arXiv (All)
open access
Disk reflection as the origin of the X-ray polarization of NGC 4151 with IXPE
We present an X-ray spectro-polarimetric study of the nearby type-1 active galactic nucleus NGC 4151 using two long IXPE observations obtained in 2022 and 2024, supported by simultaneous XMM-Newton and NuSTAR spectroscopy. IXPE measures a polarization degree of $\sim 6-7\%$ above 4 keV, with a polar
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
- Dust characterization of the HD 163296 disk with high-resolution multi-wavelength ALMA observations#820568
- Fragmentation in the massive G31.41+0.31 protocluster#948094
- The Star-forming Main Sequence and Bursty Star-formation Histories at $z>1.4$ in JADES and AURORA#984902
- Hint of bimodal Mg-Al anticorrelation in the metal-poor Globular Cluster NGC 4372#927655
- A Census of Na D-traced neutral ISM and outflows at $0.6<z<4$#1157272
Record · ID 1011129
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