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Table 1

Sample of T Tauri discs observed with JWST included in this work, and assumed properties, organised by increasing stellar mass.

ID M L log(Lacc) Distance Rdust Rgap PID Date observed σ ~15.9 µm Age
[M] [L] [L] [pc] [au] [au] [d/m/y] [mJy] [Myr]
Full discs

GW Lup 0.46A1 0.33L1 –2.17L1 155 102.3 47.5 1282 8/8/2022 0.7 0.8–5.0A1
IQ Tau 0.50L2 0.22L3 –1.40L5 132 103.0 39.3 1640 27/2/2023 1.3 2.2–8.3L2
BP Tau 0.52L2 0.4L2 –1.17L2 127 40.6 1282 19/2/2023 1.5 1.0–3.4L2
Sz 98 0.74L1 1.52L1 –0.72L1 156 147.3 8.6 1282 8/8/2022 1.5 1.7–5.6A2
CI Tau 0.89L2 0.83L3 –0.70L4 160 172.5 15.2 1640 27/2/2023 1.5 1.4–4.5L2
V1094 Sco 0.92M1 1.17L1 –1.02L1 155 239.3 15.6 1282 9/8/2022 0.3 6.0–18A2
DR Tau 0.93L2 0.63L2 –0.24L2 193 54.6 37.7 1282 3/3/2023 8.4 1.8–5.9L2
DL Tau 0.98L2 0.65L2 –0.47L2 160 147.2 13.8 1282 27/2/2023 1.2 1.9–6.3L2

Transition discs (Rring)

PDS 70 0.76A3 0.35L6 −2.81L7 114 100 70 1282 1/8/2022 0.3 4.4–6.4A3
SY Cha 0.78L8 0.47L8 –2.24L8 180 135 100 1282 10/8/2022 0.7 3A4

Notes. Masses from M1van Terwisga et al. (2018). L and Lacc from L1 Alcalá et al. (2017), L2Long et al. (2019), L3Herczeg & Hillenbrand (2014), L4Donati et al. (2020), L5Gangi et al. (2022), L6Pecaut & Mamajek (2016), L7Skinner & Audard (2022), and L8Manara et al. (2016) scaled to the updated Gaia distance where relevant. All distances from the Gaia DR2 parallax (Gaia Collaboration 2016, 2023). Outer dust and gap radii estimated from ALMA data (see Appendix C). Ages are from A1Andrews et al. (2018), A2van der Marel et al. (2019), A3Müller et al. (2018), and A4 Orihara et al. (2023). Ages are generally very uncertain and may be based on different estimation methods. Especially for Sz 98 and V1094 Sco, we found large discrepancies in the literature, and we assume they are of the order of millions of years old, similarly to the other discs.

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