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Later accepted TESS Sector 78 data show smaller 30-minute flux changes in the T CrB aperture

We test whether rapid flux changes stayed constant during the May 2024 TESS visit to T Coronae Borealis. We use public two-minute SPOC data and accept only samples with no quality flags. Every sample inside each measured pair must pass the cut. A measure of 30-minute changes, after subtraction of the quoted independent error variance, falls from 2.263 to 1.011 parts per thousand between the accepted 3–12 May and 17–21 May intervals. The later value is 0.447 of the earlier value, a decrease of 55.3 percent. Four pixel apertures preserve the decrease. Pointing and background fits remove less than one percent of raw difference power. Three bright nearby comparison targets on the same detector do not show a decrease of this size. We chose the split after inspection of daily variation. The later interval has only four daily bins, and a five-day gap in accepted data prevents an exact change time. This is an exploratory measurement of aperture flux. It does not establish a physical state change or an eruption date. The package preserves original data, source records, code, figures, tables, and checks for reproduction without network access.

T Coronae Borealis · T CrB · TESS · Sector 78 · flickering · rapid flux variation · recurrent nova · public data

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References

8
  1. doi:10.1111/j.1365-2966.2004.07747.x

    This work measured optical flickering in T CrB.

  2. doi:10.1111/j.1365-2966.2009.16068.x

    This work studied the statistics of T CrB flickering.

  3. doi:10.1093/mnras/stad735

    This work includes earlier TESS analysis and the long optical record.

  4. doi:10.3847/2515-5172/ace527

    This work reported the end of the bright accretion state in 2023.

  5. doi:10.1051/0004-6361/202348116

    This work detected T CrB flickering in earlier TESS sectors. It sets the scope of the present result.

  6. doi:10.1051/0004-6361/202555917

    This work gives the accretion history and reports a rise in blue and ultraviolet light from about May 2024.

  7. doi:10.1117/1.JATIS.1.1.014003

    This paper describes the TESS mission that supplied the data.

  8. doi:10.1117/12.2233418

    This paper describes SPOC processing for the source products.

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