Summary
 

Observation code	:	VS03l		AIPS Version	:	15OCT98
Date of Observation	:	1998/53		Difmap Version	:	2.3c
Source Name	:	J1626-29		vsop_difmap used	:	Yes
Calibration Source(s)	:	1622-253
Ground telescopes	:	Hart, Hobart, Shanghai		Model Fitted to data	:	Yes
Tracking Station(s)	:	TZ		Image made	:	Yes
Correlator	:	Penticton

 

Abstract A-priori calibration looked pretty good for this experiment. Good fringes found on ground-space baselines up to 00:00 UT, then weak fringes seen occasionally. It's possible that these weak fringes (esp after about 0100 UT) are non-detections. In this case, the data may act as an upper limit on flux density and is therefore useful? A two-component model was sufficient to fit this data.

Model
Flux (Jy)	Radius (mas)	Theta (deg)	Major (mas)	Axial ratio	Phi (deg)	TB (10^12 K)
0.390140	0.0254574	116.844	0.310405	1.00000	45.0000	0.1976
0.764621	0.310329	-80.7747	0.718325	0.765078	-52.0007	0.0945
(*) Quoted Brightness temperatures assume Gaussian components and are in the local (z=0) frame.

AIPS Input Files

INDXR.TXT ANTAB.TXT SN6.TXT SN7.TXT

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_2.PS SN_APCAL_AMP_1.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_FRING02_DEL_1.PS SN_FRING02_DEL_2.PS SN_FRING02_RAT_1.PS SN_FRING02_RAT_2.PS SN_FRING02_SNR_1.PS SN_FRING02_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 POSSM01_AP_2.PS

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