87 citations · 91 across the 5 of their papers we have counts for
6 papers
A GeV to TeV view of shell-type SNRs
Henrike Fleischhack, the HAWC collaboration, the Fermi-LAT collaboration
Shock acceleration by the shells of supernova remnants (SNRs) has been hypothesized to be the mechanism that produces the bulk of Galactic Cosmic Rays, possibly up to PeV energies.…
Investigating the Nature of Late-Time High-Energy GRB Emission Through Joint Fermi\Swift Observations
The Fermi LAT Collaboration
We use joint observations by the Neil Gehrels Swift X-ray Telescope (XRT) and the Fermi Large Area Telescope (LAT) of gamma-ray burst (GRB) afterglows to investigate the nature of…
Multiwavelength observations of the blazar BL Lacertae in June 2015
Shimpei Tsujimoto, Monica Vazquez Acosta, Elina Lindfors +9
BL Lacertae is a blazar at the redshift of z = 0.069, eponym of the BL Lac blazar type. It is also a prototype of the low-frequency-peaked BL Lac (LBL) subclass. It was first detec…
MAGIC observations of variable very-high-energy gamma-ray emission from PKS1510-089 during May 2015 outburst
Julian Sitarek, Josefa Becerra González, Vandad Fallah Ramazani Elina Lindfors +11
PKS1510-089 is a flat spectrum radio quasar located at a redshift of 0.36. It is one of only a few such sources detected in very-high-energy (VHE, >100 GeV) gamma rays. Though PKS1…
Fermi-LAT Observation of Impulsive Solar Flares
N. Omodei, V. Petrosian, M. Pesce-Rollins +1
The Fermi Large Area Telescope (LAT) is the most sensitive instrument ever deployed in space for observing gamma-ray emission >100 MeV. This sensitivity has enabled the LAT to dete…
Fermi-LAT Search for Pulsar Wind Nebulae around gamma-ray Pulsars
The Fermi LAT Collaboration, Pulsar Timing Consortium
The high sensitivity of the Fermi-LAT (Large Area Telescope) offers the first opportunity to study faint and extended GeV sources such as pulsar wind nebulae (PWNe). After one year…