Table 1.
Summary of the ALPINE-CRISTAL sample used in this work.
| Original name | CRISTAL ID | z[CII] | αJ2000 | δJ2000 | log10(M⋆) | log10(SFR) | Beam size |
|---|---|---|---|---|---|---|---|
| deg | deg | M⊙ | M⊙ yr−1 | arcsec × arcsec | |||
| CRISTAL large programme | |||||||
| DEIMOS_COSMOS_842313 | CRISTAL-01 | 4.530 | 150.2271 | +2.5762 | 10.65 ± 0.50 | 2.31 ± 0.74 | 0.18 × 0.18 |
| DEIMOS_COSMOS_848185 | CRISTAL-02 | 5.294 | 150.0896 | +2.5864 | 10.30 ± 0.23 | 1.71 ± 0.29 | 0.33 × 0.28 |
| DEIMOS_COSMOS_536534 | CRISTAL-03 | 5.689 | 149.9719 | +2.1182 | 10.40 ± 0.29 | 1.79 ± 0.31 | 0.51 × 0.40 |
| vuds_cosmos_5100822662 | CRISTAL-04a | 4.520 | 149.7413 | +2.0809 | 10.15 ± 0.29 | 1.89 ± 0.21 | 0.42 × 0.35 |
| vuds_cosmos_5100541407 | CRISTAL-06a | 4.562 | 150.2538 | +1.8094 | 10.09 ± 0.30 | 1.62 ± 0.34 | 0.37 × 0.28 |
| DEIMOS_COSMOS_873321 | CRISTAL-07ab | 5.154 | 150.0166 | +2.6266 | 10.00 ± 0.33 | 1.89 ± 0.26 | 0.45 × 0.28 |
| DEIMOS_COSMOS_519281 | CRISTAL-09a | 5.575 | 149.7537 | +2.0910 | 9.85 ± 0.39 | 1.51 ± 0.32 | 0.18 × 0.16 |
| DEIMOS_COSMOS_630594 | CRISTAL-11 | 4.439 | 150.1358 | +2.2579 | 9.68 ± 0.33 | 1.57 ± 0.31 | 0.25 × 0.21 |
| vuds_cosmos_5100994794 | CRISTAL-13 | 4.579 | 150.1715 | +2.2873 | 9.65 ± 0.34 | 1.51 ± 0.41 | 0.18 × 0.14 |
| vuds_cosmos_5101244930 | CRISTAL-15 | 4.580 | 150.1986 | +2.3006 | 9.69 ± 0.33 | 1.44 ± 0.24 | 0.23 × 0.21 |
| DEIMOS_COSMOS_494763 | CRISTAL-19 | 5.233 | 150.0213 | +2.0534 | 9.51 ± 0.36 | 1.45 ± 0.36 | 0.39 × 0.29 |
| ALPINE follow-up | |||||||
| DEIMOS_COSMOS_873756 | CRISTAL-24 | 4.546 | 150.0113 | +2.6278 | 10.53 ± 0.08 | 2.06 ± 0.22 | 0.22 × 0.15 |
| vuds_cosmos_5110377875 | Nonea | 4.551 | 150.3847 | +2.4084 | 10.16 ± 0.21 | 1.99 ± 0.26 | 0.40 × 0.35 |
Notes. The first column presents the original COSMOS survey names, while the second column shows CRISTAL IDs following the naming convention in Mitsuhashi et al. (2024). The ![$ \mathrm{z} _\mathrm{[CII]} $](/articles/aa/full_html/2025/10/aa56140-25/aa56140-25-eq1.gif)
column lists redshifts derived from ALMA [C II] line observations of the CRISTAL survey (Herrera-Camus et al. 2025), for which formal uncertainty estimates are not provided. Nonetheless, these values are consistent with those from Béthermin et al. (2020), who report typical uncertainties of approximately 0.0005. Co-ordinates are given in J2000 epoch. The integrated mass and SFR are those reported in Herrera-Camus et al. (2025), apart from for VC875, whose values are from the Béthermin et al. (2020) catalogue. Beam sizes of the ALMA observations are reported as major axis × minor axis in arcseconds. aVC875 has not been used in previous CRISTAL work, therefore it has no CRISTAL ID.
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