[daip] 31DEC15 LINUX midnite job (dave, 20150116.044352)

aipsmgr at nrao.edu aipsmgr at nrao.edu
Thu Jan 15 23:44:24 EST 2015


dave update report for 31DEC15 on Fri Jan 16 04:44:24 UTC 2015 (UT)

Copies and compiles:

AIPSUPD - Using CVS for copying files.
UPDCVS - cvs copy of 31DEC15 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 31DEC15/TIMESTAMP
U 31DEC15/APL/PGM/NOTST/HOLOG.FOR
U 31DEC15/HELP/HOLOG.HLP
P 31DEC15/HELP/LSAPROPO.HLP
U 31DEC15/HELP/PANEL.HLP
P 31DEC15/HIST/CHANGE.DOC
P 31DEC15/RUN/VLBARUN.001
P 31DEC15/UPDATE/COMLNK.UPD
U 31DEC15/UPDATE/COMLNK.UPD.SUM
U 31DEC15/UPDATE/LASTCVS.DAT
P 31DEC15/UPDATE/PUTBCK.UPD
U 31DEC15/UPDATE/PUTBCK.UPD.SUM
P 31DEC15/UPDATE/REASONS.UPD
U 31DEC15/UPDATE/REASONS.UPD.SUM
P 31DEC15/UPDATE/WHATISOUT.UPD
U 31DEC15/UPDATE/WHATISOUT.UPD.SUM
U 31DEC15/Y/PGM/PANEL.FOR
UPDCVS - cvs update of 31DEC15 completed
UPDCVS - cvs update of TEXT completed
AIPSUPD - UPDCVS apparently worked

UPDCONTROL - /home/AIPS/31DEC15/LINUX/UPDATE/LASTREMOVE.DAT = 20150115.044228
UPDCONTROL - /home/AIPS/31DEC15/LINUX/UPDATE/LASTCOPY.DAT = 20150115.044228
UPDCONTROL - /home/AIPS/31DEC15/LINUX/UPDATE/LASTCOMRPL.DAT = 20150115.044228
UPDCONTROL - /home/AIPS/31DEC15/LINUX/UPDATE/LASTCOMLNK.DAT = 20150115.044228

UPDCONTROL - Everything seems in order

UPDCOMRPL: COMRPLs


UPDCOMRPL: currently in /home/AIPS/31DEC15/LINUX/UPDATE

UPDCOMLNK: COMLNKs

16-JAN-2015 00:06:21 20150116 TST APGNOT   HOLOG.FOR     egreisen
16-JAN-2015 00:06:26 20150116 TST YPGM     PANEL.FOR     egreisen

UPDCOMLNK: currently in /home/AIPS/31DEC15/LINUX/UPDATE
UPDCOMLNK: /home/AIPS/31DEC15/APL/PGM/NOTST/HOLOG.FOR
UPDCOMLNK: /home/AIPS/31DEC15/Y/PGM/PANEL.FOR


UPDCONTROL - Reasons for file updates on Fri Jan 16 04:44:10 UTC 2015 (UT)

16-JAN-2015 00:02:25 20150116 TST RUNSYS   VLBARUN.001   fix small gotcha if aips notv is used
16-JAN-2015 00:03:10 20150116 TST HIST     CHANGE.DOC    HOLOG, PANEL
16-JAN-2015 00:04:53 20150116 TST HLPFIL   HOLOG.HLP     updated holgr
16-JAN-2015 00:05:08 20150116 TST HLPFIL   PANEL.HLP     panel adjustments from HOLOG
16-JAN-2015 00:05:48 20150116 TST APGNOT   HOLOG.FOR     updated HOLGR
16-JAN-2015 00:06:09 20150116 TST YPGM     PANEL.FOR     panel adjustments/plots from HOLOG output images

CHANGE.DOC entries:

        NEW TASK: Drift (or driven) scans through a source can produce
        in the SN-table gains a plot of the primary beam.  Made a
        version of SNPLT that can fit a 2nd or 4th order polynomial to
        such gains, solving for the time at the peak, the width, and
        the function.
14520.  January 15, 2015          HOLOG                 Eric/Rick
        NEW TASK (sort of)  - a simplified version of HOLGR which i
        will leave alone.  Rick Perley developed the simplifications
        and I have worked over the code.  The most significant changes
        were to make it play well with the UVHOL and PANEL program
        that precede and follow the HOLGR step.  The DFT routine was
        changed to use double precision internally which changed its
        answers at the 1 part in 1000-10000 level.
        Moved nowhere.

14521.  January 15, 2015            PANEL               Eric/Rick
        NEW TASK: Rick's panel.f developed initially by Mkie Kestevan
        was converted into an AIPS task.  The pgplot plots were
        replaced with AIPS plots.  The code was restructured to
        suitable subroutines.  The unformatted file inputs were
        replaced with reading the AIPS images from the AIPS files
        directly and reading text files for the panel layout (if not
        EVLA which is available without a text file).  Blanking under
        the feed legs and subreflector is now handled with a blanking
        image (the V_AMP image from HOLOG).  The task gets some of the
        parameter values (e.g. frequency, mapsize, # pointings) from
        the input image header and offers controls over which plots
        are desired and allows suppresion of portions of the plots
        (grey scale, contours, panel layout).  The fitting routine was
        enhanced to take the masking into account and to avoid
        singular matrices when a panel is fully masked.
        moved nowhere.
14522.  January



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