| Ef | B | yes | Fringe overview of all baselines (all of C181A) including Ef in LL (left for each baseline) and RR (right for each baseline). Legend: white - scheduled, but no data, blue - no fringe, red-green - fringes of different quality. D -- fourfit error, in this case due to mixing upper and lower subbands in the KVN compatibility mode, no real problem with the data. Scans 209, 210, 213-214 are missing from all diagnostic plots due to a difx2mark4 error. They are present in the final correlation products. c181a_FRINGE_RfAnt_Ef_LLRR_AllSrc.pdf Examples of fourfit fringe plots: c181a_No0199_3C273_AB_LL.pdf, c181a_No0199_3C273_AB_LR.pdf,
c181a_No0199_3C273_AB_RL.pdf, c181a_No0199_3C273_AB_RR.pdf c181a_No0208_3C273_AB_LL.pdf, c181a_No0208_3C273_AB_LR.pdf,
c181a_No0208_3C273_AB_RL.pdf, c181a_No0208_3C273_AB_RR.pdf Same for all antennas below unless otherwise noted. | In the plots EVN is "missing" all the baselines except to ALMA or GLT. This is due to a fourfit error, the baselines are missing only from some of the diagnostic plots, but are present in the final correlation products. |
| On | X | yes | c181a_FRINGE_RfAnt_On_LLRR_AllSrc.pdf c181a_No0208_3C273_AX_LL.pdf, c181a_No0208_3C273_AX_LR.pdf,
c181a_No0208_3C273_AX_RL.pdf, c181a_No0208_3C273_AX_RR.pdf | In the plots EVN is "missing" all the baselines except to ALMA or GLT. This is due to a fourfit error, the baselines are missing only from some of the diagnostic plots, but are present in the final correlation products. |
| Ys | Y | yes | c181a_FRINGE_RfAnt_Ys_LLRR_AllSrc.pdf c181a_No0208_3C273_AY_LL.pdf, c181a_No0208_3C273_AY_LR.pdf,
c181a_No0208_3C273_AY_RL.pdf, c181a_No0208_3C273_AY_RR.pdf c181a_No0220_3C273_gY_LL.pdf, c181a_No0220_3C273_gY_LR.pdf,
no RL or RR fringes | As usual, Ys observed LCP only, but it was also recorded as fake RCP, that's why there are common Ys "right" to other antenna's left fringes. In the plots EVN is "missing" all the baselines except to ALMA or GLT. This is due to a fourfit error, the baselines are missing only from some of the diagnostic plots, but are present in the final correlation products. |
| Mh | Z | yes | c181a_FRINGE_RfAnt_Mh_LLRR_AllSrc.pdf c181a_No0208_3C273_AZ_LL.pdf, c181a_No0208_3C273_AZ_LR.pdf,
c181a_No0208_3C273_AZ_RL.pdf, c181a_No0208_3C273_AZ_RR.pdf | In the plots EVN is "missing" all the baselines except to ALMA or GLT. This is due to a fourfit error, the baselines are missing only from some of the diagnostic plots, but are present in the final correlation products. |
| Pv | P | yes | c181a_FRINGE_RfAnt_Pv_LLRR_AllSrc.pdf c181a_No0208_3C273_AP_LL.pdf, c181a_No0208_3C273_AP_LR.pdf,
c181a_No0208_3C273_AP_RL.pdf, c181a_No0208_3C273_AP_RR.pdf c181a_No0220_3C273_AP_LL.pdf, c181a_No0220_3C273_AP_LR.pdf,
c181a_No0220_3C273_AP_RL.pdf, c181a_No0220_3C273_AP_RR.pdf c181a_No0220_3C273_gP_LL.pdf, c181a_No0220_3C273_gP_LR.pdf,
