activity
20112026
most citedA new nearby pulsar wind nebula overlapping the RX J0852.0-4622 supernova remnant

33 citations · 65 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026★ 1 cited

Bridging the gap between SLSNe and SE-SNe. Multi-wavelength analysis of the SLSN-Ib SN 2024jlc

A. Simongini, F. Acero, M. Imbrogno +15

The Type I super-luminous supernova SN~2024jlc (ZTF24aapadbb) exploded on the 25th of May 2024 at . Being the closest supernova of this class discovered in recent years…

astro-ph.HE2026

SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics

Emma McGinness, Rebecca Diesing, Damiano Caprioli +1

SN 1006 is a historical Type Ia supernova remnant that exhibits non-thermal emission ranging from radio to multi-TeV -rays. Most of this emission (particularly X-rays and -ra…

astro-ph.HE2026★ 2 cited

Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine

F. Acero, A. Acharyya, A. Adelfio +116

Superluminous supernovae (SLSNe) are a rare class of transients with peak luminosities 10-100 times greater than those of standard core-collapse supernovae (SNe). The mechanisms po…

astro-ph.HE2026

Isolating Sgr A East: The First Uncontaminated X-ray Maps of a Galactic Center Supernova Remnant

Mayura Balakrishnan, Adrien Picquenot, Lia Corales +3

The central few parsecs of the Milky Way host a complex X-ray-emitting environment in which several extended plasma components are blended along the line of sight, complicating att…

astro-ph.HE2025

Discovery of a Pulsar Wind Nebula Candidate Associated with the Galactic PeVatron 1LHAASO J0343+5254u

Stephen DiKerby, Shuo Zhang, Tulun Ergin +6

The astronomical origin of the most energetic galactic cosmic rays and gamma rays is still uncertain. X-ray followup of candidate "PeVatrons", systems producing cosmic rays with en…

astro-ph.HE2024

Parkes Radio and NuSTAR X-ray Observations of the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud

Jordan Eagle, Jeremy Hare, Elizabeth Hays +9

Gamma-ray emission is observed coincident in position to the evolved, composite supernova remnant (SNR) B0453-685. Prior multi-wavelength investigations of the region indicate that…

astro-ph.HE2024★ 5 cited

Bayesian insights in Tycho supernova remnant : a detailed mapping of ejecta properties

L. Godinaud, F. Acero, A. Decourchelle +1

While Tycho's supernova remnant is one of the most studied type Ia Galactic supernova remnants, a global view of the physical properties of its ejecta is lacking, to understand its…

astro-ph.HE2024

Mapping thermal emission in the synchrotron-dominated SNRs 330.2+1.0, 3C58, and RX J1713.7-3946

Adrien Picquenot, Brian J. Williams, Fabio Acero +1

Since the discovery of synchrotron X-ray emission from the shell of the supernova remnant (SNR) SN 1006, multiple observations from Chandra and XMM-Newton have shown that many youn…

astro-ph.HE2023★ 15 cited

A fresh perspective on the 3D dynamics of Tycho's supernova remnant: Ejecta asymmetries in the X-ray band

Leila Godinaud, Fabio Acero, Anne Decourchelle +1

450 years after the explosion of the Type Ia SN1572, the dynamics of the Tycho supernova remnant can give us keys to understand the explosion mechanism and the interaction of the r…

astro-ph.HE2018★ 6 cited

Discovery of a radio nebula around PSR J0855-4644

C. Maitra, S. Roy, F. Acero +1

We report the discovery of a diffuse radio emission around PSR J0855--4644 using an upgraded GMRT (uGMRT) observation at 1.35 GHz. The radio emission is spatially coincident with t…

astro-ph.HE2018★ 1 cited

Probing the nature of AX J0043-737: Not an 87 ms pulsar in the SMC

C. Maitra, J. Ballet, P. Esposito +4

AX J0043-737 is a source in the ASCA catalogue, the nature of which is uncertain. It is most commonly classified as a Crab-like pulsar in the Small Magellanic Cloud (SMC) following…

astro-ph.HE2012★ 33 cited

A new nearby pulsar wind nebula overlapping the RX J0852.0-4622 supernova remnant

F. Acero, Y. Gallant, J. Ballet +2

Energetic pulsars can be embedded in a nebula of relativistic leptons which is powered by the dissipation of the rotational energy of the pulsar. The object PSR J0855-4644 is an en…

astro-ph.HE2011★ 2 cited

A new nearby PWN overlapping the Vela Jr SNR

F. Acero, Y. Gallant, R. Terrier +2

PSR J0855-4644 is an energetic pulsar (Edot = 1.1x10^36 erg/s, P=65 ms) discovered near the South-East rim of the supernova remnant (SNR) RX J0852.0-4622 (aka Vela Jr) by the Parke…