Calibrating the Clock of JWST

Abstract JWST, despite not being designed to observe astrophysical phenomena that vary on rapid timescales, can be an unparalleled tool for such studies. If timing systematics can be controlled, JWST will be able to open up the subsecond infrared timescale regime. Rapid time-domain studies, such as lag measurements in accreting compact objects and solar system stellar occultations, require both precise interframe timing and knowing when a time series begins, down to an absolute accuracy significantly below 1 s. In this work, we present two long-duration observations of the deeply eclipsing double white dwarf system ZTF J153932.16+502738.8, which we use as a natural timing calibrator to measure the absolute timing accuracy of JWST's clock. From our two epochs, we measure an average clock accuracy of 0.12 ± 0.06 s, implying that JWST can be used for subsecond time-resolution studies down to the ∼100 ms level, a factor ∼5 improvement upon the prelaunch clock accuracy requirement. We also find an asymmetric eclipse profile in the F322W2 band, which we suggest has a physical origin.

Authors

Publication Details

Journal
The Astronomical Journal
Published
2024-12-11
DOI
https://doi.org/10.3847/1538-3881/ad8eb1
Citations
4
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
1.33

Funders

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article

Calibrating the Clock of JWST

S. P. Littlefair, C. O. Heinke, C. T. Britt, T. Shahbaz et al.
4 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
1.33
article

Calibrating the Clock of JWST

S. P. Littlefair, C. O. Heinke, C. T. Britt, T. Shahbaz, A. W. Shaw, Thomas J. Maccarone, R. G. French, David L. Kaplan, P. Santos-Sanz, G. R. Sivakoff, Michael E. Ressler, R. I. Hynes, D. A. H. Buckley, Richard M. Plotkin, C. Knigge, Abigail Stevens, V. S. Dhillon, P. Gandhi, Kevin B. Burdge, Devraj Pawar, P. A. Charles, E. S. Borowski
article en
4 citations

Abstract

Abstract JWST, despite not being designed to observe astrophysical phenomena that vary on rapid timescales, can be an unparalleled tool for such studies. If timing systematics can be controlled, JWST will be able to open up the subsecond infrared timescale regime. Rapid time-domain studies, such as lag measurements in accreting compact objects and solar system stellar occultations, require both precise interframe timing and knowing when a time series begins, down to an absolute accuracy significantly below 1 s. In this work, we present two long-duration observations of the deeply eclipsing double white dwarf system ZTF J153932.16+502738.8, which we use as a natural timing calibrator to measure the absolute timing accuracy of JWST's clock. From our two epochs, we measure an average clock accuracy of 0.12 ± 0.06 s, implying that JWST can be used for subsecond time-resolution studies down to the ∼100 ms level, a factor ∼5 improvement upon the prelaunch clock accuracy requirement. We also find an asymmetric eclipse profile in the F322W2 band, which we suggest has a physical origin.

The Astronomical JournalVol. 169(1)
National Aeronautics and Space Administration, Space Telescope Science Institute, UK Research and Innovation, Ministerio de Ciencia, Innovación y Universidades, European Commission, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council, Agencia Estatal de Investigación
Openalex Percentile: Top 19%
Stellar, planetary, and galactic studies
1.33
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