eScholarship
metadata only
CC BY
New limits from microlensing on Galactic black holes in the mass range 10 M⊙ < M < 1000 M⊙
We searched for long-duration microlensing events originating from intermediate-mass black holes (BH) in the halo of the Milky Way, using archival data from the EROS-2 and MACHO photometric surveys towards the Large Magellanic Cloud (LMC). We combined data from these two surveys to create a common d
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
- The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-Day Location#1110555
- Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network#491773
- Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network#370453
- Migration Traps as Variability Attractors. I. Optical/UV Signatures of Embedded Stellar-Mass Black Holes in Active Galactic Nucleus Disks#1048712
- Inpainting to search for premerger massive black hole binaries in realistic LISA datasets#1297131
Record · ID 1358067
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