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.

本内容为已被《Astronomy & Astrophysics》（《天文学与天体物理学》）录用的论文《错列BL Lac天体3C 371的多波段图景》中的表A.1完整版本。

作者：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 及 A. V. Zhovtan

表A.1：基于甚长基线干涉测量（Very Long Baseline Interferometry, VLBI）数据分析得到的所有观测时段及各已识别辐射成分的模型拟合结果。各列依次对应已识别的辐射成分、对应观测时段、成分的流量密度以及以毫角秒为单位的位置坐标。未附带名称的成分为那些参与模型拟合，但因噪声过高未被纳入本次分析的对象，因此不适用于运动学评估，也无法用于追踪其演化与连续性。有关模型拟合结果的更多细节可查阅Difmap软件的官方文档。