Summary
 

Observation code	:	VS08t		AIPS Version	:	15OCT99
Date of Observation	:	1999/092		Difmap Version	:	2.3c
Source Name	:	J1647-64		vsop_difmap used	:	Yes
Calibration Source(s)	:
Ground telescopes	:	HH, MP		Model Fitted to data	:	No
Tracking Station(s)	:	GZ, TZ		Image made	:	No
Correlator	:	Penticton

 

Abstract One of five survey datasets I am reducing that have only two GRT's, to determine if they are useful or require re-observation, following the July 1999 Survey Working Group meeting at ISAS. Fringes between Mopra and Hart and the last timerange between Mopra and HALCA on the shortest projected baselines ** I recommend that this observation be re-scheduled with medium priority since the source is strong enough to be detected on at least some space baselines, should do better with three GRRT experiment **. Had tape reading problem with Penticton tapes - asci junk before FITS header. No VPLOT done. Scan breaks for INDXR not used. CALIB was not run after final fringe-fit, so preliminary fringe-fit plots represent the final delay and rate solutions that were applied to the data.

AIPS Input Files

ANTAB.TXT

Comments Hart and Mopra Tsys data collected from ATNF server and processed into ANTAB format. Default Tsys of 95 deg used for HALCA. Default gain of 0.0062 used for HALCA.

AIPS Output Files

DTSUM_0.LIS DTSUM_1.LIS LISTR.LIS PRTAN.LIS UVPLT_UV.PS SN_APCAL_AMP_1.PS

SN_APCAL_AMP_2.PS SN_FRING01_DEL_1.PS SN_FRING01_DEL_2.PS SN_FRING01_RAT_1.PS SN_FRING01_RAT_2.PS SN_FRING01_SNR_1.PS

SN_FRING01_SNR_2.PS UVPLT_UVD.PS UVPLT_UVPA.PS POSSM01_AP_1.PS POSSM01_AP_2.PS