Open Access
Table A.3
Euclid-based assessment of previously identified candidate members of the σ Orionis cluster and very red sources in the region.
| Name | RA [hh mm ss.ss] | Dec [deg mm ss.s] | Comment |
|---|---|---|---|
| S Ori 69 | 05 39 18.05 | −02 28 54.1 | extended |
| SOriJ053923−021235 | 05 39 23.28 | −02 12 35.0 | extended |
| SOriJ053929−024636 | 05 39 29.36 | −02 46 37.1 | high proper motion |
| S Ori 57 | 05 39 47.05 | −02 25 24.5 | high proper motion |
| SOriJ053956−025315 | 05 39 56.81 | −02 53 14.6 | extended |
| SOriJ054004−025332 | 05 40 04.48 | −02 53 31.9 | extended |
| PBZ2012 J054011−025639 | 05 40 11.62 | −02 56 39.4 | high proper motion |
| S OriJ054014−025146 | 05 40 14.23 | −02 51 46.3 | extended |
| PBZ2012 J054024−024444 | 05 40 24.32 | −02 44 44.3 | extended |
| PBZ2012 J054025−024259 | 05 40 25.39 | −02 42 59.7 | extended |
| PBZ2012 J054026−023100 | 05 40 26.44 | −02 31 00.8 | high proper motion |
| PBZ2012 J054028−025116 | 05 40 27.99 | −02 51 16.7 | extended |
| PBZ2012 J054038−022806 | 05 40 38.42 | −02 28 06.6 | extended |
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