c181a_No0220_3C273_gP_RL.pdf, c181a_No0220_3C273_gP_RR.pdf | In the plots EVN is "missing" all the baselines except to ALMA or GLT. This is due to a fourfit error, the baselines are missing only from some of the diagnostic plots, but are present in the final correlation products. |
| VLBA: Br | b | yes | c181a_FRINGE_RfAnt_Br_LLRR_AllSrc.pdf preliminary: c181a_No0225_3C273_bg_LL.pdf, c181a_No0225_3C273_bg_LR.pdf,
c181a_No0225_3C273_bg_RL.pdf, c181a_No0225_3C273_bg_RR.pdf final: c181a_No0215_3C273_Ab_LL.pdf, c181a_No0215_3C273_Ab_LR.pdf,
c181a_No0215_3C273_Ab_RL.pdf, c181a_No0215_3C273_Ab_RR.pdf c181a_No0220_3C273_bG_LL.pdf, c181a_No0220_3C273_bG_LR.pdf,
c181a_No0220_3C273_bG_RL.pdf, c181a_No0220_3C273_bG_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: Fd | f | yes | c181a_FRINGE_RfAnt_Fd_LLRR_AllSrc.pdf c181a_No0208_3C273_Af_LL.pdf, c181a_No0208_3C273_Af_LR.pdf,
c181a_No0208_3C273_Af_RL.pdf, c181a_No0208_3C273_Af_RR.pdf c181a_No0220_3C273_fG_LL.pdf, c181a_No0220_3C273_fG_LR.pdf,
c181a_No0220_3C273_fG_RL.pdf, c181a_No0220_3C273_fG_RR.pdf c181a_No0230_3C273_fp_LL.pdf, c181a_No0230_3C273_fp_LR.pdf,
c181a_No0230_3C273_fp_RL.pdf, c181a_No0230_3C273_fp_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: Kp | k | yes | c181a_FRINGE_RfAnt_Kp_LLRR_AllSrc.pdf c181a_No0230_3C273_kp_LL.pdf, c181a_No0230_3C273_kp_LR.pdf,
c181a_No0230_3C273_kp_RL.pdf, c181a_No0230_3C273_kp_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: La | l | yes | c181a_FRINGE_RfAnt_La_LLRR_AllSrc.pdf c181a_No0230_3C273_lp_LL.pdf, c181a_No0230_3C273_lp_LR.pdf,
c181a_No0230_3C273_lp_RL.pdf, c181a_No0230_3C273_lp_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: Mk | m | yes | c181a_FRINGE_RfAnt_Mk_LLRR_AllSrc.pdf c181a_No0230_3C273_mp_LL.pdf, c181a_No0230_3C273_mp_RR.pdf,
no LR or RL fringes c181a_No0220_3C273_Gm_LL.pdf, c181a_No0220_3C273_Gm_RR.pdf,
no LR or RL fringes | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: Nl | n | yes | c181a_FRINGE_RfAnt_Nl_LLRR_AllSrc.pdf c181a_No0208_3C273_An_LL.pdf, c181a_No0208_3C273_An_LR.pdf,
c181a_No0208_3C273_An_RL.pdf, c181a_No0208_3C273_An_RR.pdf c181a_No0220_3C273_gn_LL.pdf, c181a_No0220_3C273_gn_LR.pdf,
c181a_No0220_3C273_gn_RL.pdf, c181a_No0220_3C273_gn_RR.pdf c181a_No0220_3C273_Gn_LL.pdf, c181a_No0220_3C273_Gn_LR.pdf,
c181a_No0220_3C273_Gn_RL.pdf, c181a_No0220_3C273_Gn_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: Ov | o | yes | c181a_FRINGE_RfAnt_Ov_LLRR_AllSrc.pdf c181a_No0208_3C273_Ao_LL.pdf, c181a_No0208_3C273_Ao_LR.pdf,
c181a_No0208_3C273_Ao_RL.pdf, c181a_No0208_3C273_Ao_RR.pdf c181a_No0220_3C273_go_LL.pdf, c181a_No0220_3C273_go_LR.pdf,
c181a_No0220_3C273_go_RL.pdf, c181a_No0220_3C273_go_RR.pdf c181a_No0220_3C273_Go_LL.pdf, c181a_No0220_3C273_Go_LR.pdf,
c181a_No0220_3C273_Go_RL.pdf, c181a_No0220_3C273_Go_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| VLBA: Pt | p | yes | c181a_FRINGE_RfAnt_Pt_LLRR_AllSrc.pdf preliminary c181a_No0225_3C273_gp_LL.pdf, c181a_No0225_3C273_gp_LR.pdf,
