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EMBER — Estimating Mass and Bolometric properties of Evolved Remnants

ember is a tool for fitting the spectral energy distribution of white dwarfs in Gaia. It works on calibrated BP/RP spectra, meaning that it is entirely native to Gaia-- no external survey data needed (unless you want it!). It also uses monte carlo sampling of MIST white dwarf cooling tracks to measure cooling ages and theoretical hydrogen layer masses.

Installation:

To install, first run

pip install git+https://github.com/stefanarseneau/ember

This will make ember a callable command on your system. However, in order to use it, one environment variable is required which points the scripts to the Bauer+2025 (ApJS In Prep) cooling tracks. This is not packaged with the CLI to keep it somewhat lightweight. Navigate to here and follow the instructions to unpack default_grids_full.tgz. Then run the following command:

export COOLING_PATH=/path/to/default_grids_full

Now ember should be fully functional.

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EMBER — (E)stimating (M)ass and (B)olometric properties of (E)volved (R)emnants

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