From shibata@hotaka.mtk.nao.ac.jp Mon Feb 14 01:47:01 2000
To: vsog@vsop.isas.ac.jp
From: shibata@hotaka.mtk.nao.ac.jp (SHIBATA, Katsunori, M.)
Subject: VSOP : vs02y
Cc: nakagawa@hotaka.mtk.nao.ac.jp


Dear PI, 

I will sending herewith a PI letter for vs02y. 
FITS file will be sent to you with 4 mm MT. 

Best regards, 

K. M. Shibata
Mitaka correlator

===========================================
MITAKA Correlation Summary  2000/02/10

Obscode:vs02y
Obsdate:1999/05/22

PI:       The VSOP Survey Program

  Address:  Institute of Space and Astronautical Science, Hirabayashi Lab.
            3-1-1 Yoshinodai, Sagamihara, Kanagawa 229
            JAPAN

VS02y was treated as v99142 during correlation. 
We made the following Data quick look. 

1. Baselines vs. time plots and u-v plots were made for each correlation path. 

2. Delay residuals and rate residuals plots were made for all stations.
These were the results of fringe finding, so the station in which fringes
were not found showed large scattering. 

3. Amplitude and phase plots were made for baselines in which fringes were
detected. 

4. Autocorrelation bandpass plots were generated for all antennas for scan
on 'J0836-20'. 

5. Cross-correlation bandpass plots were made for baselines in which
fringes were detected for scan on 'J0836-20'. 

NOTES: 

CD - Not observed. 

KA - Not observed. 

UZ - Fringes were detected during 09:20 - 11:25.

TZ - No fringe was detected.

NOTES for REDUCTION:
The unit of output amplitude is arbitrary. Use ACCOR just after loading to
the AIPS. 

Set DIGICOR = -1 and DELCORR = -1 in FITLD. 

Delete NX and CL tables just after FITLD, then re-build by INDXR. 

DO NOT use PHNEG!!  These FITS data are no longer necessary to use PHNEG. 

IF YOU HAVE ANY QUESTION AND PROBLEM ABOUT FITS DATA, please contact with 
mtkfx@hotaka.mtk.nao.ac.jp.