Published December 20, 2023 | Version v1
Dataset Open

Synthetic JWST MIRI-MRS Observations of Mid-IR Noble Gas Emission from T Cha

Description

Synthetic detctor images for the continuum + line emission from [Ne II], [Ne III], [Ar II], [Ar III] for T Cha made with MIRISim (Klaassen et al. 2021) for the overall best fitting model with r_in = 0.1 rG (both with and without a cavity). Also provided are backgrounds for the source observation (applicable to both with and without a cavity) and models for a synthetic standard star and its background. 

The .fits files are the underlying data cubes for the [Ne II] and [Ar II] lines which were provided as inputs to the simulator. 

For a full description, see Sellek et al. (2024a).

Files

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md5:ceae0a8021d983688ec8a46afcd55d64
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Additional details

Related works

Is supplement to
Preprint: arXiv:2403.09780 (arXiv)
Publication: 2024AJ....167..223S (Bibcode)

Funding

European Commission
DUSTBUSTERS - Dust and gas in planet forming discs 823823
UK Research and Innovation
STFC Cambridge IoA 2019 DTP ST/T505985/1
European Commission
MOLDISK - Linking chemistry and physics in the planet-forming zones of disks 101019751