Table B.2
Disk properties of sample sorted by right ascension. Columns are NIR, MIR, and FIR excesses relative to the stellar luminosity, approximate disk dust mass, category of the SPHERE image as from Sect. 4.1, measured contrast in scattered light, and reference publication of the SPHERE images shown in this work. The observing programs are listed in Table C.1.
| Target | NIR (%) | MIR (%) | FIR (%) | Mdust (M⊕) | Type | αpol | Reference |
|---|---|---|---|---|---|---|---|
| CQ Tau | 26.8 | 28.3 | 24.3 | 108 | Bright | 6.4±1.2 | Hammond et al. (2022) |
| MWC758 | 33.6 | 9.4 | 13.7 | 49 | Bright | 3.1±0.3 | Benisty et al. (2015) |
| RW Aur | 55.1 | 38.9 | 18.4 | 27 | Ambient | – | – |
| V836 Tau | 6.4 | 6.2 | 4.1 | 24 | Faint | 1.8±0.6 | – |
| MWC480 | 18.7 | 11.2 | 5.2 | 188 | Faint | 0.5±0.1 | – |
| SU Aur | 6.4 | 5.8 | 3.7 | 9 | Bright | 10.1±0.7 | Ginski et al. (2021) |
| AB Aur | 35.6 | 15.8 | 17.9 | 32 | Bright | 9.7±0.5 | Boccaletti et al. (2020) |
| GM Aur | 0 | 5.7 | 21.2 | 130 | Bright | 16.4±1.8 | – |
| UY Aur | 49.6 | 77.3 | 53.0 | 3 | Ambient | 3.5±0.3 | – |
| DS Tau | 14.8 | 8.2 | 2.3 | 12 | Faint | <0.2 | – |
| DR Tau | 47.8 | 44.6 | – | 128 | Bright | 3.0±0.6 | Mesa et al. (2022) |
| DQ Tau | 14.7 | 18.3 | 12.0 | 79 | Faint | 0.4±0.2 | – |
| EM* LkCa15 | 12.1 | 6.1 | 7.0 | 44 | Bright | 3.7±0.4 | Thalmann et al. (2016) |
| DO Tau | 78.0 | 71.0 | 56.0 | 62 | Ambient | 1.8±0.3 | Huang et al. (2022) |
| V* V1025 Tau | 0 | 0 | 0.7 | 1 | Faint | <0.2 | – |
| V* HP Tau | 39.3 | 19.8 | – | 45 | Ambient | – | – |
| HQ Tau | 14.7 | 10.9 | 4.2 | 3 | Faint | 0.4±0.1 | – |
| DN Tau | 9.2 | 8.9 | 7.9 | 41 | Faint | 0.3±0.3 | – |
| CI Tau | 20.7 | 13.9 | 9.9 | 137 | Faint | 1.4±0.4 | Garufi et al. (2022) |
| DM Tau | 0 | 6.1 | 14.3 | 56 | Faint | 2.6±0.6 | – |
| HN Tau | – | – | – | 8 | Faint | 1.7±1.5 | – |
| DL Tau | 10.5 | 23.0 | 13.5 | 130 | Faint | 0.7±0.4 | – |
| GK Tau | 30.6 | 22.0 | 8.4 | 2 | Faint | 0.3±0.3 | – |
| GI Tau | 13.3 | 17.5 | – | 6 | Faint | 0.4±0.3 | – |
| V807 Tau | 4.8 | 4.2 | 1.6 | 17 | Faint | <0.3 | – |
| UZ Tau | 26.0 | – | – | 14 | Faint | 2.5±0.4 | Zurlo et al. (2024) |
| GG Tau | 17.6 | 14.8 | 12.9 | 295 | Bright | 8.7±1.2 | Keppler et al. (2020) |
| V710 Tau | 15.9 | 10.1 | 3.6 | 34 | Faint | 2.7±0.4 | – |
| XZ Tau | 102 | 120 | 55.0 | 2 | Ambient | – | Zurlo et al. (2024) |
| DK Tau | 16.1 | 12.2 | 6.4 | 9 | Faint | <0.2 | – |
| UX Tau | 8.8 | 3.7 | 8.4 | 33 | Ambient | 8.7±0.9 | Ménard et al. (2020) |
| IQ Tau | 20.5 | 10.8 | 6.1 | 32 | Faint | 1.7±0.7 | – |
| DH Tau | 17.6 | 6.1 | 5.6 | 1 | Faint | 0.9±0.2 | van Holstein et al. (2021) |
| DG Tau | 23.2 | 53.0 | 57.1 | 162 | Ambient | 6.5±0.8 | – |
| IP Tau | 14.0 | 8.8 | 5.3 | 4 | Faint | 1.3±0.2 | – |
| T Tau | 27.9 | 55.4 | 56.0 | 67 | Ambient | – | – |
| RY Tau | 22.9 | 21.9 | 12.0 | 52 | Ambient | 3.8±0.6 | Valegård et al. (2022) |
| DE Tau | 15.7 | 11.0 | 8.3 | 15 | Faint | 0.6±0.3 | – |
| BP Tau | 13.7 | 9.8 | 5.6 | 20 | Faint | 0.5±0.3 | – |
| V409 Tau | 7.5 | 15.6 | – | 9 | Faint | 2.9±0.5 | – |
| CY Tau | 11.3 | 6.0 | 3.1 | 43 | Faint | 0.6±0.1 | – |
| CX Tau | 10.6 | 13.3 | 7.1 | 5 | Faint | 0.4±0.3 | – |
| CW Tau | 25.0 | 19.0 | 6.9 | 27 | Faint | 1.5±0.3 | – |
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