From the 1 of 8 papers with an AI index.
34 citations
- Goddard Space Flight CenterUS8 papers
- University of Maryland, College ParkUS4 papers
- University of Maryland, Baltimore CountyUS3 papers
- Centre National de la Recherche ScientifiqueFR2 papers
- Friedrich-Alexander-Universität Erlangen-NürnbergDE2 papers
- George Washington UniversityUS2 papers
- Gran Sasso Science InstituteIT2 papers
- Howard UniversityUS2 papers
- Institut d'Estudis Espacials de CatalunyaES2 papers
- Institute of Space SciencesES2 papers
- Johns Hopkins UniversityUS2 papers
- Louisiana State UniversityUS2 papers
5 papers · 1 filter
Vacuum birefringence and the polarized X-ray emission from a radio magnetar
Rachael E. Stewart, Hoa Dinh Thi, George Younes +13
The paper presents phase- and energy-resolved X‑ray polarization measurements of the radio magnetar 1E 1547.0‑5408, finding high polarization degrees that support vacuum birefringe…
Radio Follow Up of a Sub-threshold GRB in the Sky Localization Area of GW241125
Natalie Gottschlich, Alessandra Corsi, S. Bradley Cenko +5
Since the Fermi satellite's identification of a candidate -ray burst (GRB) temporally coincident with GW150914, several tentative, and often debated, associations between elect…
Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
E. Loffredo, N. Hazra, U. Dupletsa +13
Next-generation gravitational wave (GW) observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, will observe binary neutron star (BNS) mergers across cosmic history…
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…
Flux variability of the "10 keV feature" of 4U 0115+63
Katrin Berger, Ekaterina Sokolova-Lapa, Ralf Ballhausen +14
X-ray spectra of accretion-powered X-ray pulsars can often be described using a power-law continuum with a high-energy cutoff, which might be further modified by additional spectra…