Multiwavelength picture of the misaligned BL Lac object 3C 371: Table A.1 (online version)

Complete version of Table A.1 from the publication "Multiwavelength picture of the misaligned BL Lac object 3C 371" accepeted in Astronomy & Astrophysics. Authors: J. Otero-Santos, C. M. Raiteri, A. Tramacere, J. Escudero Pedrosa, J. A. Acosta-Pulido, M. I. Carnerero, M. Villata, I. Agudo, I. A. Rahimov, T. S. Andreeva, D. V. Ivanov, N. Marchili, S. Righini, M. Giroletti, M. A. Gurwell, S. S. Savchenko, D. Carosati, W. P. Chen, S. O. Kurtanidze, M. D. Joner, E. Semkov, T. Pursimo, E. Benítez, G. Damljanovic, G. Andreuzzi, G. Apolonio, G. A. Borman, V. Bozhilov, F. J. Galindo-Guil, T. S. Grishina, V. A. Hagen-Thorn, D. Hiriart, H. Y. Hsiao, S. Ibryamov, R. Z. Ivanidze, G. N. Kimeridze, E. N. Kopatskaya, O. M. Kurtanidze, V. M. Larionov, E. G. Larionova, L. V. Larionova, M. Minev, D. A. Morozova, M. G. Nikolashvili, E. Ovcharov, L. A. Sigua, M. Stojanovic, I. S. Troitskiy, Yu. V. Troitskaya, A. Tsai, A. Valcheva, A. A. Vasilyev, O. Vince, E. Zaharieva, and A. V. Zhovtan Table A.1: Modelfit results derived from the VLBI data analysis for all epochs and each identified component. Columns correspond to the identified components, the corresponding epoch, the flux density and the position of the component in milli-arcseconds. Components without an associated name correspond to those used for the modelfitting but not included in our analysis due to high noise, making them not suitable for the kinematic evaluation and for tracing their evolution and continuity. More details on the modelfit results can be consulted in the documentation of difmap.