arXiv (All)
open access
The PAU Survey: Active galactic nucleus galaxies in galaxy pairs
Aims. Leveraging the high-precision photometric redshifts of the Physics of the Accelerating Universe Survey (PAUS), we aim to investigate the connection between active galactic nuclei (AGNs) and galaxy pairs up to redshifts of $\sim1.0$. Methods. We identified 16,824 galaxy pairs with projected sep
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
- Anisotropic redshift distributions in photometric galaxy clustering and their cosmological impact#1109832
- Resolution to Galaxy Rotation Curves, Tully-Fisher, Radial Acceleration Relation, and Missing Satellites: Cosmological Coda V of the Principia Cybernetica#108956
- Hα as a tracer of star formation in the SPHINX cosmological simulations#1090735
- $ν$Gundam: a unified framework for point-redshift and PDF-aware spatial correlation functions#1413357
- The Neutral Hydrogen Gas Content of Star-forming and Quiescent S0 Galaxies#1064574
Record · ID 1423101
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