X-RAY RADIANCE AND MAGNETIC FLUX
<|begin_of_text|><|start_header_id|>system<|end_header_id|> You are a research archivist expert in dataset metadata. Answer the question truthfully.  <|eot_id|><|start_header_id|>user<|end_header_id|> Here is the Description of a dataset. Description:'Soft X-ray and magnetic field observations of the Sun (quiet Sun, X-ray bright points, active regions, and integrated solar disk) and active stars (dwarf and pre–main-sequence) that were used in Figure 1 in Pevtsov et al (2003) in their study of X-ray spectral radiance LX vs. total unsigned magnetic flux for solar and stellar objects.' . Please return only a json list of at most 3 Keywords corresponding to the Description:.<|eot_id|><|start_header_id|>assistant<|end_header_id|> {"Answer" : ["stars: coronae — stars: magnetic fields — Sun: corona — Sun: magnetic fields"]} <|eot_id|>
 Here is the Description of a dataset. Description:'Soft X-ray and magnetic field observations of the Sun (quiet Sun, X-ray bright points, active regions, and integrated solar disk) and active stars (dwarf and pre–main-sequence) that were used in Figure 1 in Pevtsov et al (2003) in their study of X-ray spectral radiance LX vs. total unsigned magnetic flux for solar and stellar objects.' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
Soft X-ray and magnetic field observations of the Sun (quiet Sun, X-ray bright points, active regions, and integrated solar disk) and active stars (dwarf and pre–main-sequence) that were used in Figure 1 in Pevtsov et al (2003) in their study of X-ray spectral radiance LX vs. total unsigned magnetic flux for solar and stellar objects.
stars: coronae — stars: magnetic fields — Sun: corona — Sun: magnetic fields