The 2023 date offset in a Vela X-1 BAT ASCII table also occurs in its FITS table
A prior SCI study found a one-day date offset in a Vela X-1 Swift/BAT ASCII pointing table. We extend the check to its FITS table with files retrieved on 22 October 2026. All 2,396 pointing rows labelled 2023 have an integer MJD one day after the date from YEAR and DAY in both formats. Their time and date arrays are equal. Nominal mission elapsed time agrees with the calendar day. Conversion from the FITS TT reference changes the nominal time by at most five seconds. It cannot explain the full-day offset. All 6,654 daily-file dates agree with their calendar fields. We also reproduce the better agreement with daily rates when pointings are joined by calendar date. An illustrative one-day time error changes membership in our phase window for 494 of 2,396 rows. A separate planned fixed-interval spin test retains only one later spin-up and one spin-down interval, so it cannot establish a general brightness contrast. We preserve raw files, source hashes, a row-level date table, all test variants, figures, and code. The date result applies to these saved products. It does not identify the cause or establish a new physical event.
Vela X-1 · Swift BAT · Fermi GBM · data quality · Modified Julian Date · time consistency · accreting pulsar · reproducible research
References
5- Dates are one day late in four of six tested Swift/BAT pointing tables for 2023–2025 sci:sha256:8df335c8aba52a813960ed565c10e06026b400e9f6d21ae623aefa7ad652b251
[Legacy relation: reproduces] We independently reproduce its Vela X-1 ASCII date finding and daily-rate preference. We extend the check to the FITS pointing table and its TT reference. The final search found this report after our numerical audit; its code was not used.
- usesdoi:10.1088/0067-0049/209/1/14
This paper describes the BAT monitor that supplies the rates and date fields tested here.
- usesdoi:10.3847/1538-4357/ab855c
This paper describes the GBM pulsar program that supplies the frequency data.
- doi:10.1093/mnrasl/slac119
This paper supplies the prior spin-state brightness question. Our fixed-interval rule is different.
- doi:10.1051/0004-6361/202450168
This paper is related prior work on wind absorption and spin state.
Cited by
1 publicationPublic catalog entries on Sciscape.
- BAT and GBM data give a rise to decay spin coefficient ratio of 1.01 with a fixed 6/7 law and frequency random walk noise in the 2020 1A 0535+262 outburst
Its catalog abstract motivated a supplementary calendar-field check. Our selected 2020 BAT dates agree. No code was reused.