Summary
 

Observation code	:	VS11q		AIPS Version	:	15OCT99
Date of Observation	:	1998/7		Difmap Version	:	2.3c
Source Name	:	J1305-1033		vsop_difmap used	:	Yes
Calibration Source(s)	:	1334-127/
Ground telescopes	:	HA, MP		Model Fitted to data	:	Yes
Tracking Station(s)	:	TZ, GZ		Image made	:	Yes
Correlator	:	Pentictn

 

Abstract This is one of two GRT experiments. Good signal with MP-TZ and HA-GZ. The pase clouser condition is fulfiled only for 10 minites, so selfflag false, 3, 4 was set before the selfcal. The source seems to be compact and amplitude vs. uv-distant plot shows 0.4-0.5 Jy upto 400Mlambda. Eventhough only one baseline is avairable at almost all time, Halca provides not too bad uv-coverage. Model fit was performed with a single circular and a elliptical gassian models, which is consistent with ground images avairable at 2.3GHz and 8GHz. For this simple structure source, further re-observation may not much improve the results. EBF 07-OCT-2005: Did combined selfcal in AIPS. VSOPx1.4 to be more consistent Fit one component and because of VSOP scaling, it is difficult to believe a core diameter. Core <0.20

Model
Flux (Jy)	Radius (mas)	Theta (deg)	Major (mas)	Axial ratio	Phi (deg)	TB (10^12 K)
0.410128	0.0187286	15.7878	0	0	0	0.0000
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.

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_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 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 POSSM01_AP_1.PS POSSM02_AP_1.PS POSSM02_AP_2.PS POSSM01_AP_2.PS POSSM01_AP_3.PS POSSM02_AP_3.PS IMAGE.FITS

More details on the Images and Modelfits are found in this page.