arXiv (All)
open access
Semiresolved Stellar Populations as Distance Indicators
Galaxy distances are central to our understanding of the Universe. Despite the success of existing approaches, independent and complementary methods remain valuable for testing systematic effects and extending the applicability range of different distance metrics. Here we demonstrate that the spectr
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
- DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics#983412
- Extragalactic Stellar Streams in Time-Dependent Cosmological Halos#819968
- (Re)Assessing Galaxy Clusters with Cosmological Models: Scales, Anisotropies, and Scientific Explanation#86429
- Is Gravity Truly What Einstein Said It Was —A Re-examination Based on Mach's Principle and the Global Inertial Vortex Force/引力，真如爱因斯坦所说的样子吗——基于马赫原理与全域惯性漩涡力的重新审视#81717
- Tracing the Evolution of $Ω_m(z)$ over the Last 10 Billion Years with Non-parametric Methods#1062866
Record · ID 821337
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