Summary
 

Observation code	:	vs04c		AIPS Version	:	15OCT99
Date of Observation	:	1997/333		Difmap Version	:	2.3c
Source Name	:	J2139+14		vsop_difmap used	:	Yes
Calibration Source(s)	:	J2253+16
Ground telescopes	:	MP, KA, HO		Model Fitted to data	:	No
Tracking Station(s)	:	TZ		Image made	:	No
Correlator	:	Mitaka

 

Abstract No space fringes were detected due to DQA1 and by extensive search in AIPS. The time avairable for the ground baseline is also quite limited by some unknown problems. Real time Tsys mesuerment is avairable only for Mopra from JPL sgr site. Other antennas are adopted nominal Gain and Tsys. All baselines with Kashima show about 1/3 of the expected amplitude from PL survey. Since we have enough data for this source from the observation in May 1998, I did not try to make image with this limited sampling data. The data contains a short time scan toward J2253+16 by Mopra and Halca in the begining of this observation without sensible fringes, but I do not if the observation for this calbrater by Halca was really tried.

AIPS Input Files

Comments - None -

AIPS Output Files

PRTAN.LIS LISTR.LIS DTSUM_0.LIS DTSUM_1.LIS UVPLT_UV.PS UVPLT_UVD.PS UVPLT_UVPA.PS SN_ACCOR_AMP_1.PS SN_ACCOR_AMP_2.PS SN_APCAL_AMP_2.PS

SN_APCAL_AMP_1.PS SN_FRING1_DEL_1.P SN_FRING1_DEL_2.P SN_FRING1_RAT_1.P SN_FRING1_RAT_2.P SN_FRING1_SNR_1.P SN_FRING1_SNR_2.P SN_CALIB_DEL_1.PS SN_CALIB_DEL_2.PS SN_CALIB_RAT_1.PS

SN_CALIB_RAT_2.PS SN_CALIB_SNR_1.PS SN_CALIB_SNR_2.PS SN_CALIB_PHA_1.PS SN_CALIB_PHA_2.PS POSSM_AP_1.PS POSSM_AP_2.PS