[daip] 31DEC06 LINUX midnite job (dave, 20060410.034335)

[aipsmgr at aoc.nrao.edu]

dave update report for 31DEC06 on Mon Apr 10 03:44:06 UTC 2006 (UT)

Copies and compiles:

AIPSUPD - Using CVS for copying files.
UPDCVS - cvs update of 31DEC06 completed
UPDCVS - cvs update of TEXT completed
AIPSUPD - UPDCVS apparently worked

UPDCONTROL - /home/AIPS/31DEC06/LINUX/UPDATE/LASTREMOVE.DAT = 20060409.034232
UPDCONTROL - /home/AIPS/31DEC06/LINUX/UPDATE/LASTCOPY.DAT = 20060409.034232
UPDCONTROL - /home/AIPS/31DEC06/LINUX/UPDATE/LASTCOMRPL.DAT = 20060409.034232
UPDCONTROL - /home/AIPS/31DEC06/LINUX/UPDATE/LASTCOMLNK.DAT = 20060409.034232

UPDCONTROL - Everything seems in order

UPDCOMRPL: COMRPLs

09-APR-2006 22:28:58 20060409 TST QOOP     PBUTIL.FOR    egreisen
09-APR-2006 22:29:00 20060409 TST QOOP     QUVUTIL.FOR   egreisen

UPDCOMRPL: currently in /home/AIPS/31DEC06/LINUX/UPDATE
UPDCOMRPL: /home/AIPS/31DEC06/Q/SUB/OOP/PBUTIL.FOR
UPDCOMRPL: /home/AIPS/31DEC06/Q/SUB/OOP/QUVUTIL.FOR

UPDCOMLNK: COMLNKs

09-APR-2006 22:38:23 20060409 TST APLPGM   CPYRT.FOR     egreisen
09-APR-2006 22:29:27 20060409 TST QPGOOP   IMAGR.FOR     egreisen

UPDCOMLNK: currently in /home/AIPS/31DEC06/LINUX/UPDATE
UPDCOMLNK: /home/AIPS/31DEC06/APL/PGM/CPYRT.FOR
UPDCOMLNK: /home/AIPS/31DEC06/Q/PGM/OOP/IMAGR.FOR


UPDCONTROL - Reasons for file updates on Mon Apr 10 03:43:47 UTC 2006 (UT)

09-APR-2006 22:28:51 20060409 TST QOOP     PBUTIL.FOR    spix
09-APR-2006 22:28:53 20060409 TST QOOP     QUVUTIL.FOR   spix
09-APR-2006 22:29:17 20060409 TST QPGOOP   IMAGR.FOR     spix
09-APR-2006 22:29:48 20060409 TST HLPFIL   IMAGR.HLP     spix
09-APR-2006 22:29:52 20060409 TST HLPFIL   SPIXR.HLP     confuses XMOM and itself
09-APR-2006 22:32:53 20060409 TST HIST     CHANGE.DOC    imagr
09-APR-2006 22:38:16 20060409 TST APLPGM   CPYRT.FOR     copy keywords
09-APR-2006 22:40:08 20060409 TST HIST     CHANGE.DOC    cpyrt

CHANGE.DOC entries:

12069.  April 9, 2006             IMAGR                  Eric
        Major new option - to use a spectral index image to alter how
        bandwidth sysnthesis component subtraction is done.  Changed:
        IMAGR    Add FQTOL and IN3NAME and IN4NAME et al adverbs,
                 create SPIX AND SPIXC object and check their
                 existence, add to HI file info.
        IMAGR    HELP file: Change description of IMAGRPRM(1) to
                 mention standard antenna beam models for VLA and
                 ATCA.  Add IMAGRPRM(17) as indicator for spectral
                 index correction and radius of an averaging circle
                 when reading the spix image.  Add IN3NAME, IN3CLASS,
                 IN3SEQ, and IN3DISK to specify a spectral index
                 image and IN4NAME, IN4CLASS, IN4SEQ, and IN4DISK to
                 specify a spectral index curvature image.  Add FQTOL
                 to control how many spectral channels are done at one
                 time when doing the primary beam and spectral index
                 corrections.
        QUVUTIL  Pick up SPIX object and call PBFSUB if there is a
                 SPIX object and/or primary beam correction requested
        POSITION If another POSTION routine was called then PSNANG
                 thought all was well when in fact the pointing
                 position was not set.  Changed all routines that call
                 SETLOC for LOCNUM=1 to zero the pointing position and
                 PSNANG to re-initialize if that position is zero or
                 the class name is different.
        PBUTIL   Changed PBFSUB and PBFDIV to pick up SPIX and FQTOL.
                 The DO loop over channels was replaced with code to
                 do as many channels together as FQTOL would suggest.
                 If the array is VLA or ATCA, PBCALC is called to get
                 the beam parameter numbers.  PBFCCT and PBFSCI have
                 new call sequences to receive the new parameters
                 (PBFINC, PBPARM, SPIX) and to call SPVALU if SPIX is
                 not blank.  PBFACT has a new call sequence to receive
                 the PBFINC, SINDEX, PBPARM parameters.  It sums over
                 the PBFINC channels, uses the PBCALC code if
                 PBPARM(1) is positive, and applies the spectral
                 index including curvature.   The correction for
                 spectral index is limited to the range 0.001 to 1000
                 to avoid gross overflows.  The average value of the
                 PBFINC channels is used compared to the average over
                 all channels to set the scaling for the current set
                 of channels.  SPVALU is new to read the spectral
                 index image(s) and get the value by interpolation or
                 averaging over a circular aperture.
        SPIXR    HELP file - removed some XMOM things, gave necessary
                 help for OPCODE, and math formula for fitting.
        Moved nowhere.
12070.  April 9, 2006              CPYRT                 Eric
        Added call to KEYCOP.
        Moved nowhere.

12071.  April