Spectroscopic detection and characterization of an irradiated substellar donor planet in an accreting white-dwarf binary system reveals a donor mass of 0.055 ± 0.008 solar masses, an average spectral type of L1 ± 1 and an average irradiation-induced temperature difference between the dayside and nightside of 57 kelvin.
- Juan V. Hernández Santisteban
- Christian Knigge
- Peter H. Hauschildt
