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Parameters of 220 million stars from Gaia BP/RP spectra

Research datakeyboard_double_arrow_right Dataset 03 Mar 2023Publisher:Zenodo
Authors: Zhang, Xiangyu; Green, Gregory M; Rix, Hans-Walter;

doi: 10.5281/zenodo.7748979 , 10.5281/zenodo.7811871 , 10.5281/zenodo.7748881 , 10.5281/zenodo.7692680 , 10.5281/zenodo.7692681

Parameters of 220 million stars from Gaia BP/RP spectra

Abstract

We present parameters of 220 million stars, based on Gaia XP spectra and near-infrared photometry from 2MASS and WISE. Instead of using ab initio stellar models, we develop a data-driven model of Gaia XP spectra as a function of the stellar parameters, with a few straightforward built-in physical assumptions. Here, we provide the resulting catalog of stellar parameters, our trained stellar model, and a few Python scripts that demonstrate how to interact with the catalog and model. See the README.md for more information.

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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