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A multi-planetary system orbiting the early-M dwarf TOI-1238
f 21 vs. logP diagram for all ZTF variables with noncharacteristic LCs.
ELM of ELM-WD: An Extremely-low-mass Hot Star Discovered in LAMOST Survey - IOPscience
Folded RV curves and LCs in different bands (V band of ASAS-SN, g and r
Amp r vs. logP diagram for all ZTF variables. Symbols are as in Figure
Poster Abstracts - Kepler - NASA
The phase-folded RV curve and the multiband light curves for
ELM of ELM-WD: An Extremely-low-mass Hot Star Discovered in LAMOST Survey - IOPscience
Attila BÓDI, Research fellow, Doctor of Astronomy, Konkoly Observatory, Budapest
Folded LCs from g, V and r band are plotted in blue, cyan and red
Two sub-Neptunes around the M dwarf TOI-1470
Two sub-Neptunes around the M dwarf TOI-1470
A multi-planetary system orbiting the early-M dwarf TOI-1238