C181F/MJ001B

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Comparing version 04:59, 12 Nov 2018 by yurii with version 06:09, 12 Nov 2018 by yurii.

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Station	Code	Fringes	Plots	Comments
VLBA: Br	b	yes	Fringe overview of all baselines of this antenna 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. c181f_FRINGE_RfAnt_Br_LLRR_AllSrc.pdf Examples of fourfit fringe plots: c181f_No0002_3C279_bp_LL.pdf c181f_No0002_3C279_bp_LR.pdf c181f_No0002_3C279_bp_RL.pdf c181f_No0002_3C279_bp_RR.pdf c181f_No0042_1921-293_Ab_LL.pdf c181f_No0042_1921-293_Ab_LR.pdf c181f_No0042_1921-293_Ab_RL.pdf c181f_No0042_1921-293_Ab_RR.pdf Same for all antennas below unless otherwise noted.
VLBA: Fd	f	yes	c181f_FRINGE_RfAnt_Fd_LLRR_AllSrc.pdf c181f_No0002_3C279_fp_LL.pdf c181f_No0002_3C279_fp_LR.pdf c181f_No0002_3C279_fp_RL.pdf c181f_No0002_3C279_fp_RR.pdf c181f_No0042_1921-293_Af_LL.pdf c181f_No0042_1921-293_Af_LR.pdf c181f_No0042_1921-293_Af_RL.pdf c181f_No0042_1921-293_Af_RR.pdf
VLBA: Kp	k	yes	c181f_FRINGE_RfAnt_Kp_LLRR_AllSrc.pdf c181f_No0042_1921-293_Ak_LL.pdf c181f_No0042_1921-293_Ak_LR.pdf c181f_No0042_1921-293_Ak_RL.pdf c181f_No0042_1921-293_Ak_RR.pdf
VLBA: La	l	yes	c181f_FRINGE_RfAnt_La_LLRR_AllSrc.pdf c181f_No0002_3C279_lp_LL.pdf c181f_No0002_3C279_lp_LR.pdf c181f_No0002_3C279_lp_RL.pdf c181f_No0002_3C279_lp_RR.pdf c181f_No0042_1921-293_Al_LL.pdf c181f_No0042_1921-293_Al_LR.pdf c181f_No0042_1921-293_Al_RL.pdf c181f_No0042_1921-293_Al_RR.pdf
VLBA: Mk	m	yes	c181f_FRINGE_RfAnt_Mk_LLRR_AllSrc.pdf c181f_No0002_3C279_mp_LL.pdf c181f_No0002_3C279_mp_LR.pdf c181f_No0002_3C279_mp_RL.pdf c181f_No0002_3C279_mp_RR.pdf c181f_No0042_1921-293_Am_LL.pdf c181f_No0042_1921-293_Am_LR.pdf c181f_No0042_1921-293_Am_RL.pdf c181f_No0042_1921-293_Am_RR.pdf
VLBA: Nl	n	yes	c181f_FRINGE_RfAnt_Nl_LLRR_AllSrc.pdf c181f_No0002_3C279_np_LL.pdf c181f_No0002_3C279_np_LR.pdf c181f_No0002_3C279_np_RL.pdf c181f_No0002_3C279_np_RR.pdf c181f_No0042_1921-293_An_LL.pdf c181f_No0042_1921-293_An_LR.pdf c181f_No0042_1921-293_An_RL.pdf c181f_No0042_1921-293_An_RR.pdf
VLBA: Ov	o	yes	c181f_FRINGE_RfAnt_Ov_LLRR_AllSrc.pdf c181f_No0002_3C279_op_LL.pdf c181f_No0002_3C279_op_LR.pdf c181f_No0002_3C279_op_RL.pdf c181f_No0002_3C279_op_RR.pdf c181f_No0042_1921-293_Ao_LL.pdf c181f_No0042_1921-293_Ao_LR.pdf c181f_No0042_1921-293_Ao_RL.pdf c181f_No0042_1921-293_Ao_RR.pdf
