Published June 8, 2021 | Version v1
Dataset Open

A characteristic optical variability timescale in astrophysical accretion disks

Creators

  • 1. University of Illinois at Urbana-Champaign
  • 2. University of California, Santa Barbara
  • 3. University of St Andrews
  • 4. Flatiron Institute
  • 5. University of Southampton
  • 6. United States Naval Academy
  • 7. University of Durham

Description

all.pdf: Full figure set showing timing analysis for each light curve in the initial sample (see caption of Fig. S5 for details).

lc_fullsample.csv: Light curve data for the initial sample. Each row corresponds to one object in the same order as Data S1. The columns are name (object used name), ra (right ascension), dec (declination), band (photometric band name), unit (flux unit), x (time; days), y (flux), yerr (1-sigma uncertainty on the flux). Note the time series data (x, y, yerr) are stored as arrays in the table entries. Negative values should be ignored. 

Files

all.pdf

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