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20182026
most citedMulti-wavelength observations of the EUV variable metal-rich white dwarf GD 394

14 citations · 20 across the 10 of their papers we have counts for

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astro-ph.EP2026★ 1 cited

Discovery of a second-generation planet candidate accreting onto a white dwarf

Jamie T. Williams, Boris T. Gänsicke, Nicholas C. Stone +10

Many white dwarfs accrete the debris of disrupted planetary bodies, detected in the form of metal-enrichment in their atmospheres, dusty or gaseous circumstellar discs, and photome…

astro-ph.IM2026

Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory

Courtney D. Dressing, Danica Adams, Evelyne Alecian +324

The Habitable Worlds Observatory (HWO) is a future NASA flagship mission concept identified by the Astro2020 Decadal Survey as the highest priority for large space missions. HWO sh…

astro-ph.EP2026

The SPACE Program II: No discernible spectral features in the transmission spectrum of the sub-Neptune HD 191939 b observed with HST/WFC3

Cyril Gapp, Lorena Acuña-Aguirre, Reza Ashtari +17

The atmospheres of sub-Neptunes provide a window into their internal structure and history, shedding light on the origin of this common, but enigmatic, class of exoplanets. However…

astro-ph.SR2026

Direct detections of white dwarfs in four WD+dM post-common envelope binaries within 20 pc

Mairi W. O'Brien, David J. Wilson, Pier-Emmanuel Tremblay +5

Characterising post-common envelope binaries (PCEBs) containing a white dwarf and a main-sequence companion is essential for improving theories of binary evolution. This paper pres…

astro-ph.IM2026

A Critical UV Legacy: A Hubble Roadmap for HWO Science Readiness

Sarah Peacock, Aiden S. Zelakewicz, Lisa Kaltenegger +14

The Habitable Worlds Observatory (HWO) will provide the first opportunity to directly image and spectrally characterize terrestrial exoplanets in the habitable zones of nearby star…

astro-ph.IM2026

The unique ability of the Hubble Space Telescope to characterize young exoplanet environments

Keighley E. Rockcliffe, Allison Youngblood, Kevin France +10

The chemical and mass evolution of exoplanet atmospheres is shaped by their specific X-ray through ultraviolet (5 - 3200 Angstroms) irradiance history. X-ray and EUV (5 - 911 Angst…

astro-ph.IM2026

White dwarf planetary systems in the ultraviolet

Jamie Williams, Amy Bonsor, Boris Gänsicke +9

Almost every known planet host will evolve into a white dwarf, and the surviving planetary material will continue to orbit this stellar remnant. Asteroids perturbed onto star-grazi…