arXiv (All)
open access
Chandra and Multiwavelength Study of Pevatron Candiate HESS J1702-420A
Aims: HESS J1702-420A is a promising Galactic PeVatron candidate whose physical nature remains unknown. Previous XMM-Newton observations revealed hard, apparently extended X-ray emission from XMMU J170147.3-421407, offset from the center of the TeV source, suggesting a possible pulsar wind nebula (P
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- A New Record Census of Dwarf AGN and a Bimodal <em>M</em><sub>BH</sub> − <em>M</em><sub>⋆</sub> Scaling Relation with DESI DR1#1221412
- X-ray grating spectroscopy as a mission enhancement#793042
- X-ray grating spectroscopy as a mission enhancement#789038
- Multiwavelength Classification of Chandra Sources in Omega Centauri#1423396
- PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field V: Unraveling X-ray Spectral Variability#1232959
Record · ID 1423170
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive