[daip] 31DEC18 LINUX midnite job (dave, 20180123.044309)

[aipsmgr at nrao.edu]

dave update report for 31DEC18 on Tue Jan 23 04:43:20 UTC 2018 (UT)

Copies and compiles:

AIPSUPD - Using CVS for copying files.
UPDCVS - cvs copy of 31DEC18 begun, 1st character means
 - U added, P updated, M your file differs from master
 - C you have a changed file needing work (error!)
 - ? you have a file not on the master (ignore)
U 31DEC18/TIMESTAMP
P 31DEC18/APL/PGM/NOTST/RLDIF.FOR
U 31DEC18/APL/PGM/NOTST/XYDIF.FOR
P 31DEC18/HELP/LSAPROPO.HLP
U 31DEC18/HELP/XYDIF.HLP
P 31DEC18/HIST/CHANGE.DOC
P 31DEC18/UPDATE/COMLNK.UPD
U 31DEC18/UPDATE/COMLNK.UPD.SUM
U 31DEC18/UPDATE/LASTCVS.DAT
P 31DEC18/UPDATE/PUTBCK.UPD
U 31DEC18/UPDATE/PUTBCK.UPD.SUM
P 31DEC18/UPDATE/REASONS.UPD
U 31DEC18/UPDATE/REASONS.UPD.SUM
UPDCVS - cvs update of 31DEC18 completed
UPDCVS - cvs update of TEXT completed
AIPSUPD - UPDCVS apparently worked

UPDCONTROL - /home/AIPS/31DEC18/LINUX/UPDATE/LASTREMOVE.DAT = 20180122.044216
UPDCONTROL - /home/AIPS/31DEC18/LINUX/UPDATE/LASTCOPY.DAT = 20180122.044216
UPDCONTROL - /home/AIPS/31DEC18/LINUX/UPDATE/LASTCOMRPL.DAT = 20180122.044216
UPDCONTROL - /home/AIPS/31DEC18/LINUX/UPDATE/LASTCOMLNK.DAT = 20180122.044216

UPDCONTROL - Everything seems in order

UPDCOMRPL: COMRPLs


UPDCOMRPL: currently in /home/AIPS/31DEC18/LINUX/UPDATE

UPDCOMLNK: COMLNKs

22-JAN-2018 22:45:08 20180122 TST APGNOT   RLDIF.FOR     egreisen
22-JAN-2018 23:25:35 20180122 TST APGNOT   XYDIF.FOR     egreisen

UPDCOMLNK: currently in /home/AIPS/31DEC18/LINUX/UPDATE
UPDCOMLNK: /home/AIPS/31DEC18/APL/PGM/NOTST/RLDIF.FOR
UPDCOMLNK: /home/AIPS/31DEC18/APL/PGM/NOTST/XYDIF.FOR


UPDCONTROL - Reasons for file updates on Tue Jan 23 04:43:14 UTC 2018 (UT)

22-JAN-2018 22:45:00 20180122 TST APGNOT   RLDIF.FOR     error bars
22-JAN-2018 23:25:18 20180122 TST APGNOT   XYDIF.FOR     rldif for linears
22-JAN-2018 23:25:25 20180122 TST HLPFIL   XYDIF.HLP     rldif for linears
22-JAN-2018 23:27:20 20180122 TST HIST     CHANGE.DOC    rldif, xydif

CHANGE.DOC entries:

15125.  January 22, 2018           RLDIF               Eric
        The error bars in the SPECTRAL solution were too large.  One
        wants to give something like the expected error - i.e. divide
        by the sqrt of the number of independent samples.  As a proxy
        for this unknown, I changed it to divide by the sqrt of the
        average number of baselines contributing at each time to the
        computation.  The results are reasonable anyway.
        Moved nowhere.

15126.  January 22, 2018          XYDIF                Eric
        For linear polarization the X-Y phase difference is found from
        source(s) that have U flux but zero V flux.  Applying all
        calibration plus DOPOL but not applying parallactic angle in
        the conversion to Stokes, one gets apparent U and V.  The
        ATAN(-Y/U) is then the phase difference.  XYDIF is much like
        RLDIF except for how it determines the phase difference.
        Moved nowhere.

15127.  January