arXiv (All)
open access
TARTARUS: A High-Performance Python Code for Ray Tracing in Curved Spacetimes
The recent observations of the supermassive black holes M87* and Sagittarius A* by the Event Horizon Telescope collaboration (EHT) have shown the need for robust, efficient, and accessible numerical tools to model light propagation in strongly curved spacetimes. Comparing theoretical accretion model
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
- An empirically constrained Covariant Modified Gravity: exact reconstruction of galactic rotation curves and lensing#1034840
- A Differentiable Parametric Model of Binary-Black-Hole Initial Data: I. Conformally flat Bowen-York punctures#997082
- A Targeted Search for Variable Gravitationally Lensed Quasars#1062751
- Broadband reverberation mapping of quasars at cosmic noon#1131944
- Detection of unresolved strongly lensed supernovae with the 7-Dimensional Telescope#1165848
Record · ID 986602
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