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exoTEDRF: An EXOplanet Transit and Eclipse Data Reduction Framework

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arxiv 2407.17541 v1 pith:M2UKLLTU submitted 2024-07-24 astro-ph.IM astro-ph.EP

classification astro-ph.IMastro-ph.EP
keywords exotedrfreductiondatastepsdesignedeclipseexoplanetframework
verification ladder T0 review T1 audit T2 compute T3 formal

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Here, I present the community with exoTEDRF (EXOplanet Transit and Eclipse Data Reduction Framework; formerly known as supreme-SPOON), an end-to-end pipeline for data reduction and light curve analysis of time series observations (TSOs) of transiting exoplanets with JWST. The pipeline is highly modular and designed to produce reliable spectra from raw JWST exposures. exoTEDRF (pronounced exo-tedorf) consists of four stages, each of which are further subdivided into a series of steps. These steps can either be run individually, for example in a Jupyter notebook, or via the command line using the provided configuration files. The steps are highly tunable, allowing full control over every parameter in the reduction. Each step also produces diagnostic plots to allow the user to verify their results at each intermediate stage, and compare outputs with other pipelines if so desired. Finally, exoTEDRF has also been designed to be run in "batch" mode: simultaneously running multiple reductions, each tweaking a subset of parameters, to understand any impacts on the resulting atmosphere spectrum.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Continuous helium absorption from the leading and trailing tails of WASP-107b

    astro-ph.EP 2025-05 conditional novelty 7.0 of 10

    Continuous JWST observations of WASP-107b reveal metastable helium absorption beginning 1.5 hours before ingress, evidence of an extended ellipsoidal thermosphere, with spot-corrected water abundance log10 H2O = -2.5 ± 0.6.

  2. TOI-421 b: A Hot Sub-Neptune with a Haze-Free, Low Mean Molecular Weight Atmosphere

    astro-ph.EP 2025-01 conditional novelty 6.0 of 10

    TOI-421 b, a 920 K sub-Neptune around a Sun-like star, has a clear, hydrogen-dominated, near-solar-metallicity atmosphere with detected water, based on JWST transmission spectroscopy.

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