Serendipitous observation of a white dwarf companion to a JWST/MIRI coronagraphic calibrator

Abstract

We present the unplanned detection of a white dwarf companion to the star HD 218261 in mid-infrared (10-16 $\mu$m) observations with JWST/MIRI. This star was observed as a calibrator for coronagraphic observations of the exoplanet host HR 8799. HD 218261 B has only previously been detected by Gaia, and only in visible light. We confidently detect the companion in the mid-infrared, where it is less luminous than the primary by a factor of ~10${}^4$. The visible and mid-infrared photometry are consistent with a white dwarf of $T_{\text{eff}}\approx 10000$ K, $M\approx 0.8M_{\odot }$, though observation of its optical spectrum is required to precisely constrain its physical parameters. These results demonstrate that precise mid-infrared photometry of white dwarf companions to bright stars can be obtained with MIRI, opening up new possibilities for studying white dwarfs in close binaries.

arXiv comment4 pages, 2 figures, 2 tables. Published in MNRAS Letters

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