VLBA: Pt	p	yes	c181f_FRINGE_RfAnt_Pt_LLRR_AllSrc.pdf c181f_No0042_1921-293_Ap_LL.pdf c181f_No0042_1921-293_Ap_LR.pdf c181f_No0042_1921-293_Ap_RL.pdf c181f_No0042_1921-293_Ap_RR.pdf c181f_No0002_3C279_bp_LL.pdf c181f_No0002_3C279_bp_LR.pdf c181f_No0002_3C279_bp_RL.pdf c181f_No0002_3C279_bp_RR.pdf c181f_No0002_3C279_fp_LL.pdf c181f_No0002_3C279_fp_LR.pdf c181f_No0002_3C279_fp_RL.pdf c181f_No0002_3C279_fp_RR.pdf c181f_No0002_3C279_lp_LL.pdf c181f_No0002_3C279_lp_LR.pdf c181f_No0002_3C279_lp_RL.pdf c181f_No0002_3C279_lp_RR.pdf c181f_No0002_3C279_mp_LL.pdf c181f_No0002_3C279_mp_LR.pdf c181f_No0002_3C279_mp_RL.pdf c181f_No0002_3C279_mp_RR.pdf c181f_No0002_3C279_np_LL.pdf c181f_No0002_3C279_np_LR.pdf c181f_No0002_3C279_np_RL.pdf c181f_No0002_3C279_np_RR.pdf c181f_No0002_3C279_op_LL.pdf c181f_No0002_3C279_op_LR.pdf c181f_No0002_3C279_op_RL.pdf c181f_No0002_3C279_op_RR.pdf	Taken out for several scans because of USNO observing.
GBT: Gb	G	no		unrecoverable read error of the Mk5 module, logs indicate bad weather, so this loss is considered non-critical
ALMA: Aa	A	yes	In this case bright red indicates false fringes (detected as the ones having abnormally high single-band delay) that fourfit in this particular case finds for all baselines for which there is no true fringe as a result of a glitch. c181f_SBD_RfAnt_Aa_LLRR_AllSrc.pdf c181f_No0002_3C279_Ap_LL.pdf c181f_No0002_3C279_Ap_LR.pdf c181f_No0002_3C279_Ap_RL.pdf c181f_No0002_3C279_Ap_RR.pdf c181f_No0042_1921-293_Ab_LL.pdf c181f_No0042_1921-293_Ab_LR.pdf c181f_No0042_1921-293_Ab_RL.pdf c181f_No0042_1921-293_Ab_RR.pdf c181f_No0042_1921-293_Af_LL.pdf c181f_No0042_1921-293_Af_LR.pdf c181f_No0042_1921-293_Af_RL.pdf c181f_No0042_1921-293_Af_RR.pdf c181f_No0042_1921-293_Ak_LL.pdf c181f_No0042_1921-293_Ak_LR.pdf c181f_No0042_1921-293_Ak_RL.pdf c181f_No0042_1921-293_Ak_RR.pdf c181f_No0042_1921-293_Al_LL.pdf c181f_No0042_1921-293_Al_LR.pdf c181f_No0042_1921-293_Al_RL.pdf c181f_No0042_1921-293_Al_RR.pdf c181f_No0042_1921-293_Am_LL.pdf c181f_No0042_1921-293_Am_LR.pdf c181f_No0042_1921-293_Am_RL.pdf c181f_No0042_1921-293_Am_RR.pdf c181f_No0042_1921-293_An_LL.pdf c181f_No0042_1921-293_An_LR.pdf c181f_No0042_1921-293_An_RL.pdf c181f_No0042_1921-293_An_RR.pdf c181f_No0042_1921-293_Ao_LL.pdf c181f_No0042_1921-293_Ao_LR.pdf c181f_No0042_1921-293_Ao_RL.pdf c181f_No0042_1921-293_Ao_RR.pdf c181f_No0042_1921-293_Ap_LL.pdf c181f_No0042_1921-293_Ap_LR.pdf c181f_No0042_1921-293_Ap_RL.pdf c181f_No0042_1921-293_Ap_RR.pdf	Observed in linear polarization, converted to circular polarization in post-correlation uning PolConvert. 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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Version from 04:59, 12 Nov 2018

This revision modified by yurii (Ban)

