arXiv (All)
open access
SN 2025wiu: A Type Ib Supernova with Post-Peak Optical Rebrightening
We present optical photometric and optical/near-infrared spectroscopic observations of SN 2025wiu, a Type Ib supernova (SN) at z = 0.046927. The r-band light curve exhibits an initial maximum of approximately -18.2 mag, followed by a weaker optical rebrightening reaching approximately -17.8 mag at +
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 prolonged plateau-to-tail transition in the Type II supernova SN2025abyc#998596
- Follow-up of SN 2025wny II: Superluminous Supernova Physics at Cosmic Noon#792423
- Follow-up of SN 2025wny II: Superluminous Supernova Physics at Cosmic Noon#788423
- First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters#1311379
- SN 2023gfo: A Peculiar Type IIP Supernova with High Luminosity and Normal Plateau Duration#617680
Record · ID 1387690
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