Published January 23, 2026
| Version v1
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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
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1.
Wayne State University
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2.
University of St Andrews
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3.
Spectral Sciences (United States)
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4.
University of Johannesburg
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5.
University of Copenhagen
- 6. University of California, Irvine
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7.
Tel Aviv University
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8.
University of Chile
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9.
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 https://ui.adsabs.harvard.edu/abs/2026MNRAS.tmp..594M/abstract.
If you make use of this data, please cite our work: Marculewicz et al. 2026, MNRAS, 548, 3.
The file has 3 columns:
- MJD: Modified Julian Date, in days
- Flux: in units of mJy
- Error: in units of mJy
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