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Version as of 06:09, 12 Nov 2018

This revision modified by yurii (Ban)

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Station	Code	Fringes	Plots	Comments
VLBA: Br	b	yes	Fringe overview of all baselines of this antenna 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. c181f_FRINGE_RfAnt_Br_LLRR_AllSrc.pdf Examples of fourfit fringe plots: c181f_No0002_3C279_bp_LL.pdf c181f_No0002_3C279_bp_LR.pdf c181f_No0002_3C279_bp_RL.pdf c181f_No0002_3C279_bp_RR.pdf c181f_No0042_1921-293_Ab_LL.pdf c181f_No0042_1921-293_Ab_LR.pdf c181f_No0042_1921-293_Ab_RL.pdf c181f_No0042_1921-293_Ab_RR.pdf Same for all antennas below unless otherwise noted.
VLBA: Fd	f	yes	c181f_FRINGE_RfAnt_Fd_LLRR_AllSrc.pdf c181f_No0002_3C279_fp_LL.pdf c181f_No0002_3C279_fp_LR.pdf c181f_No0002_3C279_fp_RL.pdf c181f_No0002_3C279_fp_RR.pdf c181f_No0042_1921-293_Af_LL.pdf c181f_No0042_1921-293_Af_LR.pdf c181f_No0042_1921-293_Af_RL.pdf c181f_No0042_1921-293_Af_RR.pdf
VLBA: Kp	k	yes	c181f_FRINGE_RfAnt_Kp_LLRR_AllSrc.pdf c181f_No0042_1921-293_Ak_LL.pdf c181f_No0042_1921-293_Ak_LR.pdf c181f_No0042_1921-293_Ak_RL.pdf c181f_No0042_1921-293_Ak_RR.pdf
VLBA: La	l	yes	c181f_FRINGE_RfAnt_La_LLRR_AllSrc.pdf c181f_No0002_3C279_lp_LL.pdf c181f_No0002_3C279_lp_LR.pdf c181f_No0002_3C279_lp_RL.pdf c181f_No0002_3C279_lp_RR.pdf c181f_No0042_1921-293_Al_LL.pdf c181f_No0042_1921-293_Al_LR.pdf c181f_No0042_1921-293_Al_RL.pdf c181f_No0042_1921-293_Al_RR.pdf
VLBA: Mk	m	yes	c181f_FRINGE_RfAnt_Mk_LLRR_AllSrc.pdf c181f_No0002_3C279_mp_LL.pdf c181f_No0002_3C279_mp_LR.pdf c181f_No0002_3C279_mp_RL.pdf c181f_No0002_3C279_mp_RR.pdf c181f_No0042_1921-293_Am_LL.pdf c181f_No0042_1921-293_Am_LR.pdf c181f_No0042_1921-293_Am_RL.pdf c181f_No0042_1921-293_Am_RR.pdf
VLBA: Nl	n	yes	c181f_FRINGE_RfAnt_Nl_LLRR_AllSrc.pdf c181f_No0002_3C279_np_LL.pdf c181f_No0002_3C279_np_LR.pdf c181f_No0002_3C279_np_RL.pdf c181f_No0002_3C279_np_RR.pdf c181f_No0042_1921-293_An_LL.pdf c181f_No0042_1921-293_An_LR.pdf c181f_No0042_1921-293_An_RL.pdf c181f_No0042_1921-293_An_RR.pdf
VLBA: Ov	o	yes	c181f_FRINGE_RfAnt_Ov_LLRR_AllSrc.pdf c181f_No0002_3C279_op_LL.pdf c181f_No0002_3C279_op_LR.pdf c181f_No0002_3C279_op_RL.pdf c181f_No0002_3C279_op_RR.pdf c181f_No0042_1921-293_Ao_LL.pdf c181f_No0042_1921-293_Ao_LR.pdf c181f_No0042_1921-293_Ao_RL.pdf c181f_No0042_1921-293_Ao_RR.pdf
