Stellar parameters from Green et al. (2019)
<|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:'Stellar parameters for 799 million stars, inferred by Green et al. (2019). The four parameters we infer are:  Distance modulus ('dm')  Reddening ('E')  Absolute rP1 magnitude ('Mr')  Metallicity ('FeH')These parameters are inferred by modeling the broad-band Pan-STARRS 1 and 2MASS photometry of the stars, as well as their Gaia DR2 parallaxes. We take into account priors on the distribution of stars of different types throughout the Milky Way.Reddening is given in an arbitrary unit, which can be converted to magnitudes of extinction in the PS1 and 2MASS passbands by multiplying by the following coefficients:  gP1: 3.518  rP1: 2.617  iP1: 1.971  zP1: 1.549' . 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" : ["interstellar extinction","interstellar reddening","stellar distances","stellar parameters"]} <|eot_id|>
 Here is the Description of a dataset. Description:'Stellar parameters for 799 million stars, inferred by Green et al. (2019). The four parameters we infer are:  Distance modulus ('dm')  Reddening ('E')  Absolute rP1 magnitude ('Mr')  Metallicity ('FeH')These parameters are inferred by modeling the broad-band Pan-STARRS 1 and 2MASS photometry of the stars, as well as their Gaia DR2 parallaxes. We take into account priors on the distribution of stars of different types throughout the Milky Way.Reddening is given in an arbitrary unit, which can be converted to magnitudes of extinction in the PS1 and 2MASS passbands by multiplying by the following coefficients:  gP1: 3.518  rP1: 2.617  iP1: 1.971  zP1: 1.549' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
Stellar parameters for 799 million stars, inferred by Green et al. (2019). The four parameters we infer are:  Distance modulus ('dm')  Reddening ('E')  Absolute rP1 magnitude ('Mr')  Metallicity ('FeH')These parameters are inferred by modeling the broad-band Pan-STARRS 1 and 2MASS photometry of the stars, as well as their Gaia DR2 parallaxes. We take into account priors on the distribution of stars of different types throughout the Milky Way.Reddening is given in an arbitrary unit, which can be converted to magnitudes of extinction in the PS1 and 2MASS passbands by multiplying by the following coefficients:  gP1: 3.518  rP1: 2.617  iP1: 1.971  zP1: 1.549
interstellar extinction; interstellar reddening; stellar distances; stellar parameters