Euclid on Sky
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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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