Imaging and Spectral Fitting of Bright Gamma-Ray Sources with the COSI Balloon Payload
The Compton Spectrometer and Imager balloon payload (COSI-Balloon) is a wide field-of-view Compton gamma-ray telescope that operates in the 0.2–5 MeV bandpass.
Jarred M. Roberts +19 more
doaj +1 more source
First Detection of Polarization in X-Rays for PSR B0540-69 and Its Nebula
We report on X-ray polarization measurements of the extragalactic Crab-like PSR B0540-69 and its Pulsar Wind Nebula (PWN) in the Large Magellanic Cloud, using a ∼850 ks Imaging X-ray Polarimetry Explorer (IXPE) exposure. The PWN is unresolved by IXPE. No
Fei Xie +103 more
doaj +1 more source
ELEMENT DISTRIBUTIONS IN THE CRAB NEBULA [PDF]
Timothy J. Satterfield +4 more
openalex +1 more source
Very high-energy gamma-ray emission beyond 10 TeV from GRB 221009A. [PDF]
LHAASO Collaboration.
europepmc +1 more source
Infrared-to-Ultraviolet Wavelength-dependent Variations Within the Pulse Profile Peaks of the Crab Nebula Pulsar [PDF]
S. S. Eikenberry +5 more
openalex +1 more source
The N(2D) + CH2CHCN (Vinyl Cyanide) Reaction: A Combined Crossed Molecular Beam and Theoretical Study and Implications for the Atmosphere of Titan. [PDF]
Vanuzzo G +10 more
europepmc +1 more source
A Cacophony of Echoes from Daily Monitoring of the Crab Pulsar at Jodrell Bank
Using archival data from the 42-foot telescope at the Jodrell Bank Observatory, we produce daily stacks of aligned giant pulses for the Crab pulsar, to study changes to the daily profiles between 2012 April and 2016 December.
Thierry Serafin Nadeau +5 more
doaj +1 more source
Spectral Signatures of Protonated Noble Gas Clusters of Ne, Ar, Kr, and Xe: From Monomers to Trimers. [PDF]
Tan JA, Kuo JL.
europepmc +1 more source
Gamma radiation from the Crab nebula above 35 MeV [PDF]
Electromagnetic radiation from the Crab nebula were observed, showing that the Crab is unique among strong X-ray sources in that major component in the low energy range (1 to 10 KeV) shows little or no temporal variation.
Bignami, G. F. +6 more
core +1 more source

