A 4.3–5.0-hour box search finds no score above 10 in WD 1145+017 TESS Sector 72 data
WD 1145+017 can show deep eclipses from orbiting dust. This study tests public TESS Sector 72 data for stable repeating eclipses. The common selection has 14487 samples at 120-second cadence over 23.17 days in November and December 2023. A box search tests 4097 periods from 4.3 to 5.0 hours. The tested widths are 4, 8, 16, and 32 minutes. Straight lines are removed from fixed 12-hour segments. The largest scores are 4.97 in SAP and 4.95 in PDCSAP. Both peaks occur at 4.49047 hours. Neither reaches the threshold of 10. All 128 block-sign control maxima are below 5.34. The score is not a calibrated Gaussian significance. Artificial stable boxes give 5600 trials across both products. Each width has 100 shared period and phase draws at seven depths. Each primary trial supplies the nearest grid period. For widths of 4 or 8 minutes, both products recover 100 of 100 trials at 32 percent target-relative depth. For widths of 16 or 32 minutes, the count is 100 of 100 at 16 percent depth. These are the lowest tested depths with at least 95 recoveries in both products. For the same finite trials, these counts also bound full-search threshold alerts from below because the supplied period is in the search grid. They do not by themselves guarantee correct period selection. Full searches of 160 of these same trials also recover the injected periods under the stated phase and drift tests. SAP and PDCSAP use the same photons. The test fixes errors, thresholds, crowding factors, and the observed noise. Signals enter the delivered photometry and do not pass through the earlier SPOC processing. The result does not exclude changing dust events or events in rejected samples and gaps. The package preserves original archive files, source hashes, code, all trials, and figures.
WD 1145+017 · TESS Sector 72 · planetary debris · white dwarf · repeating eclipses · injection recovery · public astronomical data · box least squares
References
10- usesdoi:10.17909/vejb-8661
The primary public input is the 120-second SPOC light curve of TIC 902906874 from TESS Sector 72.
- usesdoi:10.17909/mjax-wh78
The earlier comparison input is the 120-second SPOC light curve of TIC 902906874 from TESS Sector 46.
- doi:10.1038/nature15527
This study found several short periods and changing deep eclipses in WD 1145+017.
- doi:10.1093/mnras/stae750
This study reports the long changes in eclipse activity and analyzes the earlier TESS Sector 46 record. It gives the comparison context.
- doi:10.31577/caosp.2024.54.2.98
This study reports close and changing periods from earlier ground observations. It motivates the restriction of the present result to stable signals.
- usesdoi:10.1051/0004-6361:20020802
The test uses the box least squares method to search periodic eclipses.
- usesdoi:10.3847/1538-4357/ac7c74
Astropy reads the FITS data and supplies the box least squares implementation.
- doi:10.1117/1.JATIS.1.1.014003
The TESS mission supplies the observations.
- doi:10.1117/12.2233418
The SPOC pipeline supplies the delivered SAP and PDCSAP light curves.
- Three TESS sectors give a 6.9% upper probability bound for independent 46-minute K2-22 b box events with at least 1.5% depth under matched control noise sci:sha256:6ae8cf3f6b28006281e12bba65dfdf84a8ab925b42defdab511efc856ad6c5fc
This related SCI study tests independent single transit events in K2-22 b. The present study tests stable repeated eclipses in WD 1145+017. No code or data are reused.
Cited by
1 publicationPublic catalog entries on Sciscape.
- supportsTESS 2-min data of 1889 Gaia white dwarfs with G < 16 show no transiting planets; for log-uniform period and radius priors, fewer than 3.6% have 8–28 Earth-radius planets at 0.2–10 d (95%)
Our box search also does not find the irregular debris transits of WD 1145+017. This agrees with this publication.