VLBA: Pt	p	yes	c181f_FRINGE_RfAnt_Pt_LLRR_AllSrc.pdf c181f_No0042_1921-293_Ap_LL.pdf c181f_No0042_1921-293_Ap_LR.pdf c181f_No0042_1921-293_Ap_RL.pdf c181f_No0042_1921-293_Ap_RR.pdf c181f_No0002_3C279_bp_LL.pdf c181f_No0002_3C279_bp_LR.pdf c181f_No0002_3C279_bp_RL.pdf c181f_No0002_3C279_bp_RR.pdf c181f_No0002_3C279_fp_LL.pdf c181f_No0002_3C279_fp_LR.pdf c181f_No0002_3C279_fp_RL.pdf c181f_No0002_3C279_fp_RR.pdf c181f_No0002_3C279_lp_LL.pdf c181f_No0002_3C279_lp_LR.pdf c181f_No0002_3C279_lp_RL.pdf c181f_No0002_3C279_lp_RR.pdf c181f_No0002_3C279_mp_LL.pdf c181f_No0002_3C279_mp_LR.pdf c181f_No0002_3C279_mp_RL.pdf c181f_No0002_3C279_mp_RR.pdf c181f_No0002_3C279_np_LL.pdf c181f_No0002_3C279_np_LR.pdf c181f_No0002_3C279_np_RL.pdf c181f_No0002_3C279_np_RR.pdf c181f_No0002_3C279_op_LL.pdf c181f_No0002_3C279_op_LR.pdf c181f_No0002_3C279_op_RL.pdf c181f_No0002_3C279_op_RR.pdf	Taken out for several scans because of USNO observing.
GBT: Gb	G	no		unrecoverable read error of the Mk5 module, logs indicate bad weather, so this loss is considered non-critical
ALMA: Aa	A	yes	In this case bright red indicates false fringes (detected as the ones having abnormally high single-band delay) that fourfit in this particular case finds for all baselines for which there is no true fringe as a result of a glitch. c181f_SBD_RfAnt_Aa_LLRR_AllSrc.pdf c181f_No0002_3C279_Ap_LL.pdf c181f_No0002_3C279_Ap_LR.pdf c181f_No0002_3C279_Ap_RL.pdf c181f_No0002_3C279_Ap_RR.pdf c181f_No0042_1921-293_Ab_LL.pdf c181f_No0042_1921-293_Ab_LR.pdf c181f_No0042_1921-293_Ab_RL.pdf c181f_No0042_1921-293_Ab_RR.pdf c181f_No0042_1921-293_Af_LL.pdf c181f_No0042_1921-293_Af_LR.pdf c181f_No0042_1921-293_Af_RL.pdf c181f_No0042_1921-293_Af_RR.pdf c181f_No0042_1921-293_Ak_LL.pdf c181f_No0042_1921-293_Ak_LR.pdf c181f_No0042_1921-293_Ak_RL.pdf c181f_No0042_1921-293_Ak_RR.pdf c181f_No0042_1921-293_Al_LL.pdf c181f_No0042_1921-293_Al_LR.pdf c181f_No0042_1921-293_Al_RL.pdf c181f_No0042_1921-293_Al_RR.pdf c181f_No0042_1921-293_Am_LL.pdf c181f_No0042_1921-293_Am_LR.pdf c181f_No0042_1921-293_Am_RL.pdf c181f_No0042_1921-293_Am_RR.pdf c181f_No0042_1921-293_An_LL.pdf c181f_No0042_1921-293_An_LR.pdf c181f_No0042_1921-293_An_RL.pdf c181f_No0042_1921-293_An_RR.pdf c181f_No0042_1921-293_Ao_LL.pdf c181f_No0042_1921-293_Ao_LR.pdf c181f_No0042_1921-293_Ao_RL.pdf c181f_No0042_1921-293_Ao_RR.pdf c181f_No0042_1921-293_Ap_LL.pdf c181f_No0042_1921-293_Ap_LR.pdf c181f_No0042_1921-293_Ap_RL.pdf c181f_No0042_1921-293_Ap_RR.pdf	Observed in linear polarization, converted to circular polarization in post-correlation uning PolConvert. 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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Table of contents

C181F/MJ001B

Table of contents

Combined revision comparison

Version from 04:59, 12 Nov 2018

Version as of 06:09, 12 Nov 2018

Table of contents