma-rays photons generated from Dark Matter annihilating into Standard Model particles in combination with a simple power law background. …”
Get full text
Article -
188
Tracking millisecond pulsars responsible for the Fermi GeV excess
Published 2023-01-01“…More than 10 years ago, an excess of γ-ray photons coming from the Galactic center was discovered in the Fermi-LAT data. …”
Get full text
Article -
189
Kinematics of the Local Spiral Structure Revealed by Young Stars in Gaia DR3
Published 2023-01-01“…Meanwhile, the sources in the Carina Arm may move in the opposite direction from the Sun to the Galactic center and rotate marginally faster than Galactic rotation. …”
Get full text
Article -
190
The characterization of the gamma-ray signal from the central Milky Way: A case for annihilating dark matter
Published 2018“…Past studies have identified a spatially extended excess of ~1-3 GeV gamma rays from the region surrounding the Galactic Center, consistent with the emission expected from annihilating dark matter. …”
Get full text
Get full text
Get full text
Article -
191
(In)direct detection of boosted dark matter
Published 2021“…We initiate the study of novel thermal dark matter (DM) scenarios where present-day annihilation of DM in the galactic center produces boosted stable particles in the dark sector. …”
Get full text
Article -
192
(In)direct detection of boosted dark matter
Published 2022“…We initiate the study of novel thermal dark matter (DM) scenarios where present-day annihilation of DM in the galactic center produces boosted stable particles in the dark sector. …”
Get full text
Article -
193
Dark nuclei. I. Cosmology and indirect detection
Published 2015“…Notably, dark nucleosynthesis realizes a novel mechanism for indirect detection signals of asymmetric dark matter from regions such as the Galactic center, without having to rely on a symmetric dark matter component.…”
Get full text
Get full text
Article -
194
Gravitational lensing by a black-bounce-Reissner–Nordström spacetime
Published 2022-05-01“…Assuming the supermassive black holes in the Galactic Center and at the center of M87, Sgr A* and M87* respectively, as the lenses, we evaluate these observables and assess their detectability. …”
Get full text
Article -
195
The orbit of the old, metal-rich, open cluster NGC 6791
Published 2012-02-01“…To estimate the viability of one of the cluster’s proposed scenarios of origin we also follow a set of forward integrations originating closer to the Galactic center (GC) where the metal enrichment could be faster. …”
Get full text
Article -
196
Weak and strong deflection gravitational lensing by a renormalization group improved Schwarzschild black hole
Published 2019-12-01“…By taking the supermassive black holes Sgr A* and M87* respectively in the Galactic Center and at the center of M87 as lenses, we estimate these observables and analyse possibility of detecting this quantum improvement. …”
Get full text
Article -
197
Z-Distribution and Period Gradient of Classical Cepheids in the Galactic Plane
Published 1986-12-01“…The well known phenomenon that the periods of classical cepheids decrease away from the Galactic center was crudely interpreted as due to an age gradient rather than an abundance gradient under the assumption that relations between the period and galactocentric distance, and between the abundance and period are linear.…”
Get full text
Article -
198
On the Population of Wind-Accreting Neutron Stars in the Galaxy
Published 2002“…This work was motivated by recent Chandra observations of the Galactic center by Wang et al. (2002). Our calculations indicate that many of the discrete X-ray sources detected in this survey may be wind-accreting neutron stars, and that many more may be discovered with deeper X-ray observations. …”
Journal article -
199
Modeling the Radial Distribution of Pulsars in the Galaxy
Published 2024-01-01“…The radial distribution function is used to estimate the proportion of pulsars in each spiral arm and the Galactic center.…”
Get full text
Article -
200
The Hot Circumgalactic Medium of the Milky Way: New Insights from XMM-Newton Observations
Published 2023-01-01“…The presence of the super-virial phase far from the regions around the Galactic center implicates physical processes unrelated to the activity at the Galactic center. …”
Get full text
Article