517 citations · 6k across the 141 of their papers we have counts for
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Measuring the Local Diffusion Coefficient with H.E.S.S. Observations of Very High-Energy Electrons
Dan Hooper, Tim Linden
The HAWC Collaboration has recently reported the detection of bright and spatially extended multi-TeV gamma-ray emission from Geminga, Monogem, and a handful of other nearby, middl…
The Radio Synchrotron Background: Conference Summary and Report
J. Singal, J. Haider, M. Ajello +20
We summarize the radio synchrotron background workshop that took place July 19-21, 2017 at the University of Richmond. This first scientific meeting dedicated to the topic was conv…
Comment on "Characterizing the population of pulsars in the Galactic bulge with the Large Area Telescope" [arXiv:1705.00009v1]
Richard Bartels, Dan Hooper, Tim Linden +4
The -LAT Collaboration recently presented a new catalog of gamma-ray sources located within the region around the Galactic Center~(Aj…
Pulsar TeV Halos Explain the TeV Excess Observed by Milagro
Tim Linden, Benjamin J. Buckman
Milagro observations have found bright, diffuse TeV emission concentrated along the galactic plane of the Milky Way. The intensity and spectrum of this emission is difficult to exp…
Searching for Dark Matter with Neutron Star Mergers and Quiet Kilonovae
Joseph Bramante, Tim Linden, Yu-Dai Tsai
We identify new astrophysical signatures of dark matter that implodes neutron stars (NSs), which could decisively test whether NS-imploding dark matter is responsible for missing p…
TeV Gamma Rays From Galactic Center Pulsars
Dan Hooper, Ilias Cholis, Tim Linden
Measurements of the nearby pulsars Geminga and B0656+14 by the HAWC and Milagro telescopes have revealed the presence of bright TeV-emitting halos surrounding these objects. If you…
Dark Kinetic Heating of Neutron Stars and An Infrared Window On WIMPs, SIMPs, and Pure Higgsinos
Masha Baryakhtar, Joseph Bramante, Shirley Weishi Li +2
We identify a largely model-independent signature of dark matter interactions with nucleons and electrons. Dark matter in the local galactic halo, gravitationally accelerated to ov…
IceCube and HAWC constraints on very-high-energy emission from the Fermi bubbles
Ke Fang, Meng Su, Tim Linden +1
The nature of the -ray emission from the \emph{Fermi} bubbles is unknown. Both hadronic and leptonic models have been formulated to explain the peculiar -ray signal observed…
Using HAWC to Discover Invisible Pulsars
Tim Linden, Katie Auchettl, Joseph Bramante +5
Observations by HAWC and Milagro have detected bright and spatially extended TeV gamma-ray sources surrounding the Geminga and Monogem pulsars. We argue that these observations, al…
HAWC Observations Strongly Favor Pulsar Interpretations of the Cosmic-Ray Positron Excess
Dan Hooper, Ilias Cholis, Tim Linden +1
Recent measurements of the Geminga and B0656+14 pulsars by the gamma-ray telescope HAWC (along with earlier measurements by Milagro) indicate that these objects generate significan…
Possible Evidence for the Stochastic Acceleration of Secondary Antiprotons by Supernova Remnants
Ilias Cholis, Dan Hooper, Tim Linden
The antiproton-to-proton ratio in the cosmic-ray spectrum is a sensitive probe of new physics. Using recent measurements of the cosmic-ray antiproton and proton fluxes in the energ…
Low Mass X-Ray Binaries in the Inner Galaxy: Implications for Millisecond Pulsars and the GeV Excess
Daryl Haggard, Craig Heinke, Dan Hooper +1
If millisecond pulsars (MSPs) are responsible for the excess gamma-ray emission observed from the region surrounding the Galactic Center, the same region should also contain a larg…