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Table 1

Stellar parameters, G0, measured flux, and derived dust mass of the Orion sample used in this work.

Nr. Name RA (h:m:s) Dec (deg:m:s) Dist. (pc) M (M) L (L) Sp.Tp. Log10(G0) Flux (mJy) Mdust (M)
1. BF Ori* 05:37:13.3 −06:35:01.0 378 1.9 13 A2 1.87 0.8 1.1 ± 0.1
2. CO Ori 05:27:38.3 +11:25:39.0 395 2.3 23 F3 0.09 1.5 2.4 ± 0.5
3. HBC 442 05:34:14.2 −05:36:54.0 383 2.0 10 F8 2.66 4.0 7.8 ± 1.6
4. HD 244314 05:30:19.0 +11:20:20.0 398 2.1 19 A2 0.18 5.9 10.2 ± 2.0
5. HD 244604 05:31:57.3 +11:17:41.0 398 2.2 34 A2 0.27 4.4 6.5 ± 1.3
6. HD 245185* 05:35:09.6 +10:01:51.0 410 2.2 30 B9 3.19 34.6 37.5 ± 3.8
7. HD 287823 05:24:08.0 +02:27:47.0 343 1.8 12 A4 1.31 8.0 11.7 ± 2.3
8. HD 288012 05:33:04.8 +02:28:10.0 341 <1.9 14 A2 1.75 <1.4 <5.8
9. HD 290380 05:23:31.0 −01:04:24.0 343 1.6 6 F5 1.09 10.6 18.6 ± 3.7
10. HD 290409 05:27:05.5 +00:25:08.0 404 2.2 25 B9 0.90 10.1 16.8 ± 3.4
11. HD 290500 05:29:48.1 −00:23:43.0 402 1.9 13 A2 1.45 11.9 23.7 ± 4.7
12. HD 290764* 05:38:05.3 −01:15:22.0 397 2.0 22 A5 1.71 210.1 91.2 ± 9.1
13. HD 290770 05:37:02.4 −01:37:21.0 393 2.6 55 B8 1.70 3.5 4.4 ± 0.9
14. HD 34282* 05:16:00.5 −09:48:35.0 306 <1.9 14 A0 0.05 99.0 86.7 ± 8.7
15. HD 34700 05:19:41.4 +05:38:43.0 347 2.6 23 F8 0.02 8.1 10.2 ± 2.0
16. HD 35929 05:27:42.8 −08:19:39.0 377 3.5 93 A9 0.73 <0.7 <2.0
17. HD 36917 05:34:47.0 −05:34:15.0 445 4.4 407 B8 2.86 <0.8 <2.3
18. HD 36982 05:35:09.8 −05:27:53.0 404 <6.4 1349 B2 3.76 <0.8 <1.3
19. HD 37258* 05:36:59.3 −06:09:16.0 377 2.3 26 A0 2.30 1.8 2.1 ± 0.2
20. HD 37357* 05:37:47.1 −06:42:30.0 465 2.8 87 B9 2.01 2.9 3.8 ± 0.4
21. HD 37371 05:38:09.9 −00:11:01.0 405 3.1 100 B8 2.36 <0.6 <2.0
22. HD 37806 05:41:02.3 −02:43:01.0 397 3.5 200 B8 1.90 3.4 3.1 ± 0.6
23. HD 38087 05:43:00.6 −02:18:45.0 373 4.2 347 B5 1.79 <0.6 <1.2
24. HD 38120 05:43:11.9 −04:59:50.0 381 2.8 71 B8 0.13 31.9 35.6 ± 7.1
25. NV Ori 05:35:31.4 −05:33:09.0 384 2.1 59 F0 3.22 4.0 4.8 ± 1.0
26. RY Ori 05:32:09.9 −02:49:47.0 347 1.6 6 F4 0.64 10.6 19.1 ± 3.8
27. T Ori 05:35:50.5 −05:28:35.0 399 2.5 59 A0 3.25 1.5 1.9 ± 0.4
28. UX Ori 05:04:30.0 −03:47:14.0 320 1.9 13 A3 0.29 20.2 25.2 ± 5.0
29. V1012 Ori* 05:11:36.5 −02:22:48.5 386 1.3 6 A3 0.08 26.4 47.8 ± 4.8
30. V1787 Ori* 05:38:09.3 −06:49:17.0 394 2.1 28 A3 1.47 14.8 18.2 ± 1.8
31. V346 Ori 05:24:42.8 +01:43:48.0 336 1.6 7 A7 2.32 15.3 24.8 ± 5.0
32. V350 Ori 05:40:11.8 −09:42:11.0 391 <1.9 9 A1 0.27 4.4 9.1 ± 1.8
33. V351 Ori 05:44:18.8 +00:08:40.0 323 2.0 21 A7 0.18 69.4 77.4 ± 15.5
34. V380 Ori* 05:36:25.4 −06:42:58.0 374 2.8 95 B9 1.84 6.2 5.1 ± 0.5
35. V599 Ori* 05:38:58.6 −07:16:46.0 401 2.1 31 A4 0.60 55.9 69.0 ± 6.9

Notes. For the disks with an asterisk the fluxes have been taken from Stapper et al. (2022); Stapper et al. (2024) and van Terwisga et al. (2022). In addition to the fluxes there is an absolute calibration error, which is 10% for ALMA, and 20% for NOEMA. Except for the UV irradiance G0, continuum flux, and inferred dust mass which we derive in this work, all parameters are taken from Guzmán-Díaz et al. (2021), see this paper for their corresponding uncertainties. For V1012 Ori, the parameters are taken from Vioque et al. (2018), and the continuum flux is determined from the ALMA pipeline product data. HD 290764 is ALMA Band 7 data.

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