c181a_No0225_3C273_gp_RL.pdf, c181a_No0225_3C273_gp_RR.pdf final: c181a_No0208_3C273_Ap_LL.pdf, c181a_No0208_3C273_Ap_LR.pdf,
c181a_No0208_3C273_Ap_RL.pdf, c181a_No0208_3C273_Ap_RR.pdf c181a_No0230_3C273_mp_LL.pdf, c181a_No0230_3C273_mp_RR.pdf,
no LR or RL fringes c181a_No0230_3C273_kp_LL.pdf, c181a_No0230_3C273_kp_LR.pdf,
c181a_No0230_3C273_kp_RL.pdf, c181a_No0230_3C273_kp_RR.pdf c181a_No0230_3C273_lp_LL.pdf, c181a_No0230_3C273_lp_LR.pdf,
c181a_No0230_3C273_lp_RL.pdf, c181a_No0230_3C273_lp_RR.pdf c181a_No0230_3C273_fp_LL.pdf, c181a_No0230_3C273_fp_LR.pdf,
c181a_No0230_3C273_fp_RL.pdf, c181a_No0230_3C273_fp_RR.pdf | all VLBA stations were starting recording late, software glitch: low data weight, possible other problems |
| GBT: Gb | G | yes | c181a_FRINGE_RfAnt_Gb_LLRR_AllSrc.pdf preliminary: c181a_No0225_3C273_Gg_LL.pdf, c181a_No0225_3C273_Gg_LR.pdf,
c181a_No0225_3C273_Gg_RL.pdf, c181a_No0225_3C273_Gg_RR.pdf final: c181a_No0220_3C273_AG_LL.pdf, c181a_No0220_3C273_AG_LR.pdf,
c181a_No0220_3C273_AG_RL.pdf, c181a_No0220_3C273_AG_RR.pdf c181a_No0220_3C273_Gm_LL.pdf, c181a_No0220_3C273_Gm_RR.pdf,
no LR or RL fringes c181a_No0220_3C273_Gg_LL.pdf, c181a_No0220_3C273_Gg_LR.pdf,
c181a_No0220_3C273_Gg_RL.pdf, c181a_No0220_3C273_Gg_RR.pdf c181a_No0220_3C273_bG_LL.pdf, c181a_No0220_3C273_bG_LR.pdf,
c181a_No0220_3C273_bG_RL.pdf, c181a_No0220_3C273_bG_RR.pdf c181a_No0220_3C273_Gn_LL.pdf, c181a_No0220_3C273_Gn_LR.pdf,
c181a_No0220_3C273_Gn_RL.pdf, c181a_No0220_3C273_Gn_RR.pdf c181a_No0220_3C273_Go_LL.pdf, c181a_No0220_3C273_Go_LR.pdf,
c181a_No0220_3C273_Go_RL.pdf, c181a_No0220_3C273_Go_RR.pdf c181a_No0220_3C273_fG_LL.pdf, c181a_No0220_3C273_fG_LR.pdf,
c181a_No0220_3C273_fG_RL.pdf, c181a_No0220_3C273_fG_RR.pdf | |
| GLT: Gl | g | yes | c181a_FRINGE_RfAnt_Gl_LLRR_AllSrc.pdf preliminary: c181a_No0225_3C273_bg_LL.pdf, c181a_No0225_3C273_bg_LR.pdf,
c181a_No0225_3C273_bg_RL.pdf, c181a_No0225_3C273_bg_RR.pdf c181a_No0225_3C273_Gg_LL.pdf, c181a_No0225_3C273_Gg_LR.pdf,
c181a_No0225_3C273_Gg_RL.pdf, c181a_No0225_3C273_Gg_RR.pdf c181a_No0225_3C273_gp_LL.pdf, c181a_No0225_3C273_gp_LR.pdf,
c181a_No0225_3C273_gp_RL.pdf, c181a_No0225_3C273_gp_RR.pdf final: c181a_No0215_3C273_Ag_LL.pdf, c181a_No0215_3C273_Ag_LR.pdf,
c181a_No0215_3C273_Ag_RL.pdf, c181a_No0215_3C273_Ag_RR.pdf c181a_No0220_3C273_Ag_LL.pdf, c181a_No0220_3C273_Ag_LR.pdf,
c181a_No0220_3C273_Ag_RL.pdf, c181a_No0220_3C273_Ag_RR.pdf c181a_No0220_3C273_gY_LL.pdf, c181a_No0220_3C273_gY_LR.pdf,
no RL or RR fringes c181a_No0220_3C273_gP_LL.pdf, c181a_No0220_3C273_gP_LR.pdf,
c181a_No0220_3C273_gP_RL.pdf, c181a_No0220_3C273_gP_RR.pdf c181a_No0220_3C273_Gg_LL.pdf, c181a_No0220_3C273_Gg_LR.pdf,
c181a_No0220_3C273_Gg_RL.pdf, c181a_No0220_3C273_Gg_RR.pdf c181a_No0220_3C273_gn_LL.pdf, c181a_No0220_3C273_gn_LR.pdf,
c181a_No0220_3C273_gn_RL.pdf, c181a_No0220_3C273_gn_RR.pdf c181a_No0220_3C273_go_LL.pdf, c181a_No0220_3C273_go_LR.pdf,
