From shibata@hotaka.mtk.nao.ac.jp Tue Jun 8 23:25:59 1999 To: vsog@vsop.isas.ac.jp From: shibata@hotaka.mtk.nao.ac.jp (SHIBATA, Katsunori, M.) Subject: VSOP : vs04j Cc: bushi@hotaka.mtk.nao.ac.jp, kameno@hotaka.mtk.nao.ac.jp, umemoto@hotaka.mtk.nao.ac.jp, kameya@miz.nao.ac.jp Dear PI, I will sending herewith a PI letter for vs04j. FITS file will be sent to you with 4 mm MT. Best regards, K. M. Shibata Mitaka correlator =========================================== MITAKA Correlation Summary 1999/06/09 Obscode:vs04j Obsdate:1999/04/28 PI: The VSOP Survey Program Address: Institute of Space and Astronautical Science, Hirabayashi Lab. 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229 JAPAN VS04j was treated as v99118 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 between Shanghai and other stations. 4. Autocorrelation bandpass plots were generated for all antennas for scan on 'J1048+71'. 5. Cross-correlation bandpass plots were made for baselines between Shanghai and other stations for scan on 'J1048+71'. NOTES: TZ - Delay jump at about 02:40. NT - Did not observe. TR - VLBA to VSOP tape copies had not well down in the reverse path because of recording qualities. No fringe was found during 01:32 - 03:30. S/N ratios are very low. SH - A spurious was shown in auto-correlation of IF1. 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.