Phase-Reference VLBI Observations of the Compact Steep-Spectrum Source 3C 138
Phase-Reference VLBI Observations of the Compact Steep-Spectrum Source 3C 138
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DOI:
10.1093/pasj/58.6.1033
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发表时间:
2006-11
影响因子:
2.3
通讯作者:
Zhi-qiang Shen;L.-L. Shang-L.;D. Jiang;H. Cai;X. Chen
中科院分区:
文献类型:
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作者:
Zhi-qiang Shen;L.-L. Shang-L.;D. Jiang;H. Cai;X. Chen
We describe a phase-reference VLBI observation that was conducted at 15.4 GHz by fast-switching VLBA antennas between the compact steep-spectrum radio source 3C 138 and the quasar PKS 0528 + 134, which are about 4 degrees away on the sky. By comparing the phase-reference mapping with the conventional hybrid mapping, we demonstrate the feasibility of high-precision astrometric measurements for sources separated by 4 degrees. VLBI phase-reference mapping preserves the relative phase information, and thus provides an accurate relative position between 3C 138 and PKS 0528 + 134 of Delta alpha = -9(m)46.(s)531000 +/- 0.(s)000003 and Delta delta = 3 degrees 6'26."90311 +/- 0."00007 (J2000.0) in right ascension and declination, respectively. This gives an improved position of the nucleus (component A) of 3C 138 in J2000.0 to be RA = 05(h)21(m)09.(s)885748 and Dec = 16 degrees 38'22."05261 under the assumption that the position of calibrator PKS 0528 + 134 is correct. We further made a hybrid map by performing several iterations of CLEAN and self-calibration on the phase-referenced data with the phase-reference map as an input model for the first phase self-calibration. Compared with the hybrid map from the limited visibility data directly obtained from fringe fitting 3C 138 data, this map has a similar dynamic range, but a higher angular resolution. Therefore, the phase-reference technique is not only a means of phase connection, but also a means of increasing the phase coherence time, and thus allowing the self-calibration technique to be applied to much weaker sources.