ZTF J0007+4804 is the first known hot subdwarf-white dwarf binary that exhibits SU UMa-type dwarf nova outbursts with a 108.72-minute orbital period.
A., Hernández, J., et al
6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
representative citing papers
New catalogue of 1423 Gaia DR3 variable white dwarf candidates, with 141 ZTF-confirmed periodic variables classified into known types and 83 newly identified periodic stars.
Planar very metal-poor stars exhibit chemical homogeneity and dwarf-galaxy-like abundance ratios, supporting origin from one ancient accreted system tentatively called Loki.
Neural network derives LAMOST instrumental profiles from arc lamps and reduces RV dispersion by ~3 km/s.
Gaia First Look delivers daily data quality checks and early warnings by running a limited astrometric solution alongside calibrations and diagnostics.
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
citing papers explorer
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Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
ZTF J0007+4804 is the first known hot subdwarf-white dwarf binary that exhibits SU UMa-type dwarf nova outbursts with a 108.72-minute orbital period.
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Gaia DR3 Variable White Dwarfs vetted by ZTF
New catalogue of 1423 Gaia DR3 variable white dwarf candidates, with 141 ZTF-confirmed periodic variables classified into known types and 83 newly identified periodic stars.
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An ancient system hidden in the Galactic plane?
Planar very metal-poor stars exhibit chemical homogeneity and dwarf-galaxy-like abundance ratios, supporting origin from one ancient accreted system tentatively called Loki.
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Characterizing the Instrumental Profile of LAMOST
Neural network derives LAMOST instrumental profiles from arc lamps and reduces RV dispersion by ~3 km/s.
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The First Look of Gaia: Daily data quality and instrument health assessment with automated early warnings
Gaia First Look delivers daily data quality checks and early warnings by running a limited astrometric solution alongside calibrations and diagnostics.
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Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.