Prudil, Z.Z.Prudil0000-0002-9934-1352Hanke, M.M.Hanke0000-0003-0376-6928Lemasle, B.B.Lemasle0000-0001-7511-2830Crestani, J.J.Crestani0000-0001-8209-0449Braga, V. F.V. F.Braga0000-0001-5829-111XFABRIZIO, MicheleMicheleFABRIZIO0000-0003-4788-677XKoch-Hansen, A. J.A. J.Koch-HansenBono, G.G.BonoGrebel, E. K.E. K.GrebelMatsunaga, N.N.MatsunagaMarengo, M.M.MarengoOliveira Da Silva, RonaldoRonaldoOliveira Da SilvaDall'Ora, M.M.Dall'OraMartinez-Vazquez, C. E.C. E.Martinez-VazquezALTAVILLA, GiuseppeGiuseppeALTAVILLALala, H.H.LalaChaboyer, B.B.ChaboyerFerraro, I.I.FerraroFiorentino, G.G.FiorentinoGilligan, M.M.GilliganNonino, C.C.NoninoThevenin, F.F.Thevenin2025-04-102025-04-102021http://hdl.handle.net/20.500.12386/37040In our investigation, we identified 20 RR Lyrae variables (13 RRab and 7 RRc-type pulsators) to be associated with the Orphan stream based on their equatorial coordinates, proper motions, and distances, listed in table D1. <P />We recovered 54 nonvariable stars likely associated with the Orphan stream as traced by our sample of RR Lyrae variables (listed in Table D.2). <P />(2 data files).en10.26093/cds/vizier.36480078https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/648/A782021yCat..36480078PFIS/05 - ASTRONOMIA E ASTROFISICA