activity
20142026
most citedFifteen years of XMM-Newton and Chandra monitoring of Sgr A*: Evidence for a recent increase in the bright flaring rate

96 citations · 182 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission

Tong Bao, Gabriele Ponti, Xiao-jie Xu +8

The origin of the highly ionized iron emission (Fe XXV at ) characterizing the Galactic ridge X-ray emission (GRXE) remains a fundamental puzzle in high-energy a…

astro-ph.HE2025★ 2 cited

Unveiling the soft X-ray source population towards the inner Galactic disk with XMM-Newton

Tong Bao, Gabriele Ponti, Frank Haberl +5

Across the Galactic disk lies a diverse population of X-ray sources, with the fainter end remaining poorly understood due to past survey sensitivity limits. We aim to classify and…

astro-ph.HE2025

A sample of ionised Fe line-emitting X-ray sources in the inner Galactic disc

Samaresh Mondal, Gabriele Ponti, Tong Bao +4

Previous studies suggest that the Galactic diffuse X-ray emission is composed of unresolved point sources, primarily mCVs. However, nearby mCVs have a much lower 6.7 keV line equiv…

astro-ph.GA2024

A VLA Study of Newly-Discovered Southern Latitude Non-Thermal Filaments in the Galactic Center: Polarimetric and Magnetic Field Properties

Dylan M. Pare, Cornelia C. Lang, Mark R. Morris

A population of structures unique to the Galactic Center (GC), known as the non-thermal filaments (NTFs), has been studied for over 40 years, but much remains unknown about them. I…

astro-ph.GA2024★ 17 cited

A magnetised Galactic halo from inner Galaxy outflows

He-Shou Zhang, Gabriele Ponti, Ettore Carretti +12

Magnetic halos of galaxies are crucial for understanding galaxy evolution, galactic-scale outflows, and feedback from star formation activity. Identifying the magnetised halo of th…

astro-ph.HE2024★ 8 cited

Periodicity from X-ray sources within the inner Galactic disk

Samaresh Mondal, Gabriele Ponti, Tong Bao +9

For many years, it has been claimed that the Galactic ridge X-ray emission at the Galactic Center (GC) is truly diffuse in nature. However, with the advancement of modern X-ray sat…

astro-ph.HE2023★ 3 cited

X-rays from a Central "Exhaust Vent" of the Galactic Center Chimney

Scott C. Mackey, Mark R. Morris, Gabriele Ponti +2

Using deep archival observations from the Chandra X-ray Observatory, we present an analysis of linear X-ray-emitting features located within the southern portion of the Galactic ce…

astro-ph.GA2023★ 3 cited

Ionized regions in the central arcsecond of NGC 1068. YJHK spatially resolved spectroscopy

P. Vermot, B. Barna, S. Ehlerová +3

Context. Several bright emission line regions have been observed in the central 100 parsecs of the active galaxy NGC 1068. Aims. We aim to determine the properties and ionization m…

astro-ph.HE2015★ 96 cited

Fifteen years of XMM-Newton and Chandra monitoring of Sgr A*: Evidence for a recent increase in the bright flaring rate

G. Ponti, B. De Marco, M. R. Morris +13

We present a study of the X-ray flaring activity of Sgr A* during all the 150 XMM-Newton and Chandra observations pointed at the Milky Way center over the last 15 years. This inclu…

astro-ph.HE2014★ 53 cited

On the Fe K absorption - accretion state connection in the Galactic center neutron star X-ray binary AX J1745.6-2901

G. Ponti, S. Bianchi, T. Munoz-Darias +17

AX J1745.6-2901 is a high-inclination (eclipsing) neutron star Low Mass X-ray Binary (LMXB) located less than ~1.5 arcmin from Sgr A*. Ongoing monitoring campaigns have targeted Sg…