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Table A.1.

Final selection of stars in Eridanus 2 for the kinematic analysis.

ID RA (deg) Dec (deg) LOS velocity (km s−1)
1058 56.06437 −43.53266 72.3 ± 20.3
2348 56.06852 −43.52907 64.1 ± 14.7
3932 56.08301 −43.54452 67.5 ± 21.0
4448 56.07485 −43.52340 61.1 ± 21.9
4630 56.08690 −43.54593 53.9 ± 16.4
4866 56.08551 −43.54109 100.3 ± 12.3
5256 56.08346 −43.53403 73.2 ± 9.4
6227 56.08961 −43.53808 54.0 ± 22.4
6664 56.08621 −43.52849 45.1 ± 13.2
9242 56.09260 −43.52854 79.2 ± 23.8
9304 56.09734 −43.53763 47.9 ± 14.2
9653 56.09155 −43.52363 61.1 ± 25.8
11171 56.09772 −43.52349 65.7 ± 20.5
11935 56.10766 −43.53628 96.0 ± 18.2
12933 56.11073 −43.53324 59.2 ± 27.9
13257 56.11460 −43.53779 75.8 ± 25.2
13549 56.11108 −43.52766 85.4 ± 12.7
14541 56.11801 −43.53130 83.9 ± 24.0
14551 56.12156 −43.53821 47.0 ± 13.2
14927 56.12031 −43.53184 73.3 ± 18.3
1002926 56.06117 −43.52640 73.5 ± 1.2
1003016 56.06721 −43.53447 68.5 ± 8.2
1003965 56.07701 −43.55105 83.1 ± 3.0
1004032 56.07494 −43.54397 78.3 ± 7.8
1004756 56.07025 −43.53160 88.6 ± 8.8
1005369 56.06965 −43.52886 79.2 ± 5.1
1005680 56.07367 −43.53681 85.7 ± 6.8
1006056 56.08153 −43.55039 59.3 ± 3.5
1006522 56.07226 −43.52913 90.9 ± 12.5
1007072 56.07965 −43.54091 86.1 ± 9.3
1007081 56.08013 −43.54021 98.2 ± 13.3
1007232 56.08398 −43.54946 75.7 ± 4.7
1007817 56.08566 −43.54801 91.5 ± 7.7
1007943 56.08618 −43.55232 84.5 ± 1.5
1008083 56.07548 −43.52653 78.3 ± 5.6
1008946 56.07992 −43.53195 94.8 ± 5.1
1009001 56.07691 −43.52592 76.3 ± 4.3
1009750 56.07605 −43.51971 63.6 ± 11.6
1010022 56.07599 −43.52005 79.2 ± 1.4
1010255 56.07916 −43.52591 86.0 ± 3.7
1010560 56.08680 −43.54108 86.2 ± 1.0
1010966 56.08882 −43.54120 62.3 ± 9.5
1010988 56.08438 −43.53642 79.9 ± 0.9
1011039 56.08312 −43.52889 69.4 ± 4.9
1012006 56.09504 −43.54725 56.9 ± 6.4
1012321 56.09129 −43.53950 100.8 ± 8.0
1013259 56.08689 −43.52648 74.7 ± 14.9
1013271 56.09513 −43.54466 95.8 ± 3.5
1013803 56.08677 −43.52694 88.6 ± 7.1
1014555 56.09416 −43.53802 77.8 ± 9.7
1017156 56.09828 −43.53589 74.1 ± 10.2
1017445 56.09230 −43.52332 81.1 ± 6.2
1018571 56.09774 −43.52937 75.8 ± 3.8
1018845 56.09547 −43.52370 71.9 ± 7.9
1019322 56.09626 −43.52348 74.5 ± 1.2
1019765 56.10630 −43.53993 76.0 ± 5.6
1019801 56.10251 −43.53367 97.3 ± 6.4
1021252 56.10830 −43.53636 82.9 ± 4.0
1021910 56.10425 −43.52568 100.7 ± 8.9
1022334 56.10586 −43.52943 71.4 ± 3.6
1022351 56.11369 −43.54099 57.1 ± 10.1
1022417 56.10670 −43.52748 80.2 ± 9.2
1023228 56.11503 −43.53988 82.3 ± 5.2
1024420 56.11196 −43.52721 73.3 ± 4.3
1025752 56.11125 −43.52308 78.1 ± 0.9
1026606 56.11505 −43.52693 79.6 ± 1.2
1026881 56.12141 −43.53211 63.1 ± 8.1
1027080 56.12490 −43.54157 84.7 ± 1.9
1027101 56.12301 −43.53626 80.0 ± 6.3
1027929 56.11814 −43.52022 83.9 ± 5.0
1027958 56.11869 −43.52139 68.0 ± 5.6
1030234 56.12404 −43.53005 71.9 ± 0.9
2000001 56.00955 −43.53305 69.8 ± 1.6
2000002 56.02915 −43.52877 77.9 ± 1.0
2000003 56.04649 −43.51453 65.4 ± 2.3
2000004 56.05139 −43.51837 75.1 ± 2.6
2000005 56.05287 −43.50876 91.2 ± 1.5
2000007 56.06543 −43.50896 65.8 ± 1.6
2000008 56.06747 −43.54544 74.0 ± 0.8
2000010 56.08023 −43.50531 81.7 ± 3.0
2000014 56.08915 −43.50587 77.3 ± 1.1
2000016 56.10013 −43.54549 67.7 ± 0.9
2000017 56.11077 −43.54558 69.5 ± 1.1
2000019 56.11480 −43.54807 75.1 ± 2.4
2000020 56.11801 −43.54748 71.8 ± 0.8
2000021 56.12240 −43.52515 74.7 ± 1.2
2000023 56.12624 −43.51339 79.3 ± 2.4
2000024 56.12985 −43.55450 89.6 ± 1.3
2000025 56.13921 −43.55537 66.7 ± 2.0
2000026 56.16179 −43.50427 74.2 ± 1.8
2000027 56.16557 −43.51079 68.4 ± 2.2
2000028 56.19012 −43.49878 80.5 ± 1.0

Notes. The columns are the source ID, the right ascension and declination in degrees, and the line-of-sight velocity and its measurement uncertainty in km s−1. The source IDs below 2 000 000 are consistent with those in Paper I. Source IDs starting with 2 000 000 are sources from Li et al. (2017) that have no counterpart in the source extraction catalogue of Paper I. The right ascension and declination have been calibrated to Gaia Data Release 2 (Gaia Collaboration 2016, 2018; Lindegren et al. 2018).

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