c181a_No0220_3C273_go_RL.pdf, c181a_No0220_3C273_go_RR.pdf | Data analysis has shown that GLT recorded in unknown polarization instead of circular (most probably unknown elliptic). At this moment IT SHOULD NOT BE USED FOR ANY POLARIMETRYand in general dealt with very carefully. |
| ALMA: Aa | A | yes | c181a_FRINGE_RfAnt_Aa_LLRR_AllSrc.pdf c181a_No0199_3C273_AB_LL.pdf, c181a_No0199_3C273_AB_LR.pdf,
c181a_No0199_3C273_AB_RL.pdf, c181a_No0199_3C273_AB_RR.pdf c181a_No0208_3C273_AB_LL.pdf, c181a_No0208_3C273_AB_LR.pdf,
c181a_No0208_3C273_AB_RL.pdf, c181a_No0208_3C273_AB_RR.pdf c181a_No0208_3C273_Af_LL.pdf, c181a_No0208_3C273_Af_LR.pdf,
c181a_No0208_3C273_Af_RL.pdf, c181a_No0208_3C273_Af_RR.pdf c181a_No0208_3C273_An_LL.pdf, c181a_No0208_3C273_An_LR.pdf,
c181a_No0208_3C273_An_RL.pdf, c181a_No0208_3C273_An_RR.pdf c181a_No0208_3C273_Ao_LL.pdf, c181a_No0208_3C273_Ao_LR.pdf,
c181a_No0208_3C273_Ao_RL.pdf, c181a_No0208_3C273_Ao_RR.pdf c181a_No0208_3C273_Ap_LL.pdf, c181a_No0208_3C273_Ap_LR.pdf,
c181a_No0208_3C273_Ap_RL.pdf, c181a_No0208_3C273_Ap_RR.pdf c181a_No0208_3C273_AP_LL.pdf, c181a_No0208_3C273_AP_LR.pdf,
c181a_No0208_3C273_AP_RL.pdf, c181a_No0208_3C273_AP_RR.pdf c181a_No0208_3C273_AX_LL.pdf, c181a_No0208_3C273_AX_LR.pdf,
c181a_No0208_3C273_AX_RL.pdf, c181a_No0208_3C273_AX_RR.pdf c181a_No0208_3C273_AY_LL.pdf, c181a_No0208_3C273_AY_LR.pdf,
c181a_No0208_3C273_AY_RL.pdf, c181a_No0208_3C273_AY_RR.pdf c181a_No0208_3C273_AZ_LL.pdf, c181a_No0208_3C273_AZ_LR.pdf,
c181a_No0208_3C273_AZ_RL.pdf, c181a_No0208_3C273_AZ_RR.pdf c181a_No0215_3C273_Ab_LL.pdf, c181a_No0215_3C273_Ab_LR.pdf,
c181a_No0215_3C273_Ab_RL.pdf, c181a_No0215_3C273_Ab_RR.pdf c181a_No0215_3C273_Ag_LL.pdf, c181a_No0215_3C273_Ag_LR.pdf,
c181a_No0215_3C273_Ag_RL.pdf, c181a_No0215_3C273_Ag_RR.pdf c181a_No0220_3C273_Ag_LL.pdf, c181a_No0220_3C273_Ag_LR.pdf,
c181a_No0220_3C273_Ag_RL.pdf, c181a_No0220_3C273_Ag_RR.pdf c181a_No0215_3C273_AG_LL.pdf, c181a_No0215_3C273_AG_LR.pdf,
c181a_No0215_3C273_AG_RL.pdf, c181a_No0215_3C273_AG_RR.pdf c181a_No0220_3C273_AG_LL.pdf, c181a_No0220_3C273_AG_LR.pdf,
c181a_No0220_3C273_AG_RL.pdf, c181a_No0220_3C273_AG_RR.pdf c181a_No0220_3C273_AP_LL.pdf, c181a_No0220_3C273_AP_LR.pdf,
c181a_No0220_3C273_AP_RL.pdf, c181a_No0220_3C273_AP_RR.pdf ______________________________________________________________ | Observed in linear polarization, converted to circular polarization in post-correlation uning PolConvert. For technical reasons the atmospheric correction was applied twice -- both in original ALMA data and during the correlation. Although a special procedure was developed to compensate for this, we found that its application leads to other difficulties, in particular to abnormally high fringe rate jumps, so in the final production run the double atmospheric correction was left as is. |
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