Published January 23, 2026 | Version v1
Dataset Open

The unusually red delay spectrum of the low-mass black hole AGN NGC 4051 as revealed by intensive continuum reverberation mapping with the Las Cumbres Observatory

Authors/Creators

  • 1. ROR icon Wayne State University
  • 2. ROR icon University of St Andrews
  • 3. ROR icon Spectral Sciences (United States)
  • 4. ROR icon University of Johannesburg
  • 5. ROR icon University of Copenhagen
  • 6. University of California, Irvine
  • 7. ROR icon Tel Aviv University
  • 8. ROR icon University of Chile
  • 9. ROR icon Australian National University
  • 10. Instituto de Astronomía, Universidad Nacional Autónoma de México, Km 103 Carretera Tijuana-Ensenada, 22860 Ensenada B.C., México
  • 11. Department of Physics, University of California, 1 Shields Avenue, Davis, CA 95616-5270, USA

Description

LCO light curves of monitoring of the NGC 4051. For details on data reduction, see ...

The file has 3 columns:

  1. MJD: Modified Julian Date, in days
  2. Flux: in units of mJy
  3. Error: in units of mJy

Files

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