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HWO Target Stars and Systems: A Survey of Archival UV and X-Ray Data

  • Authors: Sarah Peacock, David J. Wilson, Tyler Richey-Yowell, Noah W. Tuchow, Kevin France, José A. Caballero, Riccardo Spinelli, Lía Corrales, Aiden S. Zelakiewicz, Seth Redfield, Keighley Rockcliffe, Allison Youngblood, Cynthia S. Froning, Girish M. Duvvuri, Breanna A. Binder, Natalie R. Hinkel, Eric E. Mamajek

Sarah Peacock et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Data availability across X-ray, EUV, FUV, and NUV wavelength ranges for ExEP Tier A stars, ordered by total number of observations (highest at top). Each colored block represents an individual observation, color-coded by observatory. Solid blocks indicate usable data, while hatched blocks denote flagged data with known issues. These include observations of unresolved binaries (Swift, XMM-Newton), upper limits (Swift), or data requiring linear corrections (GALEX). Blocks with solid outlines represent spectroscopic measurements (including APEC model spectra for Chandra and XMM-Newton observations), while dashed outlines represent photometry. Subplots reflect different wavelength bands.

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