Summary
 

Observation code	:	VS03l		AIPS Version	:	19OCT99
Date of Observation	:	1998/53		Difmap Version	:	2.3c
Source Name	:	J1626-29		vsop_difmap used	:	Yes
Calibration Source(s)	:	1622-253
Ground telescopes	:	HH, HO, SH		Model Fitted to data	:	Yes
Tracking Station(s)	:	TZ		Image made	:	Yes
Correlator	:	Penticton

 

Abstract Among three ground telescopes, HA, HO, SH, the Shanghai is the only telescope with which I could find Space fringes. However the signal becomes remakably lower as the SC goes away. The source is hevily resolved with longer baselines with Halca.

Model
Flux (Jy)	Radius (mas)	Theta (deg)	Major (mas)	Axial ratio	Phi (deg)	TB (10^12 K)
0.639063	0.0283747	120.731	0.371423	1.00000	-15.9454	0.2261
0.230924	0.437951	-82.9746	0.371875	0.835242	-54.3114	0.0976
0.0381851	1.51448	-92.3920	0.106620	1.00000	-59.7436	0.1639
(*) 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_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_FRING03_DEL_1.PS SN_FRING03_DEL_2.PS SN_FRING03_RAT_1.PS SN_FRING03_RAT_2.PS SN_FRING03_SNR_1.PS

SN_FRING03_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 POSSM_AP_1.PS POSSM_AP_2.PS

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