From shibata@hotaka.mtk.nao.ac.jp Mon Jan 11 17:02:39 1999 To: vsog@vsop.isas.ac.jp From: shibata@hotaka.mtk.nao.ac.jp (SHIBATA, Katsunori, M.) Subject: vs09t Cc: bushi@hotaka.mtk.nao.ac.jp, kameno@hotaka.mtk.nao.ac.jp, umemoto@hotaka.mtk.nao.ac.jp, kameya@miz.nao.ac.jp, hkobaya@vsop.isas.ac.jp ======================================== MITAKA Correlation Summary 1999/01/04 Obscode:vs09t Obsdate:1998/08/03 VS09t was treated as v98215 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 'J1540+14'. 5. Cross-correlation bandpass plots were made for baselines in which fringes were detected for scan on 'J1540+14'. NOTES: UZ - No fringe was detected. 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 shibata@hotaka.mtk.nao.ac.jp.