10.4k citations
- Goddard Space Flight CenterUS657 papers
- George Mason UniversityUS539 papers
- University of Maryland, College ParkUS484 papers
- Naval Research Laboratory Space Science Division467 papers
- Centre National de la Recherche ScientifiqueFR448 papers
- Stanford UniversityUS339 papers
- Kavli Institute for Particle Astrophysics and CosmologyUS301 papers
- National Radio Astronomy ObservatoryUS299 papers
- Center for Astrophysics Harvard & SmithsonianUS293 papers
- National Institute for AstrophysicsIT293 papers
- SLAC National Accelerator LaboratoryUS279 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR263 papers
5 papers · 2 filters
Broad-band Spectral Modeling of Large-Scale X-ray Jets in High-Redshift Quasars: An MHD-Informed Approach
Patryk Liniewicz, Łukasz Stawarz, C. C. Cheung +2
We present a systematic spectral analysis of kiloparsec-scale jets in high-redshift quasars, modeling their radio-to-X-ray emission as synchrotron radiation and inverse-comptonizat…
Exploring the nature of Galactic unassociated sources detected by the Fermi-LAT
F. Acero, A. Acharyya, A. Adelfio +120
We investigate the nature of the unassociated sources detected by the Fermi-LAT close (|b|<10°) to the Galactic plane, representing 16% of all sources in the 4FGL-DR4 catalog. The…
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…
An updated constraint for the Gravitational Wave Background from the Gamma-ray Pulsar Timing Array
Serena Valtolina, Colin J. Clark, Rutger van Haasteren +5
Fermi LAT observations of gamma-ray pulsars can be used to build a pulsar timing array (PTA) experiment to search for gravitational wave (GW) signals at nanohertz frequencies. At t…
Gravitational Wave Measurement of the - Intrinsic Scatter at High Redshift
Cayenne Matt, Kayhan Gültekin, Gabriella Agazie +109
The observed GWB spectrum is higher in amplitude than model predictions by a factor of 2-3. Using a semi-analytic model, we evaluate the effect of a high-scatter supermassive black…