25 citations · 202 across the 24 of their papers we have counts for
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Radio and infrared study of the supernova remnant candidate HESS J1912+101
Laura Duvidovich, Alberto Petriella
Aims: We provide new insights into the gamma-ray emission from HESS J1912+101, a TeV supernova remnant candidate probably associated with the radio pulsar PSR J1913+1011. Methods:…
Radio study of HESS J1857+026. Gamma-rays from a superbubble?
Alberto Petriella, Laura Duvidovich, Elsa Giacani
Aims. We provide new insights into the nature of HESS J1857+026, a very-high-energy γ-ray source whose complex morphology in the TeV band was attributed to the superposition of two…
Radio study of the extended TeV source VER J1907+062
L. Duvidovich, A. Petriella, E. Giacani
This paper aims to provide new insights on the origin of the TeV source VER J1907+062 through new high-quality radio observations. We used the Karl G. Jansky Very Large Array (VLA)…
New X-ray observations toward PSR J1826-1256
L. Duvidovich, E. Giacani, G. Castelletti +2
We present the results of XMM-Newton observations toward the pulsar PSR J18261256, which lies at 5.4 from the centroid of the TeV source HESS J1826130. These data…
New composite supernova remnant toward HESS J1844-030?
Alberto Petriella
AIMS: HESS J1844-030 is a newly confirmed TeV source in the direction of the X-ray pulsar wind nebula (PWN) candidate G29.4+0.1 and the complex radio source G29.37+0.1, which is li…
A new study towards PSR J1826-1334 and PSR J1826-1256 in the region of HESS J1825-137 and HESS J1826-130
L. Duvidovich, E. Giacani, G. Castelletti +2
Aims. The goal of this paper is to detect synchrotron emission from the relic electrons of the crushed pulsar wind nebula (PWN) HESS J1825-137 and to investigate the origin of the…
Unveiling the origin of HESS J1809-193
G. Castelletti, E. Giacani, A. Petriella
The main goal of this paper is to provide new insights on the origin of the observable flux of gamma rays from HESS J1809-193 using new high-quality observations in the radio domai…