From shibata@hotaka.mtk.nao.ac.jp Wed Feb 17 15:26:45 1999 To: vsog@vsop.isas.ac.jp From: shibata@hotaka.mtk.nao.ac.jp (SHIBATA, Katsunori, M.) Subject: VSOP: vs02b Cc: nakagawa@hotaka.mtk.nao.ac.jp, bushi@hotaka.mtk.nao.ac.jp, kameno@hotaka.mtk.nao.ac.jp, umemoto@hotaka.mtk.nao.ac.jp, kameya@miz.nao.ac.jp, shibata@hotaka.mtk.nao.ac.jp Dear PI, I will sending herewith a correlation summary for VSOP SURVEY vs02b. You will recieved one DATA tape soon. Please let me know, if you have any trouble in our FITS data. Best regards, Shibata, K.M. Mitaka Correlator, NAOJ ======================================== MITAKA Correlation Summary 1999/02/15 Obscode:vs02b Obsdate:1998/02/04 PI: The VSOP Survey Program Address: Institute of Space and Astronautical Science, Hirabayashi Lab. 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229 JAPAN VS05a was treated as v98035 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 'J1613+34'. 5. Cross-correlation bandpass plots were made for baselines in which fringes were detected for scan on 'J1613+34'. NOTES: GZ - No fringes during 21:50 - 22:10. TZ - No fringes during 00:00 - 00:20. KA - No fringes during 19:00 - 21:20 and 21:45 - 01:30 or weak fringes. 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 shibata@hotaka.mtk.nao.